The Study of Solar Activity in Relation with High Frequency Variations of Solar Radio Flux

Antony Dhivya Tharshini S.; Shanthi G.

doi:doi:10.11648/j.ajaa.20150306.11

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The Study of Solar Activity in Relation with High Frequency Variations of Solar Radio Flux

Antony Dhivya Tharshini S., Shanthi G.

Published in American Journal of Astronomy and Astrophysics (Volume 3, Issue 6)

Received: 9 October 2015 Accepted: 21 October 2015 Published: 31 October 2015

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Abstract

In recent years, radio observations of solar emission at 10.7cm wavelengths show a systematic increase compared to the sunspot number (SSN). The 10.7cm solar radio flux (F10.7) is one of the most widely used indices of solar activity. The solar magnetic field flux measured for the entire solar cycle is compared with the solar index of the effective cycles for the years 1986-2015. The solar activity indices include numerous quantities. Of these indices the two most used are the relative sunspot number, covering more than 300 years and the 10.7cm solar radio flux (F10.7), which has been measured regularly since 1947. The data published in the official website of National Oceanic and Atmospheric Administration (NOAA) has been used in the analysis. This study examines the relative sunspot number and 10.7cm solar radio flux indices individually and also the relation between them, and also what it implies on the solar behaviour for the solar cycle 22, 23 & 24.

Published in	American Journal of Astronomy and Astrophysics (Volume 3, Issue 6)
DOI	10.11648/j.ajaa.20150306.11
Page(s)	87-92
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), 2024. Published by Science Publishing Group

Keywords

SSN, Solar Radio Flux, Solar Activity, Indices, Data Analysis

References

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[4]	Chatterjee. T.N and Das. T.K.,(1995), Relation between solar UV flux and 10.7cm radio emission, RAS. 274,858-860.
[5]	Cong Huang., Dan-Dan Liu and Jing- Song Wang.,(2009), Forecast daily indices of solar activity, F10.7, using support vector regression method, Research in Astron. Astrophys. 9, 694-702.
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[8]	Ivan Kutiev., Ioanna Tsagouri., Loredana Perrone., Dora Pancheva., Plamen Mukhtarov., Andrei Mikhailov., Jan Lastovicka., Norbert Jakowski., Dalia Buresova., Estefania Blanch., Borislav Andonov., David Altadill., Sergio Magdaleno., Mario Parisi and Joan Miquel Torta., (2013), Solar activity impact on the Earth’s upper atmosphere, Journal of Space Weather Space Climate. DOI: 10.1051/swsc/2013028.
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Antony Dhivya Tharshini S., Shanthi G. (2015). The Study of Solar Activity in Relation with High Frequency Variations of Solar Radio Flux. American Journal of Astronomy and Astrophysics, 3(6), 87-92. https://doi.org/10.11648/j.ajaa.20150306.11

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Antony Dhivya Tharshini S.; Shanthi G. The Study of Solar Activity in Relation with High Frequency Variations of Solar Radio Flux. Am. J. Astron. Astrophys. 2015, 3(6), 87-92. doi: 10.11648/j.ajaa.20150306.11

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AMA Style

Antony Dhivya Tharshini S., Shanthi G. The Study of Solar Activity in Relation with High Frequency Variations of Solar Radio Flux. Am J Astron Astrophys. 2015;3(6):87-92. doi: 10.11648/j.ajaa.20150306.11

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@article{10.11648/j.ajaa.20150306.11,
  author = {Antony Dhivya Tharshini S. and Shanthi G.},
  title = {The Study of Solar Activity in Relation with High Frequency Variations of Solar Radio Flux},
  journal = {American Journal of Astronomy and Astrophysics},
  volume = {3},
  number = {6},
  pages = {87-92},
  doi = {10.11648/j.ajaa.20150306.11},
  url = {https://doi.org/10.11648/j.ajaa.20150306.11},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajaa.20150306.11},
  abstract = {In recent years, radio observations of solar emission at 10.7cm wavelengths show a systematic increase compared to the sunspot number (SSN). The 10.7cm solar radio flux (F10.7) is one of the most widely used indices of solar activity. The solar magnetic field flux measured for the entire solar cycle is compared with the solar index of the effective cycles for the years 1986-2015. The solar activity indices include numerous quantities. Of these indices the two most used are the relative sunspot number, covering more than 300 years and the 10.7cm solar radio flux (F10.7), which has been measured regularly since 1947. The data published in the official website of National Oceanic and Atmospheric Administration (NOAA) has been used in the analysis. This study examines the relative sunspot number and 10.7cm solar radio flux indices individually and also the relation between them, and also what it implies on the solar behaviour for the solar cycle 22, 23 & 24.},
 year = {2015}
}

