Comparison of empirical models of ionospheric heating to global simulations
Intense currents produced during geomagnetic storms dissipate energy in the ionosphere through Joule heating. This dissipation has significant space weather effects, and thus it is important to determine the ability of physics-based simulations to replicate real events quantitatively. Several empiri...
Main Authors: | Fatemeh Bagheri, Ramon E. Lopez |
---|---|
Format: | Article |
Language: | English |
Published: |
Frontiers Media S.A.
2023-06-01
|
Series: | Frontiers in Astronomy and Space Sciences |
Subjects: | |
Online Access: | https://www.frontiersin.org/articles/10.3389/fspas.2023.1170390/full |
Similar Items
-
Quantifying the ability of magnetohydrodynamic models to reproduce observed Birkeland current and auroral electrojet magnitudes
by: Tre’Shunda James, et al.
Published: (2023-08-01) -
Global Magnetohydrodynamic Simulations: Performance Quantification of Magnetopause Distances and Convection Potential Predictions
by: Agnit Mukhopadhyay, et al.
Published: (2021-04-01) -
Ionospheric occultation constellation: Global monitoring and simulation
by: Xiaochen Gou, et al.
Published: (2022-09-01) -
Global and local Joule heating during substorms in St. Patrick’s Day 2015 geomagnetic storm
by: K. J. Suji, et al.
Published: (2018-10-01) -
Influences of the state of ionospheric background on ionospheric heating effects
by: Shuji Hao, et al.
Published: (2014-01-01)