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Monday, November 16, 2015



In fig i, parallelogram ABCD and trapezium ABFE have a common base AB but they are not in between the same parallels. In figure ii, parallelogram ABCD and ABEF are on the same base AB and in between the same parallels (AB / DE).
In fact, two figure are said to be on the same base and in between the same parallels if they have common base and the vertices (vertex) opposite to the common base of each figure lie on a line parallel to the base.

Tuesday, September 8, 2015

Here For Free NTC GPRS
Guys here I am to give you some tips on using NTC Gprs just in free. NTC have very weak system it can easily be hacked and you will not charged any for surfing the net. Here the tips goes on

1) After you have surf the internet and you are about to close your browser don't close your browser rather search a number like 220000000 in wap page and try to make call to that number. For such number ntc says "you cannot call to this number and end the call itself. Try to call that number 5/6 times and gprs get disconnected by network and you wont get charged for the gprs and close the browser .

2)Another trick goes like this, "Just surf internet without exceedind your balance, download within the limit of balane you have in your sim and after you finish surfing, just take off your battery out of your mobile and insert your sim only after 1 hour. Check the balance now, yeah you will be not deducted any.

In Nokia 5300, so basically,  number of Nokia sets would behave the same for what I am gonna describe here.Now, getting to the main thing, I browse the web via Opera Mini (Latest Version),  when I am done with browsing and want to close the session, I would rather search for a number “202000000″(nine digits) and when the search result is presented, you can click on the number to call the number without having to close the Opera Mini. The IVR shall tell you that “You cannot make call to this number ” and shall end your call by itself.  When you call, for some 3-4 times to the same number repeatedly, the gprs connection that had been kept on hold will be closed by the network itself. So you are not billed for the data usage from your cellphone.
Try it urself, and comments are welcome.

Monday, September 7, 2015

LAYER OF ATMOSPHER]\/12

Exosphere

Main article: Exosphere
The exosphere is the outermost layer of Earth's atmosphere (i.e. the upper limit of the atmosphere). It extends from the exobase, which is located at the top of the thermosphere at an altitude of about 700 km above sea level, to about 10,000 km (6,200 mi; 33,000,000 ft). The exosphere merges with the emptiness of outer space, where there is no atmosphere.
This layer is mainly composed of extremely low densities of hydrogen, helium and several heavier molecules including nitrogen, oxygen and carbon dioxide closer to the exobase. The atoms and molecules are so far apart that they can travel hundreds of kilometers without colliding with one another. Thus, the exosphere no longer behaves like a gas, and the particles constantly escape into space. These free-moving particles follow ballistic trajectories and may migrate in and out of the magnetosphere or the solar wind.
The exosphere is located too far above Earth for any meteorological phenomena to be possible. However, the aurora borealis and aurora australis sometimes occur in the lower part of the exosphere, where they overlap into the thermosphere. The exosphere contains most of the satellites orbiting Earth.

Thermosphere

Main article: Thermosphere
The thermosphere is the second-highest layer of Earth's atmosphere. It extends from the mesopause (which separates it from the mesosphere) at an altitude of about 80 km (50 mi; 260,000 ft) up to the thermopause at an altitude range of 500–1000 km (310–620 mi; 1,600,000–3,300,000 ft). The height of the thermopause varies considerably due to changes in solar activity.[8] Because the thermopause lies at the lower boundary of the exosphere, it is also referred to as the exobase. The lower part of the thermosphere, from 80 to 550 kilometres (50 to 342 mi) above Earth's surface, contains the ionosphere.
This atmospheric layer undergoes a gradual increase in temperature with height. Unlike the stratosphere, wherein a temperature inversion is due to the absorption of radiation by ozone, the inversion in the thermosphere occurs due to the extremely low density of its molecules. The temperature of this layer can rise as high as 1500 °C (2700 °F), though the gas molecules are so far apart that its temperature in the usual sense is not very meaningful. The air is so rarefied that an individual molecule (of oxygen, for example) travels an average of 1 kilometre (0.62 mi; 3300 ft) between collisions with other molecules.[10] Even though the thermosphere has a very high proportion of molecules with immense amounts of energy, the thermosphere would not feel hot to a human in direct contact, because the low density in the thermosphere would not be able to conduct a significant amount of energy to or from the skin. In other words, a person would not feel warm because of the thermosphere's extremely low pressure.
This layer is completely cloudless and free of water vapor. However non-hydrometeorological phenomena such as the aurora borealis and aurora australis are occasionally seen in the thermosphere. The International Space Station orbits in this layer, between 320 and 380 km (200 and 240 mi).

