The loss of magnetic flux from pre-main sequence stars

Details The loss of magnetic flux from pre-main sequence stars The loss of magnetic flux from pre-main sequence stars

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..93..213m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 93, no. 1, June 1983, p. 213-216.

Astronomy and Astrophysics

Astrophysics

Magnetic Flux, Main Sequence Stars, Stellar Models, Losses, T Tauri Stars

Scientific paper

A mechanism of magnetic flux loss from mostly convective stellar models is explicitly demonstrated in response to the Piddington (1982) critique of stellar dynamo theory which rejects the widespread acceptance of the concept of turbulent resistivity and the associated, enhanced decay of large scale magnetic fields. It is noted that, even without appealing to enhanced turbulent resistivity, it is possible topologically for a convective star to lose a large part of its magnetic flux.

Affiliated with

Also associated with

No associations

Rating

The loss of magnetic flux from pre-main sequence stars 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 The loss of magnetic flux from pre-main sequence stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The loss of magnetic flux from pre-main sequence stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1504550