The General's Luck Runs Out

Does the killing of the notorious guerrilla leader Kishenji mean the end of India's four-decade Maoist insurgency, or the beginning of its next chapter?

BY JASON MIKLIAN | NOVEMBER 30, 2011

With no time to change into his customary flat green combat fatigues, Kishenji fled into the forest wearing a powder blue windbreaker and slacks. But even an intimate knowledge of the jungle's tangled paths was no match for a battalion of soldiers sporting infrared goggles. Guarded by only a small security detail, a fraction of the size of his usual phalanx, Kishenji found himself cornered, and started a firefight that lasted for over two hours. While the guerrilla leader and his loyalists desperately sprayed the forest with bullets, the CoBRAs retaliated with precision artillery. When the shooting stopped just before dusk, the advancing troops found a wiry middle-aged body bleeding out onto the forest floor. After hiding for four decades in malarial jungles and mining towns, Kishenji was dead. Forsaken by his fleeing bodyguards, he was killed less than a week after taunting the "useless and worthless" Indian forces for being completely incapable of catching him.

The Maoist insurgency may very well survive the death of its field general; there are several plausible replacement candidates, including Kishenji's brother Venugopal. A massive retaliation attack at some point in the next month seems inevitable. The Maoists themselves have been doing their best to spin the killing, leaking stories to the press about their annoyance with a man who they now claim was little more than a figurehead to them. But there is no denying that Kishenji was the lifeblood of the rebel group, the operational commander who stirred his fighters to battle to the death against a far superior force. With their great uniter gone, the movement risks degenerating into turf wars and squabbles over who controls the profitable mining extortion trade that funds guerrilla salaries.

Kishenji's demise also punctuates an incredible run for Prime Minister Manmohan Singh, who has staked much of his reputation on the fight against a rebellion he once called "the gravest internal security threat we face," one more worrying than even Islamist terrorism. After years of condemnations from the media for incompetence, from human rights organizations for a policy of targeted assassinations, and even from the Supreme Court for creating illegal militias, the government's strategic successes are undeniable. Conflict deaths this year are down by 40 percent; the Maoist organizational structure is being dismantled; and now its leader is gone.

Not everyone is celebrating. The Maoists, for all the chaos they have sowed under Kishenji's leadership, enjoy widespread support in the indigenous communities where they operate. The mining companies fear the Maoists, often acceding to the latter's extortionist demands -- payouts that have made more than few rebel fortunes, and transformed the rebellion itself from a scrappy agrarian uprising into something that often resembles an elaborate and bloody protection racket. The indigenous communities know this, but still support the Maoists; they know they have few other options. Laws to protect tribal lands exist, but they are easily sidestepped by paying off corrupt politicians and police. The Maoists have brought this hypocrisy to light, however brutally.

In a way, the offensive that claimed Kishenji bears an eerie similarity to the past. After its founding, the initial Naxal movement grew for a decade, turning increasingly violent as demands for more egalitarian economic and human rights reforms went unheeded. By the late 1970s, the government had had enough of the unrest and liquidated dozens of the movement's leaders. The violence subsided and the campaign was declared an unconditional success. But little was done to address the underlying causes for violence: inequality, a lack of justice, and a broken local government. Naxal student leaders voiced these concerns at the time, but nobody listened. Twenty years later, one of those same students tapped into the still-festering grievances to launch a new war.

Military advances may once again break the grip of Maoist violence, giving India another once-in-a-generation opportunity to stop the violence in its heartland. But the gains will be similarly short-lived this time around unless Delhi finally corrects the discriminatory practices towards its indigenous communities that have lingered since its independence. If not, it is only a matter of time before the next Kishenji heads down a jungle path into the shadows.

DESHAKALYAN CHOWDHURY/AFP/Getty Images

 

Jason Miklian is a researcher at the Peace Research Institute Oslo. He can be reached at Jason@prio.no.

JOEMILLER

11:57 PM ET

November 29, 2011

India crashes

India is in crash right now. No one wants to be with India.
India is in really bad condition. They always try to rule over the world.. This is really a bad point of them.
Considering that when India set out to be democratic, successful democracies tended to be white, rich, Christian and with a single dominant language, its success over 60 years is significant in two ways.

First, it demonstrated beyond argument that poverty, massive illiteracy and diversity on a sub-continental scale were not arguments against democracy, they were arguments for it.

Second, India's Republican democracy is premised on a national myth of pluralism, not the standard nationalist invocation of a shared history, a single language and an assimilationist culture.

Considering that when India set out to be democratic, successful democracies tended to be white, rich, Christian and with a single dominant language, its success over 60 years is significant in two ways.

First, it demonstrated beyond argument that poverty, massive illiteracy and diversity on a sub-continental scale were not arguments against democracy, they were arguments for it.