Mesosphere

Main article: Mesosphere
The mesosphere is the third highest layer of Earth's atmosphere, occupying the region above the stratosphere and below the thermosphere. It extends from the stratopause at an altitude of about 50 km (31 mi; 160,000 ft) to the mesopause at 80–85 km (50–53 mi; 260,000–280,000 ft) above sea level.
Temperatures drop with increasing altitude to the mesopause that marks the top of this middle layer of the atmosphere. It is the coldest place on Earth and has an average temperature around −85 °C (−120 °F; 190 K).[11][12]
Just below the mesopause, the air is so cold that even the very scarce water vapor at this altitude can be sublimated into polar-mesospheric noctilucent clouds. These are the highest clouds in the atmosphere and may be visible to the naked eye if sunlight reflects off them about an hour or two after sunset or a similar length of time before sunrise. They are most readily visible when the Sun is around 4 to 16 degrees below the horizon. A type of lightning referred to as either sprites orELVES, occasionally form far above tropospheric thunderclouds. The mesosphere is also the layer where most meteors burn up upon atmospheric entrance. It is too high above Earth to be accessible to aircraft and balloons, and too low to permit orbital spacecraft. The mesosphere is mainly accessed by sounding rockets.

Stratosphere

Main article: Stratosphere
The stratosphere is the second-lowest layer of Earth's atmosphere. It lies above the troposphere and is separated from it by the tropopause. This layer extends from the top of the troposphere at roughly 12 km (7.5 mi; 39,000 ft) above Earth's surface to the stratopause at an altitude of about 50 to 55 km (31 to 34 mi; 164,000 to 180,000 ft).
The atmospheric pressure at the top of the stratosphere is roughly 1/1000 the pressure at sea level. It contains the ozone layer, which is the part of Earth's atmosphere that contains relatively high concentrations of that gas. The stratosphere defines a layer in which temperatures rise with increasing altitude. This rise in temperature is caused by the absorption of ultraviolet radiation (UV) radiation from the Sun by the ozone layer, which restricts turbulence and mixing. Although the temperature may be −60 °C (−76 °F; 210 K) at the tropopause, the top of the stratosphere is much warmer, and may be near 0 °C.[13]
The stratospheric temperature profile creates very stable atmospheric conditions, so the stratosphere lacks the weather-producing air turbulence that is so prevalent in the troposphere. Consequently, the stratosphere is almost completely free of clouds and other forms of weather. However, polar stratospheric or nacreous cloudsare occasionally seen in the lower part of this layer of the atmosphere where the air is coldest. This is the highest layer that can be accessed by jet-powered aircraft.

Troposphere

Main article: Troposphere
The troposphere is the lowest layer of Earth's atmosphere. It extends from Earth's surface to an average height of about 12 km, although this altitude actually varies from about 9 km (30,000 ft) at the poles to 17 km (56,000 ft) at the equator,[9] with some variation due to weather. The troposphere is bounded above by thetropopause, a boundary marked in most places by a temperature inversion (i.e. a layer of relatively warm air above a colder one), and in others by a zone which is isothermal with height.[14][15]
Although variations do occur, the temperature usually declines with increasing altitude in the troposphere because the troposphere is mostly heated through energy transfer from the surface. Thus, the lowest part of the troposphere (i.e. Earth's surface) is typically the warmest section of the troposphere. This promotes vertical mixing (hence the origin of its name in the Greek word τρόπος, tropos, meaning "turn"). The troposphere contains roughly 80% of the mass of Earth's atmosphere.[16] The troposphere is denser than all its overlying atmospheric layers because a larger atmospheric weight sits on top of the troposphere and causes it to be most severely compressed. Fifty percent of the total mass of the atmosphere is located in the lower 5.6 km (18,000 ft) of the troposphere. It is primarily composed of nitrogen (78%) and oxygen (21%) with only small concentrations of other trace gases.
Nearly all atmospheric water vapor or moisture is found in the troposphere, so it is the layer where most of Earth's weather takes place. It has basically all the weather-associated cloud genus types generated by active wind circulation, although very tall cumulonimbus thunder clouds can penetrate the tropopause from below and rise into the lower part of the stratosphere. Most conventional aviation activity takes place in the troposphere, and it is the only layer that can be accessed by propeller-driven aircraft.
Space Shuttle Endeavour orbiting in the thermosphere. Because of the angle of the photo, it appears to straddle the stratosphere and mesosphere that actually lie more than 250 km below. The orange layer is thetroposphere, which gives way to the whitish stratosphere and then the bluemesosphere.[17]

