Radial evolution of the three-dimensional structure in CIRs between Earth and Ulysses

Author:

Broiles T. W.12,Desai M. I.23,Lee C. O.45,MacNeice P. J.6

Affiliation:

1. Department of Physics and Astronomy; University of Texas at San Antonio; San Antonio Texas USA

2. Space Sciences and Engineering Division; Southwest Research Institute; San Antonio Texas USA

3. Also at Department of Physics and Astronomy; University of Texas at San Antonio; San Antonio Texas USA

4. Institute for Scientific Research; Boston College; Chestnut Hill Massachusetts USA

5. Air Force Research Laboratory/Space Vehicles Directorate; Kirtland Air Force Base; Albuquerque New Mexico USA

6. NASA Goddard Space Flight Center; Greenbelt Maryland USA

Funder

NASA

NSF

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference41 articles.

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2. The structure and dynamics of the Corona-Heliosphere connection;Antiochos;Space Sci. Rev.,2011

3. Improvement in the prediction of solar wind conditions using near-real time solar magnetic field updates;Arge;J. Geophys. Res.,2000

4. Stream structure and coronal sources of the solar wind during the May 12th, 1997 CME;Arge;J. Atmos. Sol.-Terr. Phy.,2004

5. The magnetic field investigation on the ULYSSES mission-Instrumentation and preliminary scientific results;Balogh;Astron. Astrophys. Suppl. Ser.,1992

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