Space experiments aboard the Lomonosov MSU satellite

Abstract At present, the Institute of Nuclear Physics of Moscow State University, in cooperation with other organizations, is preparing space experiments onboard the Lomonosov satellite. The main goal of this mission is to study extreme astrophysical phenomena such as cosmic gamma-ray bursts and ult...
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Autor*in:	Sadovnichiy, V. A. [verfasserIn] Amelyushkin, A. M. Angelopoulos, V. Bengin, V. V. Bogomolov, V. V. Garipov, G. K. Gorbovskoy, E. S. Grossan, B. Klimov, P. A. Khrenov, B. A. Lee, J. Lipunov, V. M. Na, G. W. Panasyuk, M. I. Park, I. H. Petrov, V. L. Russell, C. T. Svertilov, S. I. Sigaeva, E. A. Smoot, G. F. Shprits, Yu. Vedenkin, N. N. Yashin, I. V.

Format:	Artikel
Sprache:	Englisch

Erschienen:	2013

Schlagwörter:	Cosmic Research Ultra High Energy Optical Light Curve Runaway Electron Avalanche Large Scale Ionospheric Disturbance

Anmerkung:	© Pleiades Publishing, Ltd. 2013

Übergeordnetes Werk:	Enthalten in: Cosmic research - Pleiades Publishing, 1964, 51(2013), 6 vom: Nov., Seite 427-433
Übergeordnetes Werk:	volume:51 ; year:2013 ; number:6 ; month:11 ; pages:427-433

