Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7853
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dc.contributor.authorBarve, Indrajit V-
dc.contributor.authorKathiravan, C-
dc.contributor.authorGireesh, G. V. S-
dc.contributor.authorAnand, M. N-
dc.contributor.authorRajesh, M-
dc.contributor.authorRajalingam, M-
dc.contributor.authorEbenezer, E-
dc.contributor.authorRamesh, R-
dc.date.accessioned2021-09-15T06:32:36Z-
dc.date.available2021-09-15T06:32:36Z-
dc.date.issued2021-09-
dc.identifier.citationSolar Physics, Vol. 296, No. 9, 132en_US
dc.identifier.issn1573-093X-
dc.identifier.urihttp://hdl.handle.net/2248/7853-
dc.descriptionRestricted Accessen_US
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractThe 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.isoenen_US
dc.publisherSpringer Nature B.V.en_US
dc.relation.urihttps://doi.org/10.1007/s11207-021-01879-1-
dc.rights© Springer Nature B. V.-
dc.subjectSun, radio emissionen_US
dc.subjectSun, coronaen_US
dc.subjectSun, radio burstsen_US
dc.titleKodaikanal solar observatory radio spectrographen_US
dc.typeArticleen_US
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