Open AccessThermospheric density oscillations due to periodic solar wind high‐speed streams
Author(s) -
Thayer Jeffrey P.,
Lei Jiuhou,
Forbes Jeffrey M.,
Sutton Eric K.,
Nerem R. Steven
Publication year - 2008
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2008ja013190
Subject(s) - thermosphere , solar wind , geomagnetic storm , earth's magnetic field , physics , atmospheric sciences , solar minimum , ionosphere , oscillation (cell signaling) , solar maximum , coronal mass ejection , geophysics , solar cycle , plasma , magnetic field , quantum mechanics , biology , genetics
We report on periodic oscillations in thermosphere density, measured by the accelerometer on the CHAMP satellite during 2006, and relate these periodicities to oscillations observed in solar wind speed and Kp index. Common periodic oscillations at 4–5, 6–7, and 9–11 day periods are observed in the neutral density at 400 km in the 2006 data set, with the 7 day period being the predominant oscillation. Spectral analysis reveals that similar periodicities are present in both the solar wind and the planetary magnetic index Kp but not in the EUV solar flux proxy F 10.7 . We suggest that the periodic oscillations observed in thermosphere density are a direct response to recurrent geomagnetic activity and associated high‐speed streams in the solar wind. The lack of response in F 10.7 at the 7 day period enables storm effects on the thermosphere density to be isolated from solar flux effects. The Kp index for these events correspond to moderate levels of geomagnetic activity, and the resultant perturbations in thermosphere density are ±20–30% of background levels. Although these levels of perturbation are small compared to major magnetic storms, their much higher occurrence frequency and characteristic long recovery time may lead to a cumulative effect on the state of the thermosphere and ionosphere.