Saturday, 23 February 2013

How To Install Aptoide For Android System Mobiles & Tabs

 
 
 
Aptoide is an open source approach to repositories in Android. With Aptoide you can create your own repositories of applications, and use the client to download, remove and update them, from your's or others repositories.

Install Aptoide now!

To finish Aptoide installation follow the steps:

Download de APK file to your device clicking in the button "Aptoide download"
After the download is complete, go to the notification bar and press the application name (Aptoide.apk) to start installing Aptoide
If this dialog is showing, go to Settings

And allow the installation of apps from unknown sources
Press "Install" to finish the installation

Saturday, 9 February 2013

Apple MacBook Password Recovery

I had an interesting task at work last week. I had to remove pasword from a MacBook. Doesn’t sound like much., his family, his work and his interests. None of them worked. This called for a more subversive approach.
I did some searching on Google and found a page that discusses how to hack passwords on a Mac. Various methods suggested on several pages of comments to that page had failed. Figuring I had nothing to lose I decided to try mixing the methods I had found until I found one that worked. I figured if I hosed the machine at this point it wouldn’t be a big deal. The machine was useless to me in it’s current state anyway so I would have had no qualms about clearing the hard drive and starting from scratch. The only reason I was still going at it was for the challenge. So off I went.
After only about 2 or 3 tries I came across the following method that worked for me:
  1. Click Restart at the login window
  2. While the computer is restarting, hold down “Command-S” until you see text scrolling through the window. This boots the computer into single user mode.
  3. At the Localhost% prompt type:
    /sbin/fsck -y [Enter]
    /sbin/mount -uw / [Enter]
    sh /etc/rc[Enter]
  4. When the Localhost% prompt reappears, type:
    passwd [username]
    (Replace [username] with the username you want to change and leave out the brackets.)
    You will then be prompted to type a new password for this user 2 times.
  5. After entering the new password, type:
    reboot
  6. At the login window, enter the username with the new password.Voila!

Mac OS X Password Recovery


Instructions for the Mac OS X Password Recovery.
Although there’s no real way to recover a lost root password, you can change the root password even if you do not know the current one. You must have physical access to the machine in order to accomplish this task.

1. Click Restart at the login window
2. While the computer is restarting, hold down “Command-S” until you see text scrolling through the window. This boots the computer into single user mode.
3. At the Localhost% prompt type:
/sbin/fsck -y
/sbin/mount -uw /
/sbin/SystemStarter
You will then see various services starting up.
4. When the Localhost% prompt reappears, type:
passwd [username]
It will then ask you to type the new root password twice, so do so.
(Though I’ve not tried it, it appears you can type niutil -list . /users to get a list if users if you do not know the username….if someone wants to verify this, I would be most appreciative).
5. After entering the new password, type:
reboot
6. At the login window, enter the username with the new password. Once you are logged in, you can use the Multiple Users application (/Applications/Utilities) to change your user’s password, or create a new user account.
Note: this may not work for newer versions of OS X; I think they did something about it in a security update.

What Is 3G Technology ?

3G technology is a standard of cellular phone service first approved by the International Telecommunication Union in 1999. The term 3G stands for third generation, as this level of technology follows two earlier mobile telecommunications standards, 1G and 2G. 1G was analog technology used mainly in the 1980s, while 2G, used primarily in the 1990s, was digital but only allowed voice and limited data functionality. Also known as International Mobile Telecommunications-2000, or IMT-2000, 3G offers several advantages over these previous iterations.
One of the benefits of using 3G technology is its capability to allow users access to voice and data functions at the same time. In addition to supporting traditional wireless phone calls and text messaging, Web-based applications such as streaming video, e-mail, and video conferencing are also supported. Phones designed to work with 3G, commonly known as smartphones, can also be used to browse the Internet and download data files. This allows users much more freedom to perform tasks, do work, and have access to information while they are mobile.
Another advantage of 3G technology is a faster rate of data transfer. Due to use of greater bandwidth and higher transfer rates, transmission of data is much faster than with 1G or 2G phones. Potential speed with 3G is around two to three Mbps; when compared to 2G’s maximum 144 Kbps, this is a significant increase.

Additional security features are another benefit of 3G technology. Encryption of data being transmitted is stronger and more robust than on the older 2G technology, using algorithms such as Kasumi and Advanced Encryption Standard, or AES. Equipment can also authenticate that it is accessing the correct network. Users can also choose to incorporate a VPN connection to add even more security for the data they are transmitting.
In order to offer 3G technology, wireless carriers were required to upgrade their infrastructure to allow for the greater bandwidth it requires. Some operators have had to expand the capabilities of existing networks and equipment, while others have had to build new ones. In some areas, it was necessary to license new radio frequencies to carry the signal. Due to the costs associated with all of these upgrades, rollout of 3G was at times delayed in some places. The first country to develop the capability and launch 3G was Japan in 2001, with other countries throughout the world following in the next few years.

What is Geocaching ?

Geocaching is a relatively new activity that combines hiking, treasure-hunting and the Global Positioning System (GPS). For more information on GPS,
Geocaching involves two separate parties, which are composed either of individuals or groups. One party hides a cache anywhere in the world and records the latitudinal and longitudinal coordinates using a portable GPS device. The cache is usually composed of a small plastic container that houses some small items such as toys or coins.
The coordinates and related information regarding the location of the hidden cache are publicized, usually on internet sites such as geocaching.com. Geocachers search for these hidden caches using their own portable GPS devices in conjunction with maps and clues. When they finally discover the cache, they may take a few of the items and leave a few different ones for future geocachers.
Geocaching is a popular new hobby and provides yet another reason to explore the world around us. Discovering a hidden cache after a long search is a surprisingly rewarding event. There are thousands of caches all over the world waiting to be discovered by anyone who wants to participate.

As geocaching becomes more and more popular, some participants are adding new levels of complexity to keep it interesting. For excample, some geocachers hide caches in particularly difficult locations such as underwater or up in a tree. Some geocachers hide caches in series such that a first cache includes instructions to discover another cache and so on.

What Is Natural Gas ?

Natural gas is a highly combustible odorless and colorless hydrocarbon gas largely composed of methane. It is produced in pressurized deposits located deep in the Earth's crust, commonly located just above oil deposits. The gas is created in roughly the same manner as oil, by geologic processes that act upon organic matter over millions of years. High combustibility coupled with low emissions makes it a highly valued resource. More economical than electricity, natural gas is primarily used for heating homes, cooking and running appliances such as water heaters and clothes dryers.
Early civilizations had an interesting relationship with natural gas. As it seeped from deep within the earth, occurrences such as lightening strikes occasionally ignited it. To ancient peoples, fire issuing from between rocks or from shallow marshlands with no visible combustible source took on divine or supernatural significance. One famous example is the legend of the "eternal flame" of Mount Parnassus, discovered by a Greek goat herder some 3,000 years ago. The temple of the Oracle of Delphi was purportedly erected around the fire, and the priestess issued prophecies inspired by the miraculous flames.
By 500 B.C., the Chinese found a way to put this gas to good use by creating rudimentary pipelines with bamboo stalks. Pinpointing areas where it was escaping the earth, they channeled the gas to fuel fires beneath pots of boiling seawater in order to make distilled drinking water.

