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Sökning: onr:"swepub:oai:DiVA.org:uu-376697" > Investigating the p...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00008808naa a2200889 4500
001oai:DiVA.org:uu-376697
003SwePub
008190213s2017 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-3766972 URI
024a https://doi.org/10.1093/mnras/stx27682 DOI
040 a (SwePub)uu
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Lin, Zhong-Yiu Natl Cent Univ, Inst Astron, Chungli 32054, Taiwan4 aut
2451 0a Investigating the physical properties of outbursts on comet 67P/Churyumov-Gerasimenko
264 c 2017-12-04
264 1b OXFORD UNIV PRESS,c 2017
338 a print2 rdacarrier
520 a Cometary outbursts on several comets have been observed both by ground-based telescopes and by in situ instruments on spacecraft. However, the mechanism behind these phenomena and their physical properties are still unclear. The optical, spectrocopic and infrared remote imaging system (OSIRIS) onboard the Rosetta spacecraft provided first-hand information on the outbursts from comet 67P/Churyumov-Gerasimenko during its perihelion passage in 2015. The physical properties of the outbursts can be investigated by examining the time series of these high-resolution images. An analysis is made of the wide- and narrow-angle images obtained during the monitoring of the outburst sequences, which occurred between July and September in 2015. A ring-masking technique is used to calculate the excess brightness of the outbursts. The ejected mass and expansion velocity of the outbursts is estimated from differences in images made with the same filter (orange filter). The calculated excess brightness from these outburst plumes ranges from a few per cent to 28 per cent. In some major outbursts, the brightness contribution from the outburst plume can be one or two times higher than that of the typical coma jet activities. The strongest event was the perihelion outburst detected just a few hours before perihelion. The mass ejection rate during a generic outburst could reach a few per cent of the steady-state value of the dust coma. Transient events are detected by studying the brightness slope of the outburst plume with continuous streams of outflowing gas and dust triggered by driving mechanisms, as yet not understood, which remain active for several minutes to less than a few hours.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
653 a comets: individual: 67P/Churyumov-Gerasimenko
700a Knollenberg, J.u Inst Planetenforsch, Deuisch Zentrum Luft & Raumfahri DLR, Rutherfordstr 2, D-12489 Berlin, Germany4 aut
700a Vincent, J. -B4 aut
700a A'Hearn, M. F.u Univ Maryland, Dept Astron, College Pk, MD 20742 USA4 aut
700a Ip, W-H4 aut
700a Sierks, H.u Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany4 aut
700a Barbieri, C.u Univ Padua, Dept Phys & Astron G Galilei, Vic Osservatorio 3, I-35122 Padua, Italy;Univ Padua, Ctr Ateneo Studi & Attivita Spaziali Giuseppe Col, Via Venezia 15, I-35131 Padua, Italy4 aut
700a Lamy, P. L.u CNRS, Lab Astrophys Marseille, UMR 7326, 38 Rue Frederic Joliot Curie, F-13388 Marseille, France;Aix Marseille Univ, 38 Rue Frederic Joliot Curie, F-13388 Marseille, France4 aut
700a Rodrigo, R.u CSIC, INTA, Ctr Astrobiol, ESA,ESAC, POB 78,E 8691, Madrid, Spain;Int Space Sci Inst, Hallerstr 6, CH-3012 Bern, Switzerland4 aut
700a Koschny, D.u Univ Maryland, Dept Astron, College Pk, MD 20742 USA;European Space Agcy, Res & Sci Support Dept, NL-2201 Noordwijk, Netherlands4 aut
700a Rickman, H.u PAS Space Res Ctr, Bartycka 18A, PL-00716 Warsaw, Poland4 aut
700a Keller, H. U.u Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterr Phys IGEP, D-38106 Braunschweig, Germany4 aut
700a Mottola, S.u Inst Planetenforsch, Deuisch Zentrum Luft & Raumfahri DLR, Rutherfordstr 2, D-12489 Berlin, Germany4 aut
700a Bodewits, D.4 aut
