Results 71 to 80 of about 320,975 (184)
Gas outflow and dust transport of comet 67P/Churyumov–Gerasimenko [PDF]
, 2016 International audienceBecause of the diurnal thermal cycle and the irregular shape of the nucleus, gas outflow of comet 67P/Churyumov–Gerasimenko could be highly anisotropic as indicated by the colliminated dust jet structures on the sunlit side.Jui-Chi Lee, Ian-Lin Lai, Gabor Kovacs, Davidsson, Björn, Ekkehard Kührt, Thomas, Nicolas, Xian Shi, Marzari, Francesco,, Lai, Ian-Lin,, Debei, Stefano, Knollenberg, J. Org, Francesco Marzari, Gabriele Cremonese, Shi, Xian, Steven Boudreault, Naletto, Giampiero, Philippe Lamy, Ip, Wing-Huen, Boudreault, Steven, Wu, Jong-Shinn, Bertini, Ivano, Tubiana, Cecilia, Rafael Rodrigo, Jorda, Laurent,, Zhong-Yi Lin, Horst Uwe Keller, Hofman, Marc, Bertaux, Jean-Loup,, Knollenberg, Jörg, Lin, Zhong-Yi,, Guttler, Carsten,, Keller, Horst Uwe, Küppers, Michael, Luisa M. Lara, Knollenberg, Jörg, De Cecco, Mariolino,, Ivano Bertini, Hofmann, Marc,, Vania Da Deppo, Josè J. Lopez Moreno, Kuhrt, Ekkehard,, Kovacs, Gabor, Lopez Moreno, Josè J., Boudreault, Steven,, Michael F. A’Hearn, Lazzarin, Monica,, Wu, Jong-Shinn,, Gutiérrez, Pedro J., Shi, Jong-Shinn, Björn Davidsson, Liao, Ying,, Moreno, Jose J. Lopez, Su, Cheng-Chin, Sierks, Holger, Stefano Debei, Sonia Fornasier, da Deppo, Vania, Wing-Huen Ip, Koschny, Detlef,, Hviid, Stubbe F., Cheng-Chin Su, Vincent, Jean-Baptiste, Agarwal, Jessica,, Oklay, Nilda, Cremonese, Gabriele,, Ip, Wing-Huen,, Lara, Luisa M.,, Cesare Barbieri, Olivier Groussin, Lara López, Luisa M., Fulle, Marco, A'Hearn, Michael F., Jorda, Laurent, Barbieri, Cesare, Lara, Luisa M., Moreno, Josà J. Lopez, Gutierrez, Pedro J.,, A’Hearn, Michael F., Marco Fulle, Jörg Knollenberg, Kramm, J.-Rainer, Bertaux, Jean-Loup, Pedro J. Gutiérrez, GÃ1⁄4ttler, Carsten, Koschny, Detlef, Michael Küppers, Groussin, Olivier, Naletto, Giampiero,, Rickman, Hans, Thomas, Nicolas,, KÃ1⁄4ppers, Michael, Lamy, Philippe,, Vincent, Jean-Baptiste,, Debei, Stefano,, Detlef Koschny, Keller, Horst Uwe,, Fornasier, Sonia,, Marzari, Francesco, Lin, Zhong-Yi, Fulle, Marc, Laurent Jorda, Rickman, Hans,, Rodrigo, Rafael,, KÃ1⁄4hrt, Ekkehard, Fulle, Marco,, Sierks, Holger,, Maria Antonella Barucci, Liao, Ying, Jean-Baptiste Vincent, Da Deppo, Vania,, de Cecco, Mariolino, Nilda Oklay, Jessica Agarwal, Davidsson, Björn, Barucci, Maria Antonella,, Kührt, Ekkehard, Güttler, Carsten, Bertini, Ivano,, Oklay, Nilda,, Kuppers, Michael,, Carsten Güttler, Gutiérrez, Pedro J., Su, Cheng-Chin,, Deller, Jakob,, Hviid, Stubbe F.,, Groussin, Olivier,, Cecilia Tubiana, Mariolino De Cecco, Lazzarin, Monica, Shi, Xian,, Agarwal, Jessica, Deller, Jakob, Barbieri, Cesare,, Lai, Ian-Lin, Lamy, Philippe, Hofmann, Marc, Cremonese, Gabriele, A'Hearn, Michael F.,, J.-Rainer Kramm, Hans Rickman, Rodrigo, Rafael, Marc Hofmann, Lee, Jui-Chi, Stubbe F. Hviid, Giampiero Naletto, Ying Liao, Jean-Loup Bertaux, Monica Lazzarin, Jakob Deller, Kramm, J. -Rainer,, Nicolas Thomas, Barucci, Maria Antonella, Tubiana, Cecilia,, Lee, Jui-Chi,, Fornasier, Sonia, Kramm, J. -Rainer, Gutiérrez Buenestado, Pedro J., Jong-Shinn Wu, Davidsson, Björn,, A’hearn, Michael, Holger Sierks, Kovacs, Gabor, +161 morecore +2 more sourcesComet Gas and Dust Dynamics Modeling [PDF]
