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20032024
most citedProperties of sunspots in cycle 23: I. Dependence of brightness on sunspot size and cycle phase

90 citations

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11 papers · 1 filter

astro-ph.SR202111 cited

Multiwavelength Signatures of Episodic Null Point Reconnection in a Quadrupolar Magnetic Configuration and the Cause of Failed Flux Rope Eruption

Prabir K. Mitra, Bhuwan Joshi, Astrid M. Veronig +1

In this paper, we present multiwavelength observations of the triggering of a failed-eruptive M-class flare from the active region NOAA 11302, and investigate the possible reasons…

astro-ph.SR202111 cited

Comparison of the Hall Magnetohydrodynamics and Magnetohydrodynamics evolution of a flaring solar active region

Kamlesh Bora, Ramit Bhattacharyya, Avijeet Prasad +2

This work analyzes the Hall magnetohydrodynamics (HMHD) and magnetohydrodynamics (MHD) numerical simulations of a flaring solar active region as a testbed while idealizing the coro…

astro-ph.SR20214 cited

Understanding the Origins of Problem Geomagnetic Storms Associated With "Stealth" Coronal Mass Ejections

Nariaki V. Nitta, Tamitha Mulligan, Emilia K. J. Kilpua +14

Geomagnetic storms are an important aspect of space weather and can result in significant impacts on space- and ground-based assets. The majority of strong storms are associated wi…

astro-ph.SR202116 cited

DH Type II Radio Bursts During Solar Cycles 23 and 24: Frequency-dependent Classification and their Flare-CME Associations

Binal D. Patel, Bhuwan Joshi, Kyung-Suk Cho +1

We present the characteristics of DH type II bursts for the Solar Cycles 23 and 24. The bursts are classified according to their end frequencies into three categories, i.e. Low Fre…

astro-ph.SR202121 cited

Heating of the solar chromosphere in a sunspot light bridge by electric currents

Rohan E. Louis, Avijeet Prasad, Christian Beck +2

Context: Resistive Ohmic dissipation has been suggested as a mechanism for heating the solar chromosphere, but few studies have established this association. Aim: We aim to determi…

astro-ph.SR202124 cited

Differential rotation of the solar transition region from STEREO/EUVI 30.4 nm images

Jaidev Sharma, Brajesh Kumar, Anil K Malik +1

The solar photosphere, chromosphere and corona are known to rotate differentially as a function of latitude. To date, it is unclear if the solar transition region also rotates diff…