UCL-MSSL

Summary of all UCL-MSSL GSF datasets

 

Title Date Description Product User Guide Missions and/or Targets Point of contact Digital Object Identifier (DOI)
UCL-MSSL_iMars_HRSC_V1.0 February 2019 A high spatial resolution (50m) Digital Terrain Model (DTM) and orthorectified Image (ORI) have been produced for the Martian South Polar Residual ice-Cap (SPRC)for 33 HRSC strips and the associated ORIs at 12.5m. In addition, a 50m DTM mosaic has been created alongside a 12.5m ORI mosaic. For the ORI mosaic, Individual HRSC image strips have been corrected for different surface scattering properties prior to mosaicing Link to the PUG MarsExpress
HRSC

Jan Peter Muller

Alfiah Rizky Diana Putri

UCL-MSSL

 10.5270/esa-0j79yk8
UCL-MSSL_iMars_CTX_V1.0 November 2020 High spatial resolution (18m) Digital Terrain Models (DTM) and (6m) orthorectified Images (ORI) have been produced covering the whole of Mars. The DTM products have been quality-controlled and where, available are co-registered to HRSC level-4 products. Link to the PUG

Mars Reconnaissance Orbiter
CTX

Jan Peter Muller

Yu Tao

UCL-MSSL

10.5270/esa-tk7pcfp
UCL-MSSL_MARS-CERBERUS_CTX-HIRISE-HRSC_V1.0 April 2021 1m HiRISE and 18m CTX co-registered 3D products (DTMs) and corresponding OrthoRectified Image (ORI) of 25cm and 6m respectively) of a terraced
crater in Cerberus Fossae employed to determine the thickness of lava+water ice overlying the buried streamlined island discussed in the paper. HRSC, CTX and HiRISE co-registered products are cropped over the terraced crater.		 Link to the PUG

Mars Reconnaissance Orbiter
CTX
HiRISE

Jan Peter Muller

Si-Ting Xiong

Yu Tao

UCL-MSSL

10.5270/esa-lqefjdl
UCL-MSSL_Valles-Marineris_HRSC_V1.0 2021 A high spatial resolution (50m) Digital Terrain Model (DTM) and 12.5m orthorectified Image (ORI) mosaics have been produced for the Martian Valles Marineris for 82 HRSC strips (11 from UCL fused with 71 from DLR). For the ORI mosaic, Individual HRSC image strips have been corrected for different surface scattering properties prior to mosaicing. Link to the PUG MarsExpress
HRSC

Jan Peter Muller

Yu Tao

UCL-MSSL

10.5270/esa-5m2qvh6
UCL-MSSL_Oxia-Planum_HRSC_CTX_HiRISE_MADNet_V1.0 2021 A multi-resolution DTM covering the 3-sigma landing ellipse of the 2020 for the Rosalind Franklin ExoMars rover mission. This unique dataset has been created using a novel deep learning technique called MADNet 1.0. This consists of a HRSC-DTM mosaic at 25m grid-spacing co-registered to MOLA DTM at 463m/grid-spacing. A 12m CTX DTM mosaic is co-registered to this HRSC 25m DTM. Finally a 50cm HiRISE derived DTM mosaic is co-registered to the 12m CTX DTM. Alongside this are the individual CTX 6m OrthoRectified Images (ORIs) and the 44 HiRISE 25cm ORIs Link to the PUG

MRO / CTX

MRO / HiRISE

MEX / HRSC

Yu Tao

Jan-Peter Muller

 10.5270/esa-1xyk62p

UCL-MSSL_Oxia-Planum_CaSSIS_SRR-MADNet_V1.0

 2021 Four mosaics derived from 9 single ESA-TGO-CaSSIS panchromatic images: 1m greyscale and 1m colourised (using HRSC colour) image mosaics of Super Resolution Restoration (SRR) and derived 2m DTM from 1m SRR-panchromatic and 8m DTM from 4m CaSSIS panchromatic both using MADNet 2.0 deep learning. These products are all co-registered to the previously published products from HiRISE-CTX-HRSC which are themselves co-aligned with MOLA DTMs. These products cover the 3-sigma landing ellipse of the Rosalind Franklin ExoMars rover. Link to the PUG EM16/TGO CaSSIS

Yu Tao

Jan-Peter Muller

10.5270/esa-5ahxyby
UCL-MSSL_Moon_von_Karman_V1.0 2023 A large area 1m mosaic covering 260 km × 209 km and constituent orbital strips covering the whole of the von Karman crater on the lunar farside. These mosaics include a  Digital Terrain Model (DTM) at 1m and OrthoRectified Image mosaic (ORI) at 50cm based on 0.5-1.5m LROC-NAC single scenes. In addition, the context DTM (14m) and ORI (7m) image from Chang'E-2 global mosaic which was itself co-registered to the global LOLA+SELENE dataset (59m at 128 ppd). Generated using Single Height Estimation algorithm MADNet 2.0 originally trained for Mars but re-trained for the Moon using all available good quality LROC-NAC stereo pairs. 370 LROC-NAC scenes were selected and co-registered to the CE2 ORI mosaic. The von Karman crater is the location of the Chang'E-4 rover (Yutu-2). Link to the PUG     
LRO/LROC NAC

Yu Tao

Jan-Peter Muller

 10.57780/esa-fb921t3