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Author Vats, H. O. ♦ Deshpande, M. R. ♦ Mehta, M. ♦ Shah, C. R. ♦ Shah, K. J.
Source Indian Institute of Astrophysics
Content type Text
File Format PDF
Language English
Subject Domain (in DDC) Natural sciences & mathematics ♦ Physics
Subject Keyword Radio emission ♦ Solar radio emission ♦ Coronal rotation
Description The time series of solar radio emission at 2.8 GHz is analysed using correlation methods. The analysis showed that this type of time series can be used to infer the rotation period of the source (in this case solar corona). It is found that the correlograms have a very strong persistence of rotational modulation. These values are significantly lower than those reported earlier by other methods. The reasons for this difference are unknown.
Educational Use Research
Education Level UG and PG
Learning Resource Type Article
Publisher Institution Astronomical Society of India
Journal BASI
Volume Number 27
Issue Number 1
Size (in Bytes) 250.73 kB
Page Count 3
Starting Page 61
Ending Page 63