Active-Region Sources of Solar Wind near Solar Maximum

AIP Conference Proceedings

Volumn 679, Issue , 2003, Pages 51-54

  Liewer, Paulett C ^a   Neugebauer, Marcia ^b   Zurbuchen, Thomas ^c  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b UNIVERSITY OF ARIZONA   (United States)

^c UNIVERSITY OF MICHIGAN   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

X RAY ANALYSIS; X RAYS;

ACTIVE REGIONS; CHARGE STATE; CORONAL HOLE; CORONAL STRUCTURE; MAGNETIC MODELING; MAGNETIC TOPOLOGIES; SOURCE REGION; SYNOPTIC MAPS;

SOLAR WIND;

EID: 85011608396     PISSN: 0094243X     EISSN: 15517616     Source Type: Conference Proceeding    
DOI: 10.1063/1.1618539     Document Type: Conference Paper

References (5)

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2. Neugebauer, M., Liewer, P. C., Smith, E. J., Skoug, R. M., and Zurbuchen, T. H., Sources of the Solar Wind at Solar Activity Maximum, J. Geophys. Res. (2002).
3. Levine, R. H., Large scale solar magnetic fields and coronal holes, in Coronal Holes and High Speed Wind Streams, ed. J. B. Zirker, pp. 103-143, Co. Assoc. Univ. Press, Boulder (1977).
4. Kojima, M., K. Fujiki, T. Ohmi, M. Tokamaru, A. Yokobe, and K. Hakamada, Low-speed solar wind from the vicinity of solar active regions, J. Geophys. Res., 104, 16993 (1999).
5. Zurbuchen, T. H., S. Hefti, L. A. Fisk, G. Gloeckler, and N. A. Schwadron, Magnetic structure of the slow solar wind: Constraints from composition data, J. Geophys. Res., 105, 18327 (2000).