File:Beispiel eines einzelnen HRSC-Höhenbildes (53119600361).jpg
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[edit]DescriptionBeispiel eines einzelnen HRSC-Höhenbildes (53119600361).jpg |
Deutsch: Beispiel eines einzelnen HRSC-Höhenbildes (HRSC-Orbitnummer 21,688_0000, aufgenommen am 28. Februar 2021; im Hintergrund schattiertes Reliefbild aus Höhenmessungen des Mars Observer Laser Altimeters der NASA, aufgezeichnet vor etwa 25 Jahren). Links: Rot-Grün-Blau-Bildkombination, die zeigt, wie die Oberfläche im sichtbaren Licht aussieht. Man beachte die hellblaue Färbung des nördlichen und südlichen Randes, die auf einen flacheren Blick der Kamera durch die Marsatmosphäre zurückzuführen ist, was wegen des längeren Lichtweges zu einem stärkeren atmosphärischen Einfluss auf die Bilder führt. Diese Bildteile wurden aus dem globalen Mosaik ausgeschlossen. Rechts: Infrarot-Rot-Grün-Bildkombination. Solche ungewöhnlichen Ansichten, die auch den Infrarotkanal einschließen, sind eine Möglichkeit, das Verhältnis des Oberflächenreflexionsvermögens im Infraroten zu dem der anderen Farben zu untersuchen. Sie werden auch untersucht, um Artefakte oder Lücken in den Eingabedaten zu entdecken.
Credit: ESA/DLR/FU Berlin/MOLA science team English: Example of a single HRSC elevation image (HRSC orbit number 21.688_0000, acquired 28 February 2021; background shaded relief image from elevation measurements by NASA's Mars Observer Laser Altimeter recorded approximately 25 years ago). Left: Red-green-blue image combination showing what the surface looks like in visible light. Note the light blue coloring of the northern and southern limbs, which is due to the camera looking flatter through the Martian atmosphere, resulting in more atmospheric influence on the images due to the longer light path. These parts of the image have been excluded from the global mosaic. Right: infrared red-green image combination. Such unusual views, which also include the infrared channel, are a way of examining the relationship of surface reflectance in the infrared to that of the other colors. They are also examined to discover artifacts or gaps in the input data. Credit: ESA/DLR/FU Berlin/MOLA science team |
Date | Taken on 16 August 2023, 05:40:42 |
Source | Beispiel eines einzelnen HRSC-Höhenbildes |
Author | DLR_de |
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This image was originally posted to Flickr by DLR_de at https://flickr.com/photos/48213136@N06/53119600361. It was reviewed on 17 August 2023 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-sa-2.0. |
17 August 2023
This media has been released under a free license by the Deutsches Zentrum für Luft- und Raumfahrt (DLR). Their website states: "Where expressly stated, DLR images and videos are covered by a Creative Commons Attribution 3.0 Germany (CC BY 3.0) licence. This licence grants permission to reproduce or distribute the work, to make the work and/or its contents publically available, to alter or edit the work and/or its contents and to make commercial use of the work, provided that you explicitly mention DLR as its source in a clearly legible format. Examples: 'Photo: DLR, CC-BY 3.0', 'Images: DLR, CC-BY 3.0', 'Video: DLR, CC-BY 3.0'." To the uploader: You must provide a link (URL) to the original file and the authorship information if available. |
This file is licensed under the Creative Commons Attribution 3.0 Germany license.
Attribution: DLR, CC-BY 3.0
- You are free:
- to share – to copy, distribute and transmit the work
- to remix – to adapt the work
- Under the following conditions:
- attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
This media was created by the European Space Agency (ESA).
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See the ESA Creative Commons copyright notice for complete information, and this article for additional details.
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This file is licensed under the Creative Commons Attribution-ShareAlike 3.0 IGO license. Attribution: ESA/DLR/FU Berlin, CC BY-SA IGO 3.0
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