Comment on "Properties of the recovery phase of extreme storms" by Choraghe et al. (2021)
Identificadores
Enlace permanente (URI): http://hdl.handle.net/10017/50725DOI: 10.1029/2021JA029999
ISSN: 2169-9402
Editor
AGU (American Geophysical Union)
Fecha de publicación
2021-12-20Cita bibliográfica
Cid, C. & Saiz, E. 2021, "Comment on "Properties of the recovery phase of extreme storms" by Choraghe et al. (2021)", Journal of Geophysical Research: Space Physics, vol. 127, no. 1.
Tipo de documento
info:eu-repo/semantics/article
Versión
info:eu-repo/semantics/publishedVersion
Versión del editor
https://doi.org/10.1029/2021JA029999Derechos
Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)
Derechos de acceso
info:eu-repo/semantics/openAccess
Resumen
Choraghe et al. (2021), based on a study of the recovery phase of the SYM-H index of 31 extreme
geomagnetic storms, have recently concluded that the hyperbolic decay function is only able to explain the
complete recovery phase of about one third of events and that both the exponential or the hyperbolic decay
functions fail to explain the late recovery phase of storms. Furthermore, they propose a linear function to model
the late recovery phase and claim that the proposed model could throw new light on the relative importance of
different physical processes involved during the complete recovery phase of extreme storms. We assert that the
Choraghe et al. (2021) conclusions regarding the recovery phase of extreme storms analysis are incorrect and
in particular are based on a misunderstanding of the nature of the evolution of the SYM-H index and the energy
balance of the ring current.
Ficheros en el ítem
Ficheros | Tamaño | Formato |
|
---|---|---|---|
Comment_Cid_JGR_Space_Physics_ ... | 775.4Kb |
|
Ficheros | Tamaño | Formato |
|
---|---|---|---|
Comment_Cid_JGR_Space_Physics_ ... | 775.4Kb |
|
Colecciones
- FISICA - Artículos [76]