The Dependence of the Peak Velocity of High-Speed Solar Wind Streams as Measured in the Ecliptic by ACE and the STEREO satellites on the Area and Co-latitude of Their Solar Source Coronal Holes

Author:

Hofmeister Stefan J.1ORCID,Veronig Astrid1ORCID,Temmer Manuela1ORCID,Vennerstrom Susanne2ORCID,Heber Bernd3ORCID,Vršnak Bojan4ORCID

Affiliation:

1. IGAM-Kanzelhöhe Observatory, NAWI Graz, Institute of Physics; University of Graz; Graz Austria

2. DTU Space, National Space Institute; Kongens Lyngby Denmark

3. Institut für Experimentelle und Angewandte Physik; Universität Kiel; Kiel Germany

4. Hvar Observatory; Faculty of Geodesy; Zagreb Croatia

Funder

Austrian Science Fund

Österreichische Forschungsförderungsgesellschaft

Steiermärkischen Sparkassen

Karl-Franzens-Universität Graz

Hrvatska Zaklada za Znanost

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference34 articles.

1. Parameters of the magnetic flux inside coronal holes;Abramenko;Solar Physics,2009

2. Improvement in the prediction of solar wind conditions using near-real time solar magnetic field updates;Arge;Journal of Geophysical Research,2000

3. Improved method for specifying solar wind speed near the Sun;Arge;Solar Wind Ten,2003

4. The standardized index Ks and the planetary index Kp;Bartels;International Association of Terrestrial Magnetism and Electricity Bulletin,1949

5. Large-amplitude Alfvén waves in the interplanetary medium, 2;Belcher;Journal of Geophysical Research,1971

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