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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7459
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dc.contributor.authorRamesh, R-
dc.contributor.authorMugundhan, V-
dc.contributor.authorPrabhu, K-
dc.date.accessioned2020-04-21T06:52:41Z-
dc.date.available2020-04-21T06:52:41Z-
dc.date.issued2020-01-
dc.identifier.citationThe Astrophysical Journal Letters, 2020, Vol.889, pL25en_US
dc.identifier.issn0004-637X-
dc.identifier.issn1538-4357 (online)-
dc.identifier.urihttp://hdl.handle.net/2289/7459-
dc.descriptionOpen Accessen_US
dc.description.abstractWe analyzed a group of type III radio bursts and a Hα flare from the Sun that were observed simultaneously on 2015 January 14. The radio observations were in the spectral mode over the frequency range 85–35 MHz, and separately in the imaging mode at 80 MHz. The duration of the observations was ≈6 minutes. The centroids of the type III bursts and the Hα flare were independently scattered near the associated active region. But the displacements in the centroids of the two phenomenon are correlated with each other. This indicates that the individual bursts in a group of type III radio bursts are most likely due to flaring activity at different locations in the active region at different times during the same flare interval.en_US
dc.language.isoenen_US
dc.publisherIOP Sciences for American Astronomical Societyen_US
dc.relation.urihttps://ui.adsabs.harvard.edu/abs/2020ApJ...889L..25R/abstracten_US
dc.relation.urihttps://iopscience.iop.org/article/10.3847/2041-8213/ab6a9cen_US
dc.rights2020. The American Astronomical Societyen_US
dc.titleNew Evidence for Spatio-temporal Fragmentation in the Solar Flare Energy Releaseen_US
dc.typeArticleen_US
Appears in Collections:Research Papers (A&A)

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