▪ Abstract Radio astronomy has provided evidence for the presence of ionized atmospheres
around almost all classes of nondegenerate stars. Magnetically confined coronae dominate …

Abstract The Very Large Array Sky Survey (VLASS) is a synoptic, all-sky radio sky survey
with a unique combination of high angular resolution (≈ 2 farcs 5), sensitivity (a 1σ goal of …

Significant new opportunities for astrophysics and cosmology have been identified at low
radio frequencies. The Murchison Widefield Array is the first telescope in the southern …

Transient radio sources are necessarily compact and usually are the locations of explosive
or dynamic events, therefore offering unique opportunities for probing fundamental physics …

Abstract Single-bubble sonoluminescence (SBSL,,,,) results from the extreme temperatures
and pressures achieved during bubble compression; calculations have predicted, the …

EMU is a wide-field radio continuum survey planned for the new Australian Square
Kilometre Array Pathfinder (ASKAP) telescope. The primary goal of EMU is to make a deep …

White dwarfs are compact stars, similar in size to Earth but approximately 200,000 times
more massive. Isolated white dwarfs emit most of their power from ultraviolet to near-infrared …

We discuss optimal detection of fast radio transients from astrophysical objects while taking
into account the effects of propagation through intervening ionized media, including …

Radiation belts are present in all large-scale Solar System planetary magnetospheres:
Earth, Jupiter, Saturn, Uranus and Neptune. These persistent equatorial zones of relativistic …

Aurorae are detected from all the magnetized planets in our Solar System, including Earth.
They are powered by magnetospheric current systems that lead to the precipitation of …