Search Results - (Author, Cooperation:J. Benkhoff)
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1A. Coradini ; F. Capaccioni ; S. Erard ; G. Arnold ; M. C. De Sanctis ; G. Filacchione ; F. Tosi ; M. A. Barucci ; M. T. Capria ; E. Ammannito ; D. Grassi ; G. Piccioni ; S. Giuppi ; G. Bellucci ; J. Benkhoff ; J. P. Bibring ; A. Blanco ; M. Blecka ; D. Bockelee-Morvan ; F. Carraro ; R. Carlson ; U. Carsenty ; P. Cerroni ; L. Colangeli ; M. Combes ; M. Combi ; J. Crovisier ; P. Drossart ; E. T. Encrenaz ; C. Federico ; U. Fink ; S. Fonti ; L. Giacomini ; W. H. Ip ; R. Jaumann ; E. Kuehrt ; Y. Langevin ; G. Magni ; T. McCord ; V. Mennella ; S. Mottola ; G. Neukum ; V. Orofino ; P. Palumbo ; U. Schade ; B. Schmitt ; F. Taylor ; D. Tiphene ; G. Tozzi
American Association for the Advancement of Science (AAAS)
Published 2011Staff ViewPublication Date: 2011-10-29Publisher: American Association for the Advancement of Science (AAAS)Print ISSN: 0036-8075Electronic ISSN: 1095-9203Topics: BiologyChemistry and PharmacologyComputer ScienceMedicineNatural Sciences in GeneralPhysicsPublished by: -
2G. Filacchione ; M. C. De Sanctis ; F. Capaccioni ; A. Raponi ; F. Tosi ; M. Ciarniello ; P. Cerroni ; G. Piccioni ; M. T. Capria ; E. Palomba ; G. Bellucci ; S. Erard ; D. Bockelee-Morvan ; C. Leyrat ; G. Arnold ; M. A. Barucci ; M. Fulchignoni ; B. Schmitt ; E. Quirico ; R. Jaumann ; K. Stephan ; A. Longobardo ; V. Mennella ; A. Migliorini ; E. Ammannito ; J. Benkhoff ; J. P. Bibring ; A. Blanco ; M. I. Blecka ; R. Carlson ; U. Carsenty ; L. Colangeli ; M. Combes ; M. Combi ; J. Crovisier ; P. Drossart ; T. Encrenaz ; C. Federico ; U. Fink ; S. Fonti ; W. H. Ip ; P. Irwin ; E. Kuehrt ; Y. Langevin ; G. Magni ; T. McCord ; L. Moroz ; S. Mottola ; V. Orofino ; U. Schade ; F. Taylor ; D. Tiphene ; G. P. Tozzi ; P. Beck ; N. Biver ; L. Bonal ; J. P. Combe ; D. Despan ; E. Flamini ; M. Formisano ; S. Fornasier ; A. Frigeri ; D. Grassi ; M. S. Gudipati ; D. Kappel ; F. Mancarella ; K. Markus ; F. Merlin ; R. Orosei ; G. Rinaldi ; M. Cartacci ; A. Cicchetti ; S. Giuppi ; Y. Hello ; F. Henry ; S. Jacquinod ; J. M. Reess ; R. Noschese ; R. Politi ; G. Peter
Nature Publishing Group (NPG)
Published 2016Staff ViewPublication Date: 2016-01-14Publisher: Nature Publishing Group (NPG)Print ISSN: 0028-0836Electronic ISSN: 1476-4687Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsPublished by: -
3T. Spohn ; J. Knollenberg ; A. J. Ball ; M. Banaszkiewicz ; J. Benkhoff ; M. Grott ; J. Grygorczuk ; C. Huttig ; A. Hagermann ; G. Kargl ; E. Kaufmann ; N. Komle ; E. Kuhrt ; K. J. Kossacki ; W. Marczewski ; I. Pelivan ; R. Schrodter ; K. Seiferlin
American Association for the Advancement of Science (AAAS)
Published 2015Staff ViewPublication Date: 2015-08-01Publisher: American Association for the Advancement of Science (AAAS)Print ISSN: 0036-8075Electronic ISSN: 1095-9203Topics: BiologyChemistry and PharmacologyComputer ScienceMedicineNatural Sciences in GeneralPhysicsPublished by: -
4F. Capaccioni ; A. Coradini ; G. Filacchione ; S. Erard ; G. Arnold ; P. Drossart ; M. C. De Sanctis ; D. Bockelee-Morvan ; M. T. Capria ; F. Tosi ; C. Leyrat ; B. Schmitt ; E. Quirico ; P. Cerroni ; V. Mennella ; A. Raponi ; M. Ciarniello ; T. McCord ; L. Moroz ; E. Palomba ; E. Ammannito ; M. A. Barucci ; G. Bellucci ; J. Benkhoff ; J. P. Bibring ; A. Blanco ; M. Blecka ; R. Carlson ; U. Carsenty ; L. Colangeli ; M. Combes ; M. Combi ; J. Crovisier ; T. Encrenaz ; C. Federico ; U. Fink ; S. Fonti ; W. H. Ip ; P. Irwin ; R. Jaumann ; E. Kuehrt ; Y. Langevin ; G. Magni ; S. Mottola ; V. Orofino ; P. Palumbo ; G. Piccioni ; U. Schade ; F. Taylor ; D. Tiphene ; G. P. Tozzi ; P. Beck ; N. Biver ; L. Bonal ; J. P. Combe ; D. Despan ; E. Flamini ; S. Fornasier ; A. Frigeri ; D. Grassi ; M. Gudipati ; A. Longobardo ; K. Markus ; F. Merlin ; R. Orosei ; G. Rinaldi ; K. Stephan ; M. Cartacci ; A. Cicchetti ; S. Giuppi ; Y. Hello ; F. Henry ; S. Jacquinod ; R. Noschese ; G. Peter ; R. Politi ; J. M. Reess ; A. Semery
American Association for the Advancement of Science (AAAS)
Published 2015Staff ViewPublication Date: 2015-01-24Publisher: American Association for the Advancement of Science (AAAS)Print ISSN: 0036-8075Electronic ISSN: 1095-9203Topics: BiologyChemistry and PharmacologyComputer ScienceMedicineNatural Sciences in GeneralPhysicsPublished by: -
5Piccioni, G. ; Gérard, J. C. ; Lopez-Valverde, M. A. ; Sanchez-Lavega, A. ; Zasova, L. ; Hueso, R. ; Taylor, F. W. ; Bézard, B. ; Adriani, A. ; Angrilli, F. ; Arnold, G. ; Baines, K. H. ; Bellucci, G. ; Benkhoff, J. ; Bibring, J. P. ; Blanco, A. ; Blecka, M. I. ; Carlson, R. W. ; Coradini, A. ; Di Lellis, A. ; Encrenaz, T. ; Erard, S. ; Fonti, S. ; Formisano, V. ; Fouchet, T.
[s.l.] : Nature Publishing Group
