University of Oulu

Holappa, L., & Mursula, K. (2018). Explicit IMF By dependence in high‐latitude geomagnetic activity. Journal of Geophysical Research: Space Physics, 123, 4728–4740. https://doi.org/10.1029/2018JA025517

Explicit IMF By dependence in high‐latitude geomagnetic activity

Saved in:
Author: Holappa, L.1,2,3; Mursula, K.1
Organizations: 1ReSoLVE Centre of Excellence, Space Climate Research Unit, University of Oulu, Oulu, Finland
2Solar Physics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD, USA
3Department of Physics, The Catholic University of America, Washington, DC, USA
Format: article
Version: accepted version
Access: open
Online Access: PDF Full Text (PDF, 1 MB)
Persistent link: http://urn.fi/urn:nbn:fi-fe2018082834234
Language: English
Published: American Geophysical Union, 2018
Publish Date: 2018-08-29
Description:

Abstract

The interaction of the solar wind with the Earth's magnetic field produces geomagnetic activity, which is critically dependent on the orientation of the interplanetary magnetic field (IMF). Most solar wind coupling functions quantify this dependence on the IMF orientation with the so‐called IMF clock angle in a way, which is symmetric with respect to the sign of the By component. However, recent studies have suggested that the sign of By is an additional, independent driver of high‐latitude geomagnetic activity, leading to higher (weaker) geomagnetic activity in Northern Hemisphere (NH) winter for By > 0 (By<0). In this paper we quantify the size of this explicit By effect with respect to the solar wind coupling function, both for northern and southern high‐latitude geomagnetic activity. We show that high‐latitude geomagnetic activity is significantly (by about 40%–50%) suppressed for By < 0 in NH winter and for By > 0 in Southern Hemisphere winter. When averaged over all months, high‐latitude geomagnetic activity in NH is about 12% weaker for By < 0 than for By > 0. The By effect affects the westward electrojet strongly, but hardly at all the eastward electrojet. We also show that the suppression of the westward electrojet in NH during By < 0 maximizes when the Earth's dipole axis points toward the night sector, that is, when the auroral region is maximally in darkness.

see all

Series: Journal of geophysical research. Space physics
ISSN: 2169-9380
ISSN-E: 2169-9402
ISSN-L: 2169-9380
Volume: 123
Issue: 6
Pages: 4728 - 4740
DOI: 10.1029/2018JA025517
OADOI: https://oadoi.org/10.1029/2018JA025517
Type of Publication: A1 Journal article – refereed
Field of Science: 114 Physical sciences
115 Astronomy and space science
Subjects:
Funding: We acknowledge the financial support by the Academy of Finland to the ReSoLVE Centre of Excellence (project 272157).
Academy of Finland Grant Number: 272157
Detailed Information: 272157 (Academy of Finland Funding decision)
Copyright information: © 2018. American Geophysical Union. Published in this repository with the kind permission of the publisher.