In 1785, the United Kingdom commercialized an alternative natural gas manufactured from coal. Production spread to the United States after the turn of the century, but coal-manufactured gas was less clean and less efficient. In 1821, William Hart of New York dug the first well looking for naturally occurring gas and the first American gas company soon followed. Robert Bunsen invented the Bunsen burner in 1885, and by 1938 natural gas was a regulated resource in the United States.
Aside from natural deposits, tiny microorganisms called methanogens produce natural gas by breaking down organic matter. Methanogens reside in the intestines of humans and many animals, including cattle, and can also be found near the surface of the Earth in anaerobic conditions. These microorganisms are responsible for landfill gas, more properly termed biogenic methane, as distinguished from thermogenic methane, or deposited gas. Though a great deal of natural gas escapes into the air from various biogenic sources, efforts are underway to develop technology that can harvest it from unconventional sources. This would compliment natural deposits, which by some estimates are quite extensive.
According to the Energy Information Administration's data as of 2006, Russia has about 27% of the world's total reserves for deposited natural gas — the most of any single country. The Middle Eastern countries collectively have about 40% of the world's total reserves, with Iran having the greatest portion (about 14%). Africa and Asia each have around 8% with Asia having just a bit more than Africa. Central and South America together have about a 4% share — about the same as the United States.


Just Hit The Share Button It Doesn't Bite Your Finger 

What is Food Poisoning ?

When one eats food that contains agents not meant for consumption, the result is often food poisoning. It ranges from mild illness, which ceases on its own, to severe and life-threatening illness, depending upon the cause. One can get food poisoning from eating foods that are poisonous if improperly prepared, food that is prepared by someone with a highly contagious virus, or food contaminated with numerous types of bacteria. Some people may even contract food poisoning from eating foods that contain a high amount of pesticides, or parasites. In many cases, food poisoning can be prevented by appropriate handwashing and safe preparation of food.



A few items can cause accidental and quite serious food poisoning. One risky food is wild mushrooms, particularly when harvested by non-experts. Certain mushrooms like the death cap may be accidentally eaten and can cause near fatal results. Ingesting it can cause liver failure, and many people who accidentally eat one end up needing a liver transplant. Another food of this type is the blowfish, which if improperly prepared contains a highly toxic poison that can result in death.
Certain viruses can cause food poisoning if the cook does not vigilantly wash his hands, particularly after using the bathroom. Norovirus is a common one, and has been the cause of many cases of mass food poisoning on cruise ships. Rotavirus and Hepatitis A can also be contracted in this manner. In most cases, the person preparing the food gets their own fecal matter into the food by not washing his/her hands properly. Most of these illnesses cause a few days to weeks of upset stomach, nausea, diarrhea and fever. However, young children can become significantly ill with Hepatitis A and with Rotaviruses and may require hospitalization and intravenous fluids.
Bacteria causing food poisoning is quite common. In many cases, such bacteria make a person sick for 24-48 hours with nausea and vomiting. Salmonella and campylobacter are common bacteria responsible for food poisoning. Salmonella tends to result from food that is improperly stored or in undercooked foods like eggs and poultry. Raw chicken, or raw milk may also cause Campylobacter. Though most get over food poisoning from these bacteria in a few days, young children and people with immune deficiencies may have much more severe reactions a few weeks after ingesting the bacteria.
Staphylococcus aureus can grow on foods that are not refrigerated properly. Shigella may result from water that is exposed to human waste, resulting in Traveler's Diarrhea. Vibrio Cholerae may result from eating undercooked seafood, and tends to most affect children. Botulism, listeria, and E. Coli are among the most severe of the bacteria borne types of food poisoning. Listeria is often found on fruits and vegetables and deli products, and spores of botulism can especially affect very young children and the immunosuppressed, and may be found in foods like honey.
Food poisoning due to E. Coli often is contracted from eating hamburger that is still pink or is raw. Since much of today’s ground beef contains E. Coli, the safest way to prepare it is by making sure the hamburger is no longer pink and that the juices run clear. Eating raw beef should be avoided. This should effectively help eliminate hamburger as a food poisoning source. Clearly, not placing the raw hamburger on dishes that will be reused before washing is also important.
If you suspect food poisoning, and you have not recovered in 12-24 hours, you may want to see your doctor. First you may be dehydrated from all that vomiting and diarrhea. Second, it’s hard to know exactly what bacteria or other agent poisoned you. Especially children and people with compromised immune systems should see a doctor if they suspect food poisoning.
Further, minimize food poisoning risks by avoiding foods that are known to be poisonous, washing hands and kitchen surfaces thoroughly while preparing food, keeping food refrigerated appropriately, and cooking food properly. Drink bottled water when you are traveling or hiking. If you are ill and work in the food industry, it is best to avoid working when you have a stomach virus.


Just Hit The Share Button It Doesn't Bite Your Finger 

What is Gene Expression ?

Gene expression is the process of how a gene works within a cell. Researchers study gene expression to look into the relationships between small individual differences in DNA and different responses to medications, or risks for diseases. Gene expression has been a major focus of pharmaceutical research. Obesity and risk for heart disease are two examples of topics where it is an important focus of research.
Every cell contains DNA and genes in its nucleus. Genes are the specific instructions for cells that make every person and organism unique. Cells contain many genes, and not all of them are active. Within any given cell, some genes will be “on” or “off.” When a gene is “on,” it is making proteins or RNA products and affecting the functioning of the organism in some way. If a gene is “on,” scientists consider that it is being expressed.
The “on” and “off” state of all a cell’s genes is called its gene expression profile. Each cell has a unique gene expression profile. Research methods called gene expression profiling can identify which genes in a cell or tissue sample are “on” or “off.” Then, expression profiling is used to tell researchers which genes are playing a role in the condition under study.
For example, scientists might use gene expression to study obesity. Scientists work to see if they can figure out the patterns of small genetic differences between people who are obese and those of normal weight, controlling for environmental factors like diet and exercise. If they can figure out these patterns, it could lead to drugs that help control obesity.
They might do this by designing a study that compares gene expression for groups of individuals that are obese and of normal weight but have similar heights, exercise habits, and diets. Comparing gene expression between these two groups might identify which genes are implicated in obesity. Once these genes are identified, researchers can work on developing diagnostic tests for genetic predispositions, and drugs to treat or prevent obesity. These drugs could work either by inhibiting the genes that are implicated in obesity from working, or by interacting with DNA in cells and tissues to turn different genes “on” or “off.”

What is a Nucleus ?

The term “nucleus” is used in several different ways in the sciences, although all cases reference a critical structure found at the center of something. In fact, the word “nucleus” means “kernel” or “core,” and it comes from an Ancient Greek word meaning “nut.” As a general rule, the nucleus is so critical that the surrounding structure cannot survive without it.
In biology, the nucleus is a small structure located inside the cells of eukaryotic organisms. The cell nucleus is actually one of the defining characteristics of eukaryotes, as the structure allows cells and organisms to reach a very high level of complexity. This structure without the cell contains the organism's DNA, and the nucleus is responsible for regulating gene expression, duplicating DNA as needed, and passing on hereditary traits, in the case of egg and sperm cells.
This structure was identified in cells in the early 1800s, when microscopes had finally progressed enough to allow scientists to observe the detailed and complex interiors of cells. Like other parts of the cell, nuclei are involved in the cell cycle, which includes reproduction of the cell and eventual cell death as the various components of the cell age. In stained microscope slides, the cell nuclei are usually very easy to see, thanks to the fact that DNA can be stained with a specific color to make it stand out, highlighting this structure within the cell.

In physics, the nucleus is the core of an atom. Atomic nuclei are extremely dense, containing most of the weight of the atom in the form of particles known as protons and neutrons. Electrons orbit around the atomic nucleus. Depending on the arrangement of particles within the atom, it may be extremely stable, or it may be unstable, in which case the atom can gain or lose particles, generating radioactivity. The application of “nucleus” to physics dates to the early 20th century, when physicists began exploring atoms and elements with the benefit of new technology which made such study possible.
Because nuclei are associated with the “control center” or “core” in the sciences, people sometimes refer to central structures or events as nuclei. For example, someone might say that the boiler room is the “nucleus” of the campus heating system. The older sense of “kernel” or “seed” may also be referenced when people discuss key items or events which lead to larger happenings, such as a piece of art which forms the foundation of a collection, or a protest which triggers widespread social awareness of a political issue.

