TY - JOUR
T1 - Geomagnetic Activity Effects on CO2-Driven Trend in the Thermosphere and Ionosphere
T2 - Ideal Model Experiments With GAIA
AU - Liu, Huixin
AU - Tao, Chihiro
AU - Jin, Hidekatsu
AU - Abe, Takamichi
N1 - Funding Information:
The authors thank the reviewers for their comments which helped to improve the original manuscript. H. L. acknowledges supports by JSPS KAKENHI (Grants nos. 18H01270, 18H04446, and 17KK0095) and JRPs‐LEAD with DFG. CT is supported by JSPS KAKENHI 19K03942.
Publisher Copyright:
© 2020. The Authors.
PY - 2021/1
Y1 - 2021/1
N2 - We examine impacts of geomagnetic activity (GA) on CO2-driven trend in the ionosphere and thermosphere using the Ground-to-topside Atmosphere Ionosphere model for Aeronomy whole atmosphere model. The model reveals three salient features. (1) Geomagnetic activities usually weakens the CO2-driven trend at a fixed altitude. Among the IT parameters analyzed, the thermosphere mass density is the most robust indicator for CO2 cooling effect even with GA influences. (2) Geomagnetic activities can either strengthen or weaken the CO2-driven trend in hmF2 and NmF2, depending on local time and latitudes. This renders the widely used linear fitting methods invalid for removing geomagnetic effects from observations. (3) An interdependency exists between the efficiency of CO2 forcing and geomagnetic forcing, with the former enhances at lower GA level, while the latter enhances at higher CO2 concentration. This could imply that the CO2-driven trend would accelerate in periods of declining GA, while magnetic storms may have larger space weather impacts in the future with increasing CO2. These findings provide a preliminary model framework to understand interactions between the CO2 forcing from below and the geomagnetic forcing from above.
AB - We examine impacts of geomagnetic activity (GA) on CO2-driven trend in the ionosphere and thermosphere using the Ground-to-topside Atmosphere Ionosphere model for Aeronomy whole atmosphere model. The model reveals three salient features. (1) Geomagnetic activities usually weakens the CO2-driven trend at a fixed altitude. Among the IT parameters analyzed, the thermosphere mass density is the most robust indicator for CO2 cooling effect even with GA influences. (2) Geomagnetic activities can either strengthen or weaken the CO2-driven trend in hmF2 and NmF2, depending on local time and latitudes. This renders the widely used linear fitting methods invalid for removing geomagnetic effects from observations. (3) An interdependency exists between the efficiency of CO2 forcing and geomagnetic forcing, with the former enhances at lower GA level, while the latter enhances at higher CO2 concentration. This could imply that the CO2-driven trend would accelerate in periods of declining GA, while magnetic storms may have larger space weather impacts in the future with increasing CO2. These findings provide a preliminary model framework to understand interactions between the CO2 forcing from below and the geomagnetic forcing from above.
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U2 - 10.1029/2020JA028607
DO - 10.1029/2020JA028607
M3 - Article
AN - SCOPUS:85102067045
SN - 2169-9380
VL - 126
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 1
M1 - e2020JA028607
ER -