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Parker Solar Probe Imaging of the Night Side of Venus.
Wood, Brian E; Hess, Phillip; Lustig-Yaeger, Jacob; Gallagher, Brendan; Korwan, Daniel; Rich, Nathan; Stenborg, Guillermo; Thernisien, Arnaud; Qadri, Syed N; Santiago, Freddie; Peralta, Javier; Arney, Giada N; Izenberg, Noam R; Vourlidas, Angelos; Linton, Mark G; Howard, Russell A; Raouafi, Nour E.
Afiliação
  • Wood BE; Naval Research Laboratory Space Science Division Washington DC USA.
  • Hess P; Naval Research Laboratory Space Science Division Washington DC USA.
  • Lustig-Yaeger J; The Johns Hopkins University Applied Physics Laboratory Laurel MD USA.
  • Gallagher B; Naval Research Laboratory Space Science Division Washington DC USA.
  • Korwan D; Naval Research Laboratory Remote Sensing Division Washington DC USA.
  • Rich N; Naval Research Laboratory Space Science Division Washington DC USA.
  • Stenborg G; The Johns Hopkins University Applied Physics Laboratory Laurel MD USA.
  • Thernisien A; Naval Research Laboratory Space Science Division Washington DC USA.
  • Qadri SN; Naval Research Laboratory Remote Sensing Division Washington DC USA.
  • Santiago F; Naval Research Laboratory Remote Sensing Division Washington DC USA.
  • Peralta J; Facultad de Fisica Universidad de Sevilla Sevilla Spain.
  • Arney GN; NASA Goddard Space Flight Center Greenbelt MD USA.
  • Izenberg NR; The Johns Hopkins University Applied Physics Laboratory Laurel MD USA.
  • Vourlidas A; The Johns Hopkins University Applied Physics Laboratory Laurel MD USA.
  • Linton MG; Naval Research Laboratory Space Science Division Washington DC USA.
  • Howard RA; The Johns Hopkins University Applied Physics Laboratory Laurel MD USA.
  • Raouafi NE; The Johns Hopkins University Applied Physics Laboratory Laurel MD USA.
Geophys Res Lett ; 49(3): e2021GL096302, 2022 Feb 16.
Article em En | MEDLINE | ID: mdl-35864851
ABSTRACT
We present images of Venus from the Wide-Field Imager for Parker Solar Probe (WISPR) telescope on board the Parker Solar Probe (PSP) spacecraft, obtained during PSP's third and fourth flybys of Venus on 2020 July 11 and 2021 February 20, respectively. Thermal emission from the surface is observed on the night side, representing the shortest wavelength observations of this emission ever, the first detection of the Venusian surface by an optical telescope observing below 0.8 µm. Consistent with previous observations at 1 µm, the cooler highland areas are fainter than the surrounding lowlands. The irradiances measured by WISPR are consistent with model predictions assuming a surface temperature of T = 735 K. In addition to the thermal emission, the WISPR images also show bright nightglow emission at the limb, and we compare the WISPR intensities with previous spectroscopic measurements of the molecular oxygen nightglow lines from Venus Express.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Revista: Geophys Res Lett Ano de publicação: 2022 Tipo de documento: Article

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Revista: Geophys Res Lett Ano de publicação: 2022 Tipo de documento: Article
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