Search Publications

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
Development of Chaos Terrain as Subaqueous Slide Blocks in Galilaei Crater, Mars
DOI: 10.3390/rs14091998 Bibcode: 2022RemS...14.1998N

Nizam, Nabila; Divola, Claire; Day, Mackenzie +2 more

Chaos terrain, expressed as enigmatic blocky landscapes on Mars, has poorly understood origins. Several hypotheses have been put forward to explain chaos terrain formation, but none fully account for the morphologies observed in Galilaei crater, the focus of this study. Previously inferred to be a paleolake, Galilaei crater hosts chaos terrain com…

2022 Remote Sensing
MEx 2
Petrological and Mineralogical Characteristics of Exposed Materials on the Floors of the Lavoisier and Surrounding Craters
DOI: 10.3390/rs14174313 Bibcode: 2022RemS...14.4313Y

Moon, Seulgi; Yi, Eung Seok; Kim, Kyeong Ja +3 more

Five floor-fractured craters (FFCs), Lavoisier crater and four craters surrounding it (Lavoisier C, Lavoisier E, Lavoisier F, and Lavoisier H), are distributed along the boundary between the northwestern part of the Oceanus Procellarum and the highlands. This study examines the uplifted or exposed materials on the fractured floors of these five im…

2022 Remote Sensing
Chandrayaan-1 2
Generation and Optimization of Spectral Cluster Maps to Enable Data Fusion of CaSSIS and CRISM Datasets
DOI: 10.3390/rs14112524 Bibcode: 2022RemS...14.2524F

Thomas, Nicolas; Rossi, Angelo Pio; Fernandes, Michael +2 more

Four-band color imaging of the Martian surface using the Color and Stereo Surface Imaging System (CaSSIS) onboard the European Space Agency's ExoMars Trace Gas Orbiter exhibits a high color diversity in specific regions. Not only is the correlation of color diversity maps with local morphological properties desirable, but mineralogical interpretat…

2022 Remote Sensing
ExoMars-16 2