Hostname: page-component-cc8bf7c57-n7qbj Total loading time: 0 Render date: 2024-12-12T05:52:35.233Z Has data issue: false hasContentIssue false
  • English
  • Français

Radio Emission from the Sun and Stars: New Insights into Energetic Phenomena

Published online by Cambridge University Press:  26 May 2016

T. S. Bastian
T. S. Bastian*
Affiliation:
National Radio Astronomy Observatory, Charlottesville, VA 22903 USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Energetic phenomena on the Sun and late-type stars pose a number of fascinating puzzles. These include coronal heating, flares, and coronal mass ejections, all believed to be manifestations of magnetic energy release. Radio radiation is a sensitive tracer of energetic phenomena on both the Sun and stars. Radio observations of the Sun over the past decade have produced new insights into the physics of magnetic energy release in flares and coronal mass ejections. Radio observations of late-type stars have exploited sensitive imaging and spectroscopic techniques to further constrain the nature of the relevant emission mechanisms. A surprise has been the recent discovery of radio emission from brown dwarf stars, implying the existence of substantial magnetic fields and a means of dissipating magnetic energy, neither of which are understood.

Type
Part 4: High Energy Phenomena in Sun and Stars
Information
Symposium - International Astronomical Union , Volume 219: Stars as Suns : Activity, Evolution and Planets , 2004 , pp. 145 - 158
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Abada-Simon, M., Lecacheux, A., Louarn, P. Dulk, G. A., et al. 1994, A&A, 288, 219.Google Scholar
Abada-Simon, M., & Aubier, M. 1997, A&AS, 125, 511.Google Scholar
Aschwanden, M. J., Wiehl, H. J., Benz, A. O., Kane, S. R. 1985, Solar Phys., 97, 159.Google Scholar
Aschwanden, M. J., Benz, A. O., Dennis, B. R., & Schwartz, R. A. 1995a, ApJ, 455, 347.CrossRefGoogle Scholar
Aschwanden, M. J., Montello, M. L, Dennis, B. R., & Benz, A. O. 1995b, ApJ, 440, 394.Google Scholar
Basri, G. 2000, ARA&A, 38, 485.Google Scholar
Basri, G. 2004, in Stars as Suns, IAU Symp. 219, ed. Dupree, A. K. & Benz, A. O..Google Scholar
Bastian, T. S. 2002, Innovative Telescopes and Instrumentation for Solar Astrophysics, Proc. SPIE v. 4853, eds. Keil, S. L. & Avakyan, S. V., SPIE: Bellingham, p. 98.Google Scholar
Bastian, T. S. 1996, in Radio Emission from the Sun and Stars, ed. Taylor, A. R. & Paredes, J. M., ASP Conf. Ser. 93, ASP: San Francisco, p. 447.Google Scholar
Bastian, T. S., & Bookbinder, 1987, Nature, 326, 678.Google Scholar
Bastian, T. S., Bookbinder, J., Dulk, G. A., & Davis, M. 1990, ApJ, 353, 265.Google Scholar
Bastian, T. S., & Gary, D. E. 1997, J. Geophys. Res., 102, 14031.Google Scholar
Bastian, T. S., Benz, A. O., & Gary, D. E. 1998, ARA&A, 36, 131.Google Scholar
Bastian, T. S., Maia, D., Pick, M. & Kerdraon, A. 2001, ApJ, 558, L65.Google Scholar
Bastian, T. S., Dulk, G. A., & Leblanc, Y. 2000, ApJ, 545, 1058.Google Scholar
Beasley, A. J., & Güdel, M. 2000, ApJ, 529, 961.CrossRefGoogle Scholar
Benz, A. O., Perrenoud, M. R., Fürst, E., & Hirth, W. 1981, Nature, 291, 210.Google Scholar
Benz, A. O., Alef, W., & Güdel, M. 1995, A&A, 298, 187.Google Scholar
Benz, A. O., Conway, J., & Güdel, M. 1998, A&A, 331, 596.Google Scholar
Berger, E., Ball, S., Becker, K. M., Clarke, M., et al. 2001, Nature, 410, 339.Google Scholar
Berger, E. 2002, ApJ, 572, 503.Google Scholar
Byrne, P. B., Lanzafame, A. C., Sarro, L. M., & Ryans, R. 1994, MNRAS, 270, 427.Google Scholar
Cane, H. V., & Reames, D. V. 1988, ApJ, 325, 895.Google Scholar
Classen, H. T., & Aurass, H. 2002, A&A, 384, 1098.Google Scholar
Cliver, E. W., Webb, D. F., & Howard, R. A. 1999, Solar Phys., 187, 89.Google Scholar
Dennis, B. R., Benz, A. O., Ranieri, M., & Simnett, G. M. 1984, Solar Phys., 90, 383.Google Scholar
