All-sky imaging of meteor trails at 55.25 MHz with the first station of the Long Wavelength Array

Authors


Abstract

A new capability for high-sensitivity, all-sky monitoring of VHF meteor trail reflections with the first station of the Long Wavelength Array, or “LWA1,” is described. LWA1 is a ∼100 m diameter HF/VHF array of 256 crossed-dipole antennas with a unique transient buffer mode that allows it to monitor for meteor trails via all-sky imaging with the same sensitivity as a single-dish antenna math formula in diameter. To demonstrate this capability, we have used a 2 h observing run conducted in August 2012 aimed at detecting and characterizing meteor trail reflections of analog TV transmissions at 55.25 MHz. The analysis techniques described here allowed for a detection rate of ∼9500 trails per hour, including the detection of two meteor streams with radiants in the Aries/Perseus and Aquila/Hercules regions that were not previously reported in the literature. In addition, we have found a population of relatively long-duration (∼1 to a few minutes), typically faint trails. These trails have implied horizontal speeds of 15–130 m s−1, with a typical speed of ∼30 m s−1. We have also used high-resolution time series of the brightest trails to characterize decay times over a relatively large geographical area (10°×7° in longitude and latitude) and on short (∼5 min) time scales. Potential enhancements that could be enabled by the addition of more LWA stations are discussed.

Ancillary