Second, India's Republican democracy is premised on a national myth of pluralism, not the standard nationalist invocation of a shared history, a single language and an assimilationist culture.

Pluralist nationalism in the 19th century was invented as an answer to the specific challenges of contemporary colonialism. It was founded on the claim that the anti-colonial Indian National Congress could speak for the nation-in-the-making because its membership included representatives of all of India's human species.

The challenge of representing India to a hostile colonial state and then the trauma of Partition committed the republican state to pluralist democracy.

Pluralism, a stratagem born of weakness (the early nationalist elite had no other way of demonstrating that they represented anyone but themselves), became the cornerstone of Indian political practice, because it legitimised the compromises essential for keeping hundreds of jostling identities aboard the good ship India.

This was the ultimate political goal: to keep the diversity of a subcontinent afloat in a democratic ark. Everything else was negotiable.

The political culture of the republic consisted of the balancing of special interests, procrastination, equivocation, pandering, tokenism and selective affirmative action: in a word, democratic politics.

Gender, language, religious identity, class and caste were all pressed into India's political mill, but no single identity or principle was used consistently enough to satisfy its champions.

It is a political culture that worked as agenda software, approximately but demonstrably.

Not only did it work, it allowed Indians a worldview born out of their own political experience.

This is what india think about them.

Thanks

 

MAZO

6:44 AM ET

December 2, 2011

ROFL

How nice of you to cut and paste somebody else's eloquent argument. It's a pity you don't really understand what you've posted otherwise your preface might have been completely different!

One point of contention however is that Pluralism was not an Indian invention or even a cop-out by the early nationalists, it was a direct adoption of Western ideals like secularism and the separation of Church and State that were ingrained in early nationalists who all happened to be great champions of Western ideals and philosophies of democracy, liberty and progressive ideals. (They were after all products of the finest educational institutions in the world like Cambridge and Oxford) . It was finally Gandhi who brought the message of pluralism and multicultural inclusion to the masses, however the ideal has always been part of early nationalist movements.
This pluralistic ideal however was tested when Mohamad ali Jinnah and the Muslim League became uncomfortable with the success of the Indian National Congress in early elections and saw their identity as a religious party as untenable in a pluralistic democracy. Therefore the subsequent tragedy of Partition.

 

DR. KUCHBHI

12:15 AM ET

November 30, 2011

India needs to make changes

to make sure that the new found prosperity is not the enclave of the middle class and the rich.

Ignoring the poor is going to be more than selfish, it will be short sighted as they take to violence to keep up with rising inflation.

Hoping the politicians can make political changes to empower and enrich the tribals to include them in the economic strides India is making.

 

AMINAHRIWAHBT

1:35 AM ET

November 30, 2011

perfect work. All womens are

perfect work.
All womens are ready to do strike :)

 

TRIGUN

2:12 AM ET

November 30, 2011

India needs to make changes

Ignoring the poor is going to be more perfect steps than selfish, it will be short sighted as they take to violence to keep up with dis beyazlatma rising inflation.

 

XTRAWIZE

3:05 AM ET

November 30, 2011

Insurgency is a poblem

The rise of insurgency is not always because of poverty. Poor people want jobs and respectable lives. Taking up guns doesn't get you that. What the Naxals are doing in India is more like a mafia gaining power to extract money from everyone--both rich and the poor. They don't need Hostgator code to get their websites. Free Blogger blogs are used to create websites, but printing, arms and ammunition costs money. Where does this come from.

 

MJACOBSON

5:15 AM ET

November 30, 2011

Race well run

It seems Kishenji had a pretty good run. He surely knew it's not easy having a large organized and armed power who's only reason for existence is to crush the little people and steal everything they have.

I'm sure he was happy with his run.

It does take a bit of spirit to dedicate your life to make way for your people to have decent jobs and have a respectable life while outside groups plan terrible things for you.

Let's hope the Naxal people find someone else willing to take a stand against the foreigner's machines.

 

AKKERMAN

6:27 PM ET

December 1, 2011

 

MAZO

6:49 AM ET

December 2, 2011

Brilliant Article and Analaysis.

This is truly a brilliant article that is both eloquent and extremely incisive in its arguments.

The entire spectrum of the conflict has been put into context with this one man's death as the main story. In a way, Kishenji did a lot of good, today the problem of these tribals is no longer trivial and far off as it was just 10 years ago. Today, these problems are real to the people in the big cities. The corruption and the base perfidy of the mining mafia is now exposed and people are starting to understand the "cost" of these resources and their impact on our environment, our people.

I just hope that unlike everything else in India, out of sight doesn't mean out of mind.

 

BIKRAM SINGH

6:16 AM ET

December 8, 2011

Why blast Naxalism and not causes leading to it?

Naxalism is a bad word, and indeed the path they have chosen make it look so, but what has made it do so?

