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Zesta, Eftyhia and Oliveira, Denny M., 2019. Thermospheric Heating and Cooling Times During Geomagnetic Storms, Including Extreme Events. Geophysical Research Letters, 46(22):12,739–12,746, doi:10.1029/2019GL085120.
• from the NASA Astrophysics Data System • by the DOI System •
@ARTICLE{2019GeoRL..4612739Z,
author = {{Zesta}, Eftyhia and {Oliveira}, Denny M.},
title = "{Thermospheric Heating and Cooling Times During Geomagnetic Storms, Including Extreme Events}",
journal = {\grl},
keywords = {extreme geomagnetic storms, thermosphere heating, thermosphere cooling, superposed epoch density},
year = 2019,
month = nov,
volume = {46},
number = {22},
pages = {12,739-12,746},
abstract = "{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 mass density
database of the CHAllenging Mini-satellite Payload and Gravity
Recovery And Climate Experiment missions to produce
thermospheric global system response to geomagnetic storms
caused by coronal mass ejections via superposed epoch analysis
during May 2001 to December 2015. Storm events are grouped in
five different categories based on the minimum value of the
SYM-H index. We calculate the time from storm onset for the
thermosphere to reach maximum intensification (heating time) and
the time from onset for the thermosphere to recover (cooling
time). We find that heating and cooling times decrease as storm
intensity increases and the effect is more pronounced for the
cooling times. For extreme storms, the thermospheric heating
time is 9.5 hr, while the cooling time is 22 hr.}",
doi = {10.1029/2019GL085120},
adsurl = {https://ui.adsabs.harvard.edu/abs/2019GeoRL..4612739Z},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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