Mars from Orbit (from July 2009)
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Clouds-Elysium_Mons-20080616a-PCF-LXTT-1.jpgLow altitude Clouds (or maybe "Fumes") from Elysium Mons (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)64 visitenessun commentoMareKromium
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Clouds-M0904025-PCF-LXTT-2.jpgLow-altitude Clouds over Chasma Australe (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)116 visitenessun commentoMareKromium
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Clouds-PCF-LXTT.jpgNorth Polar Clouds and Surface (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)54 visiteCaption NASA:"When winds that have swept across the North Polar Ice encounter a trough in the ice, the laminar flow slows at the base of the trough, producing a turbulent wind regime that is easily recognized in the clouds formed in the trough".
MareKromium
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Clouds-PIA13386.jpgNorth Polar Clouds (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)132 visiteCaption NASA:"Clouds are common near the North Polar Cap throughout the entire Spring and Summer. The Clouds typically cause a haze over the extensive Dunefields forming the North Polar Erg.
This VIS image shows the edge of the Cloud-front".MareKromium
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Clouds-PIA14965-PCF-LXTT.jpgClouds over Charlier Crater (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)133 visiteOrbit Number: 43473
Latitude: 68,057° South
Longitude: 190,213° East
Instrument: VIS
Captured: October, 2nd, 2011
Mars Local Time (M.L.T.): 19:45 (Early Evening Hours)
MareKromium
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Clouds-Soth_Polar_Regions-20090417a-PCF-LXTT-1.jpgSouthern Storm (1 - Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)68 visiteCaption NASA:"Right now, most of the Southern Hemisphere of Mars is covered by Dust Storms, blocking our view of the Surface. Bright cloud tops dominate these two VIS images".MareKromium
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Clouds-Soth_Polar_Regions-20090417a-PCF-LXTT-2.jpgSouthern Storm (2 - Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)72 visiteCoord.: 68,7° South Lat. and 146,4° East Long.MareKromium
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Clouds-South_Polar_Regions-20090416a-PCF-LXTT-1.jpgSouthern Storm (1 - Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)57 visiteCaption NASA:"The southern hemisphere dust storm season is in full swing this year on Mars. This VIS image shows the top of the dust clouds and thin streamers of clouds".MareKromium
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Clouds-South_Polar_Regions-20090416a-PCF-LXTT-2.jpgSouthern Storm (2 - Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)79 visiteCoord.: 68,2° South Lat. and 190,6° East Long.MareKromium
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Clouds-South_Polar_Regions-PCF-LXTT.jpgSouthern Dust Storm (Enhanced Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)53 visiteCaption NASA:"This image captured part of one of the larger storms that occurred during the latest Spring Season on Mars. Southern Spring is the season of Dust Storms and this storm is located over Promethei Terra".MareKromium
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Clouds-South_Polar_regions-20090415a-PCF-LXTT.jpgSouthern Cloud-Front (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)73 visiteCaption NASA:"This VIS image of the South Polar Region of Mars shows the edge of a front of clouds. These clouds are near enough to the Surface to be affected by surface topography".
Coord.: 73,7° South Lat. and 133,0° East LongMareKromium
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Clouds-Vastitas_Borealis_Region-PCF-LXTT-2.jpgClouds over Vastitas Borealis (Enhanced Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)54 visiteCaption NASA:"Dust Clouds often can obscure the Surface of Mars. When an image captures the edge of a Dust Storm Front, the loss of surface information is more than compensated for by the information that can be gleaned from analysis of the image.
As Dust Storm formation and location are unpredictable, any images of such features are priceless".
Coord.: 66,2° North. Lat. and 248,7° East Long.MareKromium
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