Other layers

Within the five principal layers that are largely determined by temperature, several secondary layers may be distinguished by other properties:
  • The ozone layer is contained within the stratosphere. In this layer ozone concentrations are about 2 to 8 parts per million, which is much higher than in the lower atmosphere but still very small compared to the main components of the atmosphere. It is mainly located in the lower portion of the stratosphere from about 15–35 km (9.3–21.7 mi; 49,000–115,000 ft), though the thickness varies seasonally and geographically. About 90% of the ozone in Earth's atmosphere is contained in the stratosphere.
  • The ionosphere is a region of the atmosphere that is ionized by solar radiation. It is responsible for auroras. During daytime hours, it stretches from 50 to 1,000 km (31 to 621 mi; 160,000 to 3,280,000 ft) and includes the mesosphere, thermosphere, and parts of the exosphere. However, ionization in the mesosphere largely ceases during the night, so auroras are normally seen only in the thermosphere and lower exosphere. The ionosphere forms the inner edge of themagnetosphere. It has practical importance because it influences, for example, radio propagation on Earth.
  • The homosphere and heterosphere are defined by whether the atmospheric gases are well mixed. The surface-based homosphere includes the troposphere, stratosphere, mesosphere, and the lowest part of the thermosphere, where the chemical composition of the atmosphere does not depend on molecular weight because the gases are mixed by turbulence.[18] This relatively homogeneous layer ends at the turbopause found at about 100 km (62 mi; 330,000 ft), which places it about 20 km (12 mi; 66,000 ft) above the mesopause.
Above this altitude lies the heterosphere, which includes the exosphere and most of the thermosphere. Here, the chemical composition varies with altitude. This is because the distance that particles can move without colliding with one another is large compared with the size of motions that cause mixing. This allows the gases to stratify by molecular weight, with the heavier ones, such as oxygen and nitrogen, present only near the bottom of the heterosphere. The upper part of the heterosphere is composed almost completely of hydrogen, the lightest element.
  • The planetary boundary layer is the part of the troposphere that is closest to Earth's surface and is directly affected by it, mainly through turbulent diffusion. During the day the planetary boundary layer usually is well-mixed, whereas at night it becomes stably stratified with weak or intermittent mixing. The depth of the planetary boundary layer ranges from as little as about 100 meters on clear, calm nights to 3000 m or more during the afternoon in dry regions.
The average temperature of the atmosphere at Earth's surface is 14 °C (57 °F; 287 K)[19] or 15 °C (59 °F; 288 K),[20] depending on the reference..

Saturday, August 22, 2015

exam tips

Exam Tip #1

Wake up early so that you do not need to rush through having breakfast and getting ready.

Exam Tip #2

Check the venue and time of the exam to make sure that you have not confused the day/time/venue.

Exam Tip #3

Have a balanced breakfast and eat nothing risky (probably not the best day to have a super-hot curry!). Bananas are always a good option.

Exam Tip #4

Before leaving home, check that you have everything that you will need – ID, stationery, map to the exam venue, etc.

Exam Tip #5

Head to the exam with plenty of time. A lot of unexpected events can happen on your way there and you do not want to be late!

Exam Tip #6

If there are people around who are panicking, avoid them. They are not doing you any favour!

Exam Tip #7

Go to the toilet before the exam starts. Exams can be quite long and there is no time to waste.

Exam Tip #8

Remember to write your name on the exam paper. You would not believe how many people have forgotten to do it!

Exam Tip #9

Read all the questions carefully before starting and quickly plan how much time to allocate to each.

Exam Tip #10

Start answering the questions that you feel most confident about. There is no need to answer the questions in order.

Exam Tip #11

If your brain freezes, just start writing anything and you will soon start remembering more details.

Exam Tip #12

Don’t spend more time than you planned on a particular section/question or you might run out of time to answer other questions and gain those extra marks! Also,  leave any questions that you are unsure about for the end.

Exam Tip #13

Don’t be afraid to ask the examiner if you are not clear on a question.

Exam Tip #14

Use every minute of the exam and if you have time left, review your answers before handing back the paper.

