Understanding coronal heating and solar wind acceleration: Case for in situ near-Sun measurements

Author:

McComas D. J.1,Velli M.23,Lewis W. S.1,Acton L. W.4,Balat-Pichelin M.5,Bothmer V.6,Dirling R. B.7,Feldman W. C.8,Gloeckler G.9,Habbal S. R.10,Hassler D. M.11,Mann I.12,Matthaeus W. H.13,McNutt R. L.14,Mewaldt R. A.15,Murphy N.3,Ofman L.16,Sittler E. C.17,Smith C. W.18,Zurbuchen T. H.19

Affiliation:

1. Space Science and Engineering Division; Southwest Research Institute; San Antonio Texas USA

2. Dipartimento di Astronomia e Scienza del Spazio; Università degli Studi di Firenze; Florence Italy

3. Jet Propulsion Laboratory; Pasadena California USA

4. Department of Physics; Montana State University; Bozeman Montana USA

5. Processes, Materials and Solar Energy; CNRS; Font-Romeu France

6. Institut für Astrophysik; Georg-August-Universität Göttingen; Göttingen Germany

7. Science Applications International Corporation; Fountain Valley California USA

8. Los Alamos National Laboratory; Los Alamos New Mexico USA

9. Department of Physics; University of Maryland; College Park Maryland USA

10. Institute for Astronomy; University of Hawaii at Manoa; Honolulu USA

11. Space Studies Department; Southwest Research Institute; Boulder Colorado USA

12. Department of Earth and Planetary Sciences; Kobe University; Kobe Japan

13. Bartol Research Institute; University of Delaware; Newark Delaware USA

14. Johns Hopkins University Applied Physics Laboratory; Laurel Maryland USA

15. Space Radiation Laboratory; California Institute of Technology; Pasadena California USA

16. Physics Department; Catholic University of America; Washington, D. C. USA

17. NASA Goddard Space Flight Center; Greenbelt Maryland USA

18. Department of Earth, Oceans and Space; University of New Hampshire; Durham New Hampshire USA

19. Department of Atmospheric, Oceanic, and Space Science; University of Michigan; Ann Arbor Michigan USA

Publisher

American Geophysical Union (AGU)

Subject

Geophysics

Reference151 articles.

1. Magnetic fields and the structure of the solar corona. 1: Methods of calculating coronal fields;Altschuler;Sol. Phys.,1969

2. Test particle acceleration in turbulent reconnecting magnetic fields;Ambrosiano;J. Geophys. Res.,1988

3. Kometenschweife und solare Korpuskularstrahlung;Biermann;Z. Astrophys.,1951

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