What is Astronomy ?

Astronomy is the study of celestial objects, phenomena, and origins. One of the oldest sciences, astronomy has been practiced since prehistoric times. Modern astronomy depends highly on accepted physical theories, such as Newton's Laws of Motion and general relativity. In the past, astronomy was something anyone could do, and many seers and sages made reputations for themselves by using the stars for useful functions, such as telling what time of the year it is, or navigating the seas. Columbus and his contemporaries used the stars to navigate across the Atlantic ocean.
It wasn't until the Renaissance that the theory of heliocentricity in astronomy, the idea that the Earth orbits the Sun rather than vice versa, began to acquire popular currency. Reflecting telescopes were invented in the early 1600s, and Galileo Galilei used them to take detailed observations of our Moon, which he revealed was mountainous, and observe Jupiter's four largest moons, now named the Galilean moons in his honor. Newton improved on Galileo's design, inventing the reflecting telescope, which is still used in optical telescopes to this day.
IN 1781, Sir William Herschel discovered the planet Uranus. In 1838, parallax — the slight difference in stellar position due to Earth's location in its orbit — was used to precisely determine the distance of stars. Neptune was discovered shortly thereafter. Pluto was discovered only as recently as 1930.


Modern astronomy is very complicated and expensive. Instead of only observing light rays, we observe radar, infrared, x-rays, and even cosmic rays. Orbital observatories such as the Hubble Space Telescope have produced the best images, include extremely high-resolution photographs of other galaxies.
In the mid-20th century, it was discovered that the universe was expanding. This, along with other evidence, led to the theory of the Big Bang, that the entire universe began as a point particle of extreme density. Later observations of the cosmic microwave background confirmed this, and the Big Bang continues as the primary theory of cosmological origins to this day.
The future of astronomy lies in the development of new observational technologies. One of interest is interferometry, sometimes called "hypertelescopes," which use a network of telescopes working cooperatively to resolve images. These could develop to the point where we can observe extrasolar planets with telescopes directly, instead of just detecting them from their gravitational signature.

Just Hit The Share Button It Doesn't Bite Your Finger 

Is Cell Tower Radiation Dangerous? (Mobilephone Signal towers)

Cellphone Tower Exposure Overview
What happens when human population centers are flooded with massive amounts of powerful wireless microwave radiation? Nobody knows…yet.
But we will soon. Because you’re exposed to 100 million times more Electromagnetic radiation than your grandparents were, and cell towers are making that number grow exponentially. If you can make a call on your cellphone, then you’re in an area that’s saturated with cell site microwave radiation.

Some of the most powerful cell tower installations are on mountains and hilltops outside of urban areas. These EM fields have impacted humans, animals as well as the ecological balance. Studies of people and farm animals living around high voltage wires point to extreme hazards of living up up-close to a powerful electromagnetic field (EMF) - exhibiting everything from stress and sleep disorders to birth defects, cancer and Alzheimer’s. All cell site exposure risks.
EMFs from cell phone towers are impossible to escape, but you can protect yourself with laboratory-proven SafeSpace products. We’ll examine this problem and look at recommended SafeSpace solutions below.
Electromagnetic Spectrum Exposure Diagram
Body resonates with the earth's magnetic field at 10Hz
A Closer Look at Cell Tower Exposure
Cell towers (or cell sites) that hold antennas and other communications equipment. They flood the area for miles around with powerful high frequency radio waves (known as microwaves) to support the use of cellphones as well as Wi-Fi, WiMax, Wireless LANs, 802.11 networks, Bluetooth supported devices, and more.
Cell towers (known as mobile phone masts (Britain) or base stations) typically contain transmitter/receivers transceivers, control electronics, a GPS receiver for timing, digital signal processors as well as various types of electrical power sources.
These microwaves might travel for as few as 2 miles in hilly areas, and up to 45 miles where there are fewer obstructions, and of course, they easily penetrate brick and metal.
Other forms of cell towers include:
Radio masts - Smaller versions of cell towers, often seen on rooftops and billboards, typically installed 800-1300 feet apart.
Mobile towers - Sometimes installed on the tops of buildings. Mobile towers are also used where there have been natural disasters, or when large numbers of people are temporarily expected (i.e. a major sports event)
Mobile towers are especially dangerous because they emit microwaves at a frequency of 1900 MHz. Recent studies have shown that the intense radioactivity from mobile phone towers adversely impacts every biological organism within 1 square kilometer.
Fact About Cell Towers And Cell Sites
  • The International Association for the Wireless Telecommunications Industry Worldwide estimates there are over 3 billion cell phone users.
  • In the U.S. alone, there are hundreds of thousands of cell phone towers.
  • If you type your address into AntennaSearch.com to locate the current and planned towers within eight miles of you.
  • In the next year, the number of cell phone towers in the U.S. is expected to increase by a full 48%!
  • The dangers of microwave radiation from cell towers (as well as satellite dishes) is being examined and debated all over the world, but relatively little in the U.S
Health Dangers of Cell Towers (or Mobile Phone Masts)
The human body itself is electromagnetic (at a very low level—around 10 hertz). It’s been shown that each one of our cells has its own electromagnetic field (EMF). Maintaining balance in those cellular EMFs is critical to staying healthy.

Decades of studies have demonstrated that artificial frequencies higher than 10 hertz can create stress and serious health problems. (See cell tower radiation health effects)
Cellphone tower wavelengths, microwaves have a significantly higher frequency than even radio waves. The higher the frequency, the more powerful the wave—and the more powerful effect on biological organisms. (Recall a mobile tower emit microwaves at 1900 MHz.)
These higher energy waves can actually destroy chemical and molecular bonds, creating chaos in our basic biochemical structures. (Search EMFs explained.)
The negative health effects of EMFs and microwave radiation are well documented. Studies have shown that EMFs can affect:
EMF Exposure Health Effects
  • Enzymes
  • DNA
  • Metabolism
  • Genes
  • Hormones
  • And more
Cell Tower Radiation Has Also Been Linked To:
  • Headaches
  • Memory loss
  • Low sperm count
  • Cancer, birth defects
  • Heart conditions
  • Alzheimer’s.
One of the problems is that this damage is cumulative in the tissues, and can take years, even decades to show up.





Just Hit The Share Button It Doesn't Bite Your Finger

What Is Spam ?

Spam is unsolicited e-mail sent for the purposes of advertising a product or service, usually to a potential customer that has no relationship with the company at all. Its physical world equivalent is junk mail that comes unsolicited into recipients' mail boxes. Spam is considered a major nuisance by many in the computer world and can even be harmful.
In some cases, e-mail disguised as spam may actually be malicious in nature and not intended to advertise a product or service at all. In theses cases, senders devise a way to make e-mail look like spam in hopes that recipients visit a Web site, where viruses may be downloaded onto their computers. While not true spam, unsolicited e-mails do make malicious intents harder to find.
The most malicious type of true spam may be that which downloads spyware or adware to a user's computer. In these cases, e-mails may direct users to a particular site where this software is downloaded. Then, the software may cause malfunctions or pop up messages that look very official warning users they need to purchase a certain product to clean up their computers.
Due to the problems that spam has caused, many countries have tried to regulate spam and hold accountable companies who send it. However, in some cases this has run into constitutional challenges, especially in the United States. Due to freedom of speech issues, the outlawing of spam becomes problematic and many laws have been overturned.

