Changes in the Magnetic Field Topology and the Dayside/Nightside Reconnection Rates in Response to a Solar Wind Dynamic Pressure Front: A Case Study-Reference-Cited by-同舟云学术

Changes in the Magnetic Field Topology and the Dayside/Nightside Reconnection Rates in Response to a Solar Wind Dynamic Pressure Front: A Case Study

Author:

Boudouridis A.¹²³^ORCID,Connor H. K.⁴^ORCID,Lummerzheim D.⁴^ORCID,Ridley A. J.⁵^ORCID,Zesta E.⁶^ORCID

Affiliation:

1. Space Sciences Institute Boulder CO USA

2. Cooperative Institute for Research in Environmental Sciences University of Colorado Boulder CO USA

3. National Center for Environmental Information National Oceanic and Atmospheric Administration Boulder CO USA

4. Geophysical Institute University of Alaska Fairbanks AK USA

5. University of Michigan Ann Arbor MI USA

6. NASA Goddard Space Flight Center Greenbelt MD USA

Funder

National Aeronautics and Space Administration

Office of Experimental Program to Stimulate Competitive Research

Division of Atmospheric and Geospace Sciences

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

Reference79 articles.

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