The two Voyager spacecraft have completed their planetary exploration mission and are now probing the outer realms of the heliosphere. The Voyager ultraviolet spectrometers continued to operate well after the Voyager 2 Neptune encounter in 1989. We present a complete database of diffuse radiation observations made by both Voyagers: a total of 1943 spectra (500–1600 Å) scattered throughout the sky. These include observations of dust-scattered starlight, emission lines from the hot interstellar medium, and a number of locations where no diffuse radiation was detected, with the very low upper limit of about 25 photons cm−2 s−1 sr−1 Å−1. Many of these observations were from late in the mission when there was significantly less contribution from...
International audienceUVS instrument onboard Voyager-1 has been performing measurements of the backs...
International audienceIn this work, we present for the first time the Lyman α intensities measured b...
The solar system and heliosphere are embedded in a partially ionized medium flowing past the Sun at ...
Attachments to this final report include 2 papers connected with the Voyager work: 'Voyager Observat...
The data harvest from the Voyagers' (V1 and V2) Ultraviolet Spectrometers (UVS) covers encounters wi...
The UVS spectrometer on Voyager 1 is still active in 2014. The only line still observed in the spect...
International audienceThe data harvest from the Voyagers’ (V 1 and V 2) Ultraviolet Spectrometers (U...
The Voyager Ultraviolet Spectrometer (UVS) is an objective grating spectrometer covering the wavelen...
An analysis is presented for the spectra of the diffuse ultraviolet background taken during shuttle ...
International audienceDoppler-shifted hydrogen Lyman-alpha (Lyα) emission from galaxies is currently...
Abstract. Diffuse ultraviolet background radiation may contain important information concerning the ...
Abstract. I report on progress in my ongoing work with Professor Jayant Murthy con-cerning the origi...
The detectors of the Ultraviolet Spectrographs (UVS) on Voyager 1/2 are recording a backgr...
International audienceUVS instrument onboard Voyager-1 has been performing measurements of the backs...
International audienceIn this work, we present for the first time the Lyman α intensities measured b...
The solar system and heliosphere are embedded in a partially ionized medium flowing past the Sun at ...
Attachments to this final report include 2 papers connected with the Voyager work: 'Voyager Observat...
The data harvest from the Voyagers' (V1 and V2) Ultraviolet Spectrometers (UVS) covers encounters wi...
The UVS spectrometer on Voyager 1 is still active in 2014. The only line still observed in the spect...
International audienceThe data harvest from the Voyagers’ (V 1 and V 2) Ultraviolet Spectrometers (U...
The Voyager Ultraviolet Spectrometer (UVS) is an objective grating spectrometer covering the wavelen...
An analysis is presented for the spectra of the diffuse ultraviolet background taken during shuttle ...
International audienceDoppler-shifted hydrogen Lyman-alpha (Lyα) emission from galaxies is currently...
Abstract. Diffuse ultraviolet background radiation may contain important information concerning the ...
Abstract. I report on progress in my ongoing work with Professor Jayant Murthy con-cerning the origi...
The detectors of the Ultraviolet Spectrographs (UVS) on Voyager 1/2 are recording a backgr...
International audienceUVS instrument onboard Voyager-1 has been performing measurements of the backs...
International audienceIn this work, we present for the first time the Lyman α intensities measured b...
The solar system and heliosphere are embedded in a partially ionized medium flowing past the Sun at ...