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Hybrid Volcanic Episodes within the Orientale Basin, Moon
DOI: 10.3390/rs15071801 Bibcode: 2023RemS...15.1801P

Harish; Patel, Shreekumari Mukeshbhai; Patel, Deep +2 more

Basalts from Mare Orientale are representative of lunar flood volcanism, which sheds light on the lunar farside's thermal and volcanic past. We use Chandrayaan's Moon Mineralogy Mapper data to examine the spectral and chemical makeup of the volcanic units located in the Orientale basin; the analysis specifically focuses on three formations: Mare O…

2023 Remote Sensing
Chandrayaan-1 0
Minimum Noise Fraction Analysis of TGO/NOMAD LNO Channel High-Resolution Nadir Spectra of Mars
DOI: 10.3390/rs15245741 Bibcode: 2023RemS...15.5741O

Vandaele, Ann Carine; Daerden, Frank; Ristic, Bojan +10 more

NOMAD is a suite of spectrometers on the board of the ESA-Roscosmos Trace Gas Orbiter (TGO) spacecraft and is capable of investigating the Martian environment at very high spectral resolution in the ultraviolet-visible and infrared spectral ranges by means of three separate channels: UVIS (0.2-0.65 µm), LNO (2.2-3.8 µm), and SO (2.3-4.…

2023 Remote Sensing
ExoMars-16 0
GBB-Nadir and KLIMA: Two Full Physics Codes for the Computation of the Infrared Spectrum of the Planetary Radiation Escaping to Space
DOI: 10.3390/rs15102532 Bibcode: 2023RemS...15.2532D

Dinelli, Bianca Maria; Del Bianco, Samuele; Castelli, Elisa +7 more

In 2019 the Far-Infrared Outgoing Radiation Understanding and Monitoring (FORUM) mission was selected to be the 9th Earth Explorer mission of the European Space Agency (ESA). In the preparatory phase of the mission there was the need for accurate and versatile codes to compute the spectrally resolved Earth radiation escaping to space ( outgoing lo…

2023 Remote Sensing
MEx 0
Giant Planet Atmospheres: Dynamics and Variability from UV to Near-IR Hubble and Adaptive Optics Imaging
DOI: 10.3390/rs14061518 Bibcode: 2022RemS...14.1518S

Wong, Michael H.; Fletcher, Leigh N.; Simon, Amy A. +2 more

Each of the giant planets, Jupiter, Saturn, Uranus, and Neptune, has been observed by at least one robotic spacecraft mission. However, these missions are infrequent; Uranus and Neptune have only had a single flyby by Voyager 2. The Hubble Space Telescope, particularly the Wide Field Camera 3 (WFC3) and Advanced Camera for Surveys (ACS) instrument…

2022 Remote Sensing
eHST 11
An Efficient High-Resolution Global-Local Network to Detect Lunar Features for Space Energy Discovery
DOI: 10.3390/rs14061391 Bibcode: 2022RemS...14.1391J

Liu, Lei; Jia, Yutong; Peng, Siqing +2 more

Lunar craters and rilles are significant topographic features on the lunar surface that will play an essential role in future research on space energy resources and geological evolution. However, previous studies have shown low efficiency in detecting lunar impact craters and poor accuracy in detecting lunar rilles. There is no complete automated …

2022 Remote Sensing
MEx 5
Subpixel-Scale Topography Retrieval of Mars Using Single-Image DTM Estimation and Super-Resolution Restoration
DOI: 10.3390/rs14020257 Bibcode: 2022RemS...14..257T

Tao, Yu; Michael, Greg; Muller, Jan-Peter +5 more

We propose using coupled deep learning based super-resolution restoration (SRR) and single-image digital terrain model (DTM) estimation (SDE) methods to produce subpixel-scale topography from single-view ESA Trace Gas Orbiter Colour and Stereo Surface Imaging System (CaSSIS) and NASA Mars Reconnaissance Orbiter High Resolution Imaging Science Expe…

2022 Remote Sensing
ExoMars-16 MEx 3
An Investigation on the Morphological and Mineralogical Characteristics of Posidonius Floor Fractured Lunar Impact Crater Using Lunar Remote Sensing Data
DOI: 10.3390/rs14040814 Bibcode: 2022RemS...14..814S

Salem, Imen Ben; Sharma, Manish; Kumaresan, P. R. +4 more

Lunar floor-fractured craters (FFCs) are a distinguished type of crater found on the surface of the Moon with radial, concentric, and/or polygonal fractures. In the present study, we selected the Posidonius FCC to explore the mineralogy, morphology and tectonic characteristics using remote sensing datasets. The Posidonius crater is vested with a w…

2022 Remote Sensing
Chandrayaan-1 3
Evaluation of the Capability of ExoMars-TGO NOMAD Infrared Nadir Channel for Water Ice Clouds Detection on Mars
DOI: 10.3390/rs14174143 Bibcode: 2022RemS...14.4143R

Daerden, Frank; Ristic, Bojan; Bellucci, Giancarlo +13 more

As part of the payload of the 2016 ExoMars Trace Gas Orbiter (TGO) mission, the Nadir and Occultation for MArs Discovery (NOMAD) suite instrument has been observing the Martian atmosphere since March 2018. NOMAD is mainly dedicated to the study of trace atmospheric species taking advantage of a high-spectral resolution. We demonstrate that when NO…

2022 Remote Sensing
ExoMars-16 3
The Influence of Dynamic Solar Oblateness on Tracking Data Analysis from Past and Future Mercury Missions
DOI: 10.3390/rs14174139 Bibcode: 2022RemS...14.4139V

van der Zwaard, Rens; Dirkx, Dominic

When the BepiColombo spacecraft arrives at Mercury in late 2025, it will be able to measure the orbit of the planet with unprecedented accuracy, allowing for more accurate measurements of the perihelion advance of the planet, as predicted by the Theory of General Relativity (GR). A similar effect is produced by the gravitational oblateness of the …

2022 Remote Sensing
BepiColombo 3
A New Method for Retrieving Electron Density Profiles from the MARSIS Ionograms
DOI: 10.3390/rs14081817 Bibcode: 2022RemS...14.1817L

Le, Huijun; Liu, Libo; Chen, Yiding +7 more

The Martian ionosphere was actively detected by Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) aboard the Mars Express. The detected echo signal of the MARSIS at an epoch is presented as a function of frequency and time delay to form an ionogram. Some MARSIS ionograms have been processed to obtain the electron density profiles…

2022 Remote Sensing
MEx 3