Results 21 to 30 of about 20,282 (172)

Canadian Meteor Orbit Radar (CMOR) [PDF]

open access: yesAtmospheric Chemistry and Physics, 2004
The radar system described here (CMOR) comprises a basic 5-element receiving system, co-located with a pulsed transmitter, specifically designed to observe meteor echoes and to determine their position in space with an angular resolution of ~1° and a radial resolution of ~3 km.
A. R. Webster   +5 more
openaire   +6 more sources

Initial Results of Meteor Wind with Langfang Medium Frequency Radar

open access: yesAtmosphere, 2020
We conducted meteor observations during the Leonid meteor shower on 16 November 2017 and 17 November 2018 with Langfang medium frequency (MF) radar (116° E, 40° N). This was the first nighttime meteor observation by MF radar in mid-latitude China.
Bing Cai   +3 more
doaj   +1 more source

The sporadic radiant and distribution of meteors in the atmosphere as observed by VHF radar at Arctic, Antarctic and equatorial latitudes [PDF]

open access: yesAnnales Geophysicae, 2009
Results are presented of a study of the temporal and spatial variability in meteor count rate observations from three VHF meteor radars. These radar are located in the Arctic (at Esrange, 68° N), in the Antarctic (at Rothera, 68° S) and near ...
P. T. Younger   +3 more
doaj   +1 more source

Comparison between the Mesospheric Winds Observed by Two Collocated Meteor Radars at Low Latitudes

open access: yesRemote Sensing, 2022
This study compares the hourly mesospheric horizontal winds observed by two collocated and independent low-latitude meteor radars operating at 37.5 MHz and 53.1 MHz in Kunming, China (25.6°N, 103.8°E). Upon analyzing simultaneously detected meteor echoes,
Jie Zeng   +8 more
doaj   +1 more source

A comparison of MLT wind between meteor radar chain data and SD-WACCM results

open access: yesEarth and Planetary Physics, 2022
A meteor radar chain located along the 120°E meridian in the Northern Hemisphere from low to middle latitudes provides long-term horizontal wind observations of the mesosphere and lower thermosphere (MLT) region.
BaoZhu Zhou   +8 more
doaj   +1 more source

First results of optical meteor and meteor trail irregularity from simultaneous Sanya radar and video observations

open access: yesEarth and Planetary Physics, 2018
Meteoroids entering the Earth's atmosphere can create meteor trail irregularity seriously disturbing the background ionosphere. Although numerous observations of meteor trail irregularities were performed with VHF/UHF coherent scatter radars in the past,
GuoZhu Li   +6 more
doaj   +1 more source

Multi-instrument observations of the Pajala fireball: Origin, characteristics, and atmospheric implications

open access: yesFrontiers in Astronomy and Space Sciences, 2022
Meteor observations provide information about Solar System constituents and their influx onto Earth, their interaction processes in the atmosphere, as well as the neutral dynamics of the upper atmosphere.
Juha Vierinen   +14 more
doaj   +1 more source

Identifying gravity waves launched by the Hunga Tonga–Hunga Ha′apai volcanic eruption in mesosphere/lower-thermosphere winds derived from CONDOR and the Nordic Meteor Radar Cluster [PDF]

open access: yesAnnales Geophysicae, 2023
The Hunga Tonga–Hunga Ha′apai volcano eruption was a unique event that caused many atmospheric phenomena around the globe. In this study, we investigate the atmospheric gravity waves in the mesosphere/lower-thermosphere (MLT) launched by the volcanic ...
G. Stober   +15 more
doaj   +1 more source

Validation of MIGHTI/ICON Atmospheric Wind Observations over China Region Based on Meteor Radar and Horizontal Wind Model (HWM14)

open access: yesAtmosphere, 2022
The Michelson Interferometer for Global High-resolution Thermospheric Imaging (MIGHTI) on board the ICON satellite provides effective measurement of horizontal winds in the mesosphere and lower thermosphere (MLT) region.
Zhou Chen   +5 more
doaj   +1 more source

Recombination in Radar Meteors [PDF]

open access: yesInternational Astronomical Union Colloquium, 1971
Recombination of the Electrons in the ionized column has often been considered (see, for example, Öpik, 1955), but the uncertainties in the atomic and molecular species present and in the rate constants have made it difficult to predict. Furthermore, recombination has not been recognized in the observations, so that it has been judged to be negligible (
openaire   +1 more source

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