The disconnection event (DE) consists of the periodic loss of a comet's entire plasma tail and the growth of a new one. This spectacular phenomenon is not understood. The strategy was to assemble a data base of specific events studied in detail, determine the solar wind conditions responsible for DEs, and develop a consistent physical model. Analysis is complete for the sequence of DEs that took place during 13 to 18 April 1986. The first DE correlates well with a sector boundary crossing for the comet and a group of DEs that occurred approximately a day later could have produced by polarity reversals seen in the IMP-8 data. Thus, these DEs are consistent with the frontside, magnetic reconnection mechanism
The encounters of five spacecraft with Halley's Comet during 6-14 March 1986 offered a unique opport...
Understanding of the cometary plasma environment, an ideal laboratory for magnetohydrodynamic (MHD) ...
Comets hold the key to the understanding of our solar system, its formation and its evolution, and t...
Disconnection Events are the dramatic part of the periodic morphology involving the separation of th...
Disconnection event (DE) in cometary plasma physics is the regular loss of the entire plasma tail an...
Cometary and solar wind data from December 1985 through April 1986 are presented for the purpose of ...
We present an initial overview of the disconnection events (DE's) in Comet Halley in 1986. Although ...
This work compares cometary and solar wind data with the purpose of determining the solar wind condi...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/94832/1/jgra18723.pd
In-situ measurements of comets Halley and Giacobini-Zinner have confirmed the accepted basic physics...
When comets interacting with solar wind, straight and narrow plasma tails will be often formed. The ...
Once a cometary plasma cloud has been created through ionisation of the cometary neutrals, it presen...
Bright comets display a rich variety of interesting plasma phenomena which occur over an enormous ra...
The plasma tail of Comet Austin (1989c1) showed remarkable disturbances because of the solar maximum...
Comets hold the key to the understanding of our solar system, its formation and its evolution, and t...
The encounters of five spacecraft with Halley's Comet during 6-14 March 1986 offered a unique opport...
Understanding of the cometary plasma environment, an ideal laboratory for magnetohydrodynamic (MHD) ...
Comets hold the key to the understanding of our solar system, its formation and its evolution, and t...
Disconnection Events are the dramatic part of the periodic morphology involving the separation of th...
Disconnection event (DE) in cometary plasma physics is the regular loss of the entire plasma tail an...
Cometary and solar wind data from December 1985 through April 1986 are presented for the purpose of ...
We present an initial overview of the disconnection events (DE's) in Comet Halley in 1986. Although ...
This work compares cometary and solar wind data with the purpose of determining the solar wind condi...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/94832/1/jgra18723.pd
In-situ measurements of comets Halley and Giacobini-Zinner have confirmed the accepted basic physics...
When comets interacting with solar wind, straight and narrow plasma tails will be often formed. The ...
Once a cometary plasma cloud has been created through ionisation of the cometary neutrals, it presen...
Bright comets display a rich variety of interesting plasma phenomena which occur over an enormous ra...
The plasma tail of Comet Austin (1989c1) showed remarkable disturbances because of the solar maximum...
Comets hold the key to the understanding of our solar system, its formation and its evolution, and t...
The encounters of five spacecraft with Halley's Comet during 6-14 March 1986 offered a unique opport...
Understanding of the cometary plasma environment, an ideal laboratory for magnetohydrodynamic (MHD) ...
Comets hold the key to the understanding of our solar system, its formation and its evolution, and t...