Heliolatitudinal and time variations of the solar wind mass flux: Inferences from the backscattered solar Lyman-alpha intensity maps-Reference-Cited by-同舟云学术

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Heliolatitudinal and time variations of the solar wind mass flux: Inferences from the backscattered solar Lyman-alpha intensity maps

Published:2013-06 Issue:6 Volume:118 Page:2800-2808
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Katushkina O. A.¹²,Izmodenov V. V.¹²³,Quemerais E.⁴,Sokół J. M.⁵

Affiliation:

1. Space Research Institute; Russian Academy of Sciences; Moscow Russia

2. Department of Mechanics and Mathematics; Lomonosov Moscow State University; Moscow Russia

3. Institute for Problems in Mechanics; Russian Academy of Sciences; Moscow Russia

4. LATMOS; Paris France

5. Space Research Centre; Polish Academy of Sciences; Warsaw Poland

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/jgra.50303/fullpdf

Reference31 articles.

1. Model of the solar wind interaction with the local interstellar medium-Numerical solution of self-consistent problem;Baranov;J. Geophys. Res.,1993

2. SWAN: A study of solar wind anisotropy on SOHO with Lyman alpha sky mapping;Bertaux;Sol. Phys.,1995

3. First results from SWAN Lyman alpha solar wind mapper on SOHO;Bertaux;Sol. Phys.,1997

4. Imaging the three-dimensional solar wind;Gruntman;J. Geophys. Res.,2001

5. Imaging the global solar wind flow in EUV;Gruntman;J. Geophys. Res.,2006

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