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TY - JOUR
T1 - The Study of Solar Activity in Relation with High Frequency Variations of Solar Radio Flux
AU - Antony Dhivya Tharshini S.
AU - Shanthi G.
Y1 - 2015/10/31
PY - 2015
N1 - https://doi.org/10.11648/j.ajaa.20150306.11
DO - 10.11648/j.ajaa.20150306.11
T2 - American Journal of Astronomy and Astrophysics
JF - American Journal of Astronomy and Astrophysics
JO - American Journal of Astronomy and Astrophysics
SP - 87
EP - 92
PB - Science Publishing Group
SN - 2376-4686
UR - https://doi.org/10.11648/j.ajaa.20150306.11
AB - In recent years, radio observations of solar emission at 10.7cm wavelengths show a systematic increase compared to the sunspot number (SSN). The 10.7cm solar radio flux (F10.7) is one of the most widely used indices of solar activity. The solar magnetic field flux measured for the entire solar cycle is compared with the solar index of the effective cycles for the years 1986-2015. The solar activity indices include numerous quantities. Of these indices the two most used are the relative sunspot number, covering more than 300 years and the 10.7cm solar radio flux (F10.7), which has been measured regularly since 1947. The data published in the official website of National Oceanic and Atmospheric Administration (NOAA) has been used in the analysis. This study examines the relative sunspot number and 10.7cm solar radio flux indices individually and also the relation between them, and also what it implies on the solar behaviour for the solar cycle 22, 23 & 24.
VL - 3
IS - 6
ER -

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Author Information

Antony Dhivya Tharshini S.

Department of Physics and Research Centre, Women’s Christian College, Nagercoil, India
Shanthi G.

Department of Physics and Research Centre, Women’s Christian College, Nagercoil, India

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APA Style

Antony Dhivya Tharshini S., Shanthi G. (2015). The Study of Solar Activity in Relation with High Frequency Variations of Solar Radio Flux. American Journal of Astronomy and Astrophysics, 3(6), 87-92. https://doi.org/10.11648/j.ajaa.20150306.11

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ACS Style

Antony Dhivya Tharshini S.; Shanthi G. The Study of Solar Activity in Relation with High Frequency Variations of Solar Radio Flux. Am. J. Astron. Astrophys. 2015, 3(6), 87-92. doi: 10.11648/j.ajaa.20150306.11

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AMA Style

Antony Dhivya Tharshini S., Shanthi G. The Study of Solar Activity in Relation with High Frequency Variations of Solar Radio Flux. Am J Astron Astrophys. 2015;3(6):87-92. doi: 10.11648/j.ajaa.20150306.11

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@article{10.11648/j.ajaa.20150306.11,
  author = {Antony Dhivya Tharshini S. and Shanthi G.},
  title = {The Study of Solar Activity in Relation with High Frequency Variations of Solar Radio Flux},
  journal = {American Journal of Astronomy and Astrophysics},
  volume = {3},
  number = {6},
  pages = {87-92},
  doi = {10.11648/j.ajaa.20150306.11},
  url = {https://doi.org/10.11648/j.ajaa.20150306.11},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajaa.20150306.11},
  abstract = {In recent years, radio observations of solar emission at 10.7cm wavelengths show a systematic increase compared to the sunspot number (SSN). The 10.7cm solar radio flux (F10.7) is one of the most widely used indices of solar activity. The solar magnetic field flux measured for the entire solar cycle is compared with the solar index of the effective cycles for the years 1986-2015. The solar activity indices include numerous quantities. Of these indices the two most used are the relative sunspot number, covering more than 300 years and the 10.7cm solar radio flux (F10.7), which has been measured regularly since 1947. The data published in the official website of National Oceanic and Atmospheric Administration (NOAA) has been used in the analysis. This study examines the relative sunspot number and 10.7cm solar radio flux indices individually and also the relation between them, and also what it implies on the solar behaviour for the solar cycle 22, 23 & 24.},
 year = {2015}
}

Copy | Download