WFRF:(Tiefenbacher C.)
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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 07196naa a2200697 4500 | |
| 001 | oai:DiVA.org:ltu-92498 | |
| 003 | SwePub | |
| 008 | 220816s2022 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-924982 URI |
| 024 | 7 | a https://doi.org/10.1093/mnras/stac17342 DOI |
| 040 | a (SwePub)ltu | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Lethuillier, A.u Institut für Geophysik und extraterrestrische Physik (IGeP), TU Braunschweig, Mendelssohnstr. 3, D-38106 Braunschweig, Germany4 aut |
| 245 | 1 0 | a Cometary dust analogues for physics experiments |
| 264 | c 2022-06-25 | |
| 264 | 1 | b Oxford University Press,c 2022 |
| 338 | a print2 rdacarrier | |
| 500 | a Validerad;2022;Nivå 2;2022-08-19 (hanlid);Funder: D-A-CH programme (DFG: GU 1620/3-1and BL 298/26-1 / SNF: 200021E 177964 / FWF: I 3730-N36); SwissNational National Science Foundation | |
| 520 | a The CoPhyLab (Cometary Physics Laboratory) project is designed to study the physics of comets through a series of earth-based experiments. For these experiments, a dust analogue was created with physical properties comparable to those of the non-volatile dust found on comets. This ‘CoPhyLab dust’ is planned to be mixed with water and CO2 ice and placed under cometary conditions in vacuum chambers to study the physical processes taking place on the nuclei of comets. In order to develop this dust analogue, we mixed two components representative for the non-volatile materials present in cometary nuclei. We chose silica dust as a representative for the mineral phase and charcoal for the organic phase, which also acts as a darkening agent. In this paper, we provide an overview of known cometary analogues before presenting measurements of eight physical properties of different mixtures of the two materials and a comparison of these measurements with known cometary values. The physical properties of interest are particle size, density, gas permeability, spectrophotometry, and mechanical, thermal, and electrical properties. We found that the analogue dust that matches the highest number of physical properties of cometary materials consists of a mixture of either 60 per cent/40 per cent or 70 per cent/30 per cent of silica dust/charcoal by mass. These best-fit dust analogue will be used in future CoPhyLab experiments. | |
| 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 methods: laboratory: solid state | |
| 653 | a techniques: miscellaneous | |
| 653 | a comets: general | |
| 653 | a comets: individual: 67P/Churyumov-Gerasimenko | |
| 653 | a Atmospheric science | |
| 653 | a Atmosfärsvetenskap | |
| 700 | 1 | a Feller, C.u Physikalisches Institut, Universität Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland4 aut |
| 700 | 1 | a Kaufmann, Erikau Luleå tekniska universitet,Rymdteknik,Space Research Institute, Austrian Academy of Science, Schmiedlstraße 6, A-8042 Graz, Austria4 aut0 (Swepub:ltu)erikau |
| 700 | 1 | a Becerra, P.u Physikalisches Institut, Universität Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland4 aut |
| 700 | 1 | a Hänni, N.u Physikalisches Institut, Universität Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland4 aut |
| 700 | 1 | a Diethelm, R.u Institut für Geophysik und extraterrestrische Physik (IGeP), TU Braunschweig, Mendelssohnstr. 3, D-38106 Braunschweig, Germany4 aut |
| 700 | 1 | a Kreuzig, C.u Institut für Geophysik und extraterrestrische Physik (IGeP), TU Braunschweig, Mendelssohnstr. 3, D-38106 Braunschweig, Germany4 aut |
| 700 | 1 | a Gundlach, B.u Institut für Geophysik und extraterrestrische Physik (IGeP), TU Braunschweig, Mendelssohnstr. 3, D-38106 Braunschweig, Germany4 aut |
