This paper summarizes our present understanding of the physical processes controlling the dust and gas production of cometary nuclei and the evolution of the dusty gas flow in the inner coma. Special emphasis is being made to compile a self-consistent set of governing equations describing the accelerating dusty gas flow in a cometary atmosphere.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/26895/1/0000461.pd
This research program addresses two cases of tenuous planetary atmospheres: comets and Io. The comet...
MHD simulation results of the interaction of the expanding atmosphere of comet Hale-Bopp with the ma...
On the basis of the icy conglometate model of cometary nuclei various observations demonstrate the s...
The development of the expanding atmospherefrom the evaporating cometary nucleus has traditionallyfo...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/76515/1/AIAA-2005-4832-757.pd
Comets often display narrow dust jets but more diffuse gas comae when their eccentric orbits bring t...
Because of the diurnal thermal cycle and the irregular shape of the nucleus, gas outflow of comet 6...
When viewed from Earth, most of what we observe of a comet is dust. The influence of solar radiation...
The first results of a new time-dependent, axisymmetric dusty gas dynamical model of inner cometary ...
Comets are made of volatile and refractory material and naturally experience various degrees of subl...
Context. The gas-driven dust activity of comets is still an unsolved question in cometary physics. H...
The goal was to investigate the structural properties of the surface of comet nucleus and how the su...
The gas and dust production rates of comets near the sun are intimately linked to the fate of the so...
This chapter aims at providing the tools and knowledge to understand and model the plasma environmen...
Improving our capability to interpret observations of cometary dust is necessary to deepen our under...
This research program addresses two cases of tenuous planetary atmospheres: comets and Io. The comet...
MHD simulation results of the interaction of the expanding atmosphere of comet Hale-Bopp with the ma...
On the basis of the icy conglometate model of cometary nuclei various observations demonstrate the s...
The development of the expanding atmospherefrom the evaporating cometary nucleus has traditionallyfo...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/76515/1/AIAA-2005-4832-757.pd
Comets often display narrow dust jets but more diffuse gas comae when their eccentric orbits bring t...
Because of the diurnal thermal cycle and the irregular shape of the nucleus, gas outflow of comet 6...
When viewed from Earth, most of what we observe of a comet is dust. The influence of solar radiation...
The first results of a new time-dependent, axisymmetric dusty gas dynamical model of inner cometary ...
Comets are made of volatile and refractory material and naturally experience various degrees of subl...
Context. The gas-driven dust activity of comets is still an unsolved question in cometary physics. H...
The goal was to investigate the structural properties of the surface of comet nucleus and how the su...
The gas and dust production rates of comets near the sun are intimately linked to the fate of the so...
This chapter aims at providing the tools and knowledge to understand and model the plasma environmen...
Improving our capability to interpret observations of cometary dust is necessary to deepen our under...
This research program addresses two cases of tenuous planetary atmospheres: comets and Io. The comet...
MHD simulation results of the interaction of the expanding atmosphere of comet Hale-Bopp with the ma...
On the basis of the icy conglometate model of cometary nuclei various observations demonstrate the s...