TY  - JOUR
A1  - Sadovnichii, V. A.
A1  - Panasyuk, M. I.
A1  - Amelyushkin, A. M.
A1  - Bogomolov, V. V.
A1  - Benghin, V. V.
A1  - Garipov, G. K.
A1  - Kalegaev, V. V.
A1  - Klimov, P. A.
A1  - Khrenov, B. A.
A1  - Petrov, V. L.
A1  - Sharakin, S. A.
A1  - Shirokov, A. V.
A1  - Svertilov, S. I.
A1  - Zotov, M. Y.
A1  - Yashin, I. V.
A1  - Gorbovskoy, E. S.
A1  - Lipunov, V. M.
A1  - Park, I. H.
A1  - Lee, J.
A1  - Jeong, S.
A1  - Kim, M. B.
A1  - Jeong, H. M.
A1  - Shprits, Yuri
A1  - Angelopoulos, V.
A1  - Russell, C. T.
A1  - Runov, A.
A1  - Turner, D.
A1  - Strangeway, R. J.
A1  - Caron, R.
A1  - Biktemerova, S.
A1  - Grinyuk, A.
A1  - Lavrova, M.
A1  - Tkachev, L.
A1  - Tkachenko, A.
A1  - Martinez, O.
A1  - Salazar, H.
A1  - Ponce, E.
T1  - "Lomonosov" Satellite-Space Observatory to Study Extreme Phenomena in Space
JF  - Space science reviews
N2  - The "Lomonosov" space project is lead by Lomonosov Moscow State University in collaboration with the following key partners: Joint Institute for Nuclear Research, Russia, University of California, Los Angeles (USA), University of Pueblo (Mexico), Sungkyunkwan University (Republic of Korea) and with Russian space industry organi-zations to study some of extreme phenomena in space related to astrophysics, astroparticle physics, space physics, and space biology. The primary goals of this experiment are to study: -Ultra-high energy cosmic rays (UHECR) in the energy range of the Greizen-ZatsepinKuzmin (GZK) cutoff; -Ultraviolet (UV) transient luminous events in the upper atmosphere; -Multi-wavelength study of gamma-ray bursts in visible, UV, gamma, and X-rays; -Energetic trapped and precipitated radiation (electrons and protons) at low-Earth orbit (LEO) in connection with global geomagnetic disturbances; -Multicomponent radiation doses along the orbit of spacecraft under different geomagnetic conditions and testing of space segments of optical observations of space-debris and other space objects; -Instrumental vestibular-sensor conflict of zero-gravity phenomena during space flight. This paper is directed towards the general description of both scientific goals of the project and scientific equipment on board the satellite. The following papers of this issue are devoted to detailed descriptions of scientific instruments.
KW  - Gamma-ray bursts
KW  - Ultra-high energy cosmic rays
KW  - Radiation belts
KW  - Space mission
Y1  - 2017
U6  - https://doi.org/10.1007/s11214-017-0425-x
SN  - 0038-6308
SN  - 1572-9672
VL  - 212
SP  - 1705
EP  - 1738
PB  - Springer
CY  - Dordrecht
ER  - 
TY  - JOUR
A1  - Ripoll, Jean-Francois
A1  - Loridan, Vivien
A1  - Denton, Michael H.
A1  - Cunningham, Gregory
A1  - Reeves, G.
A1  - Santolik, O.
A1  - Fennell, Joseph
A1  - Turner, Drew L.
A1  - Drozdov, Alexander
A1  - Cervantes Villa, Juan Sebastian
A1  - Shprits, Yuri
A1  - Thaller, Scott A.
A1  - Kurth, William S.
A1  - Kletzing, Craig A.
A1  - Henderson, Michael  G.
A1  - Ukhorskiy, Aleksandr Y.
T1  - Observations and Fokker-Planck Simulations of the L-Shell, Energy, and Times
JF  - Journal of geophysical research : Space physics
