Centenary of the birth of the famous Ukrainian researcher of radiometeors prof. B.L. Kashcheyev (1920-2004), his heritage and trajectory measurements today
DOI:
https://doi.org/10.18524/1810-4215.2020.33.217120Ключові слова:
meteors, ionosphere, trajectory measure- ments, meteor radar, Kashcheyev heritageАнотація
The development of meteor radar research was stimulated during World War II by air
defense requests to rule out false alarms of radars on meteoroid intrusions. After the war, many air defense radars were involved in scientific observations of meteors. An additional stimulus for interest in the study of radiometeors was the phenomenon of the Draconid meteor shower in 1946, which was recorded by the radio method as extraordinary. We can talk about the scientific and technological revolution of this period, associated with the use and boom in the development of radio technology and missile technology. The ballistics of the movement of airborne objects in the Earth’s atmosphere (and outside the atmosphere since 1957) of artificial and natural origin is becoming increasingly complex. Radio technology could not have developed without knowledge of the ionosphere and the effects of the Sun on radio communications, along with the effects of the Sun on the ionosphere. In the ionosphere, a layer at altitudes of 70-130 km is called the meteor zone, i.e. the zone where cosmic bodies, burning in the Earth’s atmosphere, cause the appearance of ionized meteor tracks, which interact with radar radiation and reflect it. This allows the radar receiver to record the reflected signal. In the presence of three receivers spaced 3-5 km apart (and located approximately at the vertices of a right triangle), it is possible to determine the guiding cosines of the trajectory of the meteoroid in the Earth’s atmosphere. Continuing the trajectory of the meteoroid to the intersection with the celestial sphere at infinity, we obtain a point called the meteor radiant. In basic optical meteor observations, the trajectory is determined differently than in the radio method. The article highlights the significance of the event of the centenary of the birth of the famous Ukrainian researcher of radiometeors Prof.KashcheyevB.L. ˙ (1920-2004) anditslegacy, aswell as the problems and solutions of trajectory measurements today.
Посилання
Andreev V.V., Babadzhanov P.B., Barsukov V.L. et al.: 1987, GOST25645.128-85.Meteorsubstance, spatial distribution model,M.:Izd.standartov, 23p.
Astapovich I.S.: 1958, Meteor phenomena in the atmosphere of the Earth, M.: Fizmatgiz, 640 p.
Bouquet A., Baratoux D., Vaubaillon J. et al.: 2014, Planetary and Space Science, 103, 238.
Catalog: Dec. 1968 – Jul. 1970, Moscow, 1975, 167.
Ceplecha Z.: 1987, Bull. of the Astron. Inst. Of Czechoslovakia, 38, 222.
Clark D., Wiegert P.: 2011, Meteorit. Planet. Sci., 46, 1217.
Gural V.P.: 2012, Planetary Science, 9, 1405.
Dmitriev V., Lupovka V., Gritsevich M.: 2015, Planetary and Space Science, 117, 223.
Hocking W.K., Kolomiyets S.V.: 2020, Radiotekhnika: All-Ukr. Sci. Interdep. Mag., 201, 78.
Fedynsky V.V., Kashcheyev B.L., Voloshchuk Yu.I. et al.: 1976, Bull. of the USSR Academy of Sciences, 10, 89.
Jenniskens P. S., Gural L., Dynneson B. J. et al.: 2016, Icarus, 40.
Kashcheyev B.L., Koval Yu.O., Gorbach V.I. et al.: 1996, Meteors today, K.: Tekhnika, 196 p.
Kashcheyev B.L., Nechitaylenko V.A.: 1983, Meteor research, 8.
Kashcheyev B.L., Lebedinets V.N., Lagutin M.F. et al.: 1967, Meteor phenomena in the Earth’s atmosphere, M.: Nauka, 260p.
Kashcheyev B.L., Tkachuk A.A.: 1980, Catalogue of meteor orbits to +12M, Moscow, 232 p.
Kashcheyev B.L., Tsesevich V.P.: 1965, The study of circulation of atmosphere in the meteor zone. Instruction manual, M.: Nauka, 64 p.
Kashcheyev B.L., Voloshchuk Yu.I., Dudnik B.S. et al.: 1977, Meteor research, 4, 11.
Kolomiyets S.V.: 2012, IEEE, 46.
Kolomiyets S.V.: 2018, in: Proc. of the IAU Simposium 339, New York, 14, 215.
Kolomiyets S.V.: 2003, Scientific-encyclopedic vision /Ed. I.B. Vavilova & Plachinda, Lviv, Kyiv, 654 p.
Kolomiyets S.V., Voloshchuk Yu.I., Slipchenko M.I. et al.: 2016, Radiotekhnika, 184, 6.
Kruchinenko V.G.: 2012, Mathematical and physical analysis of the meteoric phenomenon: monograph, MAO NASU, K.: Nauk. Dumka, 294 p.
Lebedev T.S., Sollogub V.B.: 1960, Informatsionnyy byulleten’ (Newsletter), 2, 3.
Levin B.Yu.: 1956, Physical theory of meteors and meteoric matter in the solar system, Publ. house of the Academy of Sciences of the USSR, 293 p.
List of objects that make up the national heritage: 2013, NAS of Ukraine [Electronic resource].
Moreno-Ibᘠne M. et al. 2020, MNRAS, 494, 316.
Narziev M.: 2019, Planetary and Space Science, 173.
Novoselova N.V., Tkachuk A.A.: 1971, Radiotekhnika, 16, 18.
OvezgeldyevO.G.,KashcheyevB.L.,NechitaylenkoV.A. et al.: 1986, Radiotekhnika, 9, 83.
Sansom et al.: 2019 ApJ, 885, 115.
Sidorov V.V., Kolomiyets S.V.: 2007, in: Proc. IEU SS5 Cambridge Univ. Press, 189.
Simonenko A.N.: 1975, Atlas, 68.
Tsesevich V.P.: 1957, International Geophysical Year [1957-1958], M.: Gostekhizdat, 184 p.
Tsesevich V.P.: 1957, Astronomical problems of the International Geophysical Year, M.: Znanije, 40 p.
Voloshchuk Yu.I., Kashcheyev B.L., Kruchinenko V.G.: 1989, Meteors and meteor substance, K.: Nauk.
dumka, 296 p.
Voloshchuk Yu.I., Kolomiyets S.V., Cherkas Yu.V.: 2018, Analysis of data on the small bodies of the solar system using information radio technologies: Catalog of meteor orbits. monograph., 344. DOI:10.30837/978-966-659-249-4 Corpus ID: 213952314.
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