Exam Tip #15

Stay calm, you have done your homework and have nothing to fear!

cell division


Cell division is the process by which a parent cell divides into two or more daughter cells.[1] Cell division usually occurs as part of a larger cell cycle. In eukaryotes, there are two distinct types of cell division: a vegetative division, whereby each daughter cell is genetically identical to the parent cell (mitosis),[2] and a reductive cell division, whereby the number of chromosomes in the daughter cells is reduced by half, to produce haploidgametes (meiosis). Meiosis results in four haploid daughter cells by undergoing one round of DNA replication followed by two divisions: homologous chromosomes are separated in the first division, and sister chromatids are separated in the second division.[3] Both of these cell division cycles are in sexually reproducing organisms at some point in their life cycle, and both are believed to be present in the last eukaryotic common ancestor[4]Prokaryotes also undergo a vegetative cell division known as binary fission, where their genetic material is segregated equally into two daughter cells. All cell divisions, regardless of organism, are preceded by a single round of DNA replication.
For simple unicellular organisms[Note 1] such as the amoeba, one cell division is equivalent to reproduction – an entire new organism is created. On a larger scale, mitotic cell division can create progeny from multicellular organisms, such as plants that grow from cuttings. Cell division also enables sexually reproducing organisms to develop from the one-celled zygote, which itself was produced by cell division from gametes. And after growth, cell division allows for continual construction and repair of the organism.[5] A human being's body experiences about 10 quadrillion cell divisions in a lifetime.[6]

Tuesday, July 14, 2015

MOST WATCHED NEWS ON GOOGLE

Robin McLaurin Williams (July 21, 1951 – August 11, 2014)[7] was an American actor and comedian. Starting as a stand-up comedian in San Francisco and Los Angeles in the mid-1970s, he is credited with leading San Francisco's comedy renaissance.[8]After rising to fame as Mork in the sitcom Mork & Mindy (1978–82), he went on to establish a career in both stand-up comedy and feature film acting. He was known for his improvisational skills.[9][10]
After his film debut in the musical comedy Popeye (1980), he starred or co-starred in widely acclaimed films, including the comedy-drama The World According to Garp (1982), war comedy Good Morning, Vietnam (1987), dramas Dead Poets Society (1989) andAwakenings (1990), comedy-drama The Fisher King (1991), animated musical fantasy Aladdin (1992), drama Good Will Hunting(1997), and psychological thriller One Hour Photo (2002), as well as financial successes such as the fantasy adventure film Hook(1991), comedy Mrs. Doubtfire (1993), fantasy adventure Jumanji (1995), comedy The Birdcage (1996), and fantasy adventure-comedy Night at the Museum (2006).
In 1998, Williams won the Academy Award for Best Supporting Actor for his performance as Dr. Sean Maguire in Good Will Hunting. He also received two Primetime Emmy Awards, six Golden Globe Awards, two Screen Actors Guild Awards, and four Grammy Awards throughout his career.
On August 11, 2014, after a long history of depression,[11] Williams committed suicide at his home in Paradise Cay, California. He had just been diagnosed with Parkinson's disease.[12]

