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
Kostelecky and Mewes have recently shown that sensitive constraints can be placed on some aspects of...
The whole-disk polarization of Uranus was measured over two apparitions in blue and red light. The b...
Polarization has been a powerful diagnostic tool in radio, microwave, and visible astronomy, providi...
Far infrared polarization of dust clouds is examined. The recently observed 10 micron polarization o...
Because observations of the Kleinmann-Low region of the Orion Nebula reveal significant polarization...
Polarization is a basic property of light and is fundamentally linked to the internal geometry of a ...
Terrestrial radiation measurements obtained with planetary radio astronomy experiments on Voyager-1 ...
The implications of the 10 micron polarization of the Orion Nebula were re-examined. The polarizatio...
The Dominion Radio Astrophysical Observatory Deep Field polarization study has been matched with the...
Elongated dust grains aligned by local magnetic fields are though to absorb background radiation and...
This research was supported by the Undergraduate Research Opportunities Program (UROP)
Original paper can be found at: http://161.58.115.79/pubs/cs/328.html--Copyright Astronomical Societ...
Polarization observations of the cosmic microwave background with the Cosmic Background Imager from ...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/328.html Copyright ASPAn outline...
Context. We investigate the linear polarization produced by interstellar dust aligned by the magneti...
Kostelecky and Mewes have recently shown that sensitive constraints can be placed on some aspects of...
The whole-disk polarization of Uranus was measured over two apparitions in blue and red light. The b...
Polarization has been a powerful diagnostic tool in radio, microwave, and visible astronomy, providi...
Far infrared polarization of dust clouds is examined. The recently observed 10 micron polarization o...
Because observations of the Kleinmann-Low region of the Orion Nebula reveal significant polarization...
Polarization is a basic property of light and is fundamentally linked to the internal geometry of a ...
Terrestrial radiation measurements obtained with planetary radio astronomy experiments on Voyager-1 ...
The implications of the 10 micron polarization of the Orion Nebula were re-examined. The polarizatio...
The Dominion Radio Astrophysical Observatory Deep Field polarization study has been matched with the...
Elongated dust grains aligned by local magnetic fields are though to absorb background radiation and...
This research was supported by the Undergraduate Research Opportunities Program (UROP)
Original paper can be found at: http://161.58.115.79/pubs/cs/328.html--Copyright Astronomical Societ...
Polarization observations of the cosmic microwave background with the Cosmic Background Imager from ...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/328.html Copyright ASPAn outline...
Context. We investigate the linear polarization produced by interstellar dust aligned by the magneti...
Kostelecky and Mewes have recently shown that sensitive constraints can be placed on some aspects of...
The whole-disk polarization of Uranus was measured over two apparitions in blue and red light. The b...
Polarization has been a powerful diagnostic tool in radio, microwave, and visible astronomy, providi...