Sökning: WFRF:(Andrews David. J.) > Interplanetary coro...
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000 | 07584naa a2200973 4500 | |
001 | oai:DiVA.org:uu-336648 | |
003 | SwePub | |
008 | 171215s2017 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-3366482 URI |
024 | 7 | a https://doi.org/10.1002/2017JA0238842 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 Witasse, O.u European Space Agcy, ESTEC4 aut |
245 | 1 0 | a Interplanetary coronal mass ejection observed at STEREO-A, Mars, comet 67P/Churyumov-Gerasimenko, Saturn, and New Horizons en route to Pluto :b Comparison of its Forbush decreases at 1.4, 3.1, and 9.9 AU |
264 | 1 | c 2017 |
338 | a electronic2 rdacarrier | |
520 | a We discuss observations of the journey throughout the Solar System of a large interplanetary coronal mass ejection (ICME) that was ejected at the Sun on 14 October 2014. The ICME hit Mars on 17 October, as observed by the Mars Express, Mars Atmosphere and Volatile EvolutioN Mission (MAVEN), Mars Odyssey, and Mars Science Laboratory (MSL) missions, 44h before the encounter of the planet with the Siding-Spring comet, for which the space weather context is provided. It reached comet 67P/Churyumov-Gerasimenko, which was perfectly aligned with the Sun and Mars at 3.1 AU, as observed by Rosetta on 22 October. The ICME was also detected by STEREO-A on 16 October at 1 AU, and by Cassini in the solar wind around Saturn on the 12 November at 9.9AU. Fortuitously, the New Horizons spacecraft was also aligned with the direction of the ICME at 31.6 AU. We investigate whether this ICME has a nonambiguous signature at New Horizons. A potential detection of this ICME by Voyager 2 at 110-111 AU is also discussed. The multispacecraft observations allow the derivation of certain properties of the ICME, such as its large angular extension of at least 116 degrees, its speed as a function of distance, and its magnetic field structure at four locations from 1 to 10 AU. Observations of the speed data allow two different solar wind propagation models to be validated. Finally, we compare the Forbush decreases (transient decreases followed by gradual recoveries in the galactic cosmic ray intensity) due to the passage of this ICME at Mars, comet 67P, and Saturn. | |
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 interplanetary coronal mass ejection | |
653 | a Forbush decrease | |
653 | a Mars | |
653 | a comet 67P | |
653 | a Saturn | |
653 | a New Horizons | |
700 | 1 | a Sanchez-Cano, B.u Univ Leicester, Dept Phys & Astron, Radio & Space Plasma Phys Grp4 aut |
700 | 1 | a Mays, M. L.u NASA Goddard Space Flight Ctr, Heliophys Sci Div4 aut |
700 | 1 | a Kajdic, P.u Univ Nacl Autonoma Mexico, Inst Geofis4 aut |
700 | 1 | a Opgenoorth, Hermannu Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)heropgen |
700 | 1 | a Elliott, H. A.u Southwest Res Inst, San Antonio4 aut |
700 | 1 | a Richardson, I. G.u NASA Goddard Space Flight Ctr, Heliophys Sci Div.;Univ Maryland, Dept Astron4 aut |
700 | 1 | a Zouganelis, I.u European Space Agcy, ESAC, Villanueva De La Canada4 aut |
700 | 1 | a Zender, J.u European Space Agcy, ESTEC4 aut |
700 | 1 | a Wimmer-Schweingruber, R. F.u Univ Kiel, Inst Expt & Appl Phys4 aut |
700 | 1 | a Turc, L.u European Space Agcy, ESTEC4 aut |
700 | 1 | a Taylor, M. G. G. T.u European Space Agcy, ESTEC4 aut |
700 | 1 | a Roussos, E.u Max Planck Inst Solar Syst Res Justus von Liebig4 aut |
700 | 1 | a Rouillard, A.u IRAP, Toulouse4 aut |
700 | 1 | a Richter, I.u Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterrestrial Phys4 aut |
