The detection of equivalent interplanetary Type II and III events is the goal of the FARSIDE array. Solar radio bursts can be extremely luminous, and are likely the most intense sources of ...
Radio Observatory on the Lunar Surface for Solar Studies (ROLSS), is a concept for a near-side, low frequency, interferometric radio imaging array. It would be deployed during a lunar sortie or by a ...
The beam width (in radians) is roughly the wavelength of the radio wave divided by the diameter of the antenna. For example, a 100 meter antenna observing at a wavelength of 21 centimeters (a ...
Leung, a co-author of both papers, is a lead developer of three companion telescopes -- so-called outriggers -- to the original CHIME radio array located near Penticton, British Columbia.
Leung, a co-author of both papers, is a lead developer of three companion telescopes—so-called outriggers—to the original CHIME radio array located near Penticton, British Columbia.
CHIME currently has two online outrigger radio arrays in place—companion telescopes to the original CHIME radio array in British Columbia. A third array comes online this week in Northern ...
The Allen Telescope Array (ATA) is the first radio telescope to be designed from the ground up to be used for SETI searches.Until its construction, all radio SETI efforts were dependent on the ...
We describe here an approach for searching for PBH explosions using a low-frequency radio antenna array, and as a practical example, the results of such a search using the Eight-meter-wavelength ...