NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Press Enter or click the Search button to begin your search.

Back to Results
Magnetic Reconnection in Different Environments: Similarities and DifferencesDepending on the specific situation, magnetic reconnection may involve symmetric or asymmetric inflow regions. Asymmetric reconnection applies, for example, to reconnection at the Earth's magnetopause, whereas reconnection in the nightside magnetotail tends to involve more symmetric geometries. A combination of review and new results pertaining to magnetic reconnection is being presented. The focus is on three aspects: A basic, MHD-based, analysis of the role magnetic reconnection plays in the transport of energy, followed by an analysis of a kinetic model of time dependent reconnection in a symmetric current sheet, similar to what is typically being encountered in the magnetotail of the Earth. The third element is a review of recent results pertaining to the orientation of the reconnection line in asymmetric geometries, which are typical for the magnetopause of the Earth, as well as likely to occur at other planets.
Document ID
20140017078
Acquisition Source
Goddard Space Flight Center
Document Type
Book Chapter
Authors
Hesse, Michael
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Aunai, Nicolas
(Oak Ridge Associated Universities Greenbelt, MD, United States)
Kuznetsova, Masha
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Zenitani, Seiji
(National Astronomical Observatory Tokyo, Japan)
Birn, Joachim
(Space Science Inst. Boulder, CO, United States)
Date Acquired
December 8, 2014
Publication Date
September 17, 2014
Publication Information
Publisher: AGU
Subject Category
Astrophysics
Report/Patent Number
GSFC-E-DAA-TN10927
Report Number: GSFC-E-DAA-TN10927
Funding Number(s)
CONTRACT_GRANT: NNH06CC03B
Distribution Limits
Public
Copyright
Public Use Permitted.
Keywords
Reconnection
Plasmas
Space
No Preview Available