Statistical Analysis of Associated and Non-Associated Type II Solar Radio Bursts during the Increasing Phase of Solar Cycle 23
International Journal of Astrophysics and Space Science
Volume 1, Issue 4, October 2013, Pages: 29-44
Received: Sep. 7, 2013; Published: Oct. 20, 2013
Views 1592      Downloads 49
Authors
Vijaykumar H. Doddamani, Dept of Physics, Bangalore University, Bangalore, Karnataka, India
Raveesha K. H., Dept of Physics, CMR Institute of Technology, Bangalore, Karnataka, India
K. R. Subramanian, Indian Institute of Astrophysics, Bangalore, Karnataka, India
Article Tools
PDF
Follow on us
Abstract
Type II and Type III bursts are probably the most intensively studied form of radio emission in all of astrophysics. Immense effort has gone into the elucidation of both the observational and theoretical aspects. The bursts have captured the attention of plasma theorists because a considerable body of information exists on the plasma parameters and because there is adequate space and time in the solar corona for the evolution of various particle and wave processes. In our work, we have studied the type II bursts and their association with type III bursts during the increasing phase approaching the peak phase of solar cycle 23. For the period 2000-2001, type III bursts data of Culgoora observatory is referred. The parameters such as duration drift rate, shock speed, band width of these associated/non associated bursts are compared .Results indicate that the above parameters almost remain uniform for associated and non-associated type II bursts.
Keywords
Shock Speed, Drift Rate, Plasma Frequency, Dynamic Spectrum
To cite this article
Vijaykumar H. Doddamani, Raveesha K. H., K. R. Subramanian, Statistical Analysis of Associated and Non-Associated Type II Solar Radio Bursts during the Increasing Phase of Solar Cycle 23, International Journal of Astrophysics and Space Science. Vol. 1, No. 4, 2013, pp. 29-44. doi: 10.11648/j.ijass.20130104.14
References
[1]
Alvarez. H. and Haddock. F.:1973, Solar Physics, 26, 468-473
[2]
Aschwanden. M., 2006, Physics of the solar corona, Springer, Newyork. (2004)
[3]
Aubier M, Boischot.A, 1972, A&A, 19, 343-353 Cane, H. V.; Stone, R. G.:1982, National Aeronautics and Space Administration. Goddard Space Flight Center, Greenbelt, MD.),
[4]
Cane, H. V et al (2002) American Geophysical Union, Spring Meeting 2002, abstract #SH21D-04 Knock, Stuart A.; Cairns, Iver H.; Robinson, Peter A. The Sun and the Heliosphere as an Integrated System, 25th meeting of the IAU, Joint Discussion 7, 17 July 2003, Sydney, Australia
[5]
Dulk, G. A.;Altschuler, M. D.;Smerd, S. F.1971, Astrophysical Letters, Vol. 8, p.235
[6]
Dulk, G. A.; Goldman, M. V.; Steinberg, J. L.; Hoang, S. Astronomy and Astrophysics (ISSN 0004-6361), vol. 173, no. 2, Feb. 1987, p. 366-374.
[7]
Evans, Larry.G. Fainberg, J.; Stone, R.G.:1973, Solar Physics, Volume 31, issue 2, pp.501-511
[8]
Fainberg, J.and Stone, R.G.: 1970, Solar.Phys. 15, 222
[9]
Friedman and Hamberger, 1969, Ann.IQSY, Vol.4, p. 36-56
[10]
Fomichev, V.V., Chertok, I.M.1968, Soviet Astronomy.AJ 12,477
[11]
Goldman, M. V.; Smith, D. F. Physics of the sun. Volume 2 (A86-31101 13-92). Dordrecht, D. Reidel Publishing Co., 1986, p. 325-376.
