Ionospheric response to the interplanetary magnetic field southward turning: Fast onset and slow reconfiguration-Reference-Cited by-同舟云学术

Ionospheric response to the interplanetary magnetic field southward turning: Fast onset and slow reconfiguration

Published:2002-08 Issue:A8 Volume:107 Page:SIA 2-1-SIA 2-9
ISSN:0148-0227
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res.

Author:

Lu G.¹,Holzer T. E.¹,Lummerzheim D.²,Ruohoniemi J. M.³,Stauning P.⁴,Troshichev O.⁵,Newell P. T.³,Brittnacher M.⁶,Parks G.⁷

Affiliation:

1. High Altitude Observatory; National Center for Atmospheric Research; Boulder Colorado USA

2. Geophysical Institute; University of Alaska; Fairbanks Alaska USA

3. Applied Physics Laboratory; Johns Hopkins University; Laurel Maryland USA

4. Danish Meteorological Institute; Copenhagen Denmark

5. Arctic and Antarctic Research Institute; St. Petersburg Russia

6. Earth and Space Sciences Department; University of Washington; Seattle Washington USA

7. Space Sciences Laboratory; University of California; Berkeley California USA

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference24 articles.

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3. The dependence of high-latitude dayside ionospheric flows on the north-south component of the IMF: A high time resolution correlation analysis using EISCAT “Polar” and AMPTE UKS and IRM data;Etemadi;Planet. Space Sci.,1988

4. Central polar cap convection response to short duration southward interplanetary magnetic field;Jayachandran;Ann. Geophys.,2000

5. Observations of the response time of high-latitude ionospheric convection to variations in the interplanetary magnetic field using EISCAT and IMP-8 data;Khan;Ann. Geophys.,1999

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