Fluctuation theory of starlight polarization

Details Fluctuation theory of starlight polarization Fluctuation theory of starlight polarization

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...237..471n&link_type=abstract

Astrophysical Journal, Part 1, vol. 237, Apr. 15, 1980, p. 471-481. Research supported by the National Science Council of Natio

Statistics

6

Fluctuation Theory, Interstellar Magnetic Fields, Optical Polarization, Stellar Radiation, Differential Equations, Light (Visible Radiation), Polarized Light, Statistical Correlation, Variance (Statistics)

Scientific paper

The average and the variance of absolute polarization of starlight are calculated as a function of distance based on the fluctuation theory of Langevin's scheme. The computed curves from the theory agree with the sample observational data. It estimates a correlation length of 225 pc and a fluctuating angle of 22.5 deg for the fluctuation of interstellar magnetic field for the observation direction within an l(II) range of 60-90 deg around the galactic equator.

Affiliated with

Also associated with

No associations

Rating

Fluctuation theory of starlight polarization 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 Fluctuation theory of starlight polarization, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fluctuation theory of starlight polarization will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1697807