Links:	Volltext

DOI / URN:	10.1134/S0010952513060063

Katalog-ID:	OLC2027386211

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520			\|a Abstract At present, the Institute of Nuclear Physics of Moscow State University, in cooperation with other organizations, is preparing space experiments onboard the Lomonosov satellite. The main goal of this mission is to study extreme astrophysical phenomena such as cosmic gamma-ray bursts and ultra-high-energy cosmic rays. These phenomena are associated with the processes occurring in the early universe in very distant astrophysical objects, therefore, they can provide information on the first stages of the evolution of the universe. This paper considers the main characteristics of the scientific equipment aboard the Lomonosov satellite.
650		4	\|a Cosmic Research
650		4	\|a Ultra High Energy
650		4	\|a Optical Light Curve
650		4	\|a Runaway Electron Avalanche
650		4	\|a Large Scale Ionospheric Disturbance
700	1		\|a Amelyushkin, A. M. \|4 aut
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700	1		\|a Garipov, G. K. \|4 aut
700	1		\|a Gorbovskoy, E. S. \|4 aut
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700	1		\|a Klimov, P. A. \|4 aut
700	1		\|a Khrenov, B. A. \|4 aut
700	1		\|a Lee, J. \|4 aut
700	1		\|a Lipunov, V. M. \|4 aut
700	1		\|a Na, G. W. \|4 aut
700	1		\|a Panasyuk, M. I. \|4 aut
700	1		\|a Park, I. H. \|4 aut
700	1		\|a Petrov, V. L. \|4 aut
700	1		\|a Russell, C. T. \|4 aut
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700	1		\|a Sigaeva, E. A. \|4 aut
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allfields	10.1134/S0010952513060063 doi (DE-627)OLC2027386211 (DE-He213)S0010952513060063-p DE-627 ger DE-627 rakwb eng 520 620 VZ 16,12 ssgn Sadovnichiy, V. A. verfasserin aut Space experiments aboard the Lomonosov MSU satellite 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2013 Abstract At present, the Institute of Nuclear Physics of Moscow State University, in cooperation with other organizations, is preparing space experiments onboard the Lomonosov satellite. The main goal of this mission is to study extreme astrophysical phenomena such as cosmic gamma-ray bursts and ultra-high-energy cosmic rays. These phenomena are associated with the processes occurring in the early universe in very distant astrophysical objects, therefore, they can provide information on the first stages of the evolution of the universe. This paper considers the main characteristics of the scientific equipment aboard the Lomonosov satellite. Cosmic Research Ultra High Energy Optical Light Curve Runaway Electron Avalanche Large Scale Ionospheric Disturbance Amelyushkin, A. M. aut Angelopoulos, V. aut Bengin, V. V. aut Bogomolov, V. V. aut Garipov, G. K. aut Gorbovskoy, E. S. aut Grossan, B. aut Klimov, P. A. aut Khrenov, B. A. aut Lee, J. aut Lipunov, V. M. aut Na, G. W. aut Panasyuk, M. I. aut Park, I. H. aut Petrov, V. L. aut Russell, C. T. aut Svertilov, S. I. aut Sigaeva, E. A. aut Smoot, G. F. aut Shprits, Yu. aut Vedenkin, N. N. aut Yashin, I. V. aut Enthalten in Cosmic research Pleiades Publishing, 1964 51(2013), 6 vom: Nov., Seite 427-433 (DE-627)129361909 (DE-600)160891-5 (DE-576)014734443 0010-9525 nnns volume:51 year:2013 number:6 month:11 pages:427-433 https://doi.org/10.1134/S0010952513060063 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_40 GBV_ILN_70 AR 51 2013 6 11 427-433
spelling	10.1134/S0010952513060063 doi (DE-627)OLC2027386211 (DE-He213)S0010952513060063-p DE-627 ger DE-627 rakwb eng 520 620 VZ 16,12 ssgn Sadovnichiy, V. A. verfasserin aut Space experiments aboard the Lomonosov MSU satellite 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2013 Abstract At present, the Institute of Nuclear Physics of Moscow State University, in cooperation with other organizations, is preparing space experiments onboard the Lomonosov satellite. The main goal of this mission is to study extreme astrophysical phenomena such as cosmic gamma-ray bursts and ultra-high-energy cosmic rays. These phenomena are associated with the processes occurring in the early universe in very distant astrophysical