The spacecraft missions to Comets 21P/Giacobini-Zinner and 1P/Halley in the mid-1980s revolutionized our knowledge of comets and their interaction with the solar wind. Besides the large-scale plasma structures, the spacecraft in situ measurements produced many exciting and surprising results about the ion distribution and magnetic field configuration in the inner regions of cometary comae. These earlier scientific explorations laid the foundation for the Deep Space 1 mission to Comet 19P/Borrelly and groundbased observations of recent bright comets such as Comets 1996 B2 (Hyakutake) and 1995 O1 (Hale-Bopp). In this chapter, we review the mor-phological structures of cometary ion tails, analytical and numerical simulations of comet-solar win...
In the advent of the Rosetta arrival at the comet 67P/Churyumov–Gerasimenko, we present a global 3D ...
A simple two-dimensional model is developed to examine the composition of the cometary ion coma in t...
The interaction between a comet and the solar wind has been treated extensively in the literature. S...
In-situ measurements of comets Halley and Giacobini-Zinner have confirmed the accepted basic physics...
Peer Reviewedhttps://deepblue.lib.umich.edu/bitstream/2027.42/138863/1/rog199129s2976.pd
Once a cometary plasma cloud has been created through ionisation of the cometary neutrals, it presen...
International audienceWe present preliminary results of the first 3-D fully kinetic and electromagne...
Understanding of the cometary plasma environment, an ideal laboratory for magnetohydrodynamic (MHD) ...
The nucleus of an active comet, such as comet Halley near its perihelion, produces large quantities ...
International audienceContext. The first 1000 km of the ion tail of comet 67P/Churyumov–Gerasimenko ...
The recent in-situ measurements of the plasma-neutral gas environment of comet Halley by the GIOTTO ...
International audienceContext. Solar Orbiter is expected to have flown close to the tail of comet C/...
In the advent of the Rosetta arrival at the comet 67P/Churyumov–Gerasimenko, we present a global 3D ...
A simple two-dimensional model is developed to examine the composition of the cometary ion coma in t...
The interaction between a comet and the solar wind has been treated extensively in the literature. S...
In-situ measurements of comets Halley and Giacobini-Zinner have confirmed the accepted basic physics...
Peer Reviewedhttps://deepblue.lib.umich.edu/bitstream/2027.42/138863/1/rog199129s2976.pd
Once a cometary plasma cloud has been created through ionisation of the cometary neutrals, it presen...
International audienceWe present preliminary results of the first 3-D fully kinetic and electromagne...
Understanding of the cometary plasma environment, an ideal laboratory for magnetohydrodynamic (MHD) ...
The nucleus of an active comet, such as comet Halley near its perihelion, produces large quantities ...
International audienceContext. The first 1000 km of the ion tail of comet 67P/Churyumov–Gerasimenko ...
The recent in-situ measurements of the plasma-neutral gas environment of comet Halley by the GIOTTO ...
International audienceContext. Solar Orbiter is expected to have flown close to the tail of comet C/...
In the advent of the Rosetta arrival at the comet 67P/Churyumov–Gerasimenko, we present a global 3D ...
A simple two-dimensional model is developed to examine the composition of the cometary ion coma in t...
The interaction between a comet and the solar wind has been treated extensively in the literature. S...