Published 2007Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] The upper atmosphere of a planet is a transition region in which energy is transferred between the deeper atmosphere and outer space. Molecular emissions from the upper atmosphere (90–120 km altitude) of Venus can be used to investigate the energetics and to trace the circulation ...Type of Medium: Electronic ResourceURL: -
6Staff View
ISSN: 0019-1035Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
7Staff View
ISSN: 0273-1177Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision MechanicsPhysicsType of Medium: Electronic ResourceURL: -
8Grun, E. ; Benkhoff, J. ; Fechtig, H. ; Hesselbarth, P. ; Klinger, J. ; Kochan, H. ; Kohl, H. ; Krankowsky, D. ; Thiel, K. ; Lammerzahl, P. ; Spohn, T. ; Seboldt, W.
Amsterdam : ElsevierStaff ViewISSN: 0273-1177Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision MechanicsPhysicsType of Medium: Electronic ResourceURL: -
9Staff View
ISSN: 0040-4039Keywords: Repetitive Diels-Alder reactions ; bis-dienes ; bis-dienophiles ; endo-stereoselectivitySource: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: Chemistry and PharmacologyType of Medium: Electronic ResourceURL: -
10Staff View
ISSN: 1432-1904Source: Springer Online Journal Archives 1860-2000Topics: BiologyChemistry and PharmacologyNatural Sciences in GeneralType of Medium: Electronic ResourceURL: -
11Staff View
ISSN: 1573-0794Source: Springer Online Journal Archives 1860-2000Topics: GeosciencesPhysicsType of Medium: Electronic ResourceURL: -
12Staff View
ISSN: 1573-0794Source: Springer Online Journal Archives 1860-2000Topics: GeosciencesPhysicsNotes: Abstract Sublimation of minor gases from ices inside of a porous comet nucleus strongly depends on the effective energy input. Our model meant to describe the gas flux inside and out of the porous nucleus has been used to study the influence of physical and structural parameters on the effective energy input. We solve the conservation equations for H2O and CO as the most abundant minor component of higher volatility under appropriate boundary conditions. From the calculations we obtain the gas flux from volatile, icy components inside the porous nucleus, temperature profiles, changes in relative chemical abundances, and the gas flux into the coma for each of the volatiles. We will show results from our calculations for a model comet in the orbit of Hale-Bopp (C/1995 O1). In this paper we focus on the energy balance at the surface. We will also relate measurements of molecule fluxes to available energies and try to provide hints about the evolutionary status of the comet.Type of Medium: Electronic ResourceURL: -
13Staff View
ISSN: 1573-0794Keywords: Comet nucleus ; coma ; volatile icesSource: Springer Online Journal Archives 1860-2000Topics: GeosciencesPhysicsNotes: Abstract One of the goals of comet research is the determination of the chemical composition of the nucleus because it provides us with the clues about the composition of the nebula in which comet nuclei formed. It is well accepted that photo-chemical reactions must be considered to establish the abundances of mother molecules in the coma as they are released from the comet nucleus or from distributed dust sources in the coma. However, the mixing ratios of mother molecules in the coma changes with heliocentric distance. To obtain the abundances in the nucleus relative to those in the coma, we must turn our attention to the release rates of mother molecules from the nucleus as a function of heliocentric distance. For this purpose, we assume three sources for the coma gas: the surface of the nucleus (releasing mostly water vapor), the dust in the coma (the distributed source of several species released from dust particles), and the interior of the porous nucleus (the source of many species more volatile than water). The species diffusing from the interior of the nucleus are released by heat transported into the interior. Thus, the ratio of volatiles relative to water in the coma is a function of the heliocentric distance and provides important information about the chemical composition and structure of the nucleus. Our goal is to determine the abundance ratios of various mother molecules relative to water from many remote-sensing observations of the coma as a function of heliocentric distance. Comet Hale-Bopp is ideal for this purpose since it has been observed using instruments in many different wavelength regions over large ranges of heliocentric distances. The ratios of release rates of species into the coma are than modeled assuming various chemical compositions of the spinning nucleus as it moves from large heliocentric distance through perihelion. Since the heat flow into the nucleus will be different after perihelion from that before perihelion, we can also expect different gas release rates after perihelion compared to those observed before perihelion. Since not all the data are available yet, we report on progress of these calculations.Type of Medium: Electronic ResourceURL: -
