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researcher

J. Doyle

32 papers hereh-index 353.9k citations313 works total

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

author position
  • first author2
  • middle author18
  • last author6

Across the 26 of 32 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR28
  • astro-ph3
  • astro-ph.EP1
same name
  • J. Doyle — 83 papers, h 53
  • J. Doyle — 19 papers, h 27
  • J. Doyle — 15 papers, h 58
  • J. Doyle — 14 papers, h 43
  • J. Doyle — 4 papers, h 5
  • J. Doyle — 3 papers, h 15

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
20062020
most citedConfirmation of the Electron Cyclotron Maser Instability as the Dominant Source of Radio Emission from Very Low Mass Stars and Brown Dwarfs

246 citations · 1.7k across the 32 of their papers we have counts for

collaborators
Showing astro-phShow all

3 papers · 1 filter

astro-ph2008★ 41 cited

The structure and dynamics of a bright point as seen with Hinode, SoHO and TRACE

D. Pérez-Suárez, R. C. Maclean, J. G. Doyle +1

Our aim is to determine the plasma properties of a coronal bright point and compare its magnetic topology extrapolated from magnetogram data with its appearance in X-ray images. We…

astro-ph2008★ 246 cited

Confirmation of the Electron Cyclotron Maser Instability as the Dominant Source of Radio Emission from Very Low Mass Stars and Brown Dwarfs

G. Hallinan, A. Antonova, J. G. Doyle +3

We report on radio observations of the M8.5 dwarf LSR J1835+3259 and the L3.5 dwarf 2MASS J00361617+1821104, which provide the strongest evidence to date that the electron cyclotro…

astro-ph2006★ 158 cited

Rotational Modulation of the Radio Emission from the M9 Dwarf TVLM 513-46546: Broadband Coherent Emission at the Substellar Boundary?

G. Hallinan, A. Antonova, J. G. Doyle +3

The Very Large Array was used to observe the ultracool, rapidly rotating M9 dwarf TVLM 513-46546 simultaneously at 4.88 GHz and 8.44 GHz. The radio emission was determined to be pe…

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