id:"swepub:oai:DiVA.org:ltu-10492"
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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 05021naa a2200601 4500 | |
| 001 | oai:DiVA.org:ltu-10492 | |
| 003 | SwePub | |
| 008 | 160929s2014 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-104922 URI |
| 024 | 7 | a https://doi.org/10.1002/2013JE0045142 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 Harri, A.-M.u Finnish Meteorological Institute, Helsinki, Finland4 aut |
| 245 | 1 0 | a Mars Science Laboratory relative humidity observations: Initial results |
| 264 | 1 | c 2014 |
| 338 | a print2 rdacarrier | |
| 500 | a Upprättat; 2014; 20150813 (ninhul) | |
| 520 | a The Mars Science Laboratory (MSL) made a successful landing at Gale crater early August 2012. MSL has an environmental instrument package called the Rover Environmental Monitoring Station (REMS) as a part of its scientific payload. REMS comprises instrumentation for the observation of atmospheric pressure, temperature of the air, ground temperature, wind speed and direction, relative humidity (REMS-H), and UV measurements. We concentrate on describing the REMS-H measurement performance and initial observations during the first 100 MSL sols as well as constraining the REMS-H results by comparing them with earlier observations and modeling results. The REMS-H device is based on polymeric capacitive humidity sensors developed by Vaisala Inc., and it makes use of transducer electronics section placed in the vicinity of the three humidity sensor heads. The humidity device is mounted on the REMS boom providing ventilation with the ambient atmosphere through a filter protecting the device from airborne dust. The final relative humidity results appear to be convincing and are aligned with earlier indirect observations of the total atmospheric precipitable water content. The water mixing ratio in the atmospheric surface layer appears to vary between 30 and 75 ppm. When assuming uniform mixing, the precipitable water content of the atmosphere is ranging from a few to six precipitable micrometers. | |
| 650 | 7 | a TEKNIK OCH TEKNOLOGIERx Maskinteknikx Rymd- och flygteknik0 (SwePub)203022 hsv//swe |
| 650 | 7 | a ENGINEERING AND TECHNOLOGYx Mechanical Engineeringx Aerospace Engineering0 (SwePub)203022 hsv//eng |
| 700 | 1 | a Genzer, M.u Finnish Meteorological Institute, Helsinki, Finland4 aut |
| 700 | 1 | a Kemppinen, O.u Finnish Meteorological Institute, Helsinki, Finland4 aut |
| 700 | 1 | a Gomez-Elvira, J.u Centro de Astrobiologia, Madrid, Spain4 aut |
| 700 | 1 | a Haberle, R.u NASA AMES Research Center, San Francisco, California, USA4 aut |
| 700 | 1 | a Polkko, J.u Finnish Meteorological Institute, Helsinki, Finland4 aut |
| 700 | 1 | a Savijärvi, H.u Finnish Meteorological Institute, Helsinki, Finland4 aut |
| 700 | 1 | a Rennó, N.u Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, Michigan, USA4 aut |
| 700 | 1 | a Rodriguez-Manfredi, J. A.u Centro de Astrobiologia, Madrid, Spain4 aut |
| 700 | 1 | a Schmidt, W.u Finnish Meteorological Institute, Helsinki, Finland4 aut |
| 700 | 1 | a Richardson, M.u Ashima Research Inc., Pasadena, California, USA4 aut |
| 700 | 1 | a Siili, T.u Finnish Meteorological Institute, Helsinki, Finland4 aut |
| 700 | 1 | a Paton, M.u Finnish Meteorological Institute, Helsinki, Finland4 aut |
| 700 | 1 | a De La Torre-Juarez, M.u NASA Jet Propulsion Laboratory, Pasadena, California, USA4 aut |
| 700 | 1 | a Mäkinen, T.u Finnish Meteorological Institute, Helsinki, Finland4 aut |
| 700 | 1 | a Newman, C.u Ashima Research Inc., Pasadena, California, USA4 aut |
| 700 | 1 | a Rafkin, S.u Southwest Research Institute, Boulder, Colorado, USA4 aut |
| 700 | 1 | a Mischna, M.u NASA Jet Propulsion Laboratory, Pasadena, California, USA4 aut |
| 700 | 1 | a Merikallio, S.u Finnish Meteorological Institute, Helsinki, Finland4 aut |
| 700 | 1 | a Haukka, H.u Finnish Meteorological Institute, Helsinki, Finland4 aut |
| 700 | 1 | a Martin-Torres, Javieru Centro de Astrobiologia, Madrid, Spain4 aut0 (Swepub:ltu)javmar |
| 700 | 1 | a Komu, M.u Finnish Meteorological Institute, Helsinki, Finland4 aut |
| 700 | 1 | a Zorzano, María-Pazu Centro de Astrobiologia, Madrid, Spain4 aut0 (Swepub:ltu)marzor |
| 700 | 1 | a Peinado, V.u Centro de Astrobiologia, Madrid, Spain4 aut |
| 700 | 1 | a Vazquez, L.u Department of Applied Mathematics, Complutense University of Madrid, Madrid, Spain4 aut |
| 700 | 1 | a Urqui, R.u Centro de Astrobiologia, Madrid, Spain4 aut |
| 710 | 2 | a Finnish Meteorological Institute, Helsinki, Finlandb Centro de Astrobiologia, Madrid, Spain4 org |
| 773 | 0 | t Journal of Geophysical Research - Planetsg 119:9, s. 2132-2147q 119:9<2132-2147x 2169-9097x 2169-9100 |
| 856 | 4 | u https://doi.org/10.1002/2013JE004514y Fulltext |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-10492 |
| 856 | 4 8 | u https://doi.org/10.1002/2013JE004514 |
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- Harri, A.-M.
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