Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1888
Title: Radio emission as a diagnostic for solar coronal rotation
Authors: Vats, H. O
Deshpande, M. R
Mehta, M
Shah, C. R
Shah, K. J
Keywords: Radio emission;Solar radio emission;Coronal rotation
Issue Date: 1999
Publisher: Astronomical Society of India
Citation: BASI, Vol. 27, No. 1, pp. 61 - 63
Abstract: 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.
URI: http://hdl.handle.net/2248/1888
???metadata.dc.relation.uri???: http://adsabs.harvard.edu/abs/1999BASI...27...61V
Appears in Collections:BASI Publications

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