, 2010 This software models the gas and dust dynamics of comet coma (the head region of a comet) in order to support the Microwave Instrument for Rosetta Orbiter (MIRO) project. MIRO will study the evolution of the comet 67P/Churyumov-Gerasimenko's coma system. Von Allmen, Paul A., Lee, Seungwoncore Comet 67P/Churyumov-Gerasimenko sheds dust coat accumulated over the past four years [PDF]
, 2015 International audienceComets are composed of dust and frozen gases. The ices are mixed with the refractory material either as an icy conglomerate1, or as an aggregate of pre-solar grains (grains that existed prior to the formation of the Solar System ...Godard, Marie, Letho, Harry, Paquette, John, Baklouti, Donia,, Bardyn, Anaïs, Kissel, J., Briois, Christelle,, Boris Zaprudin, Hilchenbach, Martin, Fischer, Henning, Bardyn, Anaïs,, Engrand, Cécile,, Hilchenbach, Martin,, Fray, Nicolas, Fray, Nicolas,, Jochen Kissel, Schulz, Rita,, Lehto, Harry J.,, Rynö, J., Henning Fischer, Thirkell, Laurent,, Godard, Marie,, Kurt Varmuza, Silén, Johan,, Fischer, Henning,, Jouni Rynö, Zaprudin, Boris, Sandra Siljeström, Fray, N., Siljeström, Sandra,, Langevin, Yves, Lehto, Harry, Stenzel, O., Sihane Merouane, Paquette, J., Cottin, Hervé,, Laurent Thirkell, Le Roy, Léna, Hornung, Klaus, Martin Hilchenbach, Cottin, H., Orthous-Daunay, François Régis,, Bardyn, A., Christelle Briois, Kissel, Jochen, Hilchenbach, M., Silén, Johann, Thirkell, Laurent, Marie Godard, Johan Silen, Merouane, Sihane, Baklouti, D., François-Régis Orthous-Daunay, Rynö, Jouni, Oliver Stenzel, Anaïs Bardyn, Yves Langevin, Kissel, Jochen,, Donia Baklouti, Rita Schulz, Cecile Engrand, Zaprudin, Boris,, Varmuza, Kurt, Le Roy, Léna,, Engrand, C., Fischer, H., Nicolas Fray, Hornung, K., Godard, M., Paquette, John A.,, Hervé Cottin, Harry Lehto, Orthous-Daunay, F., Zaprudin, B., Briois, Christelle, Léna Le Roy, Stenzel, Oliver,, Schulz, R., Silen, Johan, Baklouti, Donia, Langevin, Y., Merouane, Sihane,, John Paquette, Briois, C., Le Roy, L., Lehto, H., Varmuza, K., Schulz, Rita, Silen, J., Rynö, Jouni,, Orthous-Daunay, François-Régis, Siljeström, S., Langevin, Yves,, Hornung, Klaus,, Stenzel, Oliver, Merouane, S., Varmuza, Kurt,, Siljeström, Sandra, Varmuza, Kurt; orcid:, Engrand, Cecile, Cottin, Hervé, Klaus Hornung, Thirkell, L. +102 morecore +1 more sourceA Tale of Two Tails
, 2009 This paper outlines the key difference between ion tails and dust tails. It explains why meteor showers are observed when the Earth passes close to the orbit of a comet by examining the distribution of fragments within the dust tail in term of their ...Comyn-Platt, Edward, Hutchinson, James, Tebbs, Emma +2 morecore The wind-sock theory of comet tails [PDF]
, 1976 A method is reported for calculating the shapes of ionic comet tails that use the magnetic field along the tail to channel the tail plasma. The local momentum field in the solar wind determines magnetic field line locations along the tail.Rothe, E. D., Brandt, J. C.core