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Showing 10 out of a total of 35 results for community: IIAP Publications.
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Effect of beam-plasma instabilities on accretion disk flares
Krishan, V
;
Wiita, P. J
;
Ramadurai, S
(
European Southern Observatory
,
2000-04
)
Low-Frequency Observations of Drifting, Non-Thermal Continuum Radio Emission Associated With the Solar Coronal Mass Ejections
Ramesh, R
;
Kishore, P
;
Mulay, S. M
;
Barve, Indrajit V
;
Kathiravan, C
;
Wang, T. J
(
IOP Publishing
,
2013-11-20
)
An estimation of the plasma parameters in the solar corona using quasi-periodic metric type III radio burst emission
Ramesh, R
;
Satya Narayanan, A
;
Kathiravan, C
;
Sastry, Ch. V
;
Shankar, N. U
(
EDP Sciences
,
2005-02
)
On the line profile changes observed during the X2.2 class flare in the active region NOAA 11158
Bayanna, A. R
;
Kumar, B
;
Venkatakrishnan, P
;
Mathew, S. K
;
Ravindra, B
;
Mathur, S
;
Garcia, R. A
(
IOP Publishing
,
2014-02
)
SoLEXS - A low energy X-ray spectrometer for solar coronal studies
Sankarasubramanian, K
;
Ramadevi, M. C
;
Bug, M
;
Umapath, C. N
;
Seetha, S
;
Sreekumar, P
;
Kumar
(
Astronomical Society of India
,
2011
)
The location of solar metric type ii radio bursts with respect to the associated coronal mass ejections
Ramesh, R
;
Anna Lakshmi, M
;
Kathiravan, C
;
Gopalswamy, N
;
Umapathy, S
(
IOP Publishing
,
2012-06-20
)
Magnetohydrodynamic simulation of the X9.3 flare on 2017 September 6: evolving magnetic topology
Jiang, C
;
Zou, P
;
Feng, X
;
Hu, Qiang
;
Liu, Rui
;
Vemareddy, P
;
Duan, Aiying
;
Zuo, P
;
Wang, Yi
;
Wei, Fengsi
(
IOP Publishing
,
2018-12-10
)
Flares before and after coronal mass ejections
Suryanarayana, G. S
(
IOP Publishing
,
2018-03
)
Evolution of Spinning and Braiding Helicity Fluxes in Solar Active Region NOAA 10930
Ravindra, B
;
Yoshimura, K
;
Dasso, S
(
IOP Publishing
,
2011-12-10
)
Evolution of Currents of Opposite Signs in the Flare-productive Solar Active Region NOAA 10930
Ravindra, B
;
Venkatakrishnan, P
;
Tiwari, S. K
;
Bhattacharyya, R
(
IOP Publishing
,
2011-10-10
)
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Vemareddy, P (12)
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Sun: flares (35)
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Sun: coronal mass ejections (CMEs) (12)
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