14Drossart, P. ; Sanchez-Lavega, A. ; Hueso, R. ; Taylor, F. W. ; Wilson, C. F. ; Grassi, D. ; Zasova, L. ; Moriconi, M. ; Adriani, A. ; Lebonnois, S. ; Coradini, A. ; Bézard, B. ; Angrilli, F. ; Arnold, G. ; Baines, K. H. ; Bellucci, G. ; Benkhoff, J. ; Bibring, J. P. ; Blanco, A. ; Blecka, M. I. ; Carlson, R. W. ; Di Lellis, A. ; Encrenaz, T. ; Erard, S. ; Fonti, S.
[s.l.] : Nature Publishing Group
Published 2007Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] Venus has no seasons, slow rotation and a very massive atmosphere, which is mainly carbon dioxide with clouds primarily of sulphuric acid droplets. Infrared observations by previous missions to Venus revealed a bright ‘dipole’ feature surrounded by a cold ‘collar’ at ...Type of Medium: Electronic ResourceURL: -
15Staff View
ISSN: 1572-9672Keywords: Comets ; Ices ; Energy Balance ; Molecular FluxSource: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract Surface temperature and the available effective energy strongly influence the mass flux of H2O and minor volatiles from the nucleus. We perform computer simulations to model the gas flux from volatile, icy components in porous ice-dust surfaces, in order to better understand results from observations of comets. Our model assumes a porous body containing dust, one major ice component (H2O) and up to eight minor components of higher volatility (e.g. CO, CH4, CH3OH, HCN, C2H2, H2S), The body's porous structure is modeled as a bundle of tubes with a given tortuosity and an initially constant pore diameter. Heat is conducted by the matrix and carried by the vapors. The model includes radially inward and outward flowing vapor within the body, escape of outward flowing gas from the body, complete depletion of less volatile ices in outer layers, and recondensation of vapor in deeper, cooler layers. From the calculations we obtain temperature profiles and changes in relative chemical abundances, porosity and pore size distribution as a function of depth, and the gas flux into the interior and into the atmosphere for each of the volatiles at various positions of the body in its orbit. In this paper we relate the observed relative molecular abundances in the coma of Comet C/1995 O1 (Hale-Bopp) and of Comet 46P/Wirtanen to molecular fluxes at the surface calculated from our model.Type of Medium: Electronic ResourceURL: -
16Staff View
ISSN: 1572-9672Keywords: Coma ; Nucleus ; Heat Diffusion ; Gas Diffusion ; Mother MoleculesSource: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract A major goal of comet research is to determine conditions in the outer solar nebula based on the chemical composition and structure of comet nuclei. The old view was to use coma abundances directly for the chemical composition of the nucleus. However, since the composition of the coma changes with heliocentric distance, r, the new view is that the nucleus composition msut be determined from analysis of coma mixing ratios as a function of r. Taking advantage of new observing technology and the early detection of the very active Comet Hale-Bopp (C/1995 O1) allows us to determine the coma mixing ratios over a large range of heliocentric distances. In our analysis we assume three sources for the coma gas: (1) the surface of the nucleus (releasing water vapor), (2) the interior of the porous nucleus (releasing many species more volatile than water), and (3) the distributed source (releasing gases from ices and hydrocarbon polycondensates trapped and contained in coma dust). Molecules diffusing inside the nucleus are sublimated by heat transported into the interior. The mixing ratios in the coma are modeled assuming various chemical compositions and structural parameters of the spinning nucleus as it moves in its orbit from large heliocentric distance through perihelion. We have combined several sets of observational data of Comet Hale-Bopp for H2O (from OH) and CO, covering the spectrum range from radio to UV. Many inconsistencies in the data were uncovered and reported to the observers for a reanalysis. Since post-perihelion data are still sparse, we have combined pre- and post-perihelion data. The resulting mixing ratio of CO relative to H2O as a function of r is presented with a preliminary analysis that still needs to be expanded further. Our fit to the data indicates that the total CO release rate (from the nucleus and distributed sources) relative to that of H2O is 30% near perihelion.Type of Medium: Electronic ResourceURL: