activity
20092026
most citedEvidence for collapsing fields in corona and photosphere during the 15 February 2011 X2.2 flare: SDO AIA and HMI Observations

77 citations · 406 across the 34 of their papers we have counts for

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Showing 2010Show all

9 papers · 1 filter

astro-ph.SR2010

Distribution of Magnetic Shear Angle in an Emerging Flux Region

Sanjay Gosain

We study the distribution of magnetic shear in an emerging flux region using the high-resolution Hinode/SOT SP observations. The distribution of mean magnetic shear angle across th…

astro-ph.SR2010

Evolution of twist-shear and dip-shear in Faring active region NOAA 10930

Sanjay Gosain, P. Venkatakrishnan

We study the evolution of magnetic shear angle in a flare productive active region NOAA 10930. The magnetic shear angle is defined as the deviation in the orientation of the observ…

astro-ph.SR2010★ 5 cited

Acoustic Power Absorption and its Relation with Vector Magnetic Field of a Sunspot

S. Gosain, S. K. Mathew, P. Venkatakrishnan

The distribution of acoustic power over sunspots shows an enhanced absorption near the umbra--penumbra boundary. Earlier studies revealed that the region of enhanced absorption coi…

astro-ph.SR2010★ 13 cited

Magnetic Non-Potentiality of Solar Active Regions and Peak X-Ray Flux of the Associated Flares

Sanjiv Kumar Tiwari, P. Venkatakrishnan, Sanjay Gosain

Predicting the severity of the solar eruptive phenomena like flares and Coronal Mass Ejections (CMEs) remains a great challenge despite concerted efforts for several decades. The a…

astro-ph.SR2010★ 19 cited

Evolution of twist-shear and dip-shear during X-class flare of 13 December 2006: Hinode observations

Sanjay Gosain, P. Venkatakrishnan

The non-potentiality (NP) of the solar magnetic fields is measured traditionally in terms of magnetic shear angle i.e., the angle between observed and potential field azimuth. Here…

astro-ph.SR2010★ 11 cited

On the estimate of magnetic non-potentiality of sunspots derived using Hinode SOT/SP observations: Effect of polarimetric noise

Sanjay Gosain, Sanjiv Kumar Tiwari, P. Venkatakrishnan

The accuracy of Milne-Eddington (ME) inversions, used to retrieve the magnetic field vector, depends upon the signal-to-noise ratio (SNR) of the spectro-polarimetric observations.…