Resonant absorption of nonlinear slow MHD waves in isotropic steady plasmas I. Theory

Solar Physics

Volumn 180, Issue 1-2, 1998, Pages 65-79

  Ballai, István ^a,c   Erdélyi, Róbert ^b,d  

^a EÖTVÖS LORÁND UNIVERSITY   (Hungary)

^b UNIVERSITY OF ST ANDREWS   (United Kingdom)

^c FRIEDRICH SCHILLER UNIVERSITY JENA   (Germany)

^d ARMAGH OBSERVATORY   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0042224560     PISSN: 00380938     EISSN: None     Source Type: Journal    
DOI: 10.1023/a:1005068127935     Document Type: Article

References (20)

1. Ballai, I., Erdélyi, R., and Ruderman, M. S.: 1997, Phys. Plasmas, submitted.
2. Ballai, I., Ruderman, M. S., and Erdélyi, R.: 1998, Phys. Plasmas, in press.
3. Čadež, V. M. and Ballester, J. L.: 1996, Astron. Astrophys. 305, 977.
4. Čadež, V. M., Csík, A., Erdélyi, R., and Goossens, M.: 1997, Astron. Astrophys. 326, 1241.
5. Csík, A., Erdélyi, R., and Čadež, V. M.: 1997, Solar Phys. 172, 61.
6. Doyle, J. G., O'Shea, E., Erdélyi, R., Dere, K. P., Socker, D. G., and Keenan, F. P.: 1997, Solar Phys. 173, 243.
7. Erdélyi, R.: 1997, Solar Phys. 171, 49.
8. Erdélyi, R.: 1998, Solar Phys. 180, 213 (this issue).
9. Erdélyi, R. and Goossens, M.: 1996, Astron. Astrophys. 313, 664.
10. Erdélyi, R., Goossens, M., and Ruderman, M. S.: 1995, Solar Phys. 161, 123.
11. Goossens, M., Hollweg, J. V., and Sakurai, T.: 1992, Solar Phys. 138, 233.
12. Goossens, M., Ruderman, M. S., and Hollweg, J. V.: 1995, Solar Phys. 157, 75.
13. Hollweg, J. V.: 1987, Astrophys. J. 312, 880.
14. Hollweg, J. V.: 1988, Astrophys. J. 335, 1005.
15. Hollweg, J. V. and Yang, G.: 1988, J. Geophys. Res. 93, 5423.
16. Keppens, R.: 1996, Astrophys. J. 468, 907.
17. Nayfeh, A. H.: 1981, Introduction to Perturbation Techniques, Wiley Interscience, New York.
18. Ruderman, M. S., Goossens, M., and Hollweg, J. V.: 1997, Phys. Plasmas 4, 91.
19. Ruderman, M. S., Hollweg, J. V., and Goossens, M.: 1997, Phys. Plasmas 4, 75 (RHG).
20. Sakurai, T., Goossens, M., and Hollweg, J. V.: 1991, Solar Phys. 133, 227.