Elgaroy, O. 1980, A&A, 82, 308.Google Scholar
Fekel, F. C., Moffet, T. J., & Henry, G. W. 1986, ApJS, 60, 551.Google Scholar
Fleishman, G. D., & Kahler, S. W. 1992, ApJ, 394, 688.Google Scholar
Fleishman, G. D., & Melnikov, V. F. 1999, Proc. 9th European Meeting on Solar Physics, Magnetic Fields Solar Processes, Florence, Italy, ESA SP-448, p. 1247.Google Scholar
Franciosini, E., & Chiuderi Drago, F. 1995, A&A, 297, 535.Google Scholar
Gary, D. E., & Keller, C. 2004, in press.Google Scholar
Gopalswamy, N., & Kundu, M. R. 1993, Solar Phys. 143, 327.Google Scholar
Gopalswamy, N. Kundu, M. R., Manoharan, P. K. Raoult, A., Nitta, N., Zarka, P. 1997, ApJ, 486, 1036.Google Scholar
Güdel, M. 1994, ApJS, 90, 743.Google Scholar
Güdel, M. 2002, ARA&A, 40, 217.Google Scholar
Güdel, M., & Benz, A. O. 1994, ApJ, 405, L63.Google Scholar
Hall, D. S. 1976, IAU Colloq. 29, Multiple Periodic Variable Stars, ed. Fitch, W. S. (Dordrecht: Reidel), p. 287.Google Scholar
Hanaoka, Y. 1996, Solar Phys., 165, 275.Google Scholar
Hanaoka, Y. 1997, Solar Phys., 173, 319.Google Scholar
Isliker, H., & Benz, A. O. 1994, A&AS, 104, 145.Google Scholar
Kassim, N. E., Perley, R. A., Erickson, W. C., & Dwarakananth, K. S. 1993, AJ, 106, 2218.Google Scholar
Kassim, N. E., Lazio, T. J. W., Erickson, W. C., Crane, P. C., Perley, R. A., & Hicks, B. 2002, in The Universe at Low Radio Frequencies, Proc. IAU Symp. 199, ed. Rao, A. P., Swarup, G., & Krishna, G., p. 474.Google Scholar
Kathiravan, C., Ramesh, R., & Subramanian, K. R. 2002, ApJ, 567, 93.Google Scholar
Lecacheux, A., Rosolen, C., Davis, M., Bookbinder, J., et al. 1993, A&A, 275, 670.Google Scholar
Melrose, D. B., & Dulk, G. A. 1982, ApJ, 259, 844.Google Scholar
Mohanty, S., & Basri, G. 2003, ApJ, 583, 451.Google Scholar
Mutel, R. L., Lestrade, J. F., Preston, R. A., & Phillips, R. B. 1985, ApJ, 289, 262.Google Scholar
Mutel, R. L., Morris, D. H., Doiron, D. J., & Lestrade, J. F. 1987, AJ, 93, 1220.Google Scholar
Nakajima, T., Oppenheimer, B. R., Kulkarni, S. R., Golimowski, D. A., et al. 1995, Nature, 378, 463.Google Scholar
Nishio, M., Yaji, K., Kosugi, T., Nakajima, H., & Sakurai, T. 1997, ApJ, 489, 976.Google Scholar
Pestalozzi, M. R., Benz, A. O., Conway, J. E., & Güdel, M. 2000, A&A, 353, 569.Google Scholar
Ramesh, R., Kathiravan, C., & Sastry, Ch. V. 2003, ApJ, 591, 163.Google Scholar
Ransom, R. R., Bartel, N., Bietenholz, M. F., Leback, D. E., et al. 2003, ApJ, 572, 487.Google Scholar
Rutledge, R. E., Basri, G., Martín, E. L., & Bildsten, L. 2000, ApJ, 538, L141.Google Scholar
Seaquist, E. 1993, Rep. Prog. Physics., 56(9), 1145.CrossRefGoogle Scholar
Stepanov, A. V., Kliem, B., Zaitsev, V. V., Fürst, E., et al. 2001, A&A, 374, 1072.Google Scholar
Strassmeier, K. G., Hall, D. S., Fekel, F. C., & Sheck, M. 1993, A&AS, 100, 173.Google Scholar
Trigilio, C., Buerni, C. S., Umana, G., Rodonò, M., et al. 2001, A&A, 373, 181.Google Scholar
Uchida, Y. 1974, Solar Phys., 39, 431.Google Scholar
van den Oord, G. H. J. 1996, in Radio Emission from the Sun and Stars, ed. Taylor, A. R. & Paredes, J. M., ASP Conf. Ser. 93, ASP: San Francisco, p. 263.Google Scholar
Wagner, W. J., & MacQueen, R. M. 1983, A&A, 20, 136.Google Scholar
White, S. M. 2000, in Radio Interferometry: The Saga and the Science, ed. Finley, D. G. & Goss, W. M., NRAO Workshop 27, p. 86.Google Scholar
White, S. M., & Kundu, M. R. 1997, Solar Phys., 174, 31.Google Scholar
White, S. M., & Franciosini, E. 1995, ApJ, 444, 342.Google Scholar
White, S. M., Kassim, N. E., Erickson, W. C. 2002, in Innovative Telescopes and Instrumentation for Solar Astrophysics, Proc. SPIE v. 4853, ed. Keil, S. L. & Avakyan, S. V., SPIE: Bellingham, p. 111.Google Scholar
Zarka, P., Treumann, R. A., Ryabov, B. P., & Ryabov, V. B. 2001, APSS, 277, 293.Google Scholar