Implications of meteor observations by the MU radar

Geophysical Research Letters

Volumn 28, Issue 7, 2001, Pages 1399-1402

  Zhou, Qihou H ^a   Mathews, John D ^b   Nakamura, Takuji ^c  

^a ARECIBO OBSERVATORY   (Puerto Rico)

^b PENNSYLVANIA STATE UNIVERSITY   (United States)

^c KYOTO UNIVERSITY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

GEOMAGNETISM; RADAR; SCATTERING; UPPER ATMOSPHERE;

GEOMAGNETIC FIELD LINES;

GEOPHYSICS; RADAR;

METEORITE;

DETECTION LIMITS; FIELD-ALIGNED IRREGULARITIES; GEOMAGNETIC FIELD LINES; HIGH RESOLUTION; KYOTO UNIVERSITY; POTENTIAL ERRORS; SCATTERING STRUCTURES; TWO STREAM INSTABILITY;

EID: 0035302717     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2000GL012504     Document Type: Article

References (14)

1. Comparison of atmospheric parameters derived from meteor observations with CIRA
2. New narrow-beam meteor radar results at Christmas Island: Implications for diurnal wind estimation
3. Plasma wave excitation on meteor trails in the equatorial electrojet
4. Analysis of Perseid meteor head echo data collected using the advanced research projects agency long-range tracking and instrumentation radar (ALTAIR)
5. Evidence that meteor trails produce fields aligned scatter signals at VHF
6. A 50 MHz radio Doppler experiment for midlatitude E-region coherent backscatter studies: System description and first results
7. Doppler studies of near-antapex UHF radar meteors
8. Micrometeor observation using the Arecibo 430 MHz Radar: 1. Determination of the ballistic parameter from measured Doppler velocity and deceleration results
9. Development of an external interferometer for meteor wind observation attached to the MU radar
10. Electrodynamics of meteor trail evolution in the equatorial E-region ionosphere
11. Meteor fluxes and visual magnitudes from ESICAT radar event rates: A comparison with cross-section based magnitude estimates and optical data
12. Meteor trails induced backscatter in MST radar echoes
13. Simultaneous meteor echo observations by large aperture VHF and UHF radars