How the IMFByInduces a LocalByComponent During Northward IMFBzand Characteristic Timescales-Reference-Cited by-同舟云学术

How the IMFByInduces a LocalByComponent During Northward IMFBzand Characteristic Timescales

Published:2018-05 Issue:5 Volume:123 Page:3333-3348
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,Haaland S.¹²^ORCID,Snekvik K.¹^ORCID,Laundal K. M.¹^ORCID,Reistad J. P.¹^ORCID,Strangeway R.³^ORCID,Milan S. E.¹⁴^ORCID,Hesse M.¹^ORCID,Ohma A.¹^ORCID

Affiliation:

1. Birkeland Centre for Space Science, Department of Physics and Technology; University of Bergen; Bergen Norway

2. Max Planck Institute for Solar System Research; Göttingen Germany

3. Institute of Geophysics and Planetary Physics; University of California; Los Angeles CA USA

4. Department of Physics and Astronomy; University of Leicester; Leicester UK

Funder

Research Council of Norway/CoE

Science and Technology Facilities Council

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/2018JA025186/fullpdf

Reference70 articles.

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2. Magnetospheric asymmetries associated with the y-component of the IMF;Cowley;Planetary and Space Science,1981

3. Observation of an IMF sector effect in the Y-magnetic field component at geostationary orbit;Cowley;Planetary and Space Science,1983

4. Dayside merging and cusp geometry;Crooker;Journal of Geophysical Research,1979

5. Reverse convection;Crooker;Journal of Geophysical Research,1992

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