Peculiarities of using the TV broadcast signals for radar Doppler measurements of the drift velocity of meteor trails have been considered. A functional block diagram of the measuring apparatus for estimating the Doppler variations of the carrier frequency of TV broadcast signals reflected from drifting meteor trails was proposed. The developed apparatus made it possible for the first time to obtain the experimental proof of the possible use of TV broadcast signals for Doppler radiolocation of meteor trails and investigation of wind-induced motions at heights of the mesopause—lower thermosphere (80–105 km). It was shown that the variations of hourly average values of carrier frequencies of TV broadcast signals reflected from the meteor trai...
306-312A procedure for computing the Doppler frequency shift of the 54.95 MHz carrier under the mete...
The atmospheric motions in the 80-110 km height region, and methods of measuring them are discussed....
50-52Diurnal and day-to-day variation in meteor signal rates observed for a period of one year over ...
The possibility of using terrestrial television (TV) broadcast signals (TVBS) as sounding signals fo...
Summary The possibility of using terrestrial television (TV) broadcast signals (TVBS) as sounding si...
A coherent pulse radar has been addressed to the problem of tracking drifting meteor trains to deduc...
Determination of wind velocity by means of Doppler meteor radars is based on the assumption that an ...
Assuming that two VHF radio stations are communicating with each other via reflections from meteor t...
A new meteor wind radar system called Cyclone was devised to extend and update the meteor radar netw...
195-211A coherent Doppler, VHF radar specifically designed for scientific studies of atmospheric dyn...
This thesis details the application of a medium frequency (MF) Doppler radar to observations of mete...
We conducted meteor echo observations using the Buckland Park MF radar (35◦S, 138◦E) at 00:40–05:45 ...
A 50MHz doppler radar installed at Syowa Station, Antarctica, in 1982 acts as a meteor radar, when a...
This thesis details the development, construction and operation of a Doppler wind facility as an upg...
We conducted meteor echo observations using the Buckland Park MF radar (35◦S, 138◦E) at 00:40–05:45 ...
306-312A procedure for computing the Doppler frequency shift of the 54.95 MHz carrier under the mete...
The atmospheric motions in the 80-110 km height region, and methods of measuring them are discussed....
50-52Diurnal and day-to-day variation in meteor signal rates observed for a period of one year over ...
The possibility of using terrestrial television (TV) broadcast signals (TVBS) as sounding signals fo...
Summary The possibility of using terrestrial television (TV) broadcast signals (TVBS) as sounding si...
A coherent pulse radar has been addressed to the problem of tracking drifting meteor trains to deduc...
Determination of wind velocity by means of Doppler meteor radars is based on the assumption that an ...
Assuming that two VHF radio stations are communicating with each other via reflections from meteor t...
A new meteor wind radar system called Cyclone was devised to extend and update the meteor radar netw...
195-211A coherent Doppler, VHF radar specifically designed for scientific studies of atmospheric dyn...
This thesis details the application of a medium frequency (MF) Doppler radar to observations of mete...
We conducted meteor echo observations using the Buckland Park MF radar (35◦S, 138◦E) at 00:40–05:45 ...
A 50MHz doppler radar installed at Syowa Station, Antarctica, in 1982 acts as a meteor radar, when a...
This thesis details the development, construction and operation of a Doppler wind facility as an upg...
We conducted meteor echo observations using the Buckland Park MF radar (35◦S, 138◦E) at 00:40–05:45 ...
306-312A procedure for computing the Doppler frequency shift of the 54.95 MHz carrier under the mete...
The atmospheric motions in the 80-110 km height region, and methods of measuring them are discussed....
50-52Diurnal and day-to-day variation in meteor signal rates observed for a period of one year over ...