Zobrazeno 1 - 10
of 17
pro vyhledávání: '"L. V. Kurnosova"'
Autor:
A. I. Karakash, M. I. Fradkin, M. F. Runtso, A. G. Labenskii, Vladimir Kaplin, N. P. Topchiev, S.K. Chernichenko, L. V. Kurnosova, I. V. Shein, Vitalii L Ginzburg, A. P. Soldatov
Publikováno v:
Cosmic Research. 45:449-451
Autor:
L. F. Kalinkin, E. I. Chuikin, M.A. Russakovitch, N. G. Leikov, V. Y. Tugaenko, M. I. Fradkin, I. D. Blokhintsev, L. V. Kurnosova, A. R. Bazer-Bachi, V.G. Afanassyev, A. M. Galper, V. A. Rud'Ko, Nikolay Topchiev, V. M. Zemskov, J. F. Olive, J.-M. Lavigne, V. E. Nesterov, M. Gros, V. V. Akimov, M. F. Runtso, Yu. V. Ozerov
Publikováno v:
Advances in Space Research. 13:739-742
The Geminga light curve obtained with the “Gamma-1” telescope features two peaks separated by 0.5 ± 0.03 period. The light curve is pronounced for γ-quanta energies higher than 400 MeV. The pulsed flux upper limit (1σ) in the energy interval 5
Autor:
P.P Ignatiev, V. L. Ginzburg, L. V. Kurnosova, E. V. Gorchakov, L. A. Razorenov, Vladimir Kaplin, Nikolay Topchiev, M. A. Rusakovich, M. I. Fradkin, M. F. Runtso, A. G. Labensky
Publikováno v:
Advances in Space Research. 15:93-94
The observation of the galactic anticenter region by the balloon borne gamma-ray telescope Natalya-I
Autor:
V. G. Kirillov-Ugryumov, B. V. Sreekantan, S. V. Damle, Yu. D. Kotov, L. V. Kurnosova, Yu. V. Smirnov, A. F. Iyudin, G. S. Gokhale, M. I. Fradkin, P. K. Kunte
Publikováno v:
Advances in Space Research. 3:53-56
This paper presents the results of measurements of gamma radiation with energies above 5 MeV, from the galactic anticenter region. The balloon-borne gamma ray telescope “Natalya-I”, was launched on 6 November, 1980 from the Tata Institute of Fund
Autor:
V. I. Logachev, P. K. Kunte, A. M. Galper, L. V. Kurnosova, B. V. Sreekantan, N. G. Leikov, V. G. Kirillov-Ugryumov, A. V. Kurochkin, M. I. Fradkin, Yu. D. Kotov, L. A. Razorenov, S.V. Damle, Yu. V. Smirnov
Publikováno v:
Advances in Space Research. 1:101-106
The report presents some results on the cosmic radiation intensity research carried out with the high-altitude balloons for the period of 1977–1979. The intensity of gamma-radiation with the energy above 40 MeV was measured in two balloon flights a
Publikováno v:
Uspekhi Fizicheskih Nauk. 63:131-148
Publikováno v:
Fortschritte der Physik. 7:145-164
Short-Lived Intensity Increase of the Nuclear Component of Cosmic Rays as a Result of Solar Activity
Publikováno v:
ARS Journal. 32:831-834
T SECOND cosmic rocket contained equipment described in Ref. 1 for investigating the nuclear component of cosmic rays. This equipment consisted of two independently operating devices. The two devices were Cherenkov counters provided for recording nuc
Autor:
Yu. D. Kotov, Yu. V. Smirnov, V. G. Kirillov-Ugryumov, M. I. Fradkin, S.V. Damle, L. V. Kurnosova, A. F. Iyudin, Vitaly Yurov
Publikováno v:
Advances in Space Research. 6:173-175
A low mass wire spark chamber gamma ray telescope “Natalya-1” was launched on a balloon flight on November 6, 1980 from Hyderabad, India (Geomagnetic cut-off rigidity R ⋍ 16.8 GV ). The galactic anti-center region was observed during the balloo
Autor:
V. B. Kotova, M. F. Runtso, S. A. Voronov, S. V. Repin, V. M. Balebanov, I. A. Gerasimov, N. G. Leikov, V. V. Akimov, N. K. Mordvov, I. D. Blokhintsev, V. A. Volzhenskaya, S. R. Tabaldiev, M. I. Fradkin, M. B. Dobrijan, M. A. Rusakovich, Yu. T. Yurkin, A. S. Belousov, V. G. Rodin, L. F. Kalinkin, O. F. Prilutsky, V. G. Zverev, V. D. Kozlov, Y. M. Lavigne, V. P. Poluektov, L. V. Kurnosova, A. Popov, V. A. Grigoriev, V. Yu. Tugaenko, M. Gros, Nikolay Topchiev, E. I. Chuikin, A. R. Bazer-Bachi, P. Masse, J. P. Leray, V. E. Nesterov, Yu. I. Nagornih, B. Parlier, A. V. Serov, V. M. Zemskov, Yu. V. Ozerov, V. L. Prokhin, I. V. Kalinin, V. G. Kirillov-Ugriumov, A. M. Galper, F. Soroka
Publikováno v:
Space Science Reviews. 49
The ‘Gamma-1’ telescope has been developed through a collaboration of scientists in the USSR and France in order to conduct γ-ray astronomical observations within the energy range from 50 to 5000 MeV. The major characteristics of the telescope w