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Science & Technology
Guest Storage - PSA
Guest Storage Facility
In 2019, the PSA developed a new feature, the Guest Storage Facilty. This consists in an FTP file repository into which scientists from the planetary community can upload and share scientific products valuable for the community.
Inputs
Scientific products to be hosted in the Guest Storage Facilty should be of interest for the planetary science community, and overall making use or presenting new products from ESA's planetary missions.
The format of the data is entirely up to the data producer choice.
The PSA only require the "Data User Guide" to be provided, the template can be downloaded here.
An associated scientific peer-reviewed publication associated to the products is encouraged
Inquiry to the PSA for storage
Potential data producers should get in touch with the PSA, either through their known contacts, the mission archive scientsist, or simply get in touch with us.
After initial contact, the PSA will then contact the data producers to formalize the process and provides credentials for the FTP access to upload the data.
A Digital Object Identifier (DOI) could be assigned to each delivery, this is an optional functionality that is also highly encouraged.
PSA review of the GSF
While the products are looked at by the archive scientists (i.e., not all one by one), no proper full scale peer reviewed scientific analysis are done.
Content of the Guest Storage facility
| 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 UCL-MSSL |
10.5270/esa-0j79yk8 |
| IPGP_Titan_Huygens_V1.0 | August 2020 | A new digital terrain model of the river networks observed at the Huygens landing site has been computed throughout a tailor made photogrammetric workflow, by using a set of overlapping, newly re-calibrated images acquired by the DISR cameras during the Huygens probe's descent. The resulting DTM (hereafter called IPGP-DTM) provides the best available spatial sampling of Titan's landscape (18 m) and increases the size of the reconstructed region up to 10.3 km². | Link to the PUG | Cassini-Huygens DISR Titan |
Chloe Daudon Antoine Lucas Sebastien Rodriguez IPGP |
10.5270/esa-3uja374 |
| 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 MarsExpress |
Jan Peter Muller 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 HiRISE MarsExpress |
Jan Peter Muller Si-Ting Xiong Yu Tao UCL-MSSL |
10.5270/esa-lqefjdl |
| ESA-AURORA_67P-GEOMAP_OSIRIS_v1.0 | May 2021 | This dataset contains geological mapping of comet 67P/Churyumov-Gerasimenko northern hemisphere. They consist of global maps of the complete comet and regional maps of the individual geological regions. Maps are presented in different versions of the Qunincuncial Adaptive Closed Kohonen (QuACK) map projection. The geological features which have been mapped are also provided as shape files in the format of the Small Body Mapping Tool (SMBT). | Link to the PUG | Rosetta OSIRIS |
Sebastien Besse Bjorn Grieger |
10.5270/esa-kokoti7 |
| November 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 |
https://doi.org/10.5270/esa-5m2qvh6 | |
| November 2021 | The JANUS instrument team at the German Aerospace Center (DLR) has created a new global mosaic of Jupiter's moon Ganymede from NASA Voyager and Galileo images with a spatial resolution of 359 m/pxl. | Link to the PUG | Voyager & Galileo Ganymede |
Elke Kersten DLR |
https://doi.org/10.5270/esa-mqhvfjf | |
| 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 |
Mars Reconnaissance Orbiter HiRISE MarsExpress |
Yu Tao Jan-Peter Muller |
10.5270/esa-1xyk62p |
| 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 |
||
| 2022 | This dataset is comprised of shapefiles, georeferenced to the simple cylindrical projection of Mars, hereafter SimpleCylindrical_Mars, of Martian fluvial valley networks mapped using High-Resolution Stereo Camera images (15 – 25 m per pixel) in a pole-to-pole strip located from 20°W - 20°E. The purpose of this dataset is to assess the conformity between valley orientation and surface slope direction. | Links to the PUG |
Mars Express / HRSC |
Rickbir Singh Bahia | 10.5270/esa-f7rgzj6 |
|
| 2022 | The JANUS instrument team at the German Aerospace Center (DLR) has created a new global mosaic of Jupiter's moon Ganymede from NASA Voyage, Galileo and Juno images with a spatial resolution of 359 m/pxl. | Link to the PUG | Voyager Galileo JunoCam |
Elke Kersten | 10.57780/esa-fcj5pf3 | |
| 2022 | This dataset presents the geography of Oxia Planum, the landing site selected for the ExoMars Rover and Surface Platform mission. A collection of three datasets provide a framework to investigate this area. They are:
|
Link to the PUG |
Mars MRO/CTX TGO/CaSSIS |
Peter Fawdon Elliot Sefton-Nash Csilla Orgel Ines Torres |
10.5270/esa-krek4a0 | |
| 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 |
| Mars_HRSC_High-Altitude-Mosaic_V1.0 | 2023 |
A high-altitude observation campaign with the Mars Express High Resolution Stereo Camera was used to construct five global mosaics of Mars from images captured through each of its five different spectral filters: panchromatic, red, green, blue and infra-red. |
Link to the PUG | Mars Express HRSC | Greg Michael | 10.57780/esa-t4y39mj |
| ESA_Mars_TGO-MEX_Radio_Occultation_V1.0 | 2024 | Data products for most of the key steps in the processing chain that converts the raw data collected at Trace Gas Orbiter’s (TGO) Electra antenna, to the derived vertical electron density profiles. These processing steps are described in detail in §4 of Parrott et al, 2024 (https://doi.org/10.1029/2023RS007873). | Link to to the PUG |
Mars Express TGO |
Jacob Parrott, Colin Wilson, Olivier Witasse |
10.57780/esa-zdvq6sw |
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