Manmohan singh says that it is the "the gravest internal security threat we face,", but why people took arms against its own government. Why there are some who is rising against their own elected govt. (whom they didn't choose, of course) and fighting their right to survive?

People, who has never been heard, got their voice through Naxalite Movement in several states in India, where all govt. is doing is to work puppet for corporate. (Click the above link to read a nice article I found on web).

How can Mittals, Tatas, and Ambanis of the poor-third-world nation gets right on the land that belong to tribal people. The rumor has it that P. Chitambram, Home Minister of India, has been handsomely bribed to push triabal people off their land.

And PM wants them to shut up and let the corporate mechanism suck their blood. I am not a communist, and I believe in individual industry and capitalism, but not in Corporate capital, and reaping reward from collective industry of your workers.

Until the right kind of reform is brought, this is a challange (and not a problem) India has to jostle with.

 

ONEN

1:11 PM ET

December 11, 2011

Not going to change

It's not going too make much difference until India realizes that they have to make real changes. They can't keep on ignoring what is important. overdrive

 

MARIYANJONIYYAH

6:44 AM ET

December 14, 2011

This image shows the average

This image shows the average temperature profile through the Earth’s atmosphere. Temperatures in the thermosphere are very sensitive to solar activity and can vary from 500°C to 1500°C. Source: Windows to the Universe, (http://www.windows.ucar.edu), the University Corporation for Atmospheric Research (UCAR). ©1995-1999, 2000 The Regents of the University of Michigan; ©2000-04 University Corporation for Atmospheric Research.

Rain, for one, is ‘returned’ to Earth by the clouds in the atmosphere. Explaining the hydrologic cycle, Encyclopedia Britannica writes:

“Water evaporates from both the aquatic and terrestrial environments as it is heated by the Sun’s energy. The rates of evaporation and precipitation depend on solar energy, as do the patterns of circulation of moisture in the air and currents in the ocean. Evaporation exceeds precipitation over the oceans, and this water vapor is transported by the wind over land, where it returns to the land through precipitation.”[2]

Not only does the atmosphere return what was on the surface back to the surface, but it reflects back into space that which might damage the flora and fauna the earth sustains, such as excessive radiant heat. In the 1990’s, collaborations between NASA, the European Space Agency (ESA), and the Institute of Space and Astronautical Science (ISAS) of Japan resulted in the International Solar-Terrestrial Physics (ISTP) Science Initiative. Polar, Wind and Geotail are a part of this initiative, combining resources and scientific communities to obtain coordinated, simultaneous investigations of the Sun-Earth space environment over an extended period of time. They have an excellent explanation of how the atmosphere returns solar heat to space.[3]

Besides ‘returning’ rain, heat and radio waves, the atmosphere protects us like a ceiling above our heads by filtering out deadly cosmic rays, powerful ultraviolet (UV) radiation from the Sun, and even meteorites on collision course with Earth.[4]

Pennsylvania State Public Broadcasting tells us:

“The sunlight that we can see represents one group of wavelengths, visible light. Other wavelengths emitted by the sun include x-rays and ultraviolet radiation. X-rays and some ultraviolet light waves are absorbed high in Earth’s atmosphere. They heat the thin layer of gas there to very high temperatures. Ultraviolet light waves are the rays that can cause sunburn. Most ultraviolet light waves are absorbed by a thicker layer of gas closer to Earth called the ozone layer. By soaking up the deadly ultraviolet and x-rays, the atmosphere acts as a protective shield around the planet. Like a giant thermal blanket, the atmosphere also keeps temperatures from getting too hot or too cold. In addition, the atmosphere also protects us from constant bombardment by meteoroids, bits of rock and dust that travel at high speeds throughout the solar system. The falling stars we see at night are not stars at all; they are actually meteoroids burning up in our atmosphere due to the extreme heating they undergo.

This image shows the average temperature profile through the Earth’s atmosphere. Temperatures in the thermosphere are very sensitive to solar activity and can vary from 500°C to 1500°C. Source: Windows to the Universe, (http://www.windows.ucar.edu), the University Corporation for Atmospheric Research (UCAR). ©1995-1999, 2000 The Regents of the University of Michigan; ©2000-04 University Corporation for Atmospheric Research.

