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Alignment of Interstellar Grains

Citation

Goldstein, Mark Parnes (1971) Alignment of Interstellar Grains. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/F26D-K620. https://resolver.caltech.edu/CaltechTHESIS:05042018-093319359

Abstract

We calculate the alignment of inter stellar dust grains with respect to the magnetic field of our galaxy. The alignment is found for several values of magnetic field strength, internal grain temperature, and grain shape. We treat in detail the following processes which affect the alignment: (i) a dissipative magnetic torque due to Davis and Greenstein; (ii) the collisions of the grain with inter stellar hydrogen; (iii) the non-zero internal temperature of the grain.

We obtain a Fokker-Planck equation which takes account of these processes, and the solution of this equation provides the probability distribution of grain orientations. The equation is solved for these cases: (i) spherical grains in all fields; (ii) needles, prolate spheroidal grains, nearly-spherical oblate grains, and disks in strong magnetic fields; (iii) needles and nearly- spherical grains in weak fields. Using the distribution of orientations, we calculate the degrees of alignment.

Our results are in mixed agreement with those of E. M. Purcell and in good agreement with the weak-field calculation of C.R. Miller. We find that for the relatively strong magnetic field 10-5 gauss and grain temperature of 10°K, the measures of alignment are smaller than the values obtained from complete orientation of the grains.

Item Type:Thesis (Dissertation (Ph.D.))
Subject Keywords:Physics
Degree Grantor:California Institute of Technology
Division:Physics, Mathematics and Astronomy
Major Option:Physics
Thesis Availability:Public (worldwide access)
Research Advisor(s):
  • Davis, Leverett
Thesis Committee:
  • Unknown, Unknown
Defense Date:29 September 1970
Funders:
Funding AgencyGrant Number
NSFUNSPECIFIED
CaltechUNSPECIFIED
Record Number:CaltechTHESIS:05042018-093319359
Persistent URL:https://resolver.caltech.edu/CaltechTHESIS:05042018-093319359
DOI:10.7907/F26D-K620
Default Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:10845
Collection:CaltechTHESIS
Deposited By: Lisa Fischelis
Deposited On:07 May 2018 18:22
Last Modified:22 Sep 2020 23:02

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