The rotation of the Fe XIV solar corona during the recent solar activity minimum

Space Science Reviews

Volumn 87, Issue 1-2, 1999, Pages 211-214

  Inhester, B ^a   Stenborg, G ^a   Schwenn, R ^a   Srivastava, N ^a   Podlipnik, B ^a  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0039834150     PISSN: 00386308     EISSN: None     Source Type: Journal    
DOI: 10.1007/978-94-015-9167-6_29     Document Type: Article

References (6)

1. Howard, R.: 1984, 'Solar rotation,' Ann. Rev. Astron. Astrophys., 22, 131-155.
2. Lewis, D. J. et al.: 1998, 'LASCO observations of the coronal rotation,' in preparation.
3. Schwenn, R., et al.: 1997, 'First view of the green-line emission corona at solar activity minimum using the LASCO-C1 coronagraph,' Solar Phys., 175, 667-684.
4. Sime, D. G., Fisher, R. R., and Altrock, R. C.: 1989, 'Rotation characteristics of the Fe XIV solar corona,' Astrophys. J., 336, 454-467.
5. Sterlingwerf, R. F.: 1978, 'Period determination using the phase dispersion method,' Astrophys. J., 224, 953-960.
6. Wang, Y. M., Sheeley, N. R., Nash, A. G., and Shampine, L. R.: 1988, 'The quasi-rigid rotation of coronal magnetic fields,' Astrophys. J., 327, 427-450.