◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

Sanjay Kumar

13 papers hereh-index 231.6k citations134 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author5
  • middle author5
  • last author3

Across the 13 of 13 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR9
  • physics.class-ph2
  • physics.flu-dyn2
same name
  • Sanjay Kumar — 32 papers, h 23
  • Sanjay Kumar — 30 papers, h 17
  • Sanjay Kumar — 3 papers, h 2
  • Sanjay Kumar — 3 papers, h 17
  • Sanjay Kumar — 3 papers, h 2
  • Sanjay Kumar — 3 papers, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20102023
most citedMagnetohydrodynamic simulation of magnetic null-point reconnections in NOAA AR12192 initiated with an extrapolated non-force-free-field

44 citations · 183 across the 13 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

astro-ph.SR2018★ 44 cited

Magnetohydrodynamic simulation of magnetic null-point reconnections in NOAA AR12192 initiated with an extrapolated non-force-free-field

A. Prasad, R. Bhattacharyya, Qiang Hu +2

Magnetohydrodynamics of the solar corona is simulated numerically. The simulation is initialized with an extrapolated non-force-free magnetic field using the vector magnetogram of…

astro-ph.SR2018★ 2 cited

Study of magnetic field topology of active region 12192 using an extrapolated non-force-free magnetic field

A. Prasad, R. Bhattacharyya, Q. Hu +2

The solar active region (AR) 12192 was one of the most flare productive region of solar cycle 24, which produced many X-class flares; the most energetic being an X3.1 flare on Octo…

astro-ph.SR2018★ 11 cited

Fast Standing Modes in Transversely Nonuniform Solar Coronal Slabs: Effects of a Finite Plasma Beta

Shao-Xia Chen, Bo Li, Sanjay Kumar +2

We examine the dispersive properties of linear fast standing modes in transversely nonuniform solar coronal slabs with finite gas pressure, or, equivalently, finite plasma beta. We…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.