Abstract
The activity of the Lyrid meteor shower is analyzed by visual observations in the interval 1900–2007. Processing of observations over a long time interval confirmed the presence of two periods of activity of the shower, of 12 and 60 years. These periods almost coincide with the period and five times Jupiter’s orbital period, i.e., 11.8 and 59.3 years, respectively, suggesting the possible influence of Jupiter on the shower structure. High activity of the shower is observed when the epoch of observations and the commensurate moment coincide with the orbital period of Jupiter and can be registered in the next 1–2 years. The increased activity of Lyrid by visual observations suggests that ZHR exceeds 30 meteors per hour. The modeling of activity profiles of showers for different minimum masses of meteoroids has shown that there is a correlation between the longitude of the node from the orbit with the mass of particles.
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Arter, T.R. and Williams, I.P., April Lyrids, Mon. Notic. Roy. Astron. Soc., 1995, vol. 277, pp. 1087–1096.
Babadzhanov, P.B., Fragmentation and Densities of Meteoroids, Astron. Astrophys., 2002, vol. 384, pp. 317–321.
Bel’kovich, O.I., Ishmukhametova, M.G., and Suleymanov, N.I., Comparative Analysis of Meteor Shower Observations Processed by Three Different Methods, Proc. Int. Conf. “Meteoroids 2001”, Kiruna, 2001, pp. 91–93.
Bel’kovich, O.I., Ishmukhametova, M.G., and Suleimanov, N.I., Present-Day Methods of Processing of Visual Observations of Meteor Streams and Their Potentialities, Astron. Vestn., 2001, vol. 35, no. 5, pp. 440–448 [Solar Syst. Res. (Engl. Transl.), 2001, vol. 35, no. 5, p. 400].
Bel’kovich, O.I. and Ishmukhametova, M.G., Mass Distribution of Lyrid Meteoroids, Astron. Vestn., 2010, vol. 44, no. 4, pp. 345–351 [Solar Syst. Res. (Engl. Transl.), 2010, vol. 44, no. 4, p. 320].
Ceplecha, Z., Meteoroid Properties from Photographic Records of Meteors and Fireball, Proc. Int. Conf. “Asteroids, Comets, Meteors 1993”, Belgirate, June 14–18, 1993, pp. 343–349.
Dubietis, A. and Arlt, R., The Lyrids in 2003, WGN, J. Int. Meteor Organ., 2003, vol. 31, pp. 97–98.
Emel’yanenko, V.V., Dynamic of Lyrid Meteor Swarm, Astron. Vestn., 1990, vol. 24, no. 4, pp. 308–313.
Emel’yanenko, V.V., Resonance Structure of Meteoroid Streams, Proc. Meteoroids-2001 Conf., Kiruna: Swedish Inst. of Space Physics, Aug. 6–10, 2001, pp. 43–45.
GOST (State Standard) 25645.128-85: Metheoritic Matter. Model of Spatial Distribution, 1985, p. 21.
Guth, V., On the Periodicity of Lirids, Bull. Astron. Inst. Czechosl., 1947, vol. 1, pp. 1–4.
Jenniskens, P., Meteor Stream Activity. I. The Annual Streams, Astron. Astrophys., 1994, vol. 287, pp. 990–1013.
Mularczyk, K., 2004 Lyrids in CMW’s Visual Observations, WGN, J. Int. Meteor Organ., 2005, vol. 33, pp. 72–74.
Opik, E.J., Analysis of 1436 Meteor Velocities, Publ. Observ. Astron. Tartu, 1940, vol. 30, p. 33.
Opik, E.J., The Distribution of Meteor Stream Intensity over the Celestial Sphere, Mem. Soc. Roy. Soc., 1955, vol. 15, pp. 147–173.
Porubčan, V., Štohl, J., and Svoren, J., On the Origin of the 1982 Lyrids Burst, Contr. Astron. Obs. Skalnate Pleso, 1992, no. 22, pp. 25–31.
Porubčan, V., Hajduk, A., Cevolani, G., et al., Lyrids 1994 Observed by a Forward Scatter System, Earth, Moon, Planets, 1995, vol. 68, pp. 465–469.
Prentic, J.P.M., The Hourly Rate of Quadrantid Meteor Shower at Maximum, J. Brit. Astron. Assoc., 1953, vol. 63, no. 5, pp. 175–186.
Rendtel, J. and Arlt, R., The Lyrid Meteor Shower in 2006 and 2007, WGN, J. Int. Meteor Organ., 2007, vol. 35, pp. 74–77.
Schiaparelli, J.V., Entwurf einer astronomischen Theorie der sternschnuppen, Stettin: Th. v. d. Nahmer, 1871.
Tokhtas’ev, V.S., Mass Scales for Radio Meteors, Visual and Photographic Masses, Trudy Vsesoyuznogo simpoziuma “Problemy radiometricheskikh issledovanii atmosfery” (Proc. All-Union Symp. “Problems of Radiometric Researches of the Atmosphere”), Kharkov, 1977, p. 26.
Tokhtas’ev, V.S., Meteor Solids Densities in Meteor Swarms, in Meteornoe veshchestvo v mezhplanetnom prostranstve (Meteor Matter in Interplanetary Space), Moscow, 1982, pp. 184–189.
Verniani, F., Meteor Masses and Luminosity, Smithson. Contr. Astrophys., 1967, vol. 10, pp. 181–195.
Visual Meteor Database, Int. Meteor Organ, Available from: http://www.imo.net/data/visual
Zvolankova, J., Dependence of the Observed Rate of the Meteors on the Zenith Distance of the Radiant, Bull. Astron. Inst. Czechosl., 1983, vol. 34, no. 2, pp. 122–131.
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Original Russian Text © O.I. Bel’kovich, M.G. Ishmukhametova, E.D. Kondrat’eva, 2011, published in Astronomicheskii Vestnik, 2011, Vol. 45, No. 6, pp. 542–551.
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Bel’kovich, O.I., Ishmukhametova, M.G. & Kondrat’eva, E.D. On activity periods of the April Lyrids. Sol Syst Res 45, 529–538 (2011). https://doi.org/10.1134/S0038094611050029
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DOI: https://doi.org/10.1134/S0038094611050029