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researcher

S. Tiwari

70 papers hereh-index 251.9k citations145 works total

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

author position
  • sole author7
  • first author14
  • middle author36
  • last author9

Across the 66 of 70 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR60
  • physics.atom-ph5
  • cond-mat.mtrl-sci2
  • physics.optics1
  • physics.space-ph1
  • quant-ph1
same name
  • S. Tiwari — 40 papers, h 55
  • S. Tiwari — 22 papers, h 19
  • S. Tiwari — 13 papers, h 15
  • S. Tiwari — 12 papers, h 7
  • S. Tiwari — 10 papers, h 61
  • S. Tiwari — 9 papers, h 6

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
20092025
most citedSolar science with the Atacama Large Millimeter/submillimeter Array - A new view of our Sun

153 citations · 1.9k across the 70 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

astro-ph.SR2018★ 21 cited

Evidence of Twisting and Mixed-polarity Solar Photospheric Magnetic Field in Large Penumbral Jets: IRIS and Hinode Observations

Sanjiv K. Tiwari, Ronald L. Moore, Bart De Pontieu +4

A recent study using {\it Hinode} (SOT/FG) data of a sunspot revealed some unusually large penumbral jets that often repeatedly occurred at the same locations in the penumbra, name…

astro-ph.SR2018★ 67 cited

IRIS and SDO Observations of Solar Jetlets Resulting from Network-Edge Flux Cancelation

Navdeep K. Panesar, Alphonse C. Sterling, Ronald L. Moore +3

Recent observations show that the buildup and triggering of minifilament eruptions that drive coronal jets result from magnetic flux cancelation at the neutral line between merging…

astro-ph.SR2018★ 12 cited

Critical magnetic field strengths for solar coronal plumes in quiet regions and coronal holes?

Ellis A. Avallone, Sanjiv K. Tiwari, Navdeep K. Panesar +2

Coronal plumes are bright magnetic funnels found in quiet regions (QRs) and coronal holes (CHs). They extend high into the solar corona and last from hours to days. The heating pro…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.