N2  - The evolution of the radiation belts in L-shell (L), energy (E), and equatorial pitch angle (alpha(0)) is analyzed during the calm 11-day interval (4-15 March) following the 1 March 2013 storm. Magnetic Electron and Ion Spectrometer (MagEIS) observations from Van Allen Probes are interpreted alongside 1D and 3D Fokker-Planck simulations combined with consistent event-driven scattering modeling from whistler mode hiss waves. Three (L, E, alpha(0)) regions persist through 11 days of hiss wave scattering; the pitch angle-dependent inner belt core (L similar to <2.2 and E < 700 keV), pitch angle homogeneous outer belt low-energy core (L > similar to 5 and E similar to < 100 keV), and a distinct pocket of electrons (L similar to [4.5, 5.5] and E similar to [0.7, 2] MeV). The pitch angle homogeneous outer belt is explained by the diffusion coefficients that are roughly constant for alpha(0) similar to <60 degrees, E > 100 keV, 3.5 < L < L-pp similar to 6. Thus, observed unidirectional flux decays can be used to estimate local pitch angle diffusion rates in that region. Top-hat distributions are computed and observed at L similar to 3-3.5 and E = 100-300 keV.
KW  - radiation belts
KW  - wave-particle interactions
KW  - electron lifetime
KW  - pitch angle diffusion coefficient
KW  - hiss waves
Y1  - 2018
U6  - https://doi.org/10.1029/2018JA026111
SN  - 2169-9380
SN  - 2169-9402
VL  - 124
IS  - 2
SP  - 1125
EP  - 1142
PB  - American Geophysical Union
CY  - Washington
ER  - 
TY  - GEN
A1  - Sadovnichii, V. A.
A1  - Panasyuk, M. I.
A1  - Amelyushkin, A. M.
A1  - Benghin, V. V.
A1  - Garipov, G. K.
A1  - Kalegaev, V. V.
A1  - Klimov, P. A.
A1  - Khrenov, B. A.
A1  - Petrov, V. L.
A1  - Sharakin, S. A.
A1  - Shirokov, A. V.
A1  - Svertilov, S. I.
A1  - Zotov, M. Y.
A1  - Yashin, I. V.
A1  - Gorbovskoy, E. S.
A1  - Lipunov, V. M.
A1  - Park, I. H.
A1  - Lee, J.
A1  - Jeong, S.
A1  - Kim, M. B.
A1  - Jeong, H. M.
A1  - Shprits, Yuri
A1  - Angelopoulos, V.
A1  - Russell, C. T.
A1  - Runov, A.
A1  - Turner, D.
A1  - Strangeway, R. J.
A1  - Caron, R.
A1  - Biktemerova, S.
A1  - Grinyuk, A.
A1  - Lavrova, M.
A1  - Tkachev, L.
A1  - Tkachenko, A.
A1  - Martinez, O.
A1  - Salazar, H.
A1  - Ponce, E.
T1  - "Lomonosov" satellite-space observatory to study extreme phenomena in space
T2  - Postprints der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe
N2  - The "Lomonosov" space project is lead by Lomonosov Moscow State University in collaboration with the following key partners: Joint Institute for Nuclear Research, Russia, University of California, Los Angeles (USA), University of Pueblo (Mexico), Sungkyunkwan University (Republic of Korea) and with Russian space industry organi-zations to study some of extreme phenomena in space related to astrophysics, astroparticle physics, space physics, and space biology. The primary goals of this experiment are to study:

-Ultra-high energy cosmic rays (UHECR) in the energy range of the Greizen-ZatsepinKuzmin (GZK) cutoff;

-Ultraviolet (UV) transient luminous events in the upper atmosphere;

-Multi-wavelength study of gamma-ray bursts in visible, UV, gamma, and X-rays;

-Energetic trapped and precipitated radiation (electrons and protons) at low-Earth orbit (LEO) in connection with global geomagnetic disturbances;

-Multicomponent radiation doses along the orbit of spacecraft under different geomagnetic conditions and testing of space segments of optical observations of space-debris and other space objects;

-Instrumental vestibular-sensor conflict of zero-gravity phenomena during space flight.

This paper is directed towards the general description of both scientific goals of the project and scientific equipment on board the satellite. The following papers of this issue are devoted to detailed descriptions of scientific instruments.
T3  - Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe - 959 
KW  - gamma-ray bursts
KW  - ultra-high energy cosmic rays
KW  - radiation belts
KW  - space mission
Y1  - 2020
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-428185
SN  - 1866-8372
IS  - 959
SP  - 1705
EP  - 1738
ER  -