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 (
Atomic oxygen is a key species in the mesosphere and thermosphere of Venus. It peaks in the transiti...
AbstractThe dayside of the Venus ionosphere at the top of the planet׳s thick atmosphere is sustained...
Calculations are presented of the vibrational distribution of O2+ in the Venusian ionosphere for a m...
Intensities of the 1304Å resonance line of atomic oxygen averaging 20R have been recorded on the nig...
The Pioneer Venus Orbiter Ultraviolet Spectrometer has recorded continuous but variable emissions of...
Abstract. The Pioneer Venus Orbiter Ultraviolet Spec-trometer has recorded continuous but variable e...
O(1D) and O(1S), the excited states that give rise to the atomic oxygen red and green lines, are pro...
We compare the intensity of the OI 130.4 and 135.6 nm emissions calculated using the soft electron p...
The Venus airglow has been observed from spectrometers on board rockets probes and satellites such a...
We have modeled the nightside ionosphere of Venus for 11 solar zenith angles between 90° and 165° wi...
The effect of a monoenergetic flux of electrons on a model atmosphere of the nightside thermosphere ...
of atomic oxygen has been observed on the nightside of Venus with HIRES, the echelle spectrograph on...
We report the detection of electrons due to photo-ionization of atomic oxygen and carbon dioxide in ...
We compare measurements and models of the luminosity that originates in the Martian and Venusian atm...
Since its discovery in 2005 with the SPICAM spectrograph on board Mars Express, the Mars aurora has ...
Atomic oxygen is a key species in the mesosphere and thermosphere of Venus. It peaks in the transiti...
AbstractThe dayside of the Venus ionosphere at the top of the planet׳s thick atmosphere is sustained...
Calculations are presented of the vibrational distribution of O2+ in the Venusian ionosphere for a m...
Intensities of the 1304Å resonance line of atomic oxygen averaging 20R have been recorded on the nig...
The Pioneer Venus Orbiter Ultraviolet Spectrometer has recorded continuous but variable emissions of...
Abstract. The Pioneer Venus Orbiter Ultraviolet Spec-trometer has recorded continuous but variable e...
O(1D) and O(1S), the excited states that give rise to the atomic oxygen red and green lines, are pro...
We compare the intensity of the OI 130.4 and 135.6 nm emissions calculated using the soft electron p...
The Venus airglow has been observed from spectrometers on board rockets probes and satellites such a...
We have modeled the nightside ionosphere of Venus for 11 solar zenith angles between 90° and 165° wi...
The effect of a monoenergetic flux of electrons on a model atmosphere of the nightside thermosphere ...
of atomic oxygen has been observed on the nightside of Venus with HIRES, the echelle spectrograph on...
We report the detection of electrons due to photo-ionization of atomic oxygen and carbon dioxide in ...
We compare measurements and models of the luminosity that originates in the Martian and Venusian atm...
Since its discovery in 2005 with the SPICAM spectrograph on board Mars Express, the Mars aurora has ...
Atomic oxygen is a key species in the mesosphere and thermosphere of Venus. It peaks in the transiti...
AbstractThe dayside of the Venus ionosphere at the top of the planet׳s thick atmosphere is sustained...
Calculations are presented of the vibrational distribution of O2+ in the Venusian ionosphere for a m...