THE LONG WAVELENGTH ARRAY SOFTWARE LIBRARY

The Long Wavelength Array System

Flaring Stars and the Long Wavelength Array

Coherent emission appears to be a common phenomenon on radio-active late-type stars. Solar radio flare emissions below 3 GHz are rich and varied, arising from coherent processes in the upper solar atmosphere (Dulk 1985; Isliker & Benz 1994). Studies of decimetric radio emission from M dwarf flare stars have led to discovery of high brightness temperature, highly circularly polarized bursts (Bas...

A Strawman Design for the Long Wavelength Array Stations

This document presents a “strawman” design for the Long Wavelength Array (LWA) stations.

Temporal and spatial changes of incoming solar short-wave wavelength and long-wave wavelength in the region of Iran

The smallest change in energy exchange of Earth System Shifts the balance of life. In order to be aware of the solar radiation Balance, Recognition of the measure of Balance level of the input and output components of radiation of input Short wavelength to the surface of the earth and Long Output Wavelength, it is necessary from the earth. To study the energy balance of input and output in Iran...

Passive over-the-horizon radar with WWV and the first station of the Long Wavelength Array

We present a new passive, over-the-horizon (OTH) radar system consisting of the transmitters for the HF radio station WWV and the dipole-antenna array that comprises the first station of the Long Wavelength Array (LWA), or “LWA1.” We demonstrate that these two existing facilities, which are operated for separate purposes, can be used together as a relatively powerful bistatic, HF radar, capable...