@article{oai:nagano-nct.repo.nii.ac.jp:00000251,
 author = {OHNISHI, Kouji and ISHIKAWA, Toshiyuki and HATTORI, Shinobu and NISHIMURA, Osamu and MIYAZAWA, Akiko and YANAGISAWA, Masatoshi and ENDO, Makoto and KAWAMURA, Masaki and MARUYAMA, Toshiyuki and HOSAYAMA, Kai and TOKUNAGA, Mai and MAEGAWA, Kimio and ABE, Shinsuke},
 journal = {長野工業高等専門学校紀要},
 month = {Dec},
 note = {application, Ham-band Radio Observation (HRO) is one of the observational techniques for the forward scatter observation of meteors. We observe the meteor echo with two-element loop antennas (F/B ratio is 10 dB) at the Nagano National College of Technology (Nagano, JAPAN) using the continuous transmission of beacon signals for meteor observations at 53.750MHz, 50W from Fukui National College of Technology (Fukui, JAPAN). To prove that the radio echo is really the echo due to meteor, we construct the Direction Determination System using the paired antennas that can detect the direction roughly where the radio echo come from. The direction of one of this paired antennas was West toward Sabae and the other was East which has proved to be the most sensitive for this research. Using this system, we detected the change of the direction of reflection point of meteor radio signal of Geminids in 2000; from the westward to eastward before and after the culmination of the radiant which is consistent the formula of reflection point of meteors. At the same time, we detected the change of an intensity and a trend of the Doppler shift of meteor echoes. This result is consistent of the meteor wind data of MU Rader of Radio Science Center for Space & Atmosphere (RASC), Kyoto University.},
 pages = {93--100},
 title = {The Detection of the motion of radio meteor reflection point of Geminids by HRO},
 volume = {35},
 year = {2001}
}