Rain, for one, is ‘returned’ to Earth by the clouds in the atmosphere. Explaining the hydrologic cycle, Encyclopedia Britannica writes:

“Water evaporates from both the aquatic and terrestrial environments as it is heated by the Sun’s energy. The rates of evaporation and precipitation depend on solar energy, as do the patterns of circulation of moisture in the air and currents in the ocean. Evaporation exceeds precipitation over the oceans, and this water vapor is transported by the wind over land, where it returns to the land through precipitation.”[2]

Not only does the atmosphere return what was on the surface back to the surface, but it reflects back into space that which might damage the flora and fauna the earth sustains, such as excessive radiant heat. In the 1990’s, collaborations between NASA, the European Space Agency (ESA), and the Institute of Space and Astronautical Science (ISAS) of Japan resulted in the International Solar-Terrestrial Physics (ISTP) Science Initiative. Polar, Wind and Geotail are a part of this initiative, combining resources and scientific communities to obtain coordinated, simultaneous investigations of the Sun-Earth space environment over an extended period of time. They have an excellent explanation of how the atmosphere returns solar heat to space.[3]

Besides ‘returning’ rain, heat and radio waves, the atmosphere protects us like a ceiling above our heads by filtering out deadly cosmic rays, powerful ultraviolet (UV) radiation from the Sun, and even meteorites on collision course with Earth.[4]

Pennsylvania State Public Broadcasting tells us:

“The sunlight that we can see represents one group of wavelengths, visible light. Other wavelengths emitted by the sun include x-rays and ultraviolet radiation. X-rays and some ultraviolet light waves are absorbed high in Earth’s atmosphere. They heat the thin layer of gas there to very high temperatures. Ultraviolet light waves are the rays that can cause sunburn. Most ultraviolet light waves are absorbed by a thicker layer of gas closer to Earth called the ozone layer. By soaking up the deadly ultraviolet and x-rays, the atmosphere acts as a protective shield around the planet. Like a giant thermal blanket, the atmosphere also keeps temperatures from getting too hot or too cold. In addition, the atmosphere also protects us from constant bombardment by meteoroids, bits of rock and dust that travel at high speeds throughout the solar system. The falling stars we see at night are not stars at all; they are actually meteoroids burning up in our atmosphere due to the extreme heating they undergo.

This image shows the average temperature profile through the Earth’s atmosphere. Temperatures in the thermosphere are very sensitive to solar activity and can vary from 500°C to 1500°C. Source: Windows to the Universe, (http://www.windows.ucar.edu), the University Corporation for Atmospheric Research (UCAR). ©1995-1999, 2000 The Regents of the University of Michigan; ©2000-04 University Corporation for Atmospheric Research.

Rain, for one, is ‘returned’ to Earth by the clouds in the atmosphere. Explaining the hydrologic cycle, Encyclopedia Britannica writes:

“Water evaporates from both the aquatic and terrestrial environments as it is heated by the Sun’s energy. The rates of evaporation and precipitation depend on solar energy, as do the patterns of circulation of moisture in the air and currents in the ocean. Evaporation exceeds precipitation over the oceans, and this water vapor is transported by the wind over land, where it returns to the land through precipitation.”[2]

Not only does the atmosphere return what was on the surface back to the surface, but it reflects back into space that which might damage the flora and fauna the earth sustains, such as excessive radiant heat. In the 1990’s, collaborations between NASA, the European Space Agency (ESA), and the Institute of Space and Astronautical Science (ISAS) of Japan resulted in the International Solar-Terrestrial Physics (ISTP) Science Initiative. Polar, Wind and Geotail are a part of this initiative, combining resources and scientific communities to obtain coordinated, simultaneous investigations of the Sun-Earth space environment over an extended period of time. They have an excellent explanation of how the atmosphere returns solar heat to space.[3]

Besides ‘returning’ rain, heat and radio waves, the atmosphere protects us like a ceiling above our heads by filtering out deadly cosmic rays, powerful ultraviolet (UV) radiation from the Sun, and even meteorites on collision course with Earth.[4]

Pennsylvania State Public Broadcasting tells us:

“The sunlight that we can see represents one group of wavelengths, visible light. Other wavelengths emitted by the sun include x-rays and ultraviolet radiation. X-rays and some ultraviolet light waves are absorbed high in Earth’s atmosphere. They heat the thin layer of gas there to very high temperatures. Ultraviolet light waves are the rays that can cause sunburn. Most ultraviolet light waves are absorbed by a thicker layer of gas closer to Earth called the ozone layer. By soaking up the deadly ultraviolet and x-rays, the atmosphere acts as a protective shield around the planet. Like a giant thermal blanket, the atmosphere also keeps temperatures from getting too hot or too cold. In addition, the atmosphere also protects us from constant bombardment by meteoroids, bits of rock and dust that travel at high speeds throughout the solar system. The falling stars we see at night are not stars at all; they are actually meteoroids burning up in our atmosphere due to the extreme heating they undergo.

This image shows the average temperature profile through the Earth’s atmosphere. Temperatures in the thermosphere are very sensitive to solar activity and can vary from 500°C to 1500°C. Source: Windows to the Universe, (http://www.windows.ucar.edu), the University Corporation for Atmospheric Research (UCAR). ©1995-1999, 2000 The Regents of the University of Michigan; ©2000-04 University Corporation for Atmospheric Research.

