Published March 1972
| Version v1
Journal article
Large coherence intercontinental interferometry
Description
Compact radio sources have been observed over several years at 2.3 GHz by interferometers of the NASA-JPL Deep Space Network with trans- or inter-continental baselines to study the secular behaviour of fine structure appearing in these sources. A comparison of the variation in flux density of components of diameter < 0.001 arcsec with the corresponding variation in total flux density of the source at the same frequency indicated that variations could be wholly ascribed to components of this order of magnitude.
Additional details
Identifiers
Publishing Information
- Journal Title
- Publications of the Astronomical Society of Australia
- Journal Volume
- 2
- Journal Issue
- 2
- Series
- Proc. Astron. Soc. Aust.
- Journal Page Range
- 114-115
- ISSN
- 1323-3580
Conference
- Title
- Meeting of the Astronomical Society of Australia.
- Dates
- 13 Dec 1971.
- Place
- Adelaide, Australia.
INIS
- Country of Publication
- Australia
- Country of Input or Organization
- Australia
- INIS RN
- 3032974
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- COORDINATES; COSMIC RADIO SOURCES; ERRORS; GHZ RANGE 01-100; INTERFEROMETRY; POYNTING THEOREM; ZONES
- Descriptors DEC
- FREQUENCY RANGE; GHZ RANGE
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent