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The inference of the magnetic field vector in prominences

Published online by Cambridge University Press:  06 January 2014

Bruce W. Lites
Bruce W. Lites*
Affiliation:
High Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307-3000, USA email: lites@ucar.edu
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Abstract

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Prominences owe their existence to the presence of magnetic fields in the solar corona. The magnetic field determines their geometry and is crucial to their stability, energetics, and dynamics. This review summarizes techniques for measurement of the magnetic field vector in prominences. New techniques for inversions of full Stokes spectro-polarimetry, incorporating both the Zeeman and Hanle mechanisms for generation and modification of polarization, are now at the forefront. Also reviewed are measurements of the magnetic fields in the photosphere below prominences, and how they may be used to infer the field geometry in and surrounding the prominence itself.

Keywords

magnetic fieldspolarizationscatteringdata analysispolarimetricSun: prominencesSun: filaments
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S300: Nature of Prominences and their role in Space Weather , June 2013 , pp. 101 - 111
Copyright
Copyright © International Astronomical Union 2013 

References

Asensio Ramos, A., Trujillo Bueno, J., & Landi Degl'Innocenti, E. 2008, ApJ, 683, 542CrossRefGoogle Scholar
Bommier, V. 1980, A&A, 87, 109Google Scholar
Bommier, V. & Leroy, J. L. 1998, in: Webb, D. F., Schmieder, B., & Rust, D. M. (eds.) IAU Colloq. 167: New Perspectives on Solar Prominences, (Astronomical Society of the Pacific Conference Series) 150, 434Google Scholar
Bommier, V. & Sahal-Brechot, S. 1978, A&A, 69, 57Google Scholar
Bommier, V., Sahal-Brechot, S., & Leroy, J. L. 1981, A&A, 100, 231Google Scholar
Bommier, V., Sahal-Brechot, S., & Leroy, J. L. 1986, A&A, 156, 79Google Scholar
Bommier, V., Landi Degl'Innocenti, E., Leroy, J.-L., & Sahal-Brechot, S. 1994, Solar Phys., 154, 231Google Scholar
Brown, A., López Ariste, A., & Casini, R. 2003, Solar Phys., 215, 295Google Scholar
Casini, R. 2002, ApJ, 568, 1056CrossRefGoogle Scholar
Casini, R., López Ariste, A., Tomczyk, S., & Lites, B. W. 2003, ApJ, 598, L67Google Scholar
Casini, R., López Ariste, A., Paletou, F., & Léger, L. 2009, ApJ, 703, 114Google Scholar
Casini, R., Asensio Ramos, A., Lites, B. W. & López Ariste, A. 2013, ApJ, 773, 180Google Scholar
Collados, M., Lagg, A., Díaz Garcí, A. J. J., Hernández Suárez, E., López López, R., Páez Mañá, E., & Solanki, S. K. 2007, in: Heinzel, P., Dorotovič, I., & Rutten, R. J. (eds.) The Physics of Chromospheric Plasmas, (Astronomical Society of the Pacific Conference Series) 368, 611Google Scholar
Harvey, J. W. 1969, Magnetic Fields Associated with Solar Active-Region Prominences PhD thesis, (University of Colorado at Boulder)Google Scholar
House, L. L. & Smartt, R. N. 1982, Solar Phys., 80, 53CrossRefGoogle Scholar
Hyder, C. L. 1965, ApJ, 141, 1374Google Scholar
Hyder, C. L. 1966, ZfA, 63, 78Google Scholar
Kano, R.et al. 2012, in: Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, (Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series) 8443Google Scholar
