Jupiter at five microns

K. R. Armstrong, R. B. Minton, George H. Rieke, F. J. Low

Research output: Contribution to journalArticle

2 Citations (Scopus)

Abstract

Maps of Jupiter at 5 um provide detailed information about the complex of emission features at this wavelength. Previous indications of a correlation between infrared sources and visual features are confirmed with a few significant exceptions. The behavior of Jupiter at 5 um is compared with that of other bodies in the outer solar system. Recent observations indicate emission features on Jupiter at other infrared wavelengths.

Original languageEnglish (US)
Pages (from-to)287-298
Number of pages12
JournalIcarus
Volume29
Issue number2
DOIs
StatePublished - 1976

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Jupiter (planet)
Jupiter
wavelength
wavelengths
solar system
indication

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Armstrong, K. R., Minton, R. B., Rieke, G. H., & Low, F. J. (1976). Jupiter at five microns. Icarus, 29(2), 287-298. https://doi.org/10.1016/0019-1035(76)90057-9

Jupiter at five microns. / Armstrong, K. R.; Minton, R. B.; Rieke, George H.; Low, F. J.

In: Icarus, Vol. 29, No. 2, 1976, p. 287-298.

Research output: Contribution to journalArticle

Armstrong, KR, Minton, RB, Rieke, GH & Low, FJ 1976, 'Jupiter at five microns', Icarus, vol. 29, no. 2, pp. 287-298. https://doi.org/10.1016/0019-1035(76)90057-9
Armstrong KR, Minton RB, Rieke GH, Low FJ. Jupiter at five microns. Icarus. 1976;29(2):287-298. https://doi.org/10.1016/0019-1035(76)90057-9
Armstrong, K. R. ; Minton, R. B. ; Rieke, George H. ; Low, F. J. / Jupiter at five microns. In: Icarus. 1976 ; Vol. 29, No. 2. pp. 287-298.
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