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researcher

T. Johnson

4 papers hereh-index 5915.3k citations400 works total

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

author position
  • first author1
  • middle author2
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP3
  • astro-ph1
same name
  • T. Johnson — 104 papers, h 61
  • T. Johnson — 46 papers, h 24
  • T. Johnson — 34 papers, h 22
  • T. Johnson — 17 papers, h 15
  • T. Johnson — 10 papers, h 45
  • T. Johnson — 10 papers, h 9

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
20032012
most citedPlanetesimal Compositions in Exoplanet Systems

87 citations · 87 across the 1 of their papers we have counts for

collaborators

4 papers

astro-ph.EP2012★ 87 cited

Planetesimal Compositions in Exoplanet Systems

Torrence V. Johnson, Olivier Mousis, Jonathan I. Lunine +1

We have used recent surveys of the composition of exoplanet host stars to investigate the expected composition of condensed material in planetesimals formed beyond the snow line in…

astro-ph.EP2012

Nebular water depletion as the cause of Jupiter's low oxygen abundance

Olivier Mousis, Jonathan I. Lunine, Nikku Madhusudhan +1

Motivated by recent spectroscopic observations suggesting that atmospheres of some extrasolar giant-planets are carbon-rich, i.e. carbon/oxygen ratio (C/O) ≥ 1, we find that th…

astro-ph.EP2011

Carbon-rich Giant Planets: Atmospheric Chemistry, Thermal Inversions, Spectra, and Formation conditions

Nikku Madhusudhan, Olivier Mousis, Torrence V. Johnson +1

The recent inference of a carbon-rich atmosphere, with C/O >= 1, in the hot Jupiter WASP-12b motivates the exotic new class of carbon-rich planets (CRPs). We report a detailed stud…

astro-ph2003

Jovian Dust Streams: A monitor of Io's volcanic plume activity

Harald Krueger, Paul Geissler, Mihaly Horanyi +7

Streams of high speed dust particles originate from Jupiter's innermost Galilean moon Io. After release from Io, the particles collect electric charges in the Io plasma torus, gain…

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