Numerical analyses of self-generated magnetic fields with very small scale in solar corona

Details Numerical analyses of self-generated magnetic fields with very small scale in solar corona Numerical analyses of self-generated magnetic fields with very small scale in solar corona

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...364..785l&link_type=abstract

Astronomy and Astrophysics, v.364, p.785-792 (2000)

Astronomy and Astrophysics

Astrophysics

5

Sun: Corona, Sun: General, Sun: Magnetic Fields

Scientific paper

We numerically study the collapse behavior of self-generated magnetic fields described by nonlinear coupling equations. The results show that magnetic fields self-generated by transverse pumping plasmons may collapse, leading to an enhancement of the magnetic field of up to 250 - 500 Gauss in the range around 0.02 - 0.03 km, which corresponds to the inferred inhomogeneity small-scale fields in both the strength and scale in the solar corona.

Affiliated with

Also associated with

No associations

Rating

Numerical analyses of self-generated magnetic fields with very small scale in solar corona 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 Numerical analyses of self-generated magnetic fields with very small scale in solar corona, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical analyses of self-generated magnetic fields with very small scale in solar corona will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1722020