Abstract
The Stanford microwave interferometer is financed by the U.S. Air Force Office of Scientific Research under contract AF 18(603) -53 and is operated by the Stanford Radio Propagation Laboratory. Some eight persons, working under the direction of Dr. R. N. Bracewell, have carried out the design, construction, and current operation. The equipment is designed primarily for the observation of solar activity, which needs the highest possible resolution in both angle and time. At our wavelength range of 9 to 1 1 cm, the sun is by far the brightest celestial object, and it has also a moderate angular size. These circumstances permit observation with multiple antenna beams pointing in different directions without problems from confusion. These observations are achieved at moderate cost with a
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callMore From: Publications of the Astronomical Society of the Pacific
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