objects, therefore, they can provide information on the first stages of the evolution of the universe. This paper considers the main characteristics of the scientific equipment aboard the Lomonosov satellite. Cosmic Research Ultra High Energy Optical Light Curve Runaway Electron Avalanche Large Scale Ionospheric Disturbance Amelyushkin, A. M. aut Angelopoulos, V. aut Bengin, V. V. aut Bogomolov, V. V. aut Garipov, G. K. aut Gorbovskoy, E. S. aut Grossan, B. aut Klimov, P. A. aut Khrenov, B. A. aut Lee, J. aut Lipunov, V. M. aut Na, G. W. aut Panasyuk, M. I. aut Park, I. H. aut Petrov, V. L. aut Russell, C. T. aut Svertilov, S. I. aut Sigaeva, E. A. aut Smoot, G. F. aut Shprits, Yu. aut Vedenkin, N. N. aut Yashin, I. V. aut Enthalten in Cosmic research Pleiades Publishing, 1964 51(2013), 6 vom: Nov., Seite 427-433 (DE-627)129361909 (DE-600)160891-5 (DE-576)014734443 0010-9525 nnns volume:51 year:2013 number:6 month:11 pages:427-433 https://doi.org/10.1134/S0010952513060063 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_40 GBV_ILN_70 AR 51 2013 6 11 427-433
allfields_unstemmed	10.1134/S0010952513060063 doi (DE-627)OLC2027386211 (DE-He213)S0010952513060063-p DE-627 ger DE-627 rakwb eng 520 620 VZ 16,12 ssgn Sadovnichiy, V. A. verfasserin aut Space experiments aboard the Lomonosov MSU satellite 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2013 Abstract At present, the Institute of Nuclear Physics of Moscow State University, in cooperation with other organizations, is preparing space experiments onboard the Lomonosov satellite. The main goal of this mission is to study extreme astrophysical phenomena such as cosmic gamma-ray bursts and ultra-high-energy cosmic rays. These phenomena are associated with the processes occurring in the early universe in very distant astrophysical objects, therefore, they can provide information on the first stages of the evolution of the universe. This paper considers the main characteristics of the scientific equipment aboard the Lomonosov satellite. Cosmic Research Ultra High Energy Optical Light Curve Runaway Electron Avalanche Large Scale Ionospheric Disturbance Amelyushkin, A. M. aut Angelopoulos, V. aut Bengin, V. V. aut Bogomolov, V. V. aut Garipov, G. K. aut Gorbovskoy, E. S. aut Grossan, B. aut Klimov, P. A. aut Khrenov, B. A. aut Lee, J. aut Lipunov, V. M. aut Na, G. W. aut Panasyuk, M. I. aut Park, I. H. aut Petrov, V. L. aut Russell, C. T. aut Svertilov, S. I. aut Sigaeva, E. A. aut Smoot, G. F. aut Shprits, Yu. aut Vedenkin, N. N. aut Yashin, I. V. aut Enthalten in Cosmic research Pleiades Publishing, 1964 51(2013), 6 vom: Nov., Seite 427-433 (DE-627)129361909 (DE-600)160891-5 (DE-576)014734443 0010-9525 nnns volume:51 year:2013 number:6 month:11 pages:427-433 https://doi.org/10.1134/S0010952513060063 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_40 GBV_ILN_70 AR 51 2013 6 11 427-433
allfieldsGer	10.1134/S0010952513060063 doi (DE-627)OLC2027386211 (DE-He213)S0010952513060063-p DE-627 ger DE-627 rakwb eng 520 620 VZ 16,12 ssgn Sadovnichiy, V. A. verfasserin aut Space experiments aboard the Lomonosov MSU satellite 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2013 Abstract At present, the Institute of Nuclear Physics of Moscow State University, in cooperation with other organizations, is preparing space experiments onboard the Lomonosov satellite. The main goal of this mission is to study extreme astrophysical phenomena such as cosmic gamma-ray bursts and ultra-high-energy cosmic rays. These phenomena are associated with the processes occurring in the early universe in very distant astrophysical objects, therefore, they can provide information on the first stages of the evolution of the universe. This paper considers the main characteristics of the scientific equipment aboard the Lomonosov satellite. Cosmic Research Ultra High Energy Optical Light Curve Runaway Electron Avalanche Large Scale Ionospheric Disturbance Amelyushkin, A. M. aut Angelopoulos, V. aut Bengin, V. V. aut Bogomolov, V. V. aut Garipov, G. K. aut Gorbovskoy, E. S. aut Grossan, B. aut Klimov, P. A. aut Khrenov, B. A. aut Lee, J. aut Lipunov, V. M. aut Na, G. W. aut Panasyuk, M. I. aut Park, I. H. aut Petrov, V. L. aut Russell, C. T. aut Svertilov, S. I. aut Sigaeva, E. A. aut Smoot, G. F. aut Shprits, Yu. aut Vedenkin, N. N. aut Yashin, I. V. aut Enthalten in Cosmic research Pleiades Publishing, 1964 51(2013), 6 vom: Nov., Seite 427-433 (DE-627)129361909 (DE-600)160891-5 (DE-576)014734443 0010-9525 nnns volume:51 year:2013 number:6 month:11 pages:427-433 https://doi.org/10.1134/S0010952513060063 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_40 GBV_ILN_70 AR 51 2013 6 11 427-433
