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

Author:

Helmboldt J. F.1,Ellingson S. W.2,Hartman J. M.3,Lazio T. J. W.3,Taylor G. B.45,Wilson T. L.1,Wolfe C. N.2

Affiliation:

1. US Naval Research Laboratory; Washington District of Columbia USA

2. Bradley Department of Electrical and Computer Engineering; Virginia Polytechnic Institute and State University; Blacksburg Virginia USA

3. Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA

4. Department of Physics and Astronomy; University of New Mexico; Albuquerque New Mexico USA

5. National Radio Astronomy Observatory; Socorro New Mexico USA

Publisher

American Geophysical Union (AGU)

Subject

Electrical and Electronic Engineering,General Earth and Planetary Sciences,Condensed Matter Physics

Reference47 articles.

1. Sporadic E signatures revealed from multi-satellite radio occultation measurements;Arras;Adv. Radio Sci.,2010

2. The absolute spectrum of CAS A-An accurate flux density scale and a set of secondary calibrators;Baars;Astron. Astrophys. Suppl.,1977

3. The modulation of sporadic-E layers by Kelvin-Helmholtz billows in the neutral atmosphere;Bernhardt;J. Atmos. Sol. Terr. Phys.,2002

4. Characteristics of radio echoes from meteor trails IV: Polarization effects;Billam;Proc. Phys. Soc.,1956

5. A meteoroid stream survey using the Canadian Meteor Orbit Radar-III. Mass distribution indices of six major meteor showers;Blaauw;Mon. Not. R. Astron. Soc.,2011a

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