| 700 | 1 | a Blum, J.u Institut für Geophysik und extraterrestrische Physik (IGeP), TU Braunschweig, Mendelssohnstr. 3, D-38106 Braunschweig, Germany4 aut |
| 700 | 1 | a Pommerol, A.u Physikalisches Institut, Universität Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland4 aut |
| 700 | 1 | a Kargl, G.u Space Research Institute, Austrian Academy of Science, Schmiedlstraße 6, A-8042 Graz, Austria4 aut |
| 700 | 1 | a Laddha, S.u Space Research Institute, Austrian Academy of Science, Schmiedlstraße 6, A-8042 Graz, Austria4 aut |
| 700 | 1 | a Denisova, K.u Institut für Physik der Kondensierten Materie (IPKM), TU Braunschweig, Mendelssohnstr. 3, D-38106 Braunschweig, Germany4 aut |
| 700 | 1 | a Kührt, E.u Deutsches Zentrum für Luft- und Raumfahrt, Rutherfordstraße 2, D-12489 Berlin-Adlershof, Germany4 aut |
| 700 | 1 | a Capelo, H. L.u Physikalisches Institut, Universität Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland4 aut |
| 700 | 1 | a Haack, D.u Deutsches Zentrum für Luft- und Raumfahrt, Rutherfordstraße 2, D-12489 Berlin-Adlershof, Germany4 aut |
| 700 | 1 | a Zhang, X.u Qian Xuesen Laboratory of Space Technology, China Academy of Space Technology, Beijing 100094, China4 aut |
| 700 | 1 | a Knollenberg, J.u Deutsches Zentrum für Luft- und Raumfahrt, Rutherfordstraße 2, D-12489 Berlin-Adlershof, Germany4 aut |
| 700 | 1 | a Molinski, N. S.u Institut für Geophysik und extraterrestrische Physik (IGeP), TU Braunschweig, Mendelssohnstr. 3, D-38106 Braunschweig, Germany4 aut |
| 700 | 1 | a Gilke, T.u Institut für Geophysik und extraterrestrische Physik (IGeP), TU Braunschweig, Mendelssohnstr. 3, D-38106 Braunschweig, Germany4 aut |
| 700 | 1 | a Sierks, H.u Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, D-37077 Gottingen, ¨ Germany4 aut |
| 700 | 1 | a Tiefenbacher, P.u Space Research Institute, Austrian Academy of Science, Schmiedlstraße 6, A-8042 Graz, Austria4 aut |
| 700 | 1 | a Güttler, C.u Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, D-37077 Gottingen, ¨ Germany4 aut |
| 700 | 1 | a Otto, K. A.u Deutsches Zentrum für Luft- und Raumfahrt, Rutherfordstraße 2, D-12489 Berlin-Adlershof, Germany4 aut |
| 700 | 1 | a Bischoff, D.u Institut für Geophysik und extraterrestrische Physik (IGeP), TU Braunschweig, Mendelssohnstr. 3, D-38106 Braunschweig, Germany4 aut |
| 700 | 1 | a Schweighart, M.u Space Research Institute, Austrian Academy of Science, Schmiedlstraße 6, A-8042 Graz, Austria4 aut |
| 700 | 1 | a Hagermann, Axelu Luleå tekniska universitet,Rymdteknik4 aut0 (Swepub:ltu)axehag |
| 700 | 1 | a Jäggi, N.u Physikalisches Institut, Universität Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland4 aut |
| 710 | 2 | a Institut für Geophysik und extraterrestrische Physik (IGeP), TU Braunschweig, Mendelssohnstr. 3, D-38106 Braunschweig, Germanyb Physikalisches Institut, Universität Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland4 org |
| 773 | 0 | t Monthly notices of the Royal Astronomical Societyd : Oxford University Pressg 515:3, s. 3420-3438q 515:3<3420-3438x 0035-8711x 1365-2966 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-92498 |
| 856 | 4 8 | u https://doi.org/10.1093/mnras/stac1734 |
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- Lethuillier, A.
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- Kreuzig, C.
- Gundlach, B.
- Blum, J.
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- Kührt, E.
- Capelo, H. L.
- Haack, D.
- Zhang, X.
- Knollenberg, J.
- Molinski, N. S.
- Gilke, T.
- Sierks, H.
- Tiefenbacher, P.
- Güttler, C.
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- Bischoff, D.
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