Published August 1976
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Astronomical polarization studies at radio and infrared wavelengths. Part 1. Gravitational deflection of polarized radiation
Description
The gravitational field is probed in a search for polarization dependence in the light bending. This involves searching for a splitting of a source image into orthogonal polarizations as the radiation passes through the solar gravitational field. This search was carried out using the techniques of very-long- and intermediate baseline interferometry, and by seeking a relative phase delay in orthogonal polarizations of microwaves passing through the solar gravitational field. In this last technique a change in the total polarization of the Helios 1 carrier wave was sought as the spacecraft passed behind the Sun. No polarization splitting was detected
Availability note (English)
MF available from INIS under the Report Number; Available from NTIS., PC A05/MF 01.
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Additional details
Publishing Information
- Imprint Pagination
- 81 p.
- Report number
- N--77-13958
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 8341895
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- GENERAL RELATIVITY THEORY; GRAVITATIONAL FIELDS; MICROWAVE RADIATION; POLARIZATION; SUN
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; FIELD THEORIES; RADIATIONS; STARS
Optional Information
- Secondary number(s)
- NASA-CR--149215; CRSR--646-PT-1.