Study on the thermospheric density distribution pattern during geomagnetic activity
The atmospheric density of the thermosphere is a fundamental parameter for spacecraft
launch and orbit control. Under magnetic storm conditions, the thermospheric atmospheric …
launch and orbit control. Under magnetic storm conditions, the thermospheric atmospheric …
Strong disturbance of the upper thermospheric density due to magnetic storms: CHAMP observations
H Liu, H Lühr - Journal of Geophysical Research: Space …, 2005 - Wiley Online Library
Strong enhancements of the upper thermospheric total mass density were observed by the
CHAMP satellite at approximately 400 km altitude during three geomagnetic superstorms …
CHAMP satellite at approximately 400 km altitude during three geomagnetic superstorms …
Thermospheric heating and cooling times during geomagnetic storms, including extreme events
E Zesta, DM Oliveira - Geophysical Research Letters, 2019 - Wiley Online Library
We present the first quantitative calculations of thermospheric heating and cooling times for
geomagnetic storms of different intensity, including extreme events. We utilize the neutral …
geomagnetic storms of different intensity, including extreme events. We utilize the neutral …
Effects of solar variability on thermosphere density from CHAMP accelerometer data
Thermosphere densities near 410 km altitude inferred from accelerometer measurements on
the Challenging Minisatellite Payload (CHAMP) satellite are analyzed for solar irradiance …
the Challenging Minisatellite Payload (CHAMP) satellite are analyzed for solar irradiance …
[引用][C] The solar diurnal variation in the amplitude of sudden commencements of magnetic storms at the geomagnetic equator
M Sugiura - Journal of Geophysical Research, 1953 - Wiley Online Library
Tohru Araki and Atsuki Shinbori, Relationship between solar wind dynamic pressure and
amplitude of geomagnetic sudden commencement (SC), Earth, Planets and Space …
amplitude of geomagnetic sudden commencement (SC), Earth, Planets and Space …
Annual and semiannual variations of thermospheric density: EOF analysis of CHAMP and GRACE data
In this paper, observations from CHAMP and GRACE during 2002–2010 are used to study
the seasonal variations of thermospheric density by characterizing the dominant modes of …
the seasonal variations of thermospheric density by characterizing the dominant modes of …
Statistical studies of geomagnetic storms with peak Dst≤− 50 nT from 1957 to 2008
A catalog of 1377 geomagnetic storms with peak Dst (Dst p)≤− 50 nT for the period 1957–
2008 has been compiled. The dependence of Dst p on the solar cycle and annual variation …
2008 has been compiled. The dependence of Dst p on the solar cycle and annual variation …
Rapid recovery of thermosphere density during the October 2003 geomagnetic storms
Thermosphere densities from the CHAMP and GRACE satellites are utilized, for the first
time, to study the recovery of the thermosphere as a function of latitude during the October …
time, to study the recovery of the thermosphere as a function of latitude during the October …
[PDF][PDF] Analyzing the hemispheric asymmetry in the thermospheric density response to geomagnetic storms
[2] It has long been understood that the solar extreme ultraviolet (EUV) radiation, the auroral
particle precipitation, and the high-latitude Joule heating are the predominant sources of …
particle precipitation, and the high-latitude Joule heating are the predominant sources of …
Wind and temperature effects on thermosphere mass density response to the November 2004 geomagnetic storm
A unique conjunction of the Thermosphere Ionosphere Mesosphere Energetics and
Dynamics (TIMED) and the Challenging Minisatellite Payload (CHAMP) satellites provided …
Dynamics (TIMED) and the Challenging Minisatellite Payload (CHAMP) satellites provided …