Quantifying The Self-helicity Of A Flux Tubes

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

Magnetic helicity has proven to be a powerful tool for understanding energetics of the solar corona. As it is usually defined, relative helicity is an integral over the entire coronal volume. In this work we consider two different generalizations by which relative helicity of a portion of the entire coronal volume may be calculated. Such a quantity is generally called the self helicity of the sub-volume. Each definition is a natural application of the traditional helicity formula but relative to different fields. One of the generalizations, which we term "additive self-helicity", has particularly desirable properties, such as being identically zero for any portion of a potential magnetic field. During a flare it is believed that the total helicity of the volume is conserved, but as reconnection transfers flux between domains, this will change the self-helicity of those. We demonstrate how "additive self-helicity" may be evaluated in practice to find the self-helicities for flux systems, or domains, composed of all field lines connecting a designated pair of photospheric source regions. It is then possible to quantify the transfer of self-helicity which would occur when reconnection transfers flux between flux systems.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Quantifying The Self-helicity Of A Flux Tubes 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 Quantifying The Self-helicity Of A Flux Tubes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Quantifying The Self-helicity Of A Flux Tubes will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1032755

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.