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Kodaikanal solar observatory radio spectrograph

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dc.contributor.author Barve, Indrajit V
dc.contributor.author Kathiravan, C
dc.contributor.author Gireesh, G. V. S
dc.contributor.author Anand, M. N
dc.contributor.author Rajesh, M
dc.contributor.author Rajalingam, M
dc.contributor.author Ebenezer, E
dc.contributor.author Ramesh, R
dc.date.accessioned 2021-09-15T06:32:36Z
dc.date.available 2021-09-15T06:32:36Z
dc.date.issued 2021-09
dc.identifier.citation Solar Physics, Vol. 296, No. 9, 132 en_US
dc.identifier.issn 1573-093X
dc.identifier.uri http://hdl.handle.net/2248/7853
dc.description Restricted Access en_US
dc.description The original publication is available at springerlink.com
dc.description.abstract The Indian Institute of Astrophysics (IIA) has commissioned a low frequency (<100 MHz) spectrograph at its Kodaikanal Solar Observatory (KSO) for coordinated observations of transients in the solar atmosphere with other existing optical observing facilities there. The hardware set-up and initial observations are presented. The availability of different instruments in the same observatory helps to quickly plan and jointly observe the energetic phenomena and their signatures in all the three major atmospheric regions of the Sun, i.e. photosphere, chromosphere and corona. en_US
dc.language.iso en en_US
dc.publisher Springer Nature B.V. en_US
dc.relation.uri https://doi.org/10.1007/s11207-021-01879-1
dc.rights © Springer Nature B. V.
dc.subject Sun, radio emission en_US
dc.subject Sun, corona en_US
dc.subject Sun, radio bursts en_US
dc.title Kodaikanal solar observatory radio spectrograph en_US
dc.type Article en_US


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