Disconnection event (DE) in cometary plasma physics is the regular loss of the entire plasma tail and the growth of the new one. Analysis of a sequence of DEs that occurred 13-18 April, 1986 shows that they correlate well with a magnetic, sector-boundary crossing and a complex magnetic structure in the solar wind with polarity reversals that occurred about one day later. These events are entirely consistent with sunward, magnetic reconnection as the DE mechanism
Context. The Rosetta Plasma Consortium (RPC) magnetometer (MAG) data during the tail excursion in Ma...
International audienceContext. The Rosetta dayside excursion took place in September-October 2015 wh...
Disconnection of open magnetic flux by reconnection is required to balance the injection of open flu...
The disconnection event (DE) consists of the periodic loss of a comet's entire plasma tail and the g...
Disconnection Events are the dramatic part of the periodic morphology involving the separation of th...
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...
Cometary and solar wind data from December 1985 through April 1986 are presented for the purpose of ...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/94832/1/jgra18723.pd
Magnetic reconnection is an important process in many astrophysical plasma environments, which leads...
When comets interacting with solar wind, straight and narrow plasma tails will be often formed. The ...
In-situ measurements of comets Halley and Giacobini-Zinner have confirmed the accepted basic physics...
Once a cometary plasma cloud has been created through ionisation of the cometary neutrals, it presen...
Context. During their journey to perihelion, comets may appear in the field of view of space-borne o...
International audience<p>Magnetic reconnection is a fundamental process that is ubiquitous in ...
Context. The Rosetta Plasma Consortium (RPC) magnetometer (MAG) data during the tail excursion in Ma...
International audienceContext. The Rosetta dayside excursion took place in September-October 2015 wh...
Disconnection of open magnetic flux by reconnection is required to balance the injection of open flu...
The disconnection event (DE) consists of the periodic loss of a comet's entire plasma tail and the g...
Disconnection Events are the dramatic part of the periodic morphology involving the separation of th...
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...
Cometary and solar wind data from December 1985 through April 1986 are presented for the purpose of ...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/94832/1/jgra18723.pd
Magnetic reconnection is an important process in many astrophysical plasma environments, which leads...
When comets interacting with solar wind, straight and narrow plasma tails will be often formed. The ...
In-situ measurements of comets Halley and Giacobini-Zinner have confirmed the accepted basic physics...
Once a cometary plasma cloud has been created through ionisation of the cometary neutrals, it presen...
Context. During their journey to perihelion, comets may appear in the field of view of space-borne o...
International audience<p>Magnetic reconnection is a fundamental process that is ubiquitous in ...
Context. The Rosetta Plasma Consortium (RPC) magnetometer (MAG) data during the tail excursion in Ma...
International audienceContext. The Rosetta dayside excursion took place in September-October 2015 wh...
Disconnection of open magnetic flux by reconnection is required to balance the injection of open flu...