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Louth Crater (EDM - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)
This observation shows a persistent Frost Patch located on a Mound which is inside Louth Crater. The Frost Patch has remained largely stable at least since the Viking era (such as the late 1970s). The bright Frosty Region is bounded by a Dunefield on the North/East and the so-called "Size Classes" of several of the Features forming the Dunefield probably represent generations of Dunes that were created under a variety of Dominant Wind Conditions. The Frost is largely absent over the Dunes, but it is way more stable on the Ground that does not possess Dune-shaped Landforms. 

Mars Local Time: 15:14 (Early Afternoon)
Coord. (centered): 70,377° North Lat. and 103,397° East Long.
Spacecraft altitude: 317,5 Km (such as about 198,4 miles) 
Original image scale range: 63,5 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 91 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: POLAR STEREOGRAPHIC
Emission Angle: 9,3° 
Sun - Mars - MRO (or "Phase") Angle: 56,1°
Solar Incidence Angle: 64° (meaning that the Sun is about 26° above the Local Horizon)
Solar Longitude: 146,4° (Northern Summer - Southern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia
Parole chiave: Mars from orbit - Craters - Louth Crater

Louth Crater (EDM - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)

This observation shows a persistent Frost Patch located on a Mound which is inside Louth Crater. The Frost Patch has remained largely stable at least since the Viking era (such as the late 1970s). The bright Frosty Region is bounded by a Dunefield on the North/East and the so-called "Size Classes" of several of the Features forming the Dunefield probably represent generations of Dunes that were created under a variety of Dominant Wind Conditions. The Frost is largely absent over the Dunes, but it is way more stable on the Ground that does not possess Dune-shaped Landforms.

Mars Local Time: 15:14 (Early Afternoon)
Coord. (centered): 70,377° North Lat. and 103,397° East Long.
Spacecraft altitude: 317,5 Km (such as about 198,4 miles)
Original image scale range: 63,5 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 91 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: POLAR STEREOGRAPHIC
Emission Angle: 9,3°
Sun - Mars - MRO (or "Phase") Angle: 56,1°
Solar Incidence Angle: 64° (meaning that the Sun is about 26° above the Local Horizon)
Solar Longitude: 146,4° (Northern Summer - Southern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia

PSP_001700_2505-PCF-LXTT-IPF-01.jpg PSP_007805_2505-PCF-LXTT-IPF-00.jpg PSP_001700_2505-PCF-LXTT-IPF-02.jpg ESP_025296_1535-PCF-LXTT-02-B.jpg ESP_025296_1535-PCF-LXTT-02-A.jpg
Informazioni sul file
Nome del file:PSP_001700_2505-PCF-LXTT-IPF-02.jpg
Nome album:MareKromium / Mars Reconnaissance Orbiter (MRO)
Valutazione (4 voti):55555(Mostra dettagli)
Parole chiave:Mars / from / orbit / - / Craters / - / Louth / Crater
Copyright:NASA/JPL/Univ. of Arizona e Dr Paolo C. Fienga - Lunar Explorer Italia per l'additional process. e la colorizzazione
Dimensione del file:376 KiB
Data di inserimento:Lug 18, 2012
Dimensioni:3000 x 1662 pixels
Visualizzato:96 volte
URL:https://www.lunexit.it/gallery/displayimage.php?pid=30730
Preferiti:Aggiungi ai preferiti

Commento 1 a 3 di 3
Pagina: 1

MareKromium   [Ott 06, 2020 at 05:17 PM]
Brina o acque affioranti ghiacciate?
walthari   [Ott 06, 2020 at 07:35 PM]
direi brina ma comunque sia è un dato importante!!
MareKromium   [Ott 06, 2020 at 07:55 PM]
Molto!

Commento 1 a 3 di 3
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