Search Publications

Monte Carlo modeling of neutral gas and dust in the coma of Comet 1P/Halley
DOI: 10.1016/j.icarus.2011.04.006 Bibcode: 2011Icar..213..655R

Hansen, Kenneth C.; Gombosi, Tamas I.; Combi, Michael R. +4 more

The neutral gas environment of a comet is largely influenced by dissociation of parent molecules created at the surface of the comet and collisions of all the involved species. We compare the results from a kinetic model of the neutral cometary environment with measurements from the Neutral Mass Spectrometer and the Dust Impact Detection System on…

2011 Icarus
Giotto 38
Cometary dust properties retrieved from polarization observations: Application to C/1995 O1 Hale Bopp and 1P/Halley
DOI: 10.1016/j.icarus.2008.09.008 Bibcode: 2009Icar..199..129L

Lasue, J.; Levasseur-Regourd, A. C.; Hadamcik, E. +1 more

The analysis of the polarized light scattered by cometary dust particles provides information on the physical properties of the solid component of cometary comae for C/1995 O1 Hale-Bopp and 1P/Halley. A model of light scattering by a size distribution of aggregates of up to 256 submicron-sized grains (spherical or spheroidal) mixed with single sph…

2009 Icarus
Giotto 86
Ion composition and chemistry in the coma of Comet 1P/Halley—A comparison between Giotto's Ion Mass Spectrometer and our ion-chemical network
DOI: 10.1016/j.icarus.2008.10.009 Bibcode: 2009Icar..199..505R

Hansen, Kenneth C.; Gombosi, Tamas I.; Combi, Michael R. +3 more

In order to understand the cometary plasma environment it is important to track the closely linked chemical reactions that dominate ion evolution. We used a coupled MHD ion-chemistry model to analyze previously unpublished Giotto High Intensity Ion Mass Spectrometer (HIS-IMS) data. In this way we study the major species, but we also try to match s…

2009 Icarus
Giotto 43
Dust Grains in the Comae and Tails of Sungrazing Comets: Modeling of Their Mineralogical and Morphological Properties
DOI: 10.1006/icar.2002.6940 Bibcode: 2002Icar..159..529K

Kimura, Hiroshi; Mann, Ingrid; Jessberger, Elmar K. +1 more

Observations of sungrazing comets, all of which belong to the Kreutz family, provide the opportunity of studying the properties of dust in the comae and tails of the comets. On the basis of available information on cometary and interplanetary dust as well as observations of dust in the tails of sungrazers, we model dust in sungrazing comets as flu…

2002 Icarus
Giotto SOHO 77
The Dependence of the Circumnuclear Coma Structure on the Properties of the Nucleus
DOI: 10.1006/icar.1997.5690 Bibcode: 1997Icar..127..319C

Rodionov, A. V.; Crifo, J. F.

A new step of development of the 3-D circumnuclear coma (“CNC”) model described in Crifoet al.(1995) is presented: now the gas and dust production are computed from an explicit dusty-ice sublimation model and a realistic dust mass spectrum is used. For the first time, (1) a clear distinction is made betweennucleus active area fraction gandactive s…

1997 Icarus
Giotto 151
Cometary dust trails I. Survey
DOI: 10.1016/0019-1035(92)90037-8 Bibcode: 1992Icar...95..180S

Sykes, Mark V.; Walker, Russell G.

Cometary dust trails were first observed by the Infrared Astronomical Satellite and consist of large refractory particles ejected from short-period comets at low velocities. Consequently, they tend to be found near the orbital paths of their parent bodies, their long and narrow appearance reminescent of airplane contrails. An examination of the en…

1992 Icarus
Giotto 220
0.7- to 23-µm photometric observations of P/Halley 1986 III and six recent bright comets
DOI: 10.1016/0019-1035(92)90027-5 Bibcode: 1992Icar..100..162G

Gehrz, R. D.; Ney, E. P.

We report 0.7- to 23-µm observations of P/Halley 1986 III and six other recent bright comets. P/Halley was measured on 47 occasions between 1985 December 12 UT and 1986 May 6 UT, several times within hours of the perihelion passage on 1986 February 9 UT. Our data show that the strength of the 10-µm silicate emission feature and the tem…

1992 Icarus
Giotto 129
The origin of complex organic ions in the coma of Comet Halley
DOI: 10.1016/0019-1035(92)90213-Q Bibcode: 1992Icar...98..125M

Reme, H.; Korth, A.; Lin, R. P. +3 more

Heavy ion mass spectra were obtained in the inner coma of Comet Halley by the Giotto-PICCA instrument. Outside the cometary ionopause, where ≳2000 K ion temperatures limited the effective mass resolution to 3 amu, the spectra exhibit a series of distinct mass groups that are separated by a constant ≈ 15 amu and extend to at least 120 amu. We show …

1992 Icarus
Giotto 41
Modeling of the thermal behavior and of the chemical differentiation of cometary nuclei
DOI: 10.1016/0019-1035(91)90058-2 Bibcode: 1991Icar...92..350E

Schmitt, B.; Espinasse, S.; Klinger, J. +1 more

Taking into account the low values of average density reported for Comet P/Halley, a model of a porous comet nucleus has been developed. The model includes heat conduction through the solid matrix and heat and mass transfers due to the vapor phase circulating in the pore system. Sublimation and recondensation of volatile species within the nucleus…

1991 Icarus
Giotto 122
Large dust particles along the Giotto trajectory
DOI: 10.1016/0019-1035(90)90220-4 Bibcode: 1990Icar...86..305C

Keller, H. U.; Curdt, W.

Images of Comet Halley taken by the Halley Multicolour Camera (HMC) onboard ESA's Giotto spacecraft provide highly accurate information on the viewing direction. As a part of the spacecraft dynamical system, HMC was very sensitive to attitude variations that occurred during the final approach phase. HMC identified several discrete events that were…

1990 Icarus
Giotto 22