Statistical Analysis of Associated and Non-Associated Type II Solar Radio Bursts during the Increasing Phase of Solar Cycle 23

Vijaykumar H. Doddamani; Raveesha K. H.; K. R. Subramanian

doi:doi:10.11648/j.ijass.20130104.14

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Statistical Analysis of Associated and Non-Associated Type II Solar Radio Bursts during the Increasing Phase of Solar Cycle 23

Vijaykumar H. Doddamani, Raveesha K. H., K. R. Subramanian

Published in International Journal of Astrophysics and Space Science (Volume 1, Issue 4)

Received: 7 September 2013 Published: 20 October 2013

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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.

Published in	International Journal of Astrophysics and Space Science (Volume 1, Issue 4)
DOI	10.11648/j.ijass.20130104.14
Page(s)	29-44
Creative Commons	This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.
Copyright	Copyright © The Author(s), 2013. Published by Science Publishing Group

Keywords

Shock Speed, Drift Rate, Plasma Frequency, Dynamic Spectrum

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APA Style

Vijaykumar H. Doddamani, Raveesha K. H., K. R. Subramanian. (2013). 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, 1(4), 29-44. https://doi.org/10.11648/j.ijass.20130104.14

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ACS Style

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. Int. J. Astrophys. Space Sci. 2013, 1(4), 29-44. doi: 10.11648/j.ijass.20130104.14

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AMA Style

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. Int J Astrophys Space Sci. 2013;1(4):29-44. doi: 10.11648/j.ijass.20130104.14

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@article{10.11648/j.ijass.20130104.14,
  author = {Vijaykumar H. Doddamani and Raveesha K. H. and K. R. Subramanian},
  title = {Statistical Analysis of Associated and Non-Associated Type II Solar Radio Bursts during the Increasing Phase of Solar Cycle 23},
  journal = {International Journal of Astrophysics and Space Science},
  volume = {1},
  number = {4},
  pages = {29-44},
  doi = {10.11648/j.ijass.20130104.14},
  url = {https://doi.org/10.11648/j.ijass.20130104.14},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijass.20130104.14},
  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.},
 year = {2013}
}

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TY - JOUR
T1 - Statistical Analysis of Associated and Non-Associated Type II Solar Radio Bursts during the Increasing Phase of Solar Cycle 23
AU - Vijaykumar H. Doddamani
AU - Raveesha K. H.
AU - K. R. Subramanian
Y1 - 2013/10/20
PY - 2013
N1 - https://doi.org/10.11648/j.ijass.20130104.14
DO - 10.11648/j.ijass.20130104.14
T2 - International Journal of Astrophysics and Space Science
JF - International Journal of Astrophysics and Space Science
JO - International Journal of Astrophysics and Space Science
SP - 29
EP - 44
PB - Science Publishing Group
SN - 2376-7022
UR - https://doi.org/10.11648/j.ijass.20130104.14
AB - 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.
VL - 1
IS - 4
ER -

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Author Information

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

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APA Style

Vijaykumar H. Doddamani, Raveesha K. H., K. R. Subramanian. (2013). 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, 1(4), 29-44. https://doi.org/10.11648/j.ijass.20130104.14

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ACS Style

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. Int. J. Astrophys. Space Sci. 2013, 1(4), 29-44. doi: 10.11648/j.ijass.20130104.14

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AMA Style

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. Int J Astrophys Space Sci. 2013;1(4):29-44. doi: 10.11648/j.ijass.20130104.14

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@article{10.11648/j.ijass.20130104.14,
  author = {Vijaykumar H. Doddamani and Raveesha K. H. and K. R. Subramanian},
  title = {Statistical Analysis of Associated and Non-Associated Type II Solar Radio Bursts during the Increasing Phase of Solar Cycle 23},
  journal = {International Journal of Astrophysics and Space Science},
  volume = {1},
  number = {4},
  pages = {29-44},
  doi = {10.11648/j.ijass.20130104.14},
  url = {https://doi.org/10.11648/j.ijass.20130104.14},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijass.20130104.14},
  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.},
 year = {2013}
}

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