MARC details
000 -LEADER |
fixed length control field |
02322nam a2200253Ia 4500 |
003 - CONTROL NUMBER IDENTIFIER |
control field |
IN-BaIIA |
005 - DATE AND TIME OF LATEST TRANSACTION |
control field |
20211110165319.0 |
008 - FIXED-LENGTH DATA ELEMENTS--GENERAL INFORMATION |
fixed length control field |
211028s9999 xx 000 0 eng d |
040 ## - CATALOGING SOURCE |
Transcribing agency |
IIA Library |
080 ## - UNIVERSAL DECIMAL CLASSIFICATION NUMBER |
Universal Decimal Classification number |
043:52-64 |
Item number |
NAG |
100 ## - MAIN ENTRY--PERSONAL NAME |
Personal name |
Nagendra, K. N |
9 (RLIN) |
15238 |
Relator term |
Author |
245 #0 - TITLE STATEMENT |
Title |
Radiative transfer with stokes vectors |
Remainder of title |
a thesis submitted for the degree of Doctor of Philosophy in the faculty of science, Bangalore University, Bangalore |
Statement of responsibility, etc. |
K. N. Nagendra |
Medium |
[Ph.D Thesis] |
260 ## - PUBLICATION, DISTRIBUTION, ETC. |
Place of publication, distribution, etc. |
Bangalore |
Name of publisher, distributor, etc. |
Indian Institute of Astrophysics |
Date of publication, distribution, etc. |
1986 |
300 ## - PHYSICAL DESCRIPTION |
Extent |
iii, 240p. |
500 ## - GENERAL NOTE |
General note |
Thesis Supervisor A. Peraiah |
502 ## - DISSERTATION NOTE |
Degree type |
Doctor of Philosophy |
Name of granting institution |
Indian Institute of Astrophysics, Bangalore |
Year degree granted |
1986 |
520 ## - SUMMARY, ETC. |
Summary, etc. |
The solution of the radiative transfer equation taking account of the polarization state of the radiation<br/>field is an important problem. The light emitted by any physical system is polarized only if there exists an intrinsic anisotropy in the medium, in which the radiation interacts with matter. The anisotropy in both microscopic as well as macroscopic scales produces a net polarization of the diffuse radiation field in the medium. The equation of radiative transfer establishes a natural link between the microphysical quantities like absorption and scattering coefficients, refractive indices etc.and thermodynamic quantities such as temperature and radiative flux gradients as well as the geometric structure of the medium. Hence a correct theoretical<br/>interpretation of the observed polarization data using the theory of polarization radiative transfer offers a better chance to determine the physical state of the matter in the emitting regions and the spatial, temporal and geometrical parameters of these regions. These parameters are the basic data needed in further studies of any astrophysical problem. In this thesis we have made an attempt to develop general solutions of the problem of radiative transfer for polarized radintion field. We mainly use the Stokes<br/>vector representation in the polarization transfer equations.<br/> |
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM |
Topical term or geographic name entry element |
Ph.D Thesis |
9 (RLIN) |
1344 |
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM |
Topical term or geographic name entry element |
Radiative Transfer |
9 (RLIN) |
1568 |
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM |
Topical term or geographic name entry element |
Stok Vectors |
9 (RLIN) |
15239 |
700 ## - ADDED ENTRY--PERSONAL NAME |
Personal name |
A. Peraiah |
Relator term |
Supervisor |
9 (RLIN) |
48850 |
856 ## - ELECTRONIC LOCATION AND ACCESS |
Uniform Resource Identifier |
<a href="http://prints.iiap.res.in/handle/2248/100">http://prints.iiap.res.in/handle/2248/100</a> |
Link text |
Click Here to Access eThesis |
942 ## - ADDED ENTRY ELEMENTS (KOHA) |
Koha item type |
Thesis & Dissertations |
Source of classification or shelving scheme |
Dewey Decimal Classification |