"వాతావరణం" కూర్పుల మధ్య తేడాలు

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(తర్జుమా మరియు వికీకరణ)
== భూమిపై వాతావరణం==
[[Image:Top of Atmosphere.jpg|thumb|290px|right|వాతావరణ వాయువులు, తమ తరంగదైర్ఘ్యం కంటే ఎక్కువ నీలి కాంతిని వెదజల్లుతాయి. శూన్యం నుండి చూస్తే భూమి నీలి గోళంగా కానవస్తుంది.]]
[[:en:Earth's atmosphere|భూ-వాతావరణం]] లో (భూమిపైనుండి) వరుసగా క్రింది పొరలున్నాయి.
The [[Earth's atmosphere]] consists, from the ground up, of the [[troposphere]] (which includes the [[planetary boundary layer]] or peplosphere as lowest layer), [[stratosphere]], [[mesosphere]], [[thermosphere]] (which contains the [[ionosphere]] and [[exosphere]]) and also the [[magnetosphere]]. Each of the layers has a different [[lapse rate]], defining the rate of change in temperature with height.
 
* [[:en:troposphere|ట్రోపో ఆవరణం]] (which includes the [[:en:planetary boundary layer|planetary boundary layer]] or peplosphere as lowest layer),
Three quarters of the atmosphere lies within the troposphere, and the depth of this layer varies between 17 km at the equator and 7 km at the poles. The [[ozone layer]], which absorbs [[ultraviolet]] energy from the Sun, is located primarily in the stratosphere, at altitudes of 15 to 35 km. The [[Kármán line]], located within the thermosphere at an altitude of 100 km, is commonly used to define the boundary between the Earth's atmosphere and outer space. However, the exosphere can extend from 500 up to 10,000 km above the surface, where it interacts with the planet's magnetosphere.
* [[:en:stratosphere|స్ట్రాటో ఆవరణం]],
* [[:en:mesosphere|మిసో ఆవరణం]],
* [[:en:thermosphere|ఉష్ణ ఆవరణం]] (which contains the [[:en:ionosphere|అయానో ఆవరణం]] మరియుand [[::exosphere|ఎక్సో ఆవరణం]])
* మరియు [[:en:magnetosphere|అయస్కాంత ఆవరణం]]. Each of the layers has a different [[:en:lapse rate|ల్యాప్స్ రేటు]], defining the rate of change in temperature with height.
 
Three quarters of the atmosphere lies within the troposphere, and the depth of this layer varies between 17 km at the equator and 7 km at the poles. The [[:en:ozone layer|ozone layer]], which absorbs [[:en:ultraviolet|ultraviolet]] energy from the Sun, is located primarily in the stratosphere, at altitudes of 15 to 35 km. The [[:en:Kármán line|కార్మాన్ లైను]], located within the thermosphere at an altitude of 100 km, is commonly used to define the boundary between the Earth's atmosphere and outer space. However, the exosphere can extend from 500 up to 10,000 km above the surface, where it interacts with the planet's magnetosphere.
 
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