The response time of the magnetopause reconnection location to changes in the solar wind: MMS case study-Reference-Cited by-同舟云学术

The response time of the magnetopause reconnection location to changes in the solar wind: MMS case study

Published:2016-05-17 Issue:10 Volume:43 Page:4673-4682
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Trattner K. J.¹,Burch J. L.²,Ergun R.¹,Fuselier S. A.²³,Gomez R. G.²,Grimes E. W.⁴,Lewis W. S.²,Mauk B.⁵,Petrinec S. M.⁶,Pollock C. J.⁷,Phan T. D.⁸,Vines S. K.²³,Wilder F. D.¹,Young D. T.²

Affiliation:

1. Laboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder Colorado USA

2. Southwest Research Institute San Antonio Texas USA

3. Physics and Astronomy Department University of Texas at San Antonio San Antonio Texas USA

4. Institute of Geophysics and Planetary Physics, Department of Earth and Space Sciences UCLA Los Angeles California USA

5. Applied Physics Laboratory Johns Hopkins University Baltimore Maryland USA

6. Lockheed Martin ATC Palo Alto California USA

7. NASA GSFC Greenbelt Maryland USA

8. Space Physics Research Group University of California Berkeley California USA

Funder

NASA

NSF

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016GL068554

Reference40 articles.

1. Technique for increasing dynamic range of space-borne ion composition instruments

2. Magnetospheric Multiscale Overview and Science Objectives

3. Role of the magnetosheath flow in determining the motion of open flux tubes

4. The causes of convection in the Earth's magnetosphere: A review of developments during the IMS

5. A simple illustrative model of open flux tube motion over the dayside magnetopause

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