The Aurora on Venus

Jane L. Fox; A. I. F. Stewart

doi:10.1029/EO066i046p00813

The Aurora on Venus

Jane L. Fox, A. I. F. Stewart

Wright State University

Research output: Contribution to conference › Presentation

Abstract

Intensities of the 1304Å resonance line of atomic oxygen averaging 20R have been recorded on the nightside of Venus by the Pioneer Venus Orbiter Ultraviolet Spectrometer. Model calculations of the intensities of 1304Å, 1356Å and 5577Å emissions to be expected for various spectra of incident electrons will be presented. It is found that to reproduce the observed intensities, the incident electrons must be very soft (E

Original language	American English
DOIs	https://doi.org/10.1029/EO066i046p00813
State	Published - Nov 1 1985
Event	Eos - Duration: Dec 1 2000 → …

Conference

Conference	Eos
Period	12/1/00 → …

Disciplines

Physical Sciences and Mathematics
Physics

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10.1029/EO066i046p00813License: Unspecified

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title = "The Aurora on Venus",

abstract = "Intensities of the 1304{\AA} resonance line of atomic oxygen averaging 20R have been recorded on the nightside of Venus by the Pioneer Venus Orbiter Ultraviolet Spectrometer. Model calculations of the intensities of 1304{\AA}, 1356{\AA} and 5577{\AA} emissions to be expected for various spectra of incident electrons will be presented. It is found that to reproduce the observed intensities, the incident electrons must be very soft (E",

author = "Fox, {Jane L.} and Stewart, {A. I. F.}",

year = "1985",

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doi = "10.1029/EO066i046p00813",

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AU - Fox, Jane L.

AU - Stewart, A. I. F.

PY - 1985/11/1

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N2 - Intensities of the 1304Å resonance line of atomic oxygen averaging 20R have been recorded on the nightside of Venus by the Pioneer Venus Orbiter Ultraviolet Spectrometer. Model calculations of the intensities of 1304Å, 1356Å and 5577Å emissions to be expected for various spectra of incident electrons will be presented. It is found that to reproduce the observed intensities, the incident electrons must be very soft (E

AB - Intensities of the 1304Å resonance line of atomic oxygen averaging 20R have been recorded on the nightside of Venus by the Pioneer Venus Orbiter Ultraviolet Spectrometer. Model calculations of the intensities of 1304Å, 1356Å and 5577Å emissions to be expected for various spectra of incident electrons will be presented. It is found that to reproduce the observed intensities, the incident electrons must be very soft (E

UR - https://corescholar.libraries.wright.edu/physics/468

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DO - 10.1029/EO066i046p00813

M3 - Presentation

T2 - Eos

Y2 - 1 December 2000

ER -

The Aurora on Venus

Abstract

Conference

Disciplines

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