Therefore, understanding there would be constitutional challenges to outlawing spam completely, the U.S. Congress has passed legislation that regulates the use of spam. Certain things must be present in any unsolicited e-mails such as: an option to allow recipients to be removed from the mailing list, a physical address and phone number for the company, and other things. The sending of pornographic images is also restricted. Each violation can cost $11,000 US Dollars (USD), making it a very expensive way for businesses to advertise.
The problem many run into with regulating spam is that it may not originate inside the borders of the regulating country. Therefore, finding violators, known as spammers, becomes nearly impossible and prosecuting those people becomes even more problematic. Many may not be traceable and those who are may be in countries where there are very few, or no, anti-spam laws. Therefore, any laws remain only partially effective at best.
To counteract the ineffectiveness of anti-spam laws, the best option may be an e-mail system which filters perceived spam mail. Usually, this is sent to a dedicated folder within the e-mail software. However, this does not totally protect the user because most anti-spam software can unintentionally filter out valid e-mails. Therefore, users must still check the e-mail that is filtered to make sure they are not losing any legitimate e-mails.

What is a Solar Flare ?

Solar flares are mass ejections from the surface of the Sun caused by the spontaneous reconnection of magnetic field lines. Solar flares are so violent that they would be capable of incinerating entire continents if the Earth were held close to them. Solar flares pose a danger to astronauts due to the energetic particles they release over long distances.
Like some other energetic astronomical events, solar flares release massive amounts of energy across the entire electromagnetic spectrum, from the longest — wavelength radio to the shortest — wavelength gamma rays. Solar flares tend to occur in active regions around sunspots, and their frequency matches the intensity of sunspots at any given time, ranging between once a week to several per day. Solar flares are powerful enough to temporarily disrupt long-range radio communication on Earth. The magnetic reconnection events that power solar flares take place on timescales of minutes to tens of minutes.
Solar flares are related to Coronal Mass Ejections, another type of stellar phenomena whereby large quantities of solar atmosphere are ejected into space at great speeds. In a solar flare, electrons, protons, and heavy ions may be accelerated to speeds close to that of light. For an unfortunate astronaut outside the Earth’s atmosphere and lacking sufficient shielding, this could mean instant death. Therefore, scientists are very concerned about studying solar flares so they might better predict them.

The first solar flares were observed in 1856 as bright flares on the edges of sunspots. Relative to the size of the Sun itself, solar flares are quite small, but relative to the Earth and other planets, they are large. Energetic particles released by solar flares contribute to the creation of the beautiful aurora borealis and aurora australis.
Solar flares cause the release of a large cascade of particles known as a proton storm, which is what can be dangerous to astronauts. A few decades ago, it was believed that proton storms could only travel at approximately 8% the speed of light, theoretically giving astronauts two hours to reach shelter in case of an observed solar flare. But recently, in 2005, a proton storm was observed reaching the vicinity of the Earth only 15 minutes after the initial observation, indicating a speed approximately a third that of light. This increases the solar flare risk for astronauts, and provides a design challenge for engineers designing long-range spacecraft, such as journeys to Mars.

What Is Concentration ?

Concentration is the ability to focus the mind on a task or series of tasks while ignoring other distractions. There are several levels of concentration based on how the mind is dealing with extraneous stimuli. Another measure of concentration is the span of time in which focus on a single task can be maintained. Certain disorders and neurological diseases can make it impossible for a person to concentrate. Several methods also are available to help improve concentration when there is a problem.
Sustained attention is what is most commonly perceived as concentration in human beings. This is a state in which a person remains cognizant despite performing or experiencing something that does not readily keep his or her attention. The person will remain consistently focused on the task at hand for as long as it lasts, from beginning to end.
The opposite of sustained attention is focused attention. This is when a person is presented with some type of event that draws his or her attention to it. Although focused attention usually lasts only seconds, there is concentration and exclusion of other environmental events for that period of time before re-focusing on another subject.

The two remaining types of concentration are known as selective and alternating. Selective attention is the ability of a person to maintain focus on a task while other stimuli are threatening to actively draw away that attention. An example of this is called the cocktail party effect, in which a person is able to focus on a single listener while excluding all others talking in the room. Alternating attention is when a person can freely switch his or her attention between two separate tasks.
The normal mechanisms of concentration can be interrupted by diseases or neurological disorders. These disorders can hinder the operation of the brain, causing a person either to move quickly from one subject to another or to hyper-focus on a single task for an extended period of time. These types of conditions often affect short-term memory, as well. Less extreme conditions, such as attention deficit disorder (ADD), can cause a shortened attention span and difficulty learning.
There are mental exercises that can help people who have problems concentrating. These can include structured games, timed activities, meditation or even just something as simple as doing crossword puzzles. Certain medications also can help to improve the level of focus and attention in a person who has trouble concentrating.

What is Plasma ?

Plasma is a phase of matter distinct from solids, liquids, and gases. It is the most abundant phase of matter in the universe -- both stars and interstellar dust consist of plasma. Although it is its own phase of matter, plasma is often referred to as an ionized gas. This is similar to a normal gas, except that electrons have been stripped from their respective nucleons and float freely within the plasma. Even if only 1% of the atoms have lost their electrons, a gas will display plasma-like behavior.
Plasma is electrically conductive and can be manipulated by magnetic fields. It can be found in a variety of everyday contexts, including plasma displays, fluorescent lamps, neon signs, plasma balls, photolithographic etching machines, flames, lightning, aurora borealis, tesla coils, and more.
Plasmas vary widely. Some parameters used for their classification are the degree of ionization, temperature, density of the magnetic field, and particle density. For example, the gas in a candle flame is only very slightly ionized, whereas the air in the path of a lightning bolt is highly ionized. Some plasmas are very low temperature, like the intergalactic medium, while some are very high temperature, like the center of a star.



Unlike gases, which are composed of neutral atoms, charged plasmas have distinct constituents that behave on their own accord. Free electrons are negatively charged. The nuclei, lacking electrons, are positively charged ions. Most plasmas still contain whole atoms which are electrically neutral as well. Since each of these components can behave differently in response to changes in external and internal conditions, a variety of complex wave-like phenomena can emerge.
Plasma phenomena can be observed safely in your own home with the use of a plasma ball. A plasma ball runs an electric field through a charged gas contained within a glass globe. When a person touches the edge of the globe, the plasma responds by sending out visible filaments to the person's finger, demonstrating the tendency of an electric charge to "ground" itself. Complex, fractal patterns can be seen within the ball.
Because plasma can be contained by magnetic fields, it can be made very hot without diffusing heat into a surrounding medium. Plasmas measuring millions of degrees Kelvin have been produced in tokamak reactors, donut-shaped plasma traps. In the not-too-distant future, we may regularly use superheated plasmas to initiate nuclear fusion reactions that produce large amounts of power.

 Just Hit The Share Button It Doesn't Bite Your Finger

What Is Helium ?

Helium is a chemical element that occurs in great abundance throughout the universe, although it is not as widely distributed on Earth. It typically takes the form of a gas, and it heads up the list of noble gases in the periodic table of elements. Like other noble gases, helium is extremely stable, and it does not readily form compounds with other elements. There are a number of uses for this gas, and it is widely considered to be a very useful and valuable element.
The atomic number of helium is two, making it the second lightest element. It is identified on the periodic table with the symbol He, and it is the least reactive of the noble gases. As a result, helium is one of the least reactive elements on Earth. Its extreme stability makes it a popular choice for a range of uses in situations where unstable materials are being handled, or where the use of other elements might be dangerous.
The discovery of helium occurred in 1868, when astronomers observed a strange band of light during a solar eclipse. The band of light did not correlate with any known element, and the observers realized that they had identified a new gas, which they called “helium” after the Greek Helios, for “Sun.” Within 30 years, scientists had succeeded in isolating and extracting the gas from the mineral clevite.



