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AGU: Geophysical Research Letters

 

Keywords

  • solar
  • EUV
  • thermosphere
  • density

Index Terms

  • Solar Physics, Astrophysics, and Astronomy: Solar irradiance
  • Atmospheric Composition and Structure: Thermosphere: composition and chemistry
  • Atmospheric Composition and Structure: Thermosphere: energy deposition
  • Global Change: Solar variability
  • Solar Physics, Astrophysics, and Astronomy: Solar activity cycle

Abstract

GEOPHYSICAL RESEARCH LETTERS, VOL. 37, L16103, 5 PP., 2010
doi:10.1029/2010GL044468

Anomalously low solar extreme-ultraviolet irradiance and thermospheric density during solar minimum

Stanley C. Solomon

High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado, USA

Thomas N. Woods

Laboratory for Atmospheric and Space Physics, University of Colorado at Boulder, Boulder, Colorado, USA

Leonid V. Didkovsky

Space Sciences Center, University of Southern California, Los Angeles, California, USA

John T. Emmert

Space Science Division, Naval Research Laboratory, Washington, D. C., USA

Liying Qian

High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado, USA

Solar activity during 2007–2009 was very low, and during this protracted solar minimum period, the terrestrial thermosphere was cooler and lower in density than expected. Measurements from instruments on the SOHO and TIMED spacecraft, and by suborbital rocket flights, indicate that solar extreme-ultraviolet irradiance levels were lower than they were during the previous solar minimum. Analysis of atmospheric drag on satellite orbits indicate that the thermosphere was lower in density, and therefore cooler, and than at any time since the beginning of the space age. However, secular change due to increasing levels of carbon dioxide and other greenhouse gases, which cool the upper atmosphere, also plays a role in thermospheric climate. Simulations by the NCAR Thermosphere-Ionosphere-Electrodynamics General Circulation Model are compared to thermospheric density measurements, yielding evidence that the primary cause of the low thermospheric density was the unusually low level of solar extreme-ultraviolet irradiance.

Received 23 June 2010; accepted 1 July 2010; published 25 August 2010.

Citation: Solomon, S. C., T. N. Woods, L. V. Didkovsky, J. T. Emmert, and L. Qian (2010), Anomalously low solar extreme-ultraviolet irradiance and thermospheric density during solar minimum, Geophys. Res. Lett., 37, L16103, doi:10.1029/2010GL044468.

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