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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 2021Show all

3 papers · 1 filter

astro-ph.SR2021★ 156 cited

A fundamental mechanism of solar eruption initiation

Chaowei Jiang, Xueshang Feng, Rui Liu +8

Solar eruptions are spectacular magnetic explosions in the Sun's corona, and how they are initiated remains unclear. Prevailing theories often rely on special magnetic topologies t…

astro-ph.SR2021★ 4 cited

What Causes Faint Solar Coronal Jets from Emerging Flux Regions in Coronal Holes?

Abigail R. Harden, Navdeep K. Panesar, Ronald L. Moore +2

Using EUV images and line-of-sight magnetograms from Solar Dynamics Observatory, we examine eight emerging bipolar magnetic regions (BMRs) in central-disk coronal holes for whether…

astro-ph.SR2021★ 7 cited

Are the brightest coronal loops always rooted in mixed-polarity magnetic flux?

Sanjiv K. Tiwari, Caroline L. Evans, Navdeep K. Panesar +2

A recent study demonstrated that freedom of convection and strength of magnetic field in the photospheric feet of active-region (AR) coronal loops, together, can engender or quench…

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