Although helium is the second most abundant element in the universe, it can be challenging to find on Earth. It is frequently extracted from natural gas, which can contain the element in concentrations ranging from 2 to 7%. The extremely stable, non-reactive gas became a vital tool during the First World War, when access to helium was highly restricted, and this occurred again during the Second World War. Many of the potential uses of the gas can be military in nature, including use as a non-reactive buffer for arc welding and as a lifting agent for balloons of all sizes. Helium is also used as a supercoolant in scientific experimentation and nuclear reactors.
Pure helium is not toxic, and exposure to the clear, odorless, and tasteless gas should not pose a health risk. However, excessive inhalation of the gas can be dangerous, as it will act as an asphyxiate. In addition, when inhaled directly from a pressurized tank, it may cause lung damage, and commercial helium such as that found in party balloons may be contaminated with other substances that are not healthy to inhale.

What is Solar Wind ?

The solar wind is a stream of charged particles flowing out from the Sun, or any star, in all directions. The solar wind is mostly made up of free protons and electrons (plasma) with energies of about 1 keV (kilo-electron-volt). This quite energetic, but solar wind is usually harmless because of its low density. The solar wind extends outwards about 100 AU (astronomical units, Earth-Sun distances), about three times as far from the Sun as the orbit of Neptune, at which point it collides with the interstellar medium. The region where the solar wind is dominant is known as the heliosphere.
It is not completely known how the solar wind escapes the Sun and travels outward. It is partially due to the extremely high temperature of the corona, thehighest layer of the Sun's atmosphere, which ranges between 1 and 3 million Kelvin (1 and 3 million Celsius, 1.8 and 5.4 million Fahrenheit), reaching occasional highs of 10 million Kelvin. The high temperature of the corona is an unsolved question in physics itself, but the speed of the solar wind as it is ejected from the Sun -- between 400 and 700 km/s -- is another mystery. Even taking into account the high temperature of the corona, these particles must be getting some additional kinetic energy from somewhere to escape the Sun at the speed they do. The magnetic fields generated by free electrons may contribute to the acceleration of protons away from the Sun.

The solar wind is the source of various phenomena visible from Earth, including the aurorae (Northern Lights(The Northern Lights, or Aurora Borealis, are glowing bands, circles and streams of colored lights that sometimes appear in the northern latitudes.) and Southern Lights), geomagnetic storms, the most severe of which can damage power grids and put astronauts in danger, and the plasma tails of comets. The Sun emits about 6.7 billion tons of solar wind per hour, which sounds like a lot, but becomes practically nothing when spread out across the vast expanse of space. An Earth-mass of solar wind is ejected only every 150 million years, and the Sun has only lost 0.01% of its mass over its 4.57 billion year age. Other stars, especially Wolf-Rayet stars, lose much more of their mass to solar wind over time. While the Sun would require 50 trillion years to eject all its mass via the solar wind, a Wolf-Rayet star requires only about 100,000.
The solar wind is the primary phenomenon in space for a large distance, but not forever. The influence of the solar wind begins to falter at the termination shock, about 75 AU from the Sun, where the velocity of the solar wind decreases from supersonic to subsonic. The space probe Voyager 1 reached the termination shock on 23-24 May 2005. Data sent back from its sensors has given scientists a better idea of how dynamics change when the solar wind is not the primary influence on the local space environment.

What Is an Electron ?

An electron is a subatomic particle with a negative electric charge that is equal, but opposite to, the positive charge of a proton. These two particles, together with neutrons, form atoms, with the protons and neutrons residing in the nucleus, and the electrons in surrounding orbitals, held in place by the electromagnetic force. They are involved in chemical bonding, can flow through some materials as an electric current, and are responsible for the solidity of solid objects. The particles have a tiny mass, about 1/1836th of the mass of a proton, and are thought to be fundamental, that is, not made up of smaller components.
Although it is often convenient to think of electrons as tiny, point-like particles, they can, in common with other subatomic particles, sometimes behave as waves. This is known as the wave-particle duality. Since no one can actually see an electron, even using the most powerful and sensitive instruments available, it is only possible to construct models to try to explain their behavior. In some cases a “particle” model works best and in others, a “wave” model. Most of the time, however, these entities are referred to as particles.



Electrons in Everyday Life

Electrons play a fundamental role in everything that humans experience on a day-to-day basis. Their mutual electrical repulsion prevents solid objects from passing through one another, despite the fact that the atoms from which the objects are made are mostly empty space. These particles are also responsible for allowing atoms to join together to form the molecules that make up the Earth and life itself. Modern civilization and technology are heavily reliant on electricity, which involves movement of electrons.

Atoms, Elements and Molecules

The properties of the chemical elements depend on the number of electrons they have, and their arrangement within the atom. These factors determine how atoms of an element will combine with other atoms to form molecules. When atoms combine, they do so in such a way as to achieve a lower level of energy. The electrons can be thought of as being arranged into concentric shells, each with a maximum number that it can contain. Usually, the lowest energy state is achieved between two atoms when both are able to fill up their outermost shells.
There are two main ways that atoms can combine, or form a chemical bond, with one another. In ionic bonding, an atom donates one or more electrons to another atom of a different element, normally in such a way that both achieve full outer shells. Since an atom normally has the same number of electrons as protons, it is electrically neutral, but losing or gaining some will give it a positive or negative charge, forming an ion. A metal will tend to donate electrons to a non-metal to form an ionic compound. The molecule is held together by the electrical attraction between the positively charged metal and the negatively charged non-metal.
In a covalent bond — which forms between non-metals — atoms combine by sharing electrons to achieve a lower energy state, usually, again, by filling up their outer shells. For example, a carbon atom, which is four short of a full outer shell, can form covalent bonds with four hydrogen atoms, each one electron short, forming a molecule of methane (CH4). This way, all five atoms share a full shell. Covalent bonds hold together the complex organic molecules that are essential to life.

Electricity

The movement of electrons from one place to another manifests itself as electricity. This can take the form of “static” electricity, where friction causes these particles to move from one material to another, leaving both electrically charged, and able to exert an attraction toward other objects. This was first documented in ancient Greece, when the effect was produced by rubbing amber with fur. The word electron, in fact, comes from the Greek word for amber. A device called a Van de Graff generator uses this effect to generate very high voltages that can produce large sparks.
The most familiar form of electricity, however, is the electric current that is supplied to homes and industry to provide light and heat, and to power various devices and processes. It consists of a flow of electrons through a suitable material, known as a conductor. The best conductors are metals, because their outer electrons are loosely held and can move about easily. The movement of a conductor within a magnetic field can produce a flow of electrons within it, an effect that is used in the large-scale generation of electricity.

History

The idea that electricity might come in small, indivisible units had been around since the early to mid 19th century, but it was in 1894 that the Irish physicist G. Johnstone Stoney first used the term electron to describe the postulated fundamental unit of negative electric charge. Three years later, the British physicist J. J. Thompson identified it as a subatomic particle. It wasn’t until 1909 that its charge was measured by Robert Andrews Millikan, an American experimental physicist, by an ingenious experiment well known to physics students. He suspended oil droplets of various sizes in an adjustable electric field, and calculated the amounts of charge required to prevent them falling by gravity. It turned out that the values were all multiples of the same tiny unit, which was the charge on a single electron.

What Is a Gyrotron ?

A gyrotron is a form of electron tube or vacuum tube that is often referred to as a cyclotron resonance maser due to the fact that one of its most frequent uses is in high-energy physics research in cyclotrons. The advantage that a gyrotron offers is that it can generate enormous amounts of radio frequency (RF) energy in the megawatt range at very small wavelengths of only a few millimeters, which is not possible for standard vacuum tubes. The process can generate an enormous amount of heat, which can be used to sinter ceramics or heat plasma in fusion research reactors. Gyrotrons are also directly employed in nuclear magnetic resonance (NMR) imaging for observing quantum mechanical effects at the atomic level or in magnetic resonance microscopy (MRI) for medical diagnoses.
The principle behind how a gyrotron functions was first theoretically composed in the late 1950s, when relativistic effects of electron energy were being studied in cyclotrons for the first time. By injecting streams of electrons into the electromagnetic field of a cyclotron with an equal frequency, an effect known as negative mass instability was observed. The electron stream would tend to bunch together from a standard gyroradius or Larmor radius, causing the electrons to decelerate and release kinetic energy in the process as millimeter wavelength radio frequency energy or radiation.