Kuckein, C., Martínez Pillet, V., & Centeno, R. 2012, A&A, 539, A131Google Scholar
Kuckein, C., Centeno, R., Martínez Pillet, V., Casini, R., Manso Sainz, R., & Shimizu, T. 2009, A&A, 501, 1113Google Scholar
Landi Degl'Innocenti, E. 1982, Solar Phys., 79, 291Google Scholar
Landi Degl'Innocenti, E., Bommier, V., & Sahal-Brechot, S. 1987, A&A, 186, 335Google Scholar
Leroy, J. L. 1977, A&A, 60, 79Google Scholar
Leroy, J. L. 1978, A&A, 64, 247Google Scholar
Leroy, J. L., Bommier, V., & Sahal-Brechot, S. 1983, Solar Phys., 83, 135Google Scholar
Leroy, J. L., Bommier, V., & Sahal-Brechot, S. 1984, A&A, 131, 33Google Scholar
Leroy, J. L., Ratier, G., & Bommier, V. 1977, A&A, 54, 811Google Scholar
Lin, H., Penn, M. J., & Kuhn, J. R. 1998, ApJ, 493, 978CrossRefGoogle Scholar
Lin, Y., Wiik, J. E., Engvold, O., Rouppe van der Voort, L., & Frank, Z. A. (2005) Solar Phys., 227, 283Google Scholar
Lites, B. W. 2005, ApJ, 622, 1275Google Scholar
Lites, B. W., Kubo, M., Berger, T., Frank, Z., Shine, R., Tarbell, T., Title, A., Okamoto, T. J., & Otsuji, K. 2010, ApJ 718, 474Google Scholar
López Ariste, A., Casini, R., Paletou, F., Tomczyk, S., Lites, B. W., Semel, M., Landi Degl'Innocenti, E., Trujillo Bueno, J., & Balasubramaniam, K. S. 2005, ApJ. 621, L145Google Scholar
López Ariste, A., Aulanier, G., Schmieder, B. & Sainz Dalda, A. 2006, A&A, 456, 725Google Scholar
López Ariste, A. & Aulanier, G. 2007, in: Heinzel, P., Dorotovič, I., Rutten, R. J. (eds.) The Physics of Chromospheric Plasmas, (Astronomical Society of the Pacific Conference Series) 368, 291Google Scholar
López Ariste, A. & Casini, R. 2002, ApJ, 575, 529Google Scholar
López Ariste, A. & Casini, R. 2003, ApJ, 582, L51Google Scholar
Mackay, D. H., Karpen, J. T., Ballester, J. L., Schmieder, B., & Aulanier, G. 2010, Space Sci. Revs, 151, 333Google Scholar
Okamoto, T. J., Tsuneta, S., Lites, B. W., Kubo, M., Yokoyama, T., Berger, T. E., Ichimoto, K., Katsukawa, Y., Nagata, S., Shibata, K., Shimizu, T., Shine, R. A., Suematsu, Y., Tarbell, T. D., & Title, A. M. 2009, ApJ, 697, 913CrossRefGoogle Scholar
Merenda, L., Trujillo Bueno, J., Landi Degl'Innocenti, E., & Collados, M. 2006, ApJ, 642, 554CrossRefGoogle Scholar
Orozco Suárez, D., Asensio Ramos, A., & Trujillo Bueno, J. 2013, in: Highlights of Spanish Astrophysics VII, 786Google Scholar
Paletou, F. 2008, in: Charbonnel, C., Combes, F., & Samadi, R. (eds.) SF2A-2008, 559Google Scholar
Paletou, F. & Aulanier, G. 2003, in: Trujillo-Bueno, J. & Sanchez Almeida, J. (eds.) Solar Polarization, (Astronomical Society of the Pacific Conference Series) 307, 458Google Scholar
Rees, D. E., López Ariste, A., Thatcher, J., & Semel, M. 2000, A&A, 355, 759Google Scholar
Rust, D. M. 1967, ApJ, 150, 313CrossRefGoogle Scholar
Sahal-Brechot, S., Bommier, V., & Leroy, J. L. 1977, A&A, 59, 223Google Scholar
Schmieder, B., Gunár, S., Heinzel, P., & Anzer, U. 2007, Solar Phys., 241, 53Google Scholar
Schmieder, B., Kucera, T. A., Knizhnik, K., Luna, M., Lopez-Ariste, A., & Toot, D. 2013, ApJ, 777, 108Google Scholar
Tandberg-Hanssen, E. 1970, Solar Phys., 15, 359CrossRefGoogle Scholar
Trujillo Bueno, J. & Asensio Ramos, A. 2007, ApJ, 655, 642Google Scholar
Trujillo Bueno, J., Landi Degl'Innocenti, E., Collados, M., Merenda, L. & Manso Sainz, R. 2002, Nature, 415, 403Google Scholar
Zirin, H. & Severny, A. 1961, The Observatory, 81, 155Google Scholar