11 |
A high sensitivity study of the galactic north polar region at 1415 MHz /Scheer, Donald Jordan January 1966 (has links)
No description available.
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The nature and the statistical properties of the faint radio populationGeorgakakis, Antonis January 1999 (has links)
No description available.
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Polarization of Radio Sources. I. Transfer of synchrotron Radition through an Extended Radio Source with Faraday Rotation|Polarization of Radio Sources. I. Homogeneous Source of Arbitrary Optical ThicknessPacholczyk, A. G., Swihart, T. L. 11 1900 (has links)
The problem of transfer of radiation in a medium with polarized emission,
polarized absorption and Faraday rotation of the plane of polarization
is formulated. Solutions are obtained for the case of a homogeneous source.
In the range of frequencies for which a medium is optically thick the degree
of polarization of synchrotron radiation depends on the type of absorption
process and is different for synchrotron absorption and for thermal absorption.
It is therefore suggested that the low frequency polarization
measurements of radio sources with curved spectra may determine whether
synchrotron self -absorption or thermal absorption or another process is
responsible for the low frequency curvature in spectra of certain radio
sources.
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Robotic localization of hostile networked radio sources with a directional antennaHu, Qiang 25 April 2007 (has links)
One of the distinguishing characteristics of hostile networked radio sources (e.g.,
enemy sensor network nodes), is that only physical layer information and limited
medium access control (MAC) layer information of the network is observable. We
propose a scheme to localize hostile networked radio sources based on the radio signal
strength and communication protocol pattern analysis using a mobile robot with a
directional antenna. We integrate a Particle Filter algorithm with a new sensing
model which is built on a directional antenna model and Carrier Sense Multiple
Access (CSMA)-based MAC protocol model. we model and analyze the channel
idle probability and busy collision probability as a function of the number of radio
sources in the CSMA protocol modeling. Based on the sensing model, we propose a
particle-filter-based scheme to simultaneously estimate the number and the positions
of networked radio sources. We provide a localization scheme based on the method
of steepest descent for the purpose of performance comparison. Simulation results
demonstrate that our proposed localization scheme has a better success rate than the
scheme based on the steepest descent at different tolerant distances.
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15 |
Using radio sources to find galaxy clustersGay, Pamela Lynn 28 August 2008 (has links)
Not available / text
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16 |
Observations of molecular clouds in the direction of galactic and extragalactic radio sourcesNash, Ana Gomes. January 1986 (has links)
Thesis (Ph. D.)--University of Wisconsin--Madison, 1986. / Typescript. Vita. eContent provider-neutral record in process. Description based on print version record. Includes bibliographical references (leaves 62-63).
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Radio spectral line studies of the interstellar medium in the galactic planeSeacord, Andrew Wilkin, January 1975 (has links)
Thesis--University of Florida. / Description based on print version record. Typescript. Vita. Includes bibliographical references (leaves 226-233).
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18 |
Host galaxies and environments of compact extragalactic radio sources /Labiano, Álvaro. January 2006 (has links)
Thesis (Doctoral)--Rijksuniversiteit Groningen, 2006. / Bibliography: p. [143]-158.
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Radio spectral characteristics of extragalactic objects /Pacht, Erich January 1980 (has links)
No description available.
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Polarization of Radio Sources. II. Faraday Effect in the Case of Quasitransverse PropagationPacholczyk, A. G., Swihart, T. L. January 1970 (has links)
Under the conditions of quasitransverse propagation of electromagnetic
waves in a magnetoionic plasma, the effect analogous to Faraday
rotation in the quasilongítudinal case (which we will call Faraday pulsation)
can produce a large elliptical polarization of originally linearly
polarized radiation. Therefore, the presence of elliptical polarization
in the radiation cannot serve as a means for distinguishing between a
synchrotron mechanism with high energy electrons and any other type of
emission process in radio sources in which conditions suggesting quasi -
transverse propagation (large magnetic fields) may take place. The
Faraday pulsation has a wavelength dependence through which it can be
identified.
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