Helios Observations of Quasiperiodic Density Structures in the Slow Solar Wind at 0.3, 0.4, and 0.6 AU-Reference-Cited by-同舟云学术

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Helios Observations of Quasiperiodic Density Structures in the Slow Solar Wind at 0.3, 0.4, and 0.6 AU

Published:2019-02 Issue:2 Volume:124 Page:837-860
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Di Matteo S.¹²^ORCID,Viall N. M.³^ORCID,Kepko L.³^ORCID,Wallace S.³⁴^ORCID,Arge C. N.³,MacNeice P.³^ORCID

Affiliation:

1. Department of Physical and Chemical SciencesUniversity of L'Aquila L'Aquila Italy

2. Consorzio Area di Ricerca in Astrogeofisica L'Aquila Italy

3. NASA Goddard Space Flight Center Greenbelt MD USA

4. Department of Physics and AstronomyUniversity of New Mexico Albuquerque NM USA

Funder

National Aeronautics and Space Administration Heliophysics Internal Science Funding Model

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2018JA026182

Reference107 articles.

1. An MHD code for the study of magnetic structures in the solar wind

2. A MODEL FOR THE SOURCES OF THE SLOW SOLAR WIND

3. Two solar cycles of nonincreasing magnetic flux

4. Stream structure and coronal sources of the solar wind during the May 12th, 1997 CME

5. Improved Method for Specifying Solar Wind Speed Near the Sun

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