Estimating the open magnetic flux from the interplanetary and ionospheric conditions

3Citations
Citations of this article
5Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

The open magnetic flux (FPC) is a key parameter to study magnetospheric dynamical process, which is closely related to magnetic reconnections in the dayside magnetopause and magnetotail. Using global MHD simulations, we find that the open magnetic flux FPC can be estimated through a combined parameter f by FPC=0.89f/(f+0.20)+0.52, where the parameter f=vSWBSnSW1/5ΣP1/3 is a function of the solar wind velocity (vSW), the solar wind number density (nSW), the southern interplanetary magnetic field (IMF) strength (BS), and the ionospheric Pederson conductance (ΣP). The comparison with the limited observational FPCdata available in the literature shows its promise in estimating the open magnetic flux from the interplanetary and ionospheric conditions. The open magnetic flux (FPC) may be served as a key space weather forecast element in the future. Key Points Estimate open magnetic flux from interplanetary and ionospheric conditions.A combined parameter is found to estimate the open magnetic flux.The model results are confirmed by the observations. © 2013. American Geophysical Union. All Rights Reserved.

Author supplied keywords

Cite

CITATION STYLE

APA

Wang, C., Xia, Z. Y., Peng, Z., & Lu, Q. M. (2013). Estimating the open magnetic flux from the interplanetary and ionospheric conditions. Journal of Geophysical Research: Space Physics, 118(5), 1899–1903. https://doi.org/10.1002/jgra.50255

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free