Magnetic reconnection as the cause of cosmic ray excess from the heliospheric tail

Details Magnetic reconnection as the cause of cosmic ray excess from the heliospheric tail Magnetic reconnection as the cause of cosmic ray excess from the heliospheric tail

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsm41d..03d&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SM41D-03

Physics

[2723] Magnetospheric Physics / Magnetic Reconnection

Scientific paper

The observation of a broad excess of sub-TeV cosmic rays compatible with the direction of the heliospheric tail and the discovery of two significant localized excess regions of multi-TeV cosmic rays by the MILAGRO collaboration, also from the same region of the sky, have raised questions on their origin. In particular, the coincidence of the most significant localized region with the direction of the heliospheric tail and the small angular scale of the observed anisotropy (~ 10deg) is suggestive a local origin and of a possible connection to the low energy broad excess. Cosmic ray acceleration from magnetic reconnection in the magnetotail is proposed as a possible source of the energetic particles.

Affiliated with

Also associated with

No associations

Rating

Magnetic reconnection as the cause of cosmic ray excess from the heliospheric tail does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Magnetic reconnection as the cause of cosmic ray excess from the heliospheric tail, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetic reconnection as the cause of cosmic ray excess from the heliospheric tail will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1473071