Plasma properties in coronal funnels

Space Science Reviews

Volumn 87, Issue 1-2, 1999, Pages 207-210

  Hackenberg, P ^a   Mann, G ^a   Marsch, E ^b  

^a ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^b MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

Author keywords

Coronal holes; Magnetic network; Solar wind

Indexed keywords

EID: 0007613860     PISSN: 00386308     EISSN: None     Source Type: Journal    
DOI: 10.1007/978-94-015-9167-6_28     Document Type: Article

References (5)

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2. Gabriel, A. H.: 1976, 'A magnetic model of the solar transition region,' Phil. Trans. R. Soc. London, 281, 339-352.
3. Marsch, E., and Tu, C.-Y.: 1997, 'Solar wind and chromospheric network,' Sol. Phys., 176, 87-106.
4. Priest, E. R.: 1984, Solar Magnetohydrodynamics, Dordrecht: D. Reidel Publishing Company.
5. Wilhelm, K., Marsch, E., Dwivedi, B. N., Hassler, D. M., Lemaire, P., Gabriel, A. H., and Huber, M. C. E.: 1998, 'The solar corona above polar coronal holes as seen by SUMER on SOHO,' Astrophys. J., 500, 1023-1038.