allfieldsSound	10.1134/S0010952513060063 doi (DE-627)OLC2027386211 (DE-He213)S0010952513060063-p DE-627 ger DE-627 rakwb eng 520 620 VZ 16,12 ssgn Sadovnichiy, V. A. verfasserin aut Space experiments aboard the Lomonosov MSU satellite 2013 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2013 Abstract At present, the Institute of Nuclear Physics of Moscow State University, in cooperation with other organizations, is preparing space experiments onboard the Lomonosov satellite. The main goal of this mission is to study extreme astrophysical phenomena such as cosmic gamma-ray bursts and ultra-high-energy cosmic rays. These phenomena are associated with the processes occurring in the early universe in very distant astrophysical objects, therefore, they can provide information on the first stages of the evolution of the universe. This paper considers the main characteristics of the scientific equipment aboard the Lomonosov satellite. Cosmic Research Ultra High Energy Optical Light Curve Runaway Electron Avalanche Large Scale Ionospheric Disturbance Amelyushkin, A. M. aut Angelopoulos, V. aut Bengin, V. V. aut Bogomolov, V. V. aut Garipov, G. K. aut Gorbovskoy, E. S. aut Grossan, B. aut Klimov, P. A. aut Khrenov, B. A. aut Lee, J. aut Lipunov, V. M. aut Na, G. W. aut Panasyuk, M. I. aut Park, I. H. aut Petrov, V. L. aut Russell, C. T. aut Svertilov, S. I. aut Sigaeva, E. A. aut Smoot, G. F. aut Shprits, Yu. aut Vedenkin, N. N. aut Yashin, I. V. aut Enthalten in Cosmic research Pleiades Publishing, 1964 51(2013), 6 vom: Nov., Seite 427-433 (DE-627)129361909 (DE-600)160891-5 (DE-576)014734443 0010-9525 nnns volume:51 year:2013 number:6 month:11 pages:427-433 https://doi.org/10.1134/S0010952513060063 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_40 GBV_ILN_70 AR 51 2013 6 11 427-433
language	English
source	Enthalten in Cosmic research 51(2013), 6 vom: Nov., Seite 427-433 volume:51 year:2013 number:6 month:11 pages:427-433
sourceStr	Enthalten in Cosmic research 51(2013), 6 vom: Nov., Seite 427-433 volume:51 year:2013 number:6 month:11 pages:427-433
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Cosmic Research Ultra High Energy Optical Light Curve Runaway Electron Avalanche Large Scale Ionospheric Disturbance
dewey-raw	520
isfreeaccess_bool	false
container_title	Cosmic research
authorswithroles_txt_mv	Sadovnichiy, V. A. @@aut@@ Amelyushkin, A. M. @@aut@@ Angelopoulos, V. @@aut@@ Bengin, V. V. @@aut@@ Bogomolov, V. V. @@aut@@ Garipov, G. K. @@aut@@ Gorbovskoy, E. S. @@aut@@ Grossan, B. @@aut@@ Klimov, P. A. @@aut@@ Khrenov, B. A. @@aut@@ Lee, J. @@aut@@ Lipunov, V. M. @@aut@@ Na, G. W. @@aut@@ Panasyuk, M. I. @@aut@@ Park, I. H. @@aut@@ Petrov, V. L. @@aut@@ Russell, C. T. @@aut@@ Svertilov, S. I. @@aut@@ Sigaeva, E. A. @@aut@@ Smoot, G. F. @@aut@@ Shprits, Yu. @@aut@@ Vedenkin, N. N. @@aut@@ Yashin, I. V. @@aut@@
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author	Sadovnichiy, V. A.
spellingShingle	Sadovnichiy, V. A. ddc 520 ssgn 16,12 misc Cosmic Research misc Ultra High Energy misc Optical Light Curve misc Runaway Electron Avalanche misc Large Scale Ionospheric Disturbance Space experiments aboard the Lomonosov MSU satellite
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topic_title	520 620 VZ 16,12 ssgn Space experiments aboard the Lomonosov MSU satellite Cosmic Research Ultra High Energy Optical Light Curve Runaway Electron Avalanche Large Scale Ionospheric Disturbance
topic	ddc 520 ssgn 16,12 misc Cosmic Research misc Ultra High Energy misc Optical Light Curve misc Runaway Electron Avalanche misc Large Scale Ionospheric Disturbance
