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OPP-SOL1045-MI-MF-LXTT-1.jpgOn the Surface of Meridiani Planum... - Sol 1045 (Superdefinition and Hi-Def-3D; credits for the additional process.: Dr Marco Faccin - Lunexit Team)83 visitenessun commentoMareKromium
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Dust_Devil_Tracks-Noachis_Terra-20090724a-PCF-LXTT.jpgDust Devils Tracks in Noachis Terra (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)83 visitenessun commentoMareKromium
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OPP-SOL358-MI-MF-LXTT.jpgMatter of Style... - Sol 358 (Sx - credits for the additional process.: Dr Paolo C. Fienga - Lunexit team; Dx - credits: NASA/JPL-Caltech)83 visiteUn piccolissimo raffronto fra la qualità del Prodotto "Pubblico" NASA (Dx) e quello Lunexit (Sx).
I commenti, se vale la pena farli, li lasciamo a Voi.MareKromium
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Coprates_Chasma-Chaotic_Terrain-MO-PCF-LXTT.jpgChaotic Terrain in Coprates Chasma (Absolute Natural Colors; additional process.: Dr Paolo C. Fienga - Lunexit Team)83 visitenessun commentoMareKromium
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SOL052-2N130956459EFF1100P1934L0M1-PCF-LXTT.jpgMartian Dawn - Sol 52 (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)83 visiteLeft Navigation Camera Non-linearized Full frame EDR acquired on Sol 52 of Spirit's Mission to Gusev Crater at approximately 05:18:59 Mars Local Solar Time.MareKromium
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051-569825main_dawn-image-070111-43_946-710.jpgApproaching 4-Vesta83 visitenessun commentoMareKromium
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SOL094-2P134687142EDN2700P2681L5M1-PCF-IPF.jpgDawn over Gusev Crater - Sol 94 (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)83 visiteForse si tratta di frames ridondanti, ma vedere - sia pure solo in una fotografia - l'alba su un Pianeta che non è la Terra, oggi, a noi continua a sembrare un miracolo ed un evento a metà tra la Realtà e la Mètafisica.
Frame PanCam ottenuto alle ore 06:07 Mars Local Solar Time.
MareKromium
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OPP-SOL2906-GB-LXTT-01.jpgA "Postcard" from Greeley Haven n. 2 - Sol 2906 (Natural Colors; credits for the additional process. and color.: Dr Gianluigi Barca - Lunexit Team)83 visitenessun commentoMareKromium
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Titan-N00188978-86-MF-EB-LXTT-IPF-1.jpgPossible Aurora at Titan (Superdefinition; credits for the additional process. and color.: Elisabetta Bonora and Marco Faccin/Lunexit Team)83 visitenessun commentoMareKromium
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Titan-W00074172-79-CB3Filter-MF-EB-LXTT-IPF.jpgFull Titan (Superdefinition and Enhanced Natural Colors; credits for the additional process. and color.: Elisabetta Bonora and Marco Faccin/Lunexit Team)83 visitenessun commentoMareKromium
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SOL0001-673758main_PIA15974-43_full.jpgLinearized Rear-View - Sol 1 (RAW Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)83 visiteCaption NASA:"This is a version of one of the first images taken by a Rear Hazard-Avoidance Camera (HazCam) on NASA's Curiosity Rover, which landed on Mars the evening of Aug. 5 PDT (morning of Aug. 6 EDT), 2012. It was taken through a "fisheye" wide-angle lens but has been "linearized" so that the Horizon looks flat rather than curved. The image has also been cropped. It is one-half of full resolution. Part of the Rim of Gale Crater, which is a feature the size of Connecticut and Rhode Island combined, stretches from the top middle to the top right of the image. One of the Rover's Wheels can be seen at bottom right. As planned, the Rover's early engineering images are taken at Low Resolution". MareKromium
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The_Rings-PIA08306-PCF-LXTT-IPF.jpgThe beautiful and colorful Rings of Saturn (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia/Italian Planetary Foundation) 83 visiteThis is a spectacular view - obtained by the NASA - Cassini Spacecraft - that shows us the subtle golden and gray/whitish colors which characterize the Outer B-Ring, the Cassini Division and the inner part of the A-Ring of the Giant Gas-Planet Saturn. In this viewing geometry, the brightest feature in the Cassini Division is the (relatively) recently discovered diffuse Ringlet which lies near the Outer Edge of the Division (and this diffuse Ringlet shows a quite peculiar bluish cast). The colors of the Rings, as they look in this picture, appear more golden than ever because of the Viewing Geometry that was adopted: as a matter of fact, an increased scattering in the ice and rock particles forming the Rings was brought about not only by the high Phase Angle (such as the angle drawn and defined by the Sun, the Rings and the NASA - Cassini Spacecraft), but also by the circumstance that this view was obtained while the Spacecraft was watching towards the Unlit Side of the Rings, from about 30° above the Ring-Plane. The images used to create this frame were acquired by the NASA - Cassini Spacecraft narrow-angle camera on Sept. 29, 2006, at a distance of approx. 1,8 MKM (about 1,13 MMs) from the Rings of Saturn and the image scale is roughly 11 Km (such as about 7 miles) per pixel.
Remember that the NASA - CASSINI Original b/w frame has been additionally processed and then re-colorized, according to an informed speculation carried out by Dr Paolo C. Fienga (LXTT-IPF), in Absolute Natural Colors (such as the colors that a human eye would actually perceive if someone were onboard the NASA - Cassini Spacecraft and then looked outside, towards the Rings of Satun), by using an original technique created - and, in time, dramatically improved - by the Lunar Explorer Italia Team. Different colors, as well as different shades of the same color, mean, among others, the existence of different Elements in the Rings of Satun, each having a different Albedo (---> Reflectivity) and Chemical Composition.MareKromium
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