Alfvén waves in the solar corona

Science

Volumn 317, Issue 5842, 2007, Pages 1192-1196

  Tomczyk, S ^a   McIntosh, S W ^a,b   Keil, S L ^c   Judge, P G ^a   Schad, T ^d   Seeley, D H ^e   Edmondson, J ^f  

^a NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

^b SOUTHWEST RESEARCH INSTITUTE   (United States)

^c NATIONAL SOLAR OBSERVATORY   (United States)

^d UNIVERSITY OF NOTRE DAME   (United States)

^e Framingham Public Schools   (United States)

^f UNIVERSITY OF MICHIGAN   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

CONVECTION; CORONA; ENERGY FLUX; MAGNETIC FIELD; OSCILLATION; POLARIZATION; S-WAVE; SOLAR SYSTEM; WAVE PROPAGATION;

ARTICLE; FOURIER ANALYSIS; HEAT; MAGNETIC FIELD; POLARIMETRY; PRIORITY JOURNAL; SOLAR ENERGY; SUN;

EID: 36849043015     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1143304     Document Type: Article

References (32)

1. H. Alfvén, Nature 150, 405 (1942).
2. H. Alfvén, Mon. Not. R. Astron. Soc. 107, 211 (1947).
3. D. Osterbrock, Astrophys. J. 134, 347 (1961).
4. M. J. Aschwanden, L. Fletcher, C. J. Schrijver, G. Alexander, Astrophys. J. 520, 880 (1999).
5. V. M. Nakariakov, L. Ofman, E. E. DeLuca, B. Roberts, J. M. Davila, Science 285, 862 (1999).
6. C. E. DeForest, J. B. Gurman, Astrophys. J. 501, L217 (1998).
7. I. De Moortel, J. Ireland, R. W. Walsh, Astron. Astrophys. 355, L23 (2000).
8. M. A. Marsh, R. W. Walsh, Astrophys. J. 643, 540 (2006).
9. M. Minarovjech et al., Sol. Phys. 213, 269 (2003).
10. D. R. Williams et al., Mon. Not. R. Astron. Soc. 326, 428 (2001).
11. J. M. Pasachoff, F. A. Babcock, K. D. Russell, D. B. Seaton, Sol. Phys. 207, 241 (2002).
12. S. Koutchmy, I. D. Zhugzhda, V. Locans, Astron. Astrophys. 120, 185 (1983).
13. T. Sakurai, K. Ichimoto, K. P. Raju, J. Singh, Sol. Phys. 209, 265 (2002).
14. J. W. Belcher, Astrophys. J. 168, 505 (1971).
15. P. Charvin, Ann. Astrophys. 28, 877 (1965).
16. S. M. Jefferies et al., Astrophys. J. 434, 795 (1994).
17. W. Finsterle et al., Astrophys. J. 613, L185 (2004).
18. S. W. McIntosh, B. Fleck, T. D. Tarbell, Astrophys. J. 609, L95 (2004).
19. B. W. Lites, R. Rutten, W. Kalkofen, Astrophys. J. 414, 345 (1993).
20. B. De Pontieu, R. Erdélyi, I. DeMoortel, Astrophys. J. 624, L61 (2005).
21. V. H. Hansteen et al., Astrophys. J. 647, L73 (2006).
22. S. W. McIntosh, S. M. Jefferies, Astrophys. J. 647, L77 (2006).
23. S. M. Jefferies et al., Astrophys. J. 648, L151 (2006).
24. B. De Pontieu et al., Astrophys. J. 655, 624 (2007).
25. O. Wikstol, P. G. Judge, V. Hansteen, Astrophys. J. 501, 895 (1998).
26. P. G. Judge, A. Pietarila, Astrophys. J. 606, 1258 (2004).
27. D. Melrose, Aust. J. Phys. 30, 647 (1977).
28. G. L. Withbroe, R. W. Noyes, Annu. Rev. Astron. Astrophys. 15, 363 (1977).
29. E. Verwichte, C. Foullon, V. M. Nakariakov, Astron. Astrophys. 446, 1139 (2006a).
30. V. M. Nakariakov, E. Verwichte, Living Rev. Sol. Phys. 2, 3 (2005).
31. M. J. Penn et al., Space Sci. Rev. 70, 185 (1994).
32. The authors would like to thank M. Knölker and P. Weis-Taylor for comments on the manuscript. Construction of the CoMP instrument was funded by the NSF through the NCAR Strategic Initiative Fund and HAO/NCAR base funds. The effort of S.M.C. was supported by grant ATM-0541567 from NSF.