Thermosphere

S. C. Solomon, R. G. Roble

Research output: Chapter in Book/Report/Conference proceedingChapterpeer-review

13 Scopus citations

Abstract

The thermosphere is the atmospheric region from 85 to 500km altitude, containing the ionosphere. It is characterized by high temperature and large variability, in response to changes in solar ultraviolet radiation and solar-driven geomagnetic activity. The composition of the lower thermosphere is primarily N2 and O2, similar to the lower and middle atmosphere, but in the upper thermosphere atomic oxygen (O) becomes the dominant gas, due to the importance of photodissociation and molecular diffusion at high altitude. Thermospheric dynamical motions result from complex interactions between solar heating, auroral processes, the resulting pressure gradients, and dissipative processes.

Original languageEnglish
Title of host publicationEncyclopedia of Atmospheric Sciences
Subtitle of host publicationSecond Edition
PublisherElsevier Inc.
Pages402-408
Number of pages7
ISBN (Electronic)9780123822260
ISBN (Print)9780123822253
DOIs
StatePublished - 2015
Externally publishedYes

Keywords

  • Atmospheric tides
  • Aurora
  • Ionization
  • Solar heating
  • Space weather

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