TY  - JOUR
AU  - Daibog, EI
AU  - Kecskeméty, Károly
AU  - Lazutin, LL
AU  - Logachev, YI
AU  - Surova, GM
TI  - A 27-Day Period in the Flux of Jovian Electrons at the Earth’s Orbit
JF  - ASTRONOMY REPORTS
J2  - ASTRON REP+
VL  - 61
PY  - 2017
IS  - 12
SP  - 1073
EP  - 1081
PG  - 9
SN  - 1063-7729
DO  - 10.1134/S1063772917120010
UR  - https://m2.mtmt.hu/api/publication/3337341
ID  - 3337341
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Daibog, EI
AU  - Kecskeméty, Károly
AU  - Lazutin, LL
AU  - Logachev, YI
TI  - Registering Jovian electrons in the Earth’s orbit
JF  - BULLETIN OF THE RUSSIAN ACADEMY OF SCIENCES - PHYSICS
J2  - BULL RUSS ACAD SCI PHYS
VL  - 81
PY  - 2017
IS  - 2
SP  - 136
EP  - 139
PG  - 4
SN  - 1062-8738
DO  - 10.3103/S1062873817020150
UR  - https://m2.mtmt.hu/api/publication/3202712
ID  - 3202712
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Daibog, E
AU  - Kecskeméty, Károly
AU  - Lazutin, L
AU  - Logachev, Y
TI  - Jovian electrons as an instrument of investigation of the interplanetary medium structure
JF  - JOURNAL OF PHYSICS-CONFERENCE SERIES
J2  - J PHYS CONF SER
VL  - 675
PY  - 2016
PG  - 4
SN  - 1742-6588
DO  - 10.1088/1742-6596/675/3/032024
UR  - https://m2.mtmt.hu/api/publication/3062752
ID  - 3062752
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Daibog, EI
AU  - Kecskeméty, Károly
AU  - Lazutin, LL
AU  - Logachev, YI
AU  - Surova, GM
TI  - Relativistic electrons in the Earth’s magnetospheric tail during solar activity minima
JF  - BULLETIN OF THE RUSSIAN ACADEMY OF SCIENCES - PHYSICS
J2  - BULL RUSS ACAD SCI PHYS
VL  - 79
PY  - 2015
IS  - 5
SP  - 643
EP  - 645
PG  - 3
SN  - 1062-8738
DO  - 10.3103/S1062873815050184
UR  - https://m2.mtmt.hu/api/publication/2911568
ID  - 2911568
N1  - Original Russian Text © E.I. Daibog, K. Kecskemety, L.L. 
Lazutin, Yu.I. Logachev, G.M. Surova, 2015, published in 
Izvestiya Rossiiskoi Akademii Nauk. Seriya Fizicheskaya, 2015, 
Vol. 79, No. 5, pp. 697–699.
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Daibog, EI
AU  - Logachev, YI
AU  - Kahler, SW
AU  - Kecskeméty, Károly
TI  - Sequences of solar events with identical decays as a tool for isolating quasistationary states in the interplanetary space
JF  - COSMIC RESEARCH
J2  - COSMIC RES+
VL  - 42
PY  - 2004
IS  - 4
SP  - 362
EP  - 369
PG  - 8
SN  - 0010-9525
DO  - 10.1023/B:COSM.0000039735.35134.70
UR  - https://m2.mtmt.hu/api/publication/1786239
ID  - 1786239
AB  - Time profile of the fluxes of energetic solar particles generated by solar flares (including