Rain, for one, is ‘returned’ to Earth by the clouds in the atmosphere. Explaining the hydrologic cycle, Encyclopedia Britannica writes:

“Water evaporates from both the aquatic and terrestrial environments as it is heated by the Sun’s energy. The rates of evaporation and precipitation depend on solar energy, as do the patterns of circulation of moisture in the air and currents in the ocean. Evaporation exceeds precipitation over the oceans, and this water vapor is transported by the wind over land, where it returns to the land through precipitation.”[2]

Not only does the atmosphere return what was on the surface back to the surface, but it reflects back into space that which might damage the flora and fauna the earth sustains, such as excessive radiant heat. In the 1990’s, collaborations between NASA, the European Space Agency (ESA), and the Institute of Space and Astronautical Science (ISAS) of Japan resulted in the International Solar-Terrestrial Physics (ISTP) Science Initiative. Polar, Wind and Geotail are a part of this initiative, combining resources and scientific communities to obtain coordinated, simultaneous investigations of the Sun-Earth space environment over an extended period of time. They have an excellent explanation of how the atmosphere returns solar heat to space.[3]

Besides ‘returning’ rain, heat and radio waves, the atmosphere protects us like a ceiling above our heads by filtering out deadly cosmic rays, powerful ultraviolet (UV) radiation from the Sun, and even meteorites on collision course with Earth.[4]

Pennsylvania State Public Broadcasting tells us:

“The sunlight that we can see represents one group of wavelengths, visible light. Other wavelengths emitted by the sun include x-rays and ultraviolet radiation. X-rays and some ultraviolet light waves are absorbed high in Earth’s atmosphere. They heat the thin layer of gas there to very high temperatures. Ultraviolet light waves are the rays that can cause sunburn. Most ultraviolet light waves are absorbed by a thicker layer of gas closer to Earth called the ozone layer. By soaking up the deadly ultraviolet and x-rays, the atmosphere acts as a protective shield around the planet. Like a giant thermal blanket, the atmosphere also keeps temperatures from getting too hot or too cold. In addition, the atmosphere also protects us from constant bombardment by meteoroids, bits of rock and dust that travel at high speeds throughout the solar system. The falling stars we see at night are not stars at all; they are actually meteoroids burning up in our atmosphere due to the extreme heating they undergo.

This image shows the average temperature profile through the Earth’s atmosphere. Temperatures in the thermosphere are very sensitive to solar activity and can vary from 500°C to 1500°C. Source: Windows to the Universe, (http://www.windows.ucar.edu), the University Corporation for Atmospheric Research (UCAR). ©1995-1999, 2000 The Regents of the University of Michigan; ©2000-04 University Corporation for Atmospheric Research.

Rain, for one, is ‘returned’ to Earth by the clouds in the atmosphere. Explaining the hydrologic cycle, Encyclopedia Britannica writes:

“Water evaporates from both the aquatic and terrestrial environments as it is heated by the Sun’s energy. The rates of evaporation and precipitation depend on solar energy, as do the patterns of circulation of moisture in the air and currents in the ocean. Evaporation exceeds precipitation over the oceans, and this water vapor is transported by the wind over land, where it returns to the land through precipitation.”[2]

Not only does the atmosphere return what was on the surface back to the surface, but it reflects back into space that which might damage the flora and fauna the earth sustains, such as excessive radiant heat. In the 1990’s, collaborations between NASA, the European Space Agency (ESA), and the Institute of Space and Astronautical Science (ISAS) of Japan resulted in the International Solar-Terrestrial Physics (ISTP) Science Initiative. Polar, Wind and Geotail are a part of this initiative, combining resources and scientific communities to obtain coordinated, simultaneous investigations of the Sun-Earth space environment over an extended period of time. They have an excellent explanation of how the atmosphere returns solar heat to space.[3]

Besides ‘returning’ rain, heat and radio waves, the atmosphere protects us like a ceiling above our heads by filtering out deadly cosmic rays, powerful ultraviolet (UV) radiation from the Sun, and even meteorites on collision course with Earth.[4]

Pennsylvania State Public Broadcasting tells us:

“The sunlight that we can see represents one group of wavelengths, visible light. Other wavelengths emitted by the sun include x-rays and ultraviolet radiation. X-rays and some ultraviolet light waves are absorbed high in Earth’s atmosphere. They heat the thin layer of gas there to very high temperatures. Ultraviolet light waves are the rays that can cause sunburn. Most ultraviolet light waves are absorbed by a thicker layer of gas closer to Earth called the ozone layer. By soaking up the deadly ultraviolet and x-rays, the atmosphere acts as a protective shield around the planet. Like a giant thermal blanket, the atmosphere also keeps temperatures from getting too hot or too cold. In addition, the atmosphere also protects us from constant bombardment by meteoroids, bits of rock and dust that travel at high speeds throughout the solar system. The falling stars we see at night are not stars at all; they are actually meteoroids burning up in our atmosphere due to the extreme heating they undergo.
This image shows the average temperature profile through the Earth’s atmosphere. Temperatures in the thermosphere are very sensitive to solar activity and can vary from 500°C to 1500°C. Source: Windows to the Universe, (http://www.windows.ucar.edu), the University Corporation for Atmospheric Research (UCAR). ©1995-1999, 2000 The Regents of the University of Michigan; ©2000-04 University Corporation for Atmospheric Research.

