High spectral resolution line profiles and images of comet Halley

F. L. Roesler, F. Scherb, K. Magee, J. Harlander, R. J. Reynolds, R. V. Yelle, A. L. Broadfoot, R. J. Oliversen

Research output: Contribution to journalArticlepeer-review

9 Scopus citations

Abstract

High-spectral-resolution line profiles and images of comet Halley were obtained in 1986 at the National Solar Observatory McMath telescope, using a dual-etalon Fabry-Perot spectrometer. The spectrometer was designed to obtain data in four distinct modes: (1) high-resolution (R = 200,000) scanning, (2) high-resolution imaging, (3) moderate resolution (R = 30,000) scanning, and (4) moderate resolution imaging. This paper describes the instrument and some examples of data obtained in the high-resolution scanning mode.

Original languageEnglish (US)
Pages (from-to)279-282
Number of pages4
JournalAdvances in Space Research
Volume5
Issue number12
DOIs
StatePublished - 1985

ASJC Scopus subject areas

  • Aerospace Engineering
  • Astronomy and Astrophysics
  • Geophysics
  • Atmospheric Science
  • Space and Planetary Science
  • Earth and Planetary Sciences(all)

Fingerprint

Dive into the research topics of 'High spectral resolution line profiles and images of comet Halley'. Together they form a unique fingerprint.

Cite this