Search: onr:"swepub:oai:DiVA.org:uu-458293" > Regions of interest...
Fältnamn | Indikatorer | Metadata |
---|---|---|
000 | 07993naa a2200877 4500 | |
001 | oai:DiVA.org:uu-458293 | |
003 | SwePub | |
008 | 211111s2021 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-4582932 URI |
024 | 7 | a https://doi.org/10.1016/j.pss.2021.1053242 DOI |
040 | a (SwePub)uu | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Stephan, K.u German Aerosp Ctr DLR, Inst Planetary Res, D-14489 Berlin, Germany.4 aut |
245 | 1 0 | a Regions of interest on Ganymede's and Callisto's surfaces as potential targets for ESA's JUICE mission |
264 | 1 | b Elsevier,c 2021 |
338 | a print2 rdacarrier | |
520 | a The JUpiter Icy moons Explorer (JUICE) will investigate Ganymede's and Callisto's surfaces and subsurfaces from orbit to explore the geologic processes that have shaped and altered their surfaces by impact, tectonics, possible cryovolcanism, space weathering due to micrometeorites, radiation and charged particles as well as explore the structure and properties of the icy crust and liquid shell (Grasset et al., 2013). The best possible synergy of the JUICE instruments is required to answer the major science objective of this mission and to fully exploit the po-tential of the JUICE mission. Therefore, the JUICE team is aiming to define high priority targets on both Gany-mede's and Callisto's surfaces to support the coordination of the planning activities by the individual instrument teams. Based on the science objectives of the JUICE mission and the most recent knowledge of Ganymede's and Callisto's geologic evolution we propose a collection of Regions of Interest (RoIs), which characterize surface features and terrain types representing important traces of geologic processes, from past and/or present cryovolcanic and tectonic activity to space weathering processes, which are crucial to understand the geologic evolution of Ganymede and Callisto. The proposed evaluation of RoIs is based on their scientific importance as well as on the opportunities and conditions to observe them during the currently discussed mission profile. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
653 | a JUICE mission | |
653 | a Ganymede | |
653 | a Callisto | |
653 | a Surface features | |
653 | a Target regions | |
653 | a Observation planning | |
700 | 1 | a Roatsch, T.u German Aerosp Ctr DLR, Inst Planetary Res, D-14489 Berlin, Germany.4 aut |
700 | 1 | a Tosi, F.u Ist Astro Fis & Planetol Spaziali INAF IAPS, Ist Nazl AstroFis, Via Fosso Cavaliere 100, I-00133 Rome, Italy.4 aut |
700 | 1 | a Matz, K. -D4 aut |
700 | 1 | a Kersten, E.u German Aerosp Ctr DLR, Inst Planetary Res, D-14489 Berlin, Germany.4 aut |
700 | 1 | a Wagner, R.u German Aerosp Ctr DLR, Inst Planetary Res, D-14489 Berlin, Germany.4 aut |
700 | 1 | a Molyneux, P.u Southwest Res Inst, 6220 Culebra Rd, San Antonio, TX 78238 USA.4 aut |
700 | 1 | a Palumbo, P.u Ist Astro Fis & Planetol Spaziali INAF IAPS, Ist Nazl AstroFis, Via Fosso Cavaliere 100, I-00133 Rome, Italy.;Univ Napoli Parthenope, Naples, Italy.4 aut |
700 | 1 | a Poulet, F.u Univ Paris Sud, Inst Astrophys Spatiale, CNRS, Bat 121,Orsay Campus, F-91405 Orsay, France.4 aut |
700 | 1 | a Hussmann, H.u German Aerosp Ctr DLR, Inst Planetary Res, D-14489 Berlin, Germany.4 aut |
700 | 1 | a Barabash, S.u Swedish Inst Space Phys, Box 812, S-98128 Kiruna, Sweden.4 aut |
700 | 1 | a Bruzzone, L.u Univ Trento, Via Sommarive 9, I-38123 Trento, Italy.4 aut |
700 | 1 | a Dougherty, M.u Imperial Coll London, London, United Kingdom.4 aut |
700 | 1 | a Gladstone, R.u Southwest Res Inst, 6220 Culebra Rd, San Antonio, TX 78238 USA.4 aut |
700 | 1 | a Gurvits, L. I.u Joint Inst VLBI ERIC, Oude Hoogeveensedijk 4, NL-7991 PD Dwingeloo, Netherlands.;Delft Univ Technol, Dept Astrodynam & Space Missions, Kluyverweg 1, NL-2629 HS Delft, Netherlands.4 aut |
