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Comparison of Solar and Jovian Radio Emission at 20.1 MHz

  • Debojyoti HalderEmail author
  • Bipasa Raha
Conference paper
Part of the Lecture Notes in Networks and Systems book series (LNNS, volume 11)

Abstract

The Sun and the Jupiter both astronomical objects emit radiation in radio frequencies and have much importance in the Earth’s atmosphere. We have recorded data of both Solar and Jovian signal on NASA’s Radio Jove instrument at 20.1 MHz. The simultaneous visibility of the two objects—the Sun and the Jupiter—is of much importance in this study. In this paper, we have done the comparison using the Jove receiving system on those dates especially when the Jupiter rises at nighttime. It shows that the intensity of solar radio emission is well above Jovian emission intensity. It has been observed that solar radio bursts are stronger than Jovian bursts. They occur usually when there are sunspots on the visible corona while Jupiter noise storms are more likely to occur at nighttime and so they are much prominently recorded.

Keywords

Solar radio emission Jovian decametric emission Radio antenna 

References

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    Khurana, K.K., Kivelson, M.G.: The configuration of Jupiter’s magnetosphere. In: Bagenal, F., Dowling, T.E., McKinnon, W.B. (eds.) Jupiter: The Planet, Satellites and Magnetosphere. Cambridge University Press, Cambridge (2004)Google Scholar
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    Bhattacharya, A.B., Joarder, S., Nag, A., Halder, D., Debnath, M.: Reception of Jovian radio signals in a tropical station. Int. J. Eng. Sci. Technol. 2, 5704–5713 (2010)Google Scholar

Copyright information

© Springer Nature Singapore Pte Ltd. 2018

Authors and Affiliations

  1. 1.Department of PhysicsRishi Bankim Chandra Evening CollegeNaihatiIndia
  2. 2.Department of PhysicsTechno India UniversityKolkataIndia

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