The Owens Valley Long Wavelength Array (OVRO-LWA) is a low-frequency radio interferometer ... of the epoch of reionization and fast-cadence all-sky imaging for the detection of low frequency ...

The emission is produced at the fundamental and first harmonic of the plasma frequency and thus ... CMEs and SEP events. The detection of equivalent interplanetary Type II and III events is the goal ...

Urania's proposed gravitational wave detectors span a broad frequency range — from 10 to 5000 Hz — capturing signals from a wide array of cosmic events, according to the new study. This range ...