[12]
Haddock, F. T.; Alvarez, H.:1970, Bulletin of the American Astronomical Society, Vol. 2, p.318
[13]
Haddock, F. T.; Alvarez, Hector: 1973, Solar Physics, Volume 29, Issue 1, pp.183-196
[14]
Hartz, T.R.:1969, Planetary space Sci, 17, 267
[15]
Hoang, S.; Maksimovic, M.; Bougeret, J.-L.; Reiner, M. J.; Kaiser, M. L.:1998, Geophysical Research Letters, Volume 25, Issue 14, p. 2497- 2500
[16]
Jaeger, J.C. and Westfold, K.C.:1950, Australian Journal of Scientific Research (A),Physical Science,3,376
[17]
Kundu, M.R. 1965,Solar Radio Astronomy, John wiley new York
[18]
Lengyel-Frey, D.:1992, Journal of Geophysical Research (ISSN 0148-0227), vol. 97, Feb. 1, 1992, p. 1609-1617
[19]
Lin, R.P.; 1970a, solar physics, 12,266
[20]
Malitson, H. H.; Stone, R. G. :1973, Bulletin of the American Astronomical Society, Vol. 5, p.276
[21]
Malitson, Harriet H.;Erickson, William C.:1966, Astrophysical Journal, vol. 144, p.337
[22]
Mann, G.; Klassen, A.; Classen, H.-T.; Aurass, H.; Scholz, D.; MacDowall, R. J.; Stone, R. G.:1966, Astronomy and Astrophysics Supplement, v.119, p.489-498
[23]
Mclean, D. J.; 1971, Australian Journal of Physics, 24, 201
[24]
Melrose, D.B.: 1980, Space Sci Rev., 26, 3.
[25]
Newkirk, G 1961, APJ, 133, 983
[26]
Poquerusse M., Bougeret J-L., Caroubalos C., 1984, A&A 136, 10
[27]
Reames, Donald V. Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 358, Aug. 1, 1990, p. L63-L67.
[28]
Reiner, M. J.; Kaiser, M. L.; Fainberg, J.; Stone, R. G.:1998a, Journal of Geophysical Research, Volume 103, Issue A12, p. 29651-29664
[29]
Reiner, M. J.; Stone, R. G.; Fainberg, J.Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 394, no. 1, July 20, 1992, p. 340-350
[30]
Robinson 1985 Robinson, R. D.; Stewart, R. T. Solar Physics (ISSN 0038-0938), vol. 97, May 1985, p. 145-157.
[31]
Smerd, S. F.; Sheridan, K. V.; Stewart, R. T. Coronal Disturbances: Proceedings from IAU Symposium no. 57 held at Surfers Paradise, Queensland Australia, 7-11 September, 1973. Edited by Gordon Allen Newkirk. International Astronomical Union. Symposium no. 57, Dordrecht; Boston: Reidel, p.389
[32]
Steinberg, J. L.; Caroubalos, C. IAU Symposium No. 41, held in Munich, Aug. 10-14, 1970. Edited by F. Labuhn and Reimar Lust. International Astronomical Union. Symposium no. 41, Dordrecht, Reidel, p.419
[33]
Stewart, R.T., Coronal Disturbances: Proceedings from IAU Symposium no. 57 held at Surfers Paradise, Queensland Australia, 7-11 September, 1973. Edited by Gordon Allen Newkirk. International Astronomical Union. Symposium no. 57, Dordrecht; Boston: Reidel, p.161
[34]
Wang, S.J, Yan, Y.H and Fu, Q.J, 2001, Astronomy & Astrophysics, 373, 1083-1088
[35]
Westfold, K. C.:1957, Astrophysical Journal, vol. 130, p.241
[36]
Wild et al., 1954: Wild, J.P., Murray, J.D., and Rowe, W.C,1954, Australian Journal of Physics,7,439
[37]
Wild J.P.Sheridan K.V. & Neylan A.A.1959, CSIRO Australia, Provided by NASA Astrophysics Data System
[38]
Wild, J.P.1950, Aust.J.Sci.Res.Ser.A3, 541
[39]
Wild, J. P., S. F. Smerd, and A. A. Weiss, Annu. Rev. Astron. Astrophys., 1, 291, 1963.
[40]
Wild, J.P., Smerd, S.F.: 1972, Ann. Rev. Astron. Astrophys. 10, 159.
[41]
Zaitsev V.V, Mityakov N.A and Rapoport V.O., 456, 1985, Solar Physics, 24,444
[42]
Zheleznyakov, V.V.:1965, Soviet Astronomy, 9, 191 (1958)
[43]
Zongjun Ningh, Qijun Fu & Quankang Lu, 2000, Solar Physics, 1944, 137-145
ADDRESS
Science Publishing Group
548 FASHION AVENUE
NEW YORK, NY 10018
U.S.A.
Tel: (001)347-688-8931