700a Agarwal, J.u Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany4 aut
700a Barucci, M. A.u Univ Paris Diderot, LESIA Observ Paris, CNRS, UPMC Univ Paris 06, 5 Pl J Janssen, F-92195 Meudon, France4 aut
700a Bertaux, J. -L4 aut
700a Bertini, I.u Univ Padua, Dept Phys & Astron G Galilei, Vic Osservatorio 3, I-35122 Padua, Italy4 aut
700a Cremonese, G.u INAF, Osservatorio Astron Padova, Vic Osservatorio 5, I-35122 Padua, Italy4 aut
700a Deller, J.u Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany4 aut
700a Da Deppo, V.u CNR IFN UOS Padova LUXOR, Via Trasea 7, I-35131 Padua, Italy4 aut
700a Davidsson, Björnu Uppsala universitet,Teoretisk astrofysik4 aut0 (Swepub:uu)bjoda312
700a Debei, S.u Univ Padua, Dept Ind Engn, Via Venezia 1, I-35131 Padua, Italy4 aut
700a De Cecco, M.u Univ Trento, Via Sommarive 9, I-38123 Trento, Italy4 aut
700a Fornasier, S.u Univ Paris Diderot, LESIA Observ Paris, CNRS, UPMC Univ Paris 06, 5 Pl J Janssen, F-92195 Meudon, France4 aut
700a Fulle, M.u INAF, Osservatorio Astron Trieste, Via Tiepolo 11, I-34143 Trieste, Italy4 aut
700a Groussin, O.u CNRS, Lab Astrophys Marseille, UMR 7326, 38 Rue Frederic Joliot Curie, F-13388 Marseille, France;Aix Marseille Univ, 38 Rue Frederic Joliot Curie, F-13388 Marseille, France4 aut
700a Gutierrez, P. J.u CSIC, Inst Astrofis Andalucia, C Glorieta Astron, E-18008 Granada, Spain4 aut
700a Guettler, C.u Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany4 aut
700a Hofmann, M.u Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany4 aut
700a Hviid, S. F.u Inst Planetenforsch, Deuisch Zentrum Luft & Raumfahri DLR, Rutherfordstr 2, D-12489 Berlin, Germany4 aut
700a Jorda, L.u CNRS, Lab Astrophys Marseille, UMR 7326, 38 Rue Frederic Joliot Curie, F-13388 Marseille, France;Aix Marseille Univ, 38 Rue Frederic Joliot Curie, F-13388 Marseille, France4 aut
700a Kovacs, G.u Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany4 aut
700a Kramm, J. -R4 aut
700a Kuehrt, E.u Inst Planetenforsch, Deuisch Zentrum Luft & Raumfahri DLR, Rutherfordstr 2, D-12489 Berlin, Germany4 aut
700a Kuppers, M.u CSIC, INTA, Ctr Astrobiol, ESA,ESAC, POB 78,E 8691, Madrid, Spain4 aut
700a Lai, I. -L4 aut
700a Lara, L. M.u CSIC, Inst Astrofis Andalucia, C Glorieta Astron, E-18008 Granada, Spain4 aut
700a Lazzarin, M.u Univ Padua, Ctr Ateneo Studi & Attivita Spaziali Giuseppe Col, Via Venezia 15, I-35131 Padua, Italy4 aut
700a Lee, J-C4 aut
700a Lopez-Moreno, J. J.u CSIC, Inst Astrofis Andalucia, C Glorieta Astron, E-18008 Granada, Spain4 aut
700a Marzari, F.u Univ Padua, Dept Phys & Astron G Galilei, Vic Osservatorio 3, I-35122 Padua, Italy4 aut
700a Naletto, G.u Univ Padua, Dept Informat Engn, Via Gradenigo 6-B, I-35131 Padua, Italy4 aut
700a Oklay, N.u Inst Planetenforsch, Deuisch Zentrum Luft & Raumfahri DLR, Rutherfordstr 2, D-12489 Berlin, Germany;Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany4 aut
700a Ott, T.u Carl von Ossietzky Univ Oldenburg, Ammerlander Heerstr 114, D-26111 Oldenburg, Germany4 aut
700a Drolshagen, E.u Carl von Ossietzky Univ Oldenburg, Ammerlander Heerstr 114, D-26111 Oldenburg, Germany4 aut
700a Shi, X.u Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany4 aut
700a Thomas, N.u Univ Bern, Phys Inst, Sidlerstr 5, CH-3012 Bern, Switzerland4 aut
700a Tubiana, C.u Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany4 aut
710a Natl Cent Univ, Inst Astron, Chungli 32054, Taiwanb Inst Planetenforsch, Deuisch Zentrum Luft & Raumfahri DLR, Rutherfordstr 2, D-12489 Berlin, Germany4 org
773t Monthly notices of the Royal Astronomical Societyd : OXFORD UNIV PRESSg 469, s. S731-S740q 469<S731-S740x 0035-8711x 1365-2966
856u https://academic.oup.com/mnras/article-pdf/469/Suppl_2/S731/22218333/stx2768.pdf
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-376697
8564 8u https://doi.org/10.1093/mnras/stx2768

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