Rain, for one, is ‘returned’ to Earth by the clouds in the atmosphere. Explaining the hydrologic cycle, Encyclopedia Britannica writes:

“Water evaporates from both the aquatic and terrestrial environments as it is heated by the Sun’s energy. The rates of evaporation and precipitation depend on solar energy, as do the patterns of circulation of moisture in the air and currents in the ocean. Evaporation exceeds precipitation over the oceans, and this water vapor is transported by the wind over land, where it returns to the land through precipitation.”[2]

Not only does the atmosphere return what was on the surface back to the surface, but it reflects back into space that which might damage the flora and fauna the earth sustains, such as excessive radiant heat. In the 1990’s, collaborations between NASA, the European Space Agency (ESA), and the Institute of Space and Astronautical Science (ISAS) of Japan resulted in the International Solar-Terrestrial Physics (ISTP) Science Initiative. Polar, Wind and Geotail are a part of this initiative, combining resources and scientific communities to obtain coordinated, simultaneous investigations of the Sun-Earth space environment over an extended period of time. They have an excellent explanation of how the atmosphere returns solar heat to space.[3]

Besides ‘returning’ rain, heat and radio waves, the atmosphere protects us like a ceiling above our heads by filtering out deadly cosmic rays, powerful ultraviolet (UV) radiation from the Sun, and even meteorites on collision course with Earth.[4]

Pennsylvania State Public Broadcasting tells us:

“The sunlight that we can see represents one group of wavelengths, visible light. Other wavelengths emitted by the sun include x-rays and ultraviolet radiation. X-rays and some ultraviolet light waves are absorbed high in Earth’s atmosphere. They heat the thin layer of gas there to very high temperatures. Ultraviolet light waves are the rays that can cause sunburn. Most ultraviolet light waves are absorbed by a thicker layer of gas closer to Earth called the ozone layer. By soaking up the deadly ultraviolet and x-rays, the atmosphere acts as a protective shield around the planet. Like a giant thermal blanket, the atmosphere also keeps temperatures from getting too hot or too cold. In addition, the atmosphere also protects us from constant bombardment by meteoroids, bits of rock and dust that travel at high speeds throughout the solar system. The falling stars we see at night are not stars at all; they are actually meteoroids burning up in our atmosphere due to the extreme heating they undergo.
This image shows the average temperature profile through the Earth’s atmosphere. Temperatures in the thermosphere are very sensitive to solar activity and can vary from 500°C to 1500°C. Source: Windows to the Universe, (http://www.windows.ucar.edu), the University Corporation for Atmospheric Research (UCAR). ©1995-1999, 2000 The Regents of the University of Michigan; ©2000-04 University Corporation for Atmospheric Research.

Rain, for one, is ‘returned’ to Earth by the clouds in the atmosphere. Explaining the hydrologic cycle, Encyclopedia Britannica writes:

“Water evaporates from both the aquatic and terrestrial environments as it is heated by the Sun’s energy. The rates of evaporation and precipitation depend on solar energy, as do the patterns of circulation of moisture in the air and currents in the ocean. Evaporation exceeds precipitation over the oceans, and this water vapor is transported by the wind over land, where it returns to the land through precipitation.”[2]

Not only does the atmosphere return what was on the surface back to the surface, but it reflects back into space that which might damage the flora and fauna the earth sustains, such as excessive radiant heat. In the 1990’s, collaborations between NASA, the European Space Agency (ESA), and the Institute of Space and Astronautical Science (ISAS) of Japan resulted in the International Solar-Terrestrial Physics (ISTP) Science Initiative. Polar, Wind and Geotail are a part of this initiative, combining resources and scientific communities to obtain coordinated, simultaneous investigations of the Sun-Earth space environment over an extended period of time. They have an excellent explanation of how the atmosphere returns solar heat to space.[3]

Besides ‘returning’ rain, heat and radio waves, the atmosphere protects us like a ceiling above our heads by filtering out deadly cosmic rays, powerful ultraviolet (UV) radiation from the Sun, and even meteorites on collision course with Earth.[4]

Pennsylvania State Public Broadcasting tells us:

