Sentence examples for evolution of atmospheres from inspiring English sources

For details on solar wind influence on the evolution of atmospheres we refer to Lammer et al. (2008) and references therein.

In situ measurements by the Gas Chromatograph and Mass Spectrometer (GCMS) instrument on board of ESA's Huygens entry probe can be used as a confirmation of the Earth-based isotope anomaly observations and will be of great importance for understanding the formation and evolution of atmospheres around bodies in the solar system.

Also, we outline some evidence for and possible causes of a solar connection in the evolution of atmosphere and climate.

The lidargram of course includes the effects of neutral atmosphere dynamics on the Na layer as these atoms have a long lifetime relative to the evolution of atmospheric dynamics and they are collisionally well-embedded in the atmosphere.

Finally, the implications of the results for the evolution of the atmospheres of Earth-like planets are discussed.

We present measurements for the production of nitrogen oxides (NO and N2O) in CO2-N2 mixthatsimulateimulate different stages of the evolution of the atmospheres of the Earth, Venus and Mars.

Long-term solar forcing and its consequences – which has come to be known as Space Climate – has important consequences for the formation and evolution of planetary atmospheres, the evolution of life and global climate on Earth.

They can help quantify the contribution of cometary impacts to terrestrial oceans and help elucidate on the formation history of comets and their role in the formation and evolution of planetary atmospheres.

If the young Sun was more active than today, one has to study the consequences this might have had for the development of the planetary environments, including the formation and evolution of planetary atmospheres and initial H2O inventories.

We show that the extreme radiation and plasma environments of the young Sun/stars have important implications for the evolution of planetary atmospheres and may be responsible for the fact that planets with low gravity like early Mars most likely never build up a dense atmosphere during the first few 100 Myr after their origin.

It is shown that the evolution of planetary atmospheres can only be understood if one recognizes the fact that the radiation and particle environment of the Sun or a planet's host star were not always on the same level as at present.