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Showing 10 out of a total of 13 results for community: Aryabhatta Research Institute of Observational Sciences. (0.099 seconds)

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Observation of Kink Instability as Driver of Recurrent Flares in AR 10960

Srivastava, A. K.; Kumar, Pankaj; Zaqarashvili, T. V.; Filippov, B. P.; Uddin, W. (Adv. Geo., 2011)
A multiwavelength study of eruptive events on January 23, 2012 associated with a major solar energetic particle event

Joshi, N. C.; Uddin, W.; Srivastava, A. K.; Kayshap, P. (Science Direct, 2013-07-01)
A study of a failed coronal mass ejection core associated with an asymmetric filament eruption

Joshi, N. C.; Srivastava, A. K.; Filippov, B.; Uddin, W.; Kayshap, P.; Chandra, R. (2013)
Observations of multiple surges associated with magnetic activities in AR 10484 on 2003 October 25

Uddin, W.; Schmieder, B.; Chandra, R.; Srivastava, A. K.; Kumar, P.; Bisht, S. (2012)
Evidence of solar flare triggering due to loop-loop interaction caused by footpoint shear motion

Kumar, P.; Srivastava, A. K.; Somov, B. V.; Manoharan, P. K.; Erdelyi, R.; Uddin, W. (2010)
Solar magnetic flux ropes

Filippov, B.; Martsenyuk, O.; Srivastava, A. K.; Uddin, W. (Indian Academy of Sciences, 2015-03)
Evidence of solar flare triggering due to loop-loop interaction caused by footpoint shear motion

Kumar, P.; Srivastava, A. K.; Somov, B. V.; Manoharan, P. K.; Erdelyi, R.; Uddin, W. (2010-11-10)
Flux emergence, flux imbalance, magnetic free energy and solar flares

Choudhary, D. P., et al.; Uddin, W.; Srivastava, A. K.; Joshi, N. C.; Kashyap, P. (Elsevier, 2013)
Height of shock formation in the solar corona inferred from observations of type II radio bursts and coronal mass ejections

Gopalswamy, N. et. al.; Uddin, W.; Srivastava, A. K.; Joshi, N. C. (2013)
Formation of a rotating jet during the filament eruption on 2013 April 10-11

Filippov, B; Srivastava, A. K.; Dwivedi, B. N.; Masson, S.; Aulanier, G.; Joshi, N. C.; Uddin, W. (Wiley, 2015-07)

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