700 | 1 | a Hartogh, P.u Max Planck Inst Sonnensyst Forsch, Gottingen, Germany.4 aut |
700 | 1 | a Iess, L.u Univ Sapienza Rome, Via Eudossiana 18, I-00186 Rome, Italy.4 aut |
700 | 1 | a Wahlund, Jan-Eriku Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)janewahl |
700 | 1 | a Wurz, P.u Univ Bern, Phys Inst, Weltraum & Planetol, Sidlerstr 5, CH-3012 Bern, Switzerland.4 aut |
700 | 1 | a Witasse, O.u European Space Agcy, European Space Res & Technol Ctr ESTEC, NL-2200 AG Noordwijk, Netherlands.4 aut |
700 | 1 | a Grasset, O.u Univ Nantes, Lab Planetol & Geodynam, UMR CNRS 6112, BP 92208, F-44322 Nantes 3, France.4 aut |
700 | 1 | a Altobelli, N.4 aut |
700 | 1 | a Carter, J.u Southwest Res Inst, 6220 Culebra Rd, San Antonio, TX 78238 USA.4 aut |
700 | 1 | a Cavalie, T.u Univ Bordeaux, Lab Astrophys Bordeaux, CNRS, B18N, Allee Georoy St Hilaire, F-33615 Pessac, France.;Univ Paris, UPMC Univ Paris 06, Sorbonne Univ, PSL Res Univ,CNRS,Observ Paris,LESIA,Sorbonne Par, Meudon, Paris, France.4 aut |
700 | 1 | a d'Aversa, E.u Ist Astro Fis & Planetol Spaziali INAF IAPS, Ist Nazl AstroFis, Via Fosso Cavaliere 100, I-00133 Rome, Italy.4 aut |
700 | 1 | a Della Corte, V.u Ist Astro Fis & Planetol Spaziali INAF IAPS, Ist Nazl AstroFis, Via Fosso Cavaliere 100, I-00133 Rome, Italy.4 aut |
700 | 1 | a Filacchione, G.u Ist Astro Fis & Planetol Spaziali INAF IAPS, Ist Nazl AstroFis, Via Fosso Cavaliere 100, I-00133 Rome, Italy.4 aut |
700 | 1 | a Galli, A.u Univ Bern, Phys Inst, Weltraum & Planetol, Sidlerstr 5, CH-3012 Bern, Switzerland.4 aut |
700 | 1 | a Galluzzi, V.u Ist Astro Fis & Planetol Spaziali INAF IAPS, Ist Nazl AstroFis, Via Fosso Cavaliere 100, I-00133 Rome, Italy.4 aut |
700 | 1 | a Gwinner, K.u German Aerosp Ctr DLR, Inst Planetary Res, D-14489 Berlin, Germany.4 aut |
700 | 1 | a Hauber, E.u German Aerosp Ctr DLR, Inst Planetary Res, D-14489 Berlin, Germany.4 aut |
700 | 1 | a Jaumann, R.u Free Univ Berlin, Planetary Sci & Remote Sensing, Malteserstr 74-100, D-12249 Berlin, Germany.4 aut |
700 | 1 | a Krohn, K.u German Aerosp Ctr DLR, Inst Planetary Res, D-14489 Berlin, Germany.4 aut |
700 | 1 | a Langevin, Y.u Univ Paris Sud, Inst Astrophys Spatiale, CNRS, Bat 121,Orsay Campus, F-91405 Orsay, France.4 aut |
700 | 1 | a Lucchetti, A.u INAF Osservatorio Astron Padova, Vicolo Osserv 5, I-35122 Padua, Italy.4 aut |
700 | 1 | a Migliorini, A.u Ist Astro Fis & Planetol Spaziali INAF IAPS, Ist Nazl AstroFis, Via Fosso Cavaliere 100, I-00133 Rome, Italy.4 aut |
700 | 1 | a Piccioni, G.u Ist Astro Fis & Planetol Spaziali INAF IAPS, Ist Nazl AstroFis, Via Fosso Cavaliere 100, I-00133 Rome, Italy.4 aut |
700 | 1 | a Solomonidou, A.u CALTECH, Pasadena, CA 91125 USA.4 aut |
700 | 1 | a Stark, A.u German Aerosp Ctr DLR, Inst Planetary Res, D-14489 Berlin, Germany.4 aut |
700 | 1 | a Tobie, G.4 aut |
700 | 1 | a Tubiana, C.u Ist Astro Fis & Planetol Spaziali INAF IAPS, Ist Nazl AstroFis, Via Fosso Cavaliere 100, I-00133 Rome, Italy.4 aut |
700 | 1 | a Vallat, C.u RHEA Grp ESA ESAC, 28 Villanueva Canada, Madrid 28692, Spain.4 aut |
700 | 1 | a Van Hoolst, T.u Royal Observ Belgium, Brussels, Belgium.;Katholieke Univ Leuven, Inst Sterrenkunde, Leuven, Belgium.4 aut |
710 | 2 | a German Aerosp Ctr DLR, Inst Planetary Res, D-14489 Berlin, Germany.b Ist Astro Fis & Planetol Spaziali INAF IAPS, Ist Nazl AstroFis, Via Fosso Cavaliere 100, I-00133 Rome, Italy.4 org |
773 | 0 | t Planetary and Space Scienced : Elsevierg 208q 208x 0032-0633x 1873-5088 |
856 | 4 | u https://doi.org/10.1016/j.pss.2021.105324y Fulltext |
856 | 4 | u https://doi.org/10.1016/j.pss.2021.105324 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-458293 |
856 | 4 8 | u https://doi.org/10.1016/j.pss.2021.105324 |
Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.
Copy and save the link in order to return to this view