Magnetospheric response and reconfiguration times following IMF B y reversals-Reference-Cited by-同舟云学术

Magnetospheric response and reconfiguration times following IMF B y reversals

Published:2017-01 Issue:1 Volume:122 Page:417-431
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Tenfjord P.¹^ORCID,Østgaard N.¹^ORCID,Strangeway R.²^ORCID,Haaland S.¹³^ORCID,Snekvik K.¹^ORCID,Laundal K. M.¹^ORCID,Reistad J. P.¹^ORCID,Milan S. E.¹⁴^ORCID

Affiliation:

1. Birkeland Centre for Space Science, Department of Physics and TechnologyUniversity of Bergen Bergen Norway

2. Institute of Geophysics and Planetary PhysicsUniversity of California Los Angeles California USA

3. Department of Physics and AstronomyUniversity of Leicester Leicester UK

4. Max Planck Institute for Solar System Research Göttingen Germany

Funder

Science and Technology Facilities Council

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016JA023018

Reference53 articles.

1. Bursty bulk flows in the inner central plasma sheet

2. Bursty bulk flows and dipolarization in MHD simulations of magnetotail reconnection

3. Substorm and interplanetary magnetic field effects on the geomagnetic tail lobes

4. Dependence of IMFBypenetration into the neutral sheet on IMFBzand geomagnetic activity

5. Magnetospheric asymmetries associated with the y-component of the IMF

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