“The sunlight that we can see represents one group of wavelengths, visible light. Other wavelengths emitted by the sun include x-rays and ultraviolet radiation. X-rays and some ultraviolet light waves are absorbed high in Earth’s atmosphere. They heat the thin layer of gas there to very high temperatures. Ultraviolet light waves are the rays that can cause sunburn. Most ultraviolet light waves are absorbed by a thicker layer of gas closer to Earth called the ozone layer. By soaking up the deadly ultraviolet and x-rays, the atmosphere acts as a protective shield around the planet. Like a giant thermal blanket, the atmosphere also keeps temperatures from getting too hot or too cold. In addition, the atmosphere also protects us from constant bombardment by meteoroids, bits of rock and dust that travel at high speeds throughout the solar system. The falling stars we see at night are not stars at all; they are actually meteoroids burning up in our atmosphere due to the extreme heating they undergo.
This image shows the average temperature profile through the Earth’s atmosphere. Temperatures in the thermosphere are very sensitive to solar activity and can vary from 500°C to 1500°C. Source: Windows to the Universe, (http://www.windows.ucar.edu), the University Corporation for Atmospheric Research (UCAR). ©1995-1999, 2000 The Regents of the University of Michigan; ©2000-04 University Corporation for Atmospheric Research.

Rain, for one, is ‘returned’ to Earth by the clouds in the atmosphere. Explaining the hydrologic cycle, Encyclopedia Britannica writes:

“Water evaporates from both the aquatic and terrestrial environments as it is heated by the Sun’s energy. The rates of evaporation and precipitation depend on solar energy, as do the patterns of circulation of moisture in the air and currents in the ocean. Evaporation exceeds precipitation over the oceans, and this water vapor is transported by the wind over land, where it returns to the land through precipitation.”[2]

Not only does the atmosphere return what was on the surface back to the surface, but it reflects back into space that which might damage the flora and fauna the earth sustains, such as excessive radiant heat. In the 1990’s, collaborations between NASA, the European Space Agency (ESA), and the Institute of Space and Astronautical Science (ISAS) of Japan resulted in the International Solar-Terrestrial Physics (ISTP) Science Initiative. Polar, Wind and Geotail are a part of this initiative, combining resources and scientific communities to obtain coordinated, simultaneous investigations of the Sun-Earth space environment over an extended period of time. They have an excellent explanation of how the atmosphere returns solar heat to space.[3]

Besides ‘returning’ rain, heat and radio waves, the atmosphere protects us like a ceiling above our heads by filtering out deadly cosmic rays, powerful ultraviolet (UV) radiation from the Sun, and even meteorites on collision course with Earth.[4]

Pennsylvania State Public Broadcasting tells us:

“The sunlight that we can see represents one group of wavelengths, visible light. Other wavelengths emitted by the sun include x-rays and ultraviolet radiation. X-rays and some ultraviolet light waves are absorbed high in Earth’s atmosphere. They heat the thin layer of gas there to very high temperatures. Ultraviolet light waves are the rays that can cause sunburn. Most ultraviolet light waves are absorbed by a thicker layer of gas closer to Earth called the ozone layer. By soaking up the deadly ultraviolet and x-rays, the atmosphere acts as a protective shield around the planet. Like a giant thermal blanket, the atmosphere also keeps temperatures from getting too hot or too cold. In addition, the atmosphere also protects us from constant bombardment by meteoroids, bits of rock and dust that travel at high speeds throughout the solar system. The falling stars we see at night are not stars at all; they are actually meteoroids burning up in our atmosphere due to the extreme heating they undergo.This image shows the average temperature profile through the Earth’s atmosphere. Temperatures in the thermosphere are very sensitive to solar activity and can vary from 500°C to 1500°C. Source: Windows to the Universe, (http://www.windows.ucar.edu), the University Corporation for Atmospheric Research (UCAR). ©1995-1999, 2000 The Regents of the University of Michigan; ©2000-04 University Corporation for Atmospheric Research.

Rain, for one, is ‘returned’ to Earth by the clouds in the atmosphere. Explaining the hydrologic cycle, Encyclopedia Britannica writes:

“Water evaporates from both the aquatic and terrestrial environments as it is heated by the Sun’s energy. The rates of evaporation and precipitation depend on solar energy, as do the patterns of circulation of moisture in the air and currents in the ocean. Evaporation exceeds precipitation over the oceans, and this water vapor is transported by the wind over land, where it returns to the land through precipitation.”[2]

Not only does the atmosphere return what was on the surface back to the surface, but it reflects back into space that which might damage the flora and fauna the earth sustains, such as excessive radiant heat. In the 1990’s, collaborations between NASA, the European Space Agency (ESA), and the Institute of Space and Astronautical Science (ISAS) of Japan resulted in the International Solar-Terrestrial Physics (ISTP) Science Initiative. Polar, Wind and Geotail are a part of this initiative, combining resources and scientific communities to obtain coordinated, simultaneous investigations of the Sun-Earth space environment over an extended period of time. They have an excellent explanation of how the atmosphere returns solar heat to space.[3]

