MHD heliosphere with boundary conditions from a tomographic reconstruction using interplanetary scintillation data-Reference-Cited by-同舟云学术

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MHD heliosphere with boundary conditions from a tomographic reconstruction using interplanetary scintillation data

Published:2014-10 Issue:10 Volume:119 Page:7981-7997
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Kim T. K.¹,Pogorelov N. V.¹,Borovikov S. N.¹,Jackson B. V.²,Yu H.-S.²,Tokumaru M.³

Affiliation:

1. Center for Space Plasma and Aeronomic Research; University of Alabama in Huntsville; Huntsville Alabama USA

2. Center for Astrophysics and Space Sciences; University of California, San Diego; La Jolla California USA

3. Solar-Terrestrial Environment Laboratory; Nagoya University; Nagoya Japan

Funder

NASA

NSF PRAC

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/2013JA019755/fullpdf

Reference99 articles.

1. Analysis of three-station interplanetary scintillation;Armstrong;J. Geophys. Res.,1972

2. Heliospheric tomography using interplanetary scintillation observations. III-Correlation between speed and electron density fluctuations in the solar wind;Asai;J. Geophys. Res.,1998

3. The Ulysses solar wind plasma experiment;Bame;Astron. Astrophys. Suppl. Ser.,1992

4. Large-scale structure of the fast solar wind;Bisi;J. Geophys. Res.,2007

5. Three-dimensional reconstructions of the early November 2004 coordinated data analysis workshop geomagnetic storms: Analyses of STELab IPS speed and SMEI density data;Bisi;J. Geophys. Res.,2008

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