700 | 1 | a Richardson, J. D.u MIT, Ctr Space Res, Cambridge4 aut |
700 | 1 | a Ramstad, R.u Swedish Inst Space Phys, IRF, Kiruna4 aut |
700 | 1 | a Provan, G.u Univ Leicester, Dept Phys & Astron, Radio & Space Plasma Phys Grp4 aut |
700 | 1 | a Posner, A.u NASA Headquarters, Sci Miss Directorate4 aut |
700 | 1 | a Plaut, J. J.u Jet Prop Lab, Pasadena4 aut |
700 | 1 | a Odstrcil, D.u George Mason Univ, Dept Phys & Astron.;NASA Goddard Space Flight Ctr, Space Weather Lab4 aut |
700 | 1 | a Nilsson, H.u Swedish Inst Space Phys, IRF, Kiruna4 aut |
700 | 1 | a Niemenen, P.u European Space Agcy, ESTEC4 aut |
700 | 1 | a Milan, S. E.u Univ Leicester, Dept Phys & Astron, Radio & Space Plasma Phys Grp4 aut |
700 | 1 | a Mandt, K.u Southwest Res Inst, San Antonio.; UTSA, Dept Phys & Astron, San Antonio4 aut |
700 | 1 | a Lohf, H.u Univ Kiel, Inst Expt & Appl Phys4 aut |
700 | 1 | a Lester, M.u Univ Leicester, Dept Phys & Astron, Radio & Space Plasma Phys Grp4 aut |
700 | 1 | a Lebreton, J. -Pu Univ Orleans, CNRS, LPC2E4 aut |
700 | 1 | a Kuulkers, E.u European Space Agcy, ESTEC4 aut |
700 | 1 | a Krupp, N.u Max Planck Inst Solar Syst Res Justus von Liebig4 aut |
700 | 1 | a Koenders, C.u Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterrestrial Phys4 aut |
700 | 1 | a James, M. K.u Univ Leicester, Dept Phys & Astron, Radio & Space Plasma Phys Grp4 aut |
700 | 1 | a Intzekara, D.u European Space Agcy, ESTEC.; European Space Agcy, ESAC, Villanueva De La Canada4 aut |
700 | 1 | a Holmstrom, M.u Swedish Inst Space Phys, IRF, Kiruna4 aut |
700 | 1 | a Hassler, D. M.u Southwest Res Inst, Boulder.; Inst Astrophys Spatiale, Orsay4 aut |
700 | 1 | a Hall, B. E. S.u Univ Leicester, Dept Phys & Astron, Radio & Space Plasma Phys Grp4 aut |
700 | 1 | a Guo, J.u Univ Kiel, Inst Expt & Appl Phys4 aut |
700 | 1 | a Goldstein, R.u Southwest Res Inst, San Antonio4 aut |
700 | 1 | a Goetz, C.u Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterrestrial Phys4 aut |
700 | 1 | a Glassmeier, K. H.u Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterrestrial Phys4 aut |
700 | 1 | a Genot, V.u IRAP, Toulouse4 aut |
700 | 1 | a Evans, H.u European Space Agcy, ESTEC4 aut |
700 | 1 | a Espley, J.u Goddard Space Flight Ctr, Lab Planetary Magnetospheres, Greenbelt4 aut |
700 | 1 | a Edberg, N. J. T.u Swedish Inst Space Phys, IRF, Uppsala, Sweden.4 aut |
700 | 1 | a Edberg, Niklas J. T.u Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)niked861 |
700 | 1 | a Cowley, S. W. H.u Univ Leicester, Dept Phys & Astron, Radio & Space Plasma Phys Grp4 aut |
700 | 1 | a Burch, J.u Southwest Res Inst, San Antonio4 aut |
700 | 1 | a Behar, E.u Swedish Inst Space Phys, IRF, Kiruna4 aut |
700 | 1 | a Barabash, S.u Swedish Inst Space Phys, IRF, Kiruna4 aut |
700 | 1 | a Andrews, David J.u Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)davan153 |
700 | 1 | a Altobelli, N.u European Space Agcy, ESAC, Villanueva De La Canada4 aut |
710 | 2 | a European Space Agcy, ESTECb Univ Leicester, Dept Phys & Astron, Radio & Space Plasma Phys Grp4 org |
773 | 0 | t Journal of Geophysical Research - Space Physicsg 122:8, s. 7865-7890q 122:8<7865-7890x 2169-9380x 2169-9402 |
856 | 4 | u https://doi.org/10.1002/2017JA023884y Fulltext |
856 | 4 | u https://uu.diva-portal.org/smash/get/diva2:1166639/FULLTEXT01.pdfx primaryx Raw objecty fulltext:print |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-336648 |
856 | 4 8 | u https://doi.org/10.1002/2017JA023884 |
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