Besides ‘returning’ rain, heat and radio waves, the atmosphere protects us like a ceiling above our heads by filtering out deadly cosmic rays, powerful ultraviolet (UV) radiation from the Sun, and even meteorites on collision course with Earth.[4]

Pennsylvania State Public Broadcasting tells us:

“The sunlight that we can see represents one group of wavelengths, visible light. Other wavelengths emitted by the sun include x-rays and ultraviolet radiation. X-rays and some ultraviolet light waves are absorbed high in Earth’s atmosphere. They heat the thin layer of gas there to very high temperatures. Ultraviolet light waves are the rays that can cause sunburn. Most ultraviolet light waves are absorbed by a thicker layer of gas closer to Earth called the ozone layer. By soaking up the deadly ultraviolet and x-rays, the atmosphere acts as a protective shield around the planet. Like a giant thermal blanket, the atmosphere also keeps temperatures from getting too hot or too cold. In addition, the atmosphere also protects us from constant bombardment by meteoroids, bits of rock and dust that travel at high speeds throughout the solar system. The falling stars we see at night are not stars at all; they are actually meteoroids burning up in our atmosphere due to the extreme heating they undergo.
This image shows the average temperature profile through the Earth’s atmosphere. Temperatures in the thermosphere are very sensitive to solar activity and can vary from 500°C to 1500°C. Source: Windows to the Universe, (http://www.windows.ucar.edu), the University Corporation for Atmospheric Research (UCAR). ©1995-1999, 2000 The Regents of the University of Michigan; ©2000-04 University Corporation for Atmospheric Research.

Rain, for one, is ‘returned’ to Earth by the clouds in the atmosphere. Explaining the hydrologic cycle, Encyclopedia Britannica writes:

“Water evaporates from both the aquatic and terrestrial environments as it is heated by the Sun’s energy. The rates of evaporation and precipitation depend on solar energy, as do the patterns of circulation of moisture in the air and currents in the ocean. Evaporation exceeds precipitation over the oceans, and this water vapor is transported by the wind over land, where it returns to the land through precipitation.”[2]

Not only does the atmosphere return what was on the surface back to the surface, but it reflects back into space that which might damage the flora and fauna the earth sustains, such as excessive radiant heat. In the 1990’s, collaborations between NASA, the European Space Agency (ESA), and the Institute of Space and Astronautical Science (ISAS) of Japan resulted in the International Solar-Terrestrial Physics (ISTP) Science Initiative. Polar, Wind and Geotail are a part of this initiative, combining resources and scientific communities to obtain coordinated, simultaneous investigations of the Sun-Earth space environment over an extended period of time. They have an excellent explanation of how the atmosphere returns solar heat to space.[3]

Besides ‘returning’ rain, heat and radio waves, the atmosphere protects us like a ceiling above our heads by filtering out deadly cosmic rays, powerful ultraviolet (UV) radiation from the Sun, and even meteorites on collision course with Earth.[4]

Pennsylvania State Public Broadcasting tells us:

“The sunlight that we can see represents one group of wavelengths, visible light. Other wavelengths emitted by the sun include x-rays and ultraviolet radiation. X-rays and some ultraviolet light waves are absorbed high in Earth’s atmosphere. They heat the thin layer of gas there to very high temperatures. Ultraviolet light waves are the rays that can cause sunburn. Most ultraviolet light waves are absorbed by a thicker layer of gas closer to Earth called the ozone layer. By soaking up the deadly ultraviolet and x-rays, the atmosphere acts as a protective shield around the planet. Like a giant thermal blanket, the atmosphere also keeps temperatures from getting too hot or too cold. pro travel In addition, the atmosphere also protects us from constant bombardment by meteoroids, bits of rock and dust that travel at high speeds throughout the solar system. The falling stars we see at night are not stars at all; they are actually meteoroids burning up in our atmosphere due to the extreme heating they undergo.
Thanks

 

MINDINVENTORY

7:01 AM ET

December 15, 2011

Maoist insurgency in india

Maoist is the danger than terrorist,so must be clear Maoist in India.This is effect in Indian economy,so many protection money need against Maoist.

 

RICKY ZEN

11:10 AM ET

December 20, 2011

Government should take strong steps

Indian government should take strong steps and appoint special forces against naxalism to eradicate them completely.

 

YARINSIZ

4:14 PM ET

December 24, 2011

This pluralistic ideal

This pluralistic ideal however was tested when Mohamad ali Jinnah and the Muslim League became uncomfortable with the success of the Indian National Congress in early elections and saw their identity as a religious party as untenable in a pluralistic democracy. seslichat Therefore the subsequent tragedy of Partition.