THE POLARIZATION OF RADIO SOURCES AT 3.75 CENTIMETER WAVELENGTH. PDF Download
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Author: ROBERT WESLEY HOBBS
Publisher:
ISBN:
Category :
Languages : en
Pages : 261
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Book Description
Author: ROBERT WESLEY HOBBS
Publisher:
ISBN:
Category :
Languages : en
Pages : 261
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Author: R.W. Hobbs
Publisher:
ISBN:
Category :
Languages : en
Pages : 248
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Author: Richard Carl Bignell
Publisher: c1972.
ISBN:
Category : Polarization (Light)
Languages : en
Pages : 186
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Author: George Samuel Downs
Publisher:
ISBN:
Category : Polarization (Electricity)
Languages : en
Pages : 376
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Book Description
Author: F. F. Gardner
Publisher:
ISBN:
Category :
Languages : en
Pages : 18
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Book Description
Linear polarization measurements at 6 cm wavelength with the Parkes 210 ft telescope are given for 706 sources. Comparison of polarization parameters and flux densities with other published data is made. For the variable sources it is found that changes in polarized flux and position angle can accompany changes in intensity. (Author).
Author: G. L. Berge
Publisher:
ISBN:
Category :
Languages : en
Pages : 23
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Book Description
The two-element interferometer at the Owens Valley Radio Observatory was used in late 1967 to measure the integrated polarization, both linear and circular, of 32 extragalactic radio sources at a wavelength of 3.12 cm. In addition, flux densities of 103 radio sources were also measured. (Author).
Author: F. F. Gardner
Publisher:
ISBN:
Category : Radio sources (Astronomy)
Languages : en
Pages : 36
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Author: P. Maltby
Publisher:
ISBN:
Category :
Languages : en
Pages : 5
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The interferometer at the Owens Valley Radio Observatory has been used to study the linear polarization of 54 radio sources at a wavelength of 10.6 cm. The measurements were made with two 90-ft antennas spaced 100 feet (289 lambda) in the east-west direction. (Author).
Author: F. F. Gardner
Publisher:
ISBN:
Category :
Languages : en
Pages : 7
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Book Description
The dependence on galactic latitude of the 11 and 20 cm polarization of 355 extragalactic sources reveals no definite evidence of depolarization within the Galaxy. The distribution of Faraday rotation can be explained in terms of a field along the local spiral arm, deformed by magnetic 'loops' in the solar neighbourhood. (Author).
Author: Daniel R. Altschuler
Publisher:
ISBN:
Category : Polarization (Light)
Languages : en
Pages : 67
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