The development of the expanding atmospherefrom the evaporating cometary nucleus has traditionallyfocused on observing and modeling the separatedevelopment of two distinct components, gas and dust,which are coupled dynamically with one another atdistances out to a few tens of cometary radii. In the lastdecade or so, however, direct evidence from observationsand suggestions from theory suggest that the dusty-gascoma is a tightly coupled system where material is transferredbetween the solid and gaseous phase as an importantintegral part of the basic development of the coma.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/43256/1/11038_2004_Article_239224.pd
The composition, origins, and evolution of comets were studied. The composition was studied using sp...
Improving our capability to interpret observations of cometary dust is necessary to deepen our under...
This review presents our understanding of cometary dust at the end of 2017. For decades, insight abo...
Comets often display narrow dust jets but more diffuse gas comae when their eccentric orbits bring t...
When viewed from Earth, most of what we observe of a comet is dust. The influence of solar radiation...
Comet Hale–Bopp was the largest comet by almost any definition,observed at least since the advent of...
Comets are made of volatile and refractory material and naturally experience various degrees of subl...
This paper summarizes our present understanding of the physical processes controlling the dust and g...
Comets often display narrow dust jets but more diffuse gas comae when their eccentric orbits bring t...
This is an Open Access article distributed under the terms of the Creative Commons Attribution Licen...
Because of the diurnal thermal cycle and the irregular shape of the nucleus, gas outflow of comet 6...
The distribution of dust-scattered intensity in Halley's inner coma is measured with the Vega three-...
Post-Halley comets are known to be irregular objects with most nucleus activity very localized and w...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/76515/1/AIAA-2005-4832-757.pd
We have investigated the dust and gas coma of the comet C/2000 WM1 (LINEAR) during Dec. 2-4, 2001, i...
The composition, origins, and evolution of comets were studied. The composition was studied using sp...
Improving our capability to interpret observations of cometary dust is necessary to deepen our under...
This review presents our understanding of cometary dust at the end of 2017. For decades, insight abo...
Comets often display narrow dust jets but more diffuse gas comae when their eccentric orbits bring t...
When viewed from Earth, most of what we observe of a comet is dust. The influence of solar radiation...
Comet Hale–Bopp was the largest comet by almost any definition,observed at least since the advent of...
Comets are made of volatile and refractory material and naturally experience various degrees of subl...
This paper summarizes our present understanding of the physical processes controlling the dust and g...
Comets often display narrow dust jets but more diffuse gas comae when their eccentric orbits bring t...
This is an Open Access article distributed under the terms of the Creative Commons Attribution Licen...
Because of the diurnal thermal cycle and the irregular shape of the nucleus, gas outflow of comet 6...
The distribution of dust-scattered intensity in Halley's inner coma is measured with the Vega three-...
Post-Halley comets are known to be irregular objects with most nucleus activity very localized and w...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/76515/1/AIAA-2005-4832-757.pd
We have investigated the dust and gas coma of the comet C/2000 WM1 (LINEAR) during Dec. 2-4, 2001, i...
The composition, origins, and evolution of comets were studied. The composition was studied using sp...
Improving our capability to interpret observations of cometary dust is necessary to deepen our under...
This review presents our understanding of cometary dust at the end of 2017. For decades, insight abo...