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Venusian South Polar Vortex through Venus Express (1)
This composite video sequence was obtained by the Ultraviolet, Visible and Near-Infrared Mapping Spectrometer (VIRTIS) on board ESA’s Venus Express. 
The single images were taken from 7 to 11 April 2007 over 5 different orbits. In each orbit the images were collected over a time span of 8 hours and were separated by about half an hour. The average distance from the Planet was about 65.000 Km. 
The Latitude of the observed area spans 50 to 90° South. The Longitude spans about 20 to 150° East. 
The video shows details of the Planet’s South Pole in RGB colour. The data obtained at 1.7 microns is shown in blue, while those obtained at 3.8 microns is represented in red. 
Using specific wavelengths (3.8 and 1.7 microns, respectively), the observations allowed the imaging of the day and night areas around the South Pole simultaneously, at different depths (at about 65 Km and below the cloud deck, respectively) simultaneously. The intersection between the polar atmospheric structures seen at different wavelengths is visible well, due to the optical properties of the clouds. 

Parole chiave: Venus - Upper Atmosphere

Venusian South Polar Vortex through Venus Express (1)

This composite video sequence was obtained by the Ultraviolet, Visible and Near-Infrared Mapping Spectrometer (VIRTIS) on board ESA’s Venus Express.
The single images were taken from 7 to 11 April 2007 over 5 different orbits. In each orbit the images were collected over a time span of 8 hours and were separated by about half an hour. The average distance from the Planet was about 65.000 Km.
The Latitude of the observed area spans 50 to 90° South. The Longitude spans about 20 to 150° East.
The video shows details of the Planet’s South Pole in RGB colour. The data obtained at 1.7 microns is shown in blue, while those obtained at 3.8 microns is represented in red.
Using specific wavelengths (3.8 and 1.7 microns, respectively), the observations allowed the imaging of the day and night areas around the South Pole simultaneously, at different depths (at about 65 Km and below the cloud deck, respectively) simultaneously. The intersection between the polar atmospheric structures seen at different wavelengths is visible well, due to the optical properties of the clouds.

Venusian_Atmosphere_and_the_Solar_Wind-Interaction.jpg Venus-PIA10123.jpg South_Polar_Regions-0.gif South_Polar_Regions-1.gif Z-Venus~1.jpg
Informazioni sul file
Nome del file:South_Polar_Regions-0.gif
Nome album:MareKromium / Venus
Valutazione (3 voti):55555(Mostra dettagli)
Parole chiave:Venus / - / Upper / Atmosphere
Copyright:ESA/VIRTIS/INAF-IASF/Obs. de Paris-LESIA
Dimensione del file:530 KiB
Data di inserimento:Mag 15, 2007
Dimensioni:400 x 300 pixels
Visualizzato:59 volte
URL:https://www.lunexit.it/gallery/displayimage.php?pid=16834
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