Early electron cyclotron resonance energies demonstrated the potential to heat plasmas in fusion research, but the technology and scientific understanding to create a gyrotron system that was reliably capable of this did not become a mature science until the first decade of the 21st century. As the science and technology advanced, gyrotron applications split into high-energy megawatt systems for fusion research, and low-energy 10- to 1,000-watt systems for NMR spectroscopy. Where the devices produce terahertz radiation in the 100 gigahertz to 1 terahertz range, they are used in industrial applications such as plasma diagnostics and high-temperature heating of ceramic compounds. Research in Japan has also increased the efficiency of mid-range to high-power gyrotron devices by 50% as of 1994 by using an integrated mode converter to more efficiently convert electron beam energy to heat.
Since a gyrotron is a form of Microwave Amplification by Stimulated Emission of Radiation (MASER) device or free electron laser that generates electromagnetic fields, it has some similarity to the principle behind how a standard microwave oven operates. A portable gyrotron can be operated in a range of frequencies typically from 2 to 235 gigahertz, and this makes them useful devices for non-lethal weapons systems that the US military refers to as Active Denial System (ADS) technology. An ADS device based on a gyrotron can be targeted against human beings with the effect that it heats up water molecules under the skin without causing permanent damage to tissue. This acts as a deterrent field that has theoretical applications in crowd control to prevent riots, or to keep enemy soldiers or civilians from approaching military installations and downed aircraft.



 Just Hit The Share Button It Doesn't Bite Your Finger

What is a Charge Card ?

Not to be confused with a credit card, a charge card, is a means by which to purchase products and services on short-term credit. The most recognized company dealing in charge cards is American Express. Some other companies, including Diner's Club. In certain situations, MasterCard has also been trying to build a presence in the charge card market.
A charge card differs from a credit in a number of important factors. Understanding these factors is critical before using such a card. While many appreciate credit cards because they have the opportunity to make purchases and pay back the balance over time, often months or years, the charge card offers no such generous time frame. A charge card must be paid back by the due date of the next billing statement in full.
Unlike a credit card, a charge card usually comes with no preset maximum credit line. However, if the charge card issuer believes you may be unable to pay the company back when a statement is issued, charging privileges could be suspended. So while there is no preset limit, there is certainly a limit that a company will allow a consumer to charge before cutting off privileges. This is done purely as a protection for the company.

There is usually no interest associated with a charge card because there is no long-term debt. Charge card companies make their money in usually one of two ways: by charging for the use of the card and charging penalties in the event that a charge card balance is not paid or is not paid in full. Often times, the penalty on a balance not paid in full can be as much as 5 percent.
However, while charge cards often make it a general practice to collect the entire outstanding balance each month, some are starting to make exceptions to this rule. For example, American Express, in some cases and if a charge card holder enrolls, will allow an individual to charge travel expenses and pay them back over time. In addition, if single purchase is more than a preset benchmark, usually $200 US Dollars, that amount can also be paid back over a period of time. In this way, charge cards are very similar to credit cards.
Still, before making a major purchase or putting all travel-related expenses on a charge card, it is important for the cardholder to make sure these are options. If not, the cardholder could be left with a large balance and be assessed a significant penalty.

What Is a SSN ?

SSN is the widely accepted acronym that stands for Social Security Number. It is a 9-digit, personal identification number issued to U.S. citizens and permanent residents by the United States Social Security Administration. The SSN is one of the most important numbers an individual can have. People must have this number to apply for a job, receive any government assistance, file taxes, and obtain a mortgage or credit. For all of these reasons, it is also one of the most private pieces of personal information an individual uses, and should be kept private.
Though SSNs weren't issued until 1936, they were originally created as part of the New Deal Social Security Program and were used only for tax purposes. This meant that most children weren't required to have one before the age of 14. However, in 1986, a new law was instated requiring children over 5 to have a SSN before they could be claimed as dependents by their parents. Today, children need one before their first birthday.




The Social Security Administration is an office of the United States Federal Government and the only source for obtaining a legally issued Social Security number. In recent years, the SSN has become interconnected with more than just taxes, because it used by banks, colleges, and other primary business entities as proof of identification. This is how the number has become the prime target for identity theft. With an individual's SSN in their possession, thieves can easily apply for credit and obtain other identity and financial means fraudulently.
For newly born citizens or new permanent residents to obtain a SSN, they must contact their local Social Security office. If a person believes that his or her number has been compromised, it is important that he or she contact the administration for information on the steps necessary to protect his or her credit and identity. They can offer assistance and tell the person what can be done to avoid potential personal and financial devastation.

What is a Lender ?

A lender is any institution or individual who loans a borrower money. There are a number of types of lending organizations, including educational lenders, commercial lenders, hard money lenders, lenders of last resort, and mutual organizations. The most traditional type of lender is a commercial lender. Often a commercial lender is a banking institution, though it may also be a private financial group. This type of lender makes an offer to the borrower of certain terms, including interest rate and length of loan, with the goal of maximizing their profit in relation to the borrower's risk of defaulting on the loan.
Often a loan is brokered, meaning that the borrower is evaluated by a third-party who then proposes the loan request to a number of different lenders. These lenders are chosen based on their likelihood of accepting the particular borrower, and may negotiate small changes in the terms to attract the borrower if they find her desirable.
A hard money lender specializes in short-term loans which are backed primarily with real estate as collateral. A hard money lender in general offers worse rates than a traditional banking organization, in exchange for more flexible terms and a broader range of deals they are willing to back. In some states within the US, hard money lenders are forced to operate differently than they do in the country as a whole, because of conflicts between their standard practices and those states' usury laws.



A mutual organization is a financial cooperative operating to lend money to its members. The constituents of a mutual organization put money into a collective, where it may then be disbursed to members in need of loans, at amiable rates and with good terms. By eliminating the need to turn a profit, mutual organizations are able to give higher interest rates on deposits and lower rates on loans than traditional banking organizations. Types of mutual organizations include community credit unions and friendly societies.
A lender of last resort is a special type of lender which focuses on protecting a country's national economy from collapse. A lender of last resort will lend to banking institutions on the edge of collapse, in order to protect their depositors and to stop total panic from pushing the economy quickly downhill.
The term lender of last resort has also come to refer to private institutions which give loans to people with a very low credit score or an otherwise extremely high risk of default. This type of lender offers loans at exorbitant interest rates as a way of covering losses from the high default rate they experience with their borrowers. A lender of last resort may also refer clients to a loan shark, offering loans at even higher interest rates for virtually any purpose.


Just Hit The Share Button It Doesn't Bite Your Finger 

What is a Microwave Oven ?

A microwave oven is a cooking device that can cook or reheat food much faster than a conventional oven. Using microwave technology, water and particles within the food are heated incredibly fast, turning cold or frozen food into steaming and hot meals. Although the technology behind microwave ovens has been around for nearly seventy years, many people still believe there are some health risks associated with using this type of oven for cooking.
A microwave is a type of radio wave that can be absorbed by water and certain molecules, like those found in sugar. The absorption of these waves causes the atoms in the food to become highly active, effectively creating heat. Most microwave ovens use a common wave frequency of 2.5 gigahertz (2500 megahertz) that has proved most effective in the food heating process. This specific wave frequency cannot be absorbed in high quantities by glass, plaster or ceramics, meaning that in a microwave oven, only the food will be affected by the heat.
Like many of science's most interesting discoveries, microwave cooking was an accidental find. In the 1940s, so legend goes, a scientist working for the American defense contractor Raytheon accidentally melted a candy bar in his pocket by hitting it with microwaves. In just a few short years, the technology had grown to revolutionize the way food is cooked.




