A classical theory of coronal emission line polarization

Astrophysical Journal

Volumn 542, Issue 1 PART 1, 2000, Pages 528-534

  Lin, Haosheng ^a   Casini, Roberto ^b  

^a NATIONAL SOLAR OBSERVATORY   (United States)

^b NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

Author keywords

Line: formation; Polarization; Radiation mechanisms: thermal; Sun: corona; Sun: magnetic fields

Indexed keywords

EID: 0034633459     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/309499     Document Type: Article

References (13)

1. Arnaud, J., & Newkirk, G. N., Jr. 1987, A&A, 178, 263
2. Babel, J., & North, P. 1997, A&A, 325, 195
3. Casini, R., & Judge, P. G. 1999, ApJ, 522, 524 (erratum 533, 574)
4. Charvin, P. 1965, Ann. d'Astrophys., 28, 877
5. Harvey, J. W. 1969, Ph.D. thesis, Univ. Colorado
6. House, L. L. 1974, PASP, 86, 490
7. _. 1977, ApJ, 214, 632
8. Kuhn, J. R. 1995, in IR Tools for Solar Astrophysics: What's Next?, ed. J. R. Kuhn & M. J. Penn (Singapore: World Scientific), 89
9. Lin, H., Penn, M. J., & Kuhn, J. R. 1998, ApJ, 493, 978 (Paper I)
10. Querfeld, C. W., & Smartt, R. N. 1984, Sol. Phys., 91, 299
11. Reitz, J. R., & Milford, F. J. 1967, Foundations of Electromagnetic Theory (Reading: Addison-Wesley)
12. Sahal-Bréchot, S. 1974, A&A, 36, 355
13. _. 1977, ApJ, 213, 887