Planned improvements to the Owens Valley frequency-agile interferometer

Details Planned improvements to the Owens Valley frequency-agile interferometer Planned improvements to the Owens Valley frequency-agile interferometer

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988fnsm.work...98h&link_type=abstract

In NASA, Goddard Space Flight Center, Max 1991: Flare Research at the Next Solar Maximum. Workshop 1: Scientific Objectives p 98

Computer Science

Antenna Arrays, Equipment Specifications, Interferometers, Magnetic Fields, Microwave Spectrometers, Solar Corona, Brightness Temperature, Emission Spectra

Scientific paper

Three small antennas will be added to the OVRO interferometer to form a five-element solar-dedicated array. This would provide up to 7 or 10 baselines (compared to the present 1 or 3). This would be sufficient to apply microwave diagnostics to most active region and burst sources. By using frequency-synthesis it would also provide an imaging capability comparable to that of an approximately 100 baseline interferometer. Expansion of the array is discussed.

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