A microwave oven can be a useful appliance to have in your home or office, particularly if you are pressed for time. With microwavable versions of everything from oatmeal to turkey dinners, it might be possible today to make all of your cooked food with a microwave, though this is not generally practiced. There are several types of microwave ovens available on the market, from easily transportable countertop versions to built-in kitchen versions.
You can purchase a microwave at most stores that carry large kitchen appliances. A basic countertop oven will typically cost between $50-$80 US Dollars (USD). More expensive versions offer features like weight sensors to prevent burning or undercooking, rotating turntables, and pre-programmed settings for dozens of foods. While these high end models make an easy job even easier, they can easily cost upwards of $300 USD and may not be necessary for the casual microwave oven user.
While microwave ovens may sound like a dream come true for the time-pressed, some people have expressed concerns over health risks posed by these ovens. Some foods, like eggs, require a specific internal temperature to be fully cooked, and can put the eater at serious risk for food poisoning or salmonella if undercooked. Others also worry about radiation leakage from the ovens, though most studies have shown that while leakage is possible, it is typically in very small doses. To avoid health risks such as food poisoning, be sure to read all directions carefully and cook accordingly.
Despite its detractors, a microwave oven is a wonderful boon when you have no time to cook a hot meal. Although not a total substitute for traditional cooking methods, they can easily mean the difference between having a bag of chips or a hot bowl of soup for a quick lunch.


Just Hit The Share Button It Doesn't Bite Your Finger

What is Infrared Radiation ?

Infrared radiation, also known as “IR,” is just one type of radiation that exists within the electromagnetic spectrum. The radiation that is used in microwave ovens is a type of radiation that has a place on the electromagnetic spectrum, while the radiation that is used in hospitals to create X-ray images is another. The light rays that allow humans to see the world around them and the radio waves that are used to deliver news and music are also types of radiation that exist within the electromagnetic spectrum.
Infrared radiation is so named because the wavelength of infrared rays is just a bit longer than that of red rays. The only types of radiation that humans can detect are light rays. If humans could see infrared rays on the color spectrum, it would appear just after or below red. The Latin infra translates to “below”.
Infrared radiation is an incredibly important part of every human being’s life. This is because IR is quite literally heat. Although human eyes cannot visibly detect IR, they can surely feel it. Wrapping a hand around a cup of hot chocolate, take a walk in balmy weather, or enjoy sizzling fajitas; in all of these experiences are interacting directly with IR.



Although the human eye cannot detect radiation, scientists have developed mechanical eyes that can. IR cameras can take pictures of objects and beings that relay their topography in terms of the amount of heat that they are giving off. For example, in an IR photo of a snake eating a mouse, the cold blooded snake would be nearly invisible, but humans would be able to see the thermal outline of the warm blooded mouse.
There are many uses for infrared radiation cameras. They are used by the military to gain information about a target or place of interest. They are also used by astronomers to learn more about the cosmos. Meteorologists also use cameras that are sensitive to IR in order to predict temperatures and oncoming weather.

What Is Indigo ?

Indigo is a rich blue dye that was widely used throughout the ancient world, from Indonesia to Europe. The distinctive dark blue color has made this dye famous, with a variety of synthetics being used today to produce indigo which is colorfast and fade-resistant, in contrast with that of natural origins used historically. Many craft stores sell it in their dye sections for people who want to work with this dye directly.
The earliest records of indigo date to around 1600 BCE, and seem to suggest that the use of this dye probably originated in India, spreading out to the Middle East and China and diffusing from there. In fact, the name comes from the Latin indicum, which means “of India.” Indigo quickly became a very popular color thanks to its depth and saturation, which made wool, cotton, and linen garments incredibly dark.
This dye was historically sourced from plants in the genus Indigofera, a member of the pea family native to Asia. Indigo could also be extracted from woad, as it was in the British Isles, and from some shellfish in the genus Murex, also used by the Phoenicians to make another famous dye, Tyrian Purple. The compound that creates the blue color is actually not soluble in water, so in order to turn it into a dye, people had to subject it to chemical treatments. Some of these treatments were quite harsh, leading to health problems at textile manufacturing facilities and occasionally attracting attention from social reformers



Historically, many people simply soaked their indigo in stale urine to turn it into a dying compound, leading dyemakers to be exiled to the fringes of cities in some regions due to the smell. Indigo could also be fermented to make a dye, as was done in Asia, and some people simply painted it directly onto substances they wished to dye. Textiles also had to go through multiple dye cycles for the color to take, and it usually only penetrated the upper layers, leaving behind a white core.
Since 1900, most companies that want to work with indigo use synthetic dyes. These dyes are stronger than the natural ones, and also more predictable, ensuring that batches retain consistent coloration. Denim is one famous product traditionally made with indigo; the distinctive wear of jeans is the result of the wear patterns of the dye, which naturally fades out through repeated washes.

What Is an Electromagnetic Wave ?

The term electromagnetic wave describes the way electromagnetic radiation (EMR) moves through space. Different forms of EMR are distinguished by their wavelengths, which vary from many yards (meters) to a distance smaller than the diameter of an atomic nucleus. The full range, in decreasing order of wavelength, goes from radio waves through microwaves, visible light, ultraviolet and X-rays to gamma rays and is known as the electromagnetic spectrum. Electromagnetic waves have many applications, both in science and in everyday life.

Light Waves

In many respects, an electromagnetic wave behaves similarly to ripples on water, or to sound travelling through a medium such as air. For example, if a light is shone onto a screen through a barrier with two narrow slits, a pattern of light and dark stripes is seen. This is called an interference pattern: where the crests of the waves from one slit meet those from the other, they reinforce one another, forming a bright stripe, but where a crest meets a trough, they cancel out, leaving a dark stripe. Light can also bend around an obstacle, like ocean breakers around a harbor wall: this is known as diffraction. These phenomena provide evidence of the wave-like nature of light.

It was long assumed that, like sound, light must travel through some kind of medium. This was given the name “ether,” sometimes spelt “aether,” and was thought to be an invisible material that filled space, but through which solid objects could pass unhindered. Experiments designed to detect the ether by its effect on the speed of light in different directions all failed to find any evidence for it, and the idea was finally rejected. It was apparent that light, and other forms of EMR, did not require any medium and could travel through empty space.

Wavelength and Frequency

Just like an ocean wave, an electromagnetic wave has peaks and troughs. The wavelength is the distance between two identical points of the wave from cycle to cycle, for instance, the distance between one peak, or crest, and the next. EMR can also be defined in terms of its frequency, which is the number of crests that pass by in a given time interval. All forms of EMR travel at the same speed: the speed of light. Therefore, the frequency depends entirely on the wavelength: the shorter the wavelength, the higher the frequency.

Energy

Shorter wavelength, or higher frequency, EMR carries more energy than longer wavelengths or lower frequencies. The energy carried by an electromagnetic wave determines how it affects matter. Low frequency radio waves mildly perturb atoms and molecules, while microwaves cause them to move about more vigorously: the material heats up. X-rays and gamma rays pack much more of a punch: they can break chemical bonds and knock electrons from atoms, forming ions. For this reason, they are described as ionizing radiation.

The Origin of Electromagnetic Waves

The relationship between light and electromagnetism was established by the work of the physicist James Clerk Maxwell in the 19th century. This led to the study of electrodynamics, in which electromagnetic waves, such as light, are regarded as disturbances, or “ripples,” in an electromagnetic field, created by the movement of electrically charged particles. Unlike the non-existent ether, the electromagnetic field is simply the sphere of influence of a charged particle, and not a tangible, material thing.
Later work, in the early 20th century, showed that EMR also had particle-like properties. The particles that make up electromagnetic radiation are called photons. Although it seems contradictory, EMR can behave as waves or as particles, depending on the type of experiment that is carried out. This is known as the wave-particle duality. It also applies to subatomic particles, whole atoms and even quite large molecules, all of which can sometimes behave as waves.
The wave-particle duality emerged as quantum theory was being developed. According to this theory, the “wave” represents the probability of finding a particle, such as a photon, at a given location. The wave-like nature of particles and the particle-like nature of waves have given rise to a great deal of scientific debate and some mind-boggling ideas, but no overall consensus about what it actually means.
In quantum theory, electromagnetic radiation is produced when subatomic particles release energy. For example, an electron in an atom can absorb energy, but it must eventually drop to a lower energy level and release the energy as EMR. Depending on how it is observed, this radiation can appear as a particle or an electromagnetic wave.

Uses

A great deal of modern technology depends upon electromagnetic waves. Radio, television, mobile phones and the Internet rely on the transmission of radio frequency,
(Radio frequency refers to an alternating electrical current with certain properties that allow it to be broadcast from an antenna.)
 EMR through air, space or fiber optic cables. The lasers used to record and play DVDs and audio CDs use light waves to write to and read from the discs. X-ray machines are an essential tool in medicine and airport security. In science, our knowledge of the universe comes largely from analysis of light, radio waves and X-rays from distant stars and galaxies.

Hazards

It is not thought that low energy electromagnetic waves, such as radio waves, are harmful. At higher energies, however, EMR poses risks. Ionizing radiation, such as X-rays and gamma rays can kill or damage living cells. They can also alter DNA, which can lead to cancer. The risk to patients from medical X-rays is considered negligible, but radiographers, who are exposed to them regularly, wear lead aprons — which X-rays cannot penetrate — to protect themselves. Ultraviolet light, present in sunlight, can cause sunburn and can also cause skin cancer if exposure is excessive.


Just Hit The Share Button It Doesn't Bite Your Finger

What Is an Electromagnetic Field ?


An electromagnetic field is a field which possesses magnetic and electrical properties and surrounds objects with an electrical charge. The field also interacts with charged objects within the field. Electromagnetic fields are present on a basic level across the universe, in varying degrees of strength. The Earth, for example, is surrounded by an electromagnetic field generated by the movement of electrons inside the Earth, and this field is taken advantage of every day when people use compasses to orient themselves. The behavior of such fields is determined by the wavelengths of energy generated, and the frequency of their oscillations. Long wavelengths oscillate at a low frequency, while short wavelengths oscillate at a high frequency.
Whenever voltage is present, an electric field forms. In a simple example, when a light is plugged into a socket but not turned on, a small electric field is generated. When the light is turned on, causing a flow of current, the movement of electrons creates a magnetic field. The electric field is still present, so an electromagnetic field is being generated. Changes in an electric field can generate magnetic activity, while changes in a magnetic field can generate electrical activity.



A classic example of an electromagnetic field is the field generated around high energy power lines. Many people have noted that they can feel a hum of energy around power lines, and studies have shown that the electromagnetic field which surrounds high energy power lines can actually impact the growth of plants inside the field, illustrating the way in which an electromagnetic field can act on charged particles inside the field.
The electromagnetic spectrum runs all the way from radio waves, which have long wavelengths and a low frequency, to gamma rays, with short wavelengths and a high frequency. Electromagnetic radiation on the higher end of the electromagnetic spectrum is known as ionizing radiation because it can remove electrons from the molecules and atoms they pass through. One area of the electromagnetic spectrum is of special interest: the range of visible light. When someone sees the orange of a carrot(carrot is an edible tuber with a feathery spray of leafy greens which makes it readily identifiable to gardeners.), for example, it is because the eye is sensitive to wavelengths reflected by the carrot.
Certain types of electromagnetic fields have been linked with health concerns. Several studies on cancer have shown that some childhood cancers have been linked with exposure to high energy electromagnetic fields. Even as an electromagnetic field causes health problems, however, it can also be beneficial. For example, in the medical community, people use x-rays, a form of electromagnetic radiation, to see the inside of the body, and lasers, another form of electromagnetic radiation, to perform surgery.


Just Hit The Share Button It Doesn't Bite Your Finger 

What Is a Gauss ?


Named for German mathematician Carl Frederich Gauss, the gauss is a unit of magnetic field measurement. Often abbreviated as G when referred to in official publications and in scientific formulas, gauss is understood to equate to one Maxwell per square centimeter. The essential idea behind this measurement is to be able to quantify the amount of magnetic flux density with a magnetic field.
Along with being an excellent mathematician, Gauss was also renowned as a top German physicist. While investigating the phenomenon of the creation and manipulation of magnetic energy, Gauss developed his formula for the measurement of changes within a magnetic field, including the identification of a base unit that would help to identify the degree of flux present at a given time and under specific conditions. As is true with many scientific discoveries, his name came to be the common name for that identifying unit.
It is important to make the distinction that a gauss relates only to the rate of flux within the magnetic density of a field. A separate unit of measurement, known as the oersted, is employed when the intensity of the magnetic field is the subject under consideration. While similar in nature, each unit helps to provide different information about the function and form of the field under consideration.




The gauss can be utilized in the measurement of the flux density of just about any material that is understood to possess a magnetic field. For example, a magnet made from iron and of a size that would fit into a hand would probably have a unit measurement of 100 gauss. In comparison, a large industrial size electromagnet would most likely account for a measurement of roughly 15,000 gauss. The method for determining the measurement is considered to be so accurate that physicists can even use the gauss to calculate a measurement for various stars, based on information about the magnetic field related to the star. 

What Is An Electric Field ?

An electric field can be regarded as the sphere of influence of an electrically charged object. Anything that has an electrical charge will affect, and be affected by, other charged bodies. If two charged objects are placed sufficiently close to one another, each will experience a measureable force acting upon it. The field is theoretically infinite in extent, but its magnitude diminishes with distance from the source according to the inverse square law. This means that if the distance is doubled, the strength of the field is divided by four, and at three times the distance, the strength is divided by nine, and so on; the field therefore becomes negligible at large distances.
Since an electric charge can be positive or negative, the electric field is a vector field, which means that it has a direction as well as a magnitude. Two electrically charged objects will experience a repulsive force if they have the same type of charge and an attractive force if they have different types of charge. The force experienced by a charged object in an electric field can be calculated as F = Eq, where F is the force in Newtons, E is the electric field in volts per meter (v/m) and q is the charge in Coulombs. This equation can be rearranged to give the strength of the field, E, in volts per meter: E = F/q. These examples apply to small, point-like, objects; for more complex, or multiple, charged bodies, the calculations are more complicated.


The direction of an electric field is defined as the direction in which the electric force would be felt by an object with a positive charge placed in the field. Thus, the field would point away from a positive charge and toward a negative charge, since like charges repel and unlike charges attract. In the case of two bodies with the same type of charge, each would experience a force — calculable by the F = Eq equation — directed away from the other object. Conversely, for two oppositely charged bodies, each would experience a force directed toward the other object.
An electric field line can be drawn with an arrow pointing away from a positive charge and pointing toward a negative charge. Thus, a positively charged object would be depicted with field lines pointing away from it in all directions, and a negatively charged object with field lines converging upon it. This, however, is just a convention and does not indicate that there is anything physical pointing in a particular direction.
The concept of an electric field as described above is part of “classical” physics. The classical description works well for everyday applications, but does not explain what is actually happening when charged objects attract or repel one another. A branch of quantum theory known as quantum electrodynamics (QED), attempts to do this in terms of the exchange of photons, the carriers of the electromagnetic force.