Monday, July 13, 2015

AMAZING FCTS ABOUT FACEBOOK

Of course, it hasn’t always been smooth sailing for the social media site.
Founder Mark Zuckerberg was accused of stealing the idea and has earned a reputation for being able to flawlessly fire people. It’s also been estimated that scammers can earn $200 million per year on Facebook. And, companies have sold user profiles along with some instances of human trafficking and extortion.
Even the future of Facebook is in doubt. A study through Princeton University discovered that the site may lose around 80% of its users over the next three years. There was another recent study that found between January 2011 and January 2014, Facebook lost over 3 million users in the age 13 to 17 year old demographic.
However, it’s not all doom and gloom for Facebook. As of today, the site remains one of the most popular in the world. In fact, Alexa has ranked Facebook second in its Top 500 Global Sites right behind search engine powerhouse Google.
So, in honor of Facebook’s decade-long dominance, here are 25 things that you should know about the social network.
  1. In 2007, Facebook underwent a major homepage redesign which replaced a man’s partly obscured face behind a cloud of binary code. But, who was the mystery “Facebook guy”? David Kirkpatrick revealed in his book The Facebook Effect that the image is actually a manipulated photo of legendary actor Al Pacino. The effect was created by a friend and classmate of Mark Zuckerberg.
  2. During Facebook’s first summer, the Zuckerberg family spent $85,000 to keep the company afloat. As of September 2013, Mark Zuckerberg is worth $19 billion.
  3. When Facebook began selling stock to the public and trading on the NASDAQ on May 18, 2012, its shares were priced at $38, which meant the company was valued at over $100 billion. It also meant that Facebook was worth more than eBay, Yahoo, Groupon, LinkedIn, Netflix, IAC, AOL, Zynga and Pandora… combined.
  4. Facebook’s first corporate partnerships, launched May 2006, were Apple and Microsoft along with Intel, EA and Amazon. Some of the other early partnerships also included Accenture, Gap, Intuit, Pepsi, PricewaterhouseCoopers and the non-profit organization Teach for America. Everyone else had to wait until September 2006 to join Facebook.
  5. Napster co-founder Sean Parker transitioned Facebook from a college project into an actual company. As dramatized in the 2010 film The Social Network, Parker changed the site’s name from Thefacebook.com by acquiring the domain Facebook.com for $200,000. Furthermore, it was Parker who insisted that the site add its most popular feature: photo sharing.
  6. Who’s on Facebook? 42% of users are male, however, the site is more gender neutral than Pinterest and Google +. About 75% of all U.S. Internet users have had some sort of college education. 73% of users in the U.S. have incomes above $75,000 (compared to 17% on Twitter, and 13% on Pinterest).
  7. The most checked-in locations in the U.S. during 2013, excluding transportation hubs, were: Disneyland & Disney California Adventure, Anaheim, Calif.; Times Square, New York City; Epcot Center, Walt Disney World, Lake Buena Vista, Fla.; Dodger Stadium, Los Angeles; AT&T Park, San Francisco; Rangers Ballpark, Arlington, Texas; Universal Studios Hollywood, Universal City, Calif.; Fenway Park, Boston; MGM Grand Hotel & Casino, Las Vegas; Houston Livestock Show & Rodeo, Houston.
  8. As of September, 2013 the percentage of 15-34 year olds on Facebook are 66%. Interestingly, 45% of internet users who are 65 years or older are also on Facebook. And, don’t be embarrassed if you’re Facebook friends with your parents; 70% of users are friends with their parents.
  9. Every morning when they wake up, 48% of 18-34 year olds check their Facebook account. 28% of that demographic actually check Facebook before they even get out of bed.
  10. Users are exposed to 1500 pieces of potential content every day.
  11. Approximately 7.5 million sites contain the the Facebook Like or Share Buttons.
  12. California is the most social state with 15,267,160 users. That means 41% of the state’s population is in Facebook. Texas is second with 9 million users and New York comes in at third with 8 million.
  13. In the United States, the five most popular brands on Facebook are: Walmart, Target, Amazon, Samsung Mobile USA and Subway.
  14. Despite being blocked, there are roughly 95 million Facebook users in China.
  15. Approximately 86% of their daily active users are outside the U.S. and Canada, with 29% logging in from Asian countries.
  16. There are 70 different languages available for users on Facebook.
  17. In 2013, the Super Bowl was the most talked about topic in the United States. Globally, the most talked about topic was Pope Francis.
  18. The average person spends between 18 and 20 minutes viewing their Facebook account. If you combine every user, that what would be around 20 billion minutes!
  19. Originally, engineers wanted to call the “Like” button the “Awesome” button.
  20. Every 20 minutes on Facebook 1 million links are shared, 2 million friends are requested and 3 million messages are sent.
  21. The most common life event added for users in 2013 was: Relationship/Got Engaged/Got Married. This was followed by Traveled, Moved, Ended a Relationship and First Met a Friend.
  22. Between 2012 and 2013, there was an increase in Facebook users by 22%.
  23. Ever since Facebook launched there have been a 150 billion friend connections, 1.13 trillion likes and 250 billion photos uploaded.
  24. On a daily basis there are 350 million photos uploaded, 4.5 billion likes, 10 billion messages sent and 22 billion times that the Like or Share buttons are viewed.
  25. Total monthly users: 1,310,000,000 with 680 million of them on mobile devices.

Thursday, June 25, 2015

gravitational force

Newton's law of universal gravitation states that any two bodies in the universe attract each other with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.[note 1] This is a general physical law derived from empirical observations by what Isaac Newton called induction.[2] It is a part of classical mechanicsand was formulated in Newton's work Philosophiæ Naturalis Principia Mathematica ("the Principia"), first published on 5 July 1687. (When Newton's book was presented in 1686 to the Royal SocietyRobert Hooke made a claim that Newton had obtained the inverse square law from him; see the History section below.)
In modern language, the law states: Every point mass attracts every single other point mass by a force pointing along the lineintersecting both points. The force is proportional to the product of the two masses and inversely proportional to the square of the distance between them.[3] The first test of Newton's theory of gravitation between masses in the laboratory was the Cavendish experiment conducted by the British scientist Henry Cavendish in 1798.[4] It took place 111 years after the publication of Newton'sPrincipia and 71 years after his death.
Newton's law of gravitation resembles Coulomb's law of electrical forces, which is used to calculate the magnitude of electrical force arising between two charged bodies. Both are inverse-square laws, where force is inversely proportional to the square of the distance between the bodies. Coulomb's law has the product of two charges in place of the product of the masses, and theelectrostatic constant in place of the gravitational constant