topic_unstemmed	ddc 520 ssgn 16,12 misc Cosmic Research misc Ultra High Energy misc Optical Light Curve misc Runaway Electron Avalanche misc Large Scale Ionospheric Disturbance
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title	Space experiments aboard the Lomonosov MSU satellite
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title_full	Space experiments aboard the Lomonosov MSU satellite
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author_browse	Sadovnichiy, V. A. Amelyushkin, A. M. Angelopoulos, V. Bengin, V. V. Bogomolov, V. V. Garipov, G. K. Gorbovskoy, E. S. Grossan, B. Klimov, P. A. Khrenov, B. A. Lee, J. Lipunov, V. M. Na, G. W. Panasyuk, M. I. Park, I. H. Petrov, V. L. Russell, C. T. Svertilov, S. I. Sigaeva, E. A. Smoot, G. F. Shprits, Yu. Vedenkin, N. N. Yashin, I. V.
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title_sort	space experiments aboard the lomonosov msu satellite
title_auth	Space experiments aboard the Lomonosov MSU satellite
abstract	Abstract At present, the Institute of Nuclear Physics of Moscow State University, in cooperation with other organizations, is preparing space experiments onboard the Lomonosov satellite. The main goal of this mission is to study extreme astrophysical phenomena such as cosmic gamma-ray bursts and ultra-high-energy cosmic rays. These phenomena are associated with the processes occurring in the early universe in very distant astrophysical objects, therefore, they can provide information on the first stages of the evolution of the universe. This paper considers the main characteristics of the scientific equipment aboard the Lomonosov satellite. © Pleiades Publishing, Ltd. 2013
abstractGer	Abstract At present, the Institute of Nuclear Physics of Moscow State University, in cooperation with other organizations, is preparing space experiments onboard the Lomonosov satellite. The main goal of this mission is to study extreme astrophysical phenomena such as cosmic gamma-ray bursts and ultra-high-energy cosmic rays. These phenomena are associated with the processes occurring in the early universe in very distant astrophysical objects, therefore, they can provide information on the first stages of the evolution of the universe. This paper considers the main characteristics of the scientific equipment aboard the Lomonosov satellite. © Pleiades Publishing, Ltd. 2013
abstract_unstemmed	Abstract At present, the Institute of Nuclear Physics of Moscow State University, in cooperation with other organizations, is preparing space experiments onboard the Lomonosov satellite. The main goal of this mission is to study extreme astrophysical phenomena such as cosmic gamma-ray bursts and ultra-high-energy cosmic rays. These phenomena are associated with the processes occurring in the early universe in very distant astrophysical objects, therefore, they can provide information on the first stages of the evolution of the universe. This paper considers the main characteristics of the scientific equipment aboard the Lomonosov satellite. © Pleiades Publishing, Ltd. 2013
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title_short	Space experiments aboard the Lomonosov MSU satellite
url	https://doi.org/10.1134/S0010952513060063
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author2	Amelyushkin, A. M. Angelopoulos, V. Bengin, V. V. Bogomolov, V. V. Garipov, G. K. Gorbovskoy, E. S. Grossan, B. Klimov, P. A. Khrenov, B. A. Lee, J. Lipunov, V. M. Na, G. W. Panasyuk, M. I. Park, I. H. Petrov, V. L. Russell, C. T. Svertilov, S. I. Sigaeva, E. A. Smoot, G. F. Shprits, Yu Vedenkin, N. N. Yashin, I. V.
author2Str	Amelyushkin, A. M. Angelopoulos, V. Bengin, V. V. Bogomolov, V. V. Garipov, G. K. Gorbovskoy, E. S. Grossan, B. Klimov, P. A. Khrenov, B. A. Lee, J. Lipunov, V. M. Na, G. W. Panasyuk, M. I. Park, I. H. Petrov, V. L. Russell, C. T. Svertilov, S. I. Sigaeva, E. A. Smoot, G. F. Shprits, Yu Vedenkin, N. N. Yashin, I. V.
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up_date	2024-07-03T15:07:40.144Z
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