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researcher

R. Moore

50 papers hereh-index 456.4k citations293 works total

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

author position
  • first author6
  • middle author32
  • last author12

Across the 50 of 50 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR50
same name
  • R. Moore — 125 papers, h 61
  • R. Moore — 77 papers, h 24
  • R. Moore — 68 papers, h 73
  • R. Moore — 48 papers, h 27
  • R. Moore — 46 papers, h 12
  • R. Moore — 24 papers, h 19

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
20132023
most citedSmall-scale filament eruptions as the driver of solar coronal hole X-ray jets

357 citations · 2.2k across the 50 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.SR2023★ 14 cited

Formation of an observed eruptive flux rope above the torus instability threshold through tether-cutting magnetic reconnection

Avijeet Prasad, Sanjay Kumar, Alphonse C. Sterling +4

Erupting magnetic flux ropes (MFRs) play a crucial role in producing solar flares. However, the formation of erupting MFRs in complex coronal magnetic configurations and their subs…

astro-ph.SR2023★ 7 cited

Prospective Implications of EUV Coronal Plumes for Magnetic-network Genesis of Coronal Heating, Coronal-hole Solar Wind, and Solar-wind Magnetic-field Switchbacks

Ronald L. Moore, Sanjiv K. Tiwari, Navdeep K. Panesar +1

We propose that coronal heating in EUV coronal plumes is weaker, not stronger, than in adjacent non-plume coronal magnetic funnels. This expectation stems from (i) the observation…

astro-ph.SR2023

Future High-Resolution and High-Cadence Observations for Unraveling Small-Scale Explosive Solar Features

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

Solar coronal jets are frequently occurring collimated ejections of solar plasma, originating from magnetically mixed polarity locations on the Sun of size scale comparable to that…

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