Zobrazeno 1 - 10
of 13
pro vyhledávání: '"B. N. Bakhtin"'
Publikováno v:
Solar System Research. 56:291-298
Autor:
A. B. Sanin, I. G. Mitrofanov, A. A. Anikin, S. Yu. Nikiforov, Dmitry Golovin, B. N. Bakhtin, Maxim Litvak
Publikováno v:
Solar System Research. 54:477-487
The article proposes a “tagged cosmic particle” method that uses the natural flux of high-energy particles of Galactic Cosmic Rays to study the composition of the near-surface soil layer of a celestial body by gamma spectrometry methods, with a h
Autor:
Yu. I. Bobrovnitskii, I. A. Karpov, A. S. Grebennikov, S. A. Asfandiyarov, B. N. Bakhtin, A. A. Kim, T. M. Tomilina
Publikováno v:
Acoustical Physics. 66:324-332
The article describes an experimental facility for studying and testing sound-absorbing linings made of acoustic metamaterials designed to reduce the noise generated by a source in a finite waveguide. The main focus is on the features of acoustic fie
In April 2001 Mars Odyssey spacecraft with High Energy Neutron Detector (HEND) onboard was launched to Mars. HEND/Odyssey was switched on measurement mode most of transit to Mars to monitor variations of spacecraft background and solar activity. Alth
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5bde8bd4846d0fefbd457a20cd0959f8
https://doi.org/10.5194/epsc2020-972
https://doi.org/10.5194/epsc2020-972
It is well known that methods of nuclear physics allow one to study distribution of hydrogen-bearing compounds in the upper 1–2 m subsurface soil layer of atmosphereless celestial bodies or planets with thin atmospheres like Mars by measuring neutr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7859fd61e77f09eb8086ee83ce792c5d
https://doi.org/10.5194/egusphere-egu2020-8685
https://doi.org/10.5194/egusphere-egu2020-8685
Autor:
T. M. Tomilina, M. M. Laktionova, Maxim Mokrousov, Yu. I. Bobrovnitskiy, B. N. Bakhtin, Maxim Litvak, Dmitry Golovin, Andrey Vostrukhin, Alexey Malakhov, A V Sotov, A. S. Grebennikov, I. G. Mitrofanov, A. S. Kozyrev
Publikováno v:
Cosmic Research. 56:208-212
The results of testing a number of space-based detectors that contain PMTs or high-voltage electrodes for the noise from the microphonics that occurs in the signal path due to external mechanical action have been presented. A method for the vibration
Autor:
Gordon Chin, K. Harshman, Alexey Malakhov, Dmitry Golovin, Larry G. Evans, William V. Boynton, A. B. Sanin, Maxim Mokrousov, F. Fedosov, Timothy A. Livengood, A. S. Kozyrev, J.G. Bodnarik, I. G. Mitrofanov, R. Z. Sagdeev, B. N. Bakhtin, Maxim Litvak, T. P. McClanahan, Andrey Vostrukhin, Vladislav Tretyakov, R. D. Starr
Publikováno v:
Icarus. 283:20-30
We present a method of conversion of the lunar neutron counting rate measured by the Lunar Reconnaissance Orbiter (LRO) Lunar Exploration Neutron Detector (LEND) instrument collimated neutron detectors, to water equivalent hydrogen (WEH) in the top
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 82:542-544
A model of an efficient sound absorber with an internal structure consisting of several compact resonators with different parameters is considered. Maximum efficiency is achieved by matching the impedance characteristics of the sound absorber and the
Autor:
Igor Nuzhdin, I. G. Mitrofanov, K. Harshman, V. V. Shevchenko, A. B. Sanin, A. S. Kosyrev, T. P. McClanahan, B. N. Bakhtin, Maxim Litvak, V. N. Shvetsov, William V. Boynton, Vladislav Tretyakov, Andrey Vostrukhin, F. Fedosov, Maxim Mokrousov, Dmitry Golovin, A. V. Malakhov, R. D. Starr
Publikováno v:
Instruments and Experimental Techniques. 59:578-591
Results of physical calibrations of the LEND neutron telescope operating on board the NASA’s LRO lunar satellite since June 2009 are described. The main goal of the LEND telescope is to measure the epithermal neutron flux in polar areas of the luna
Autor:
I. G. Mitrofanov, Maxim Mokrousov, R. Z. Sagdeev, Т.P. McClanahan, M. L. Litvak, T. A. Livengood, A. V. Malakhov, R. D. Starr, B. N. Bakhtin, Larry G. Evans, K. Harshman, J.G. Bodnarik, A. B. Sanin, William V. Boynton, Gordon Chin
Publikováno v:
Planetary and Space Science. 122:53-65
Lunar neutron flux data measured by the Lunar Exploration Neutron Detector (LEND) on board NASA's Lunar Reconnaissance Orbiter (LRO) were analyzed for the period 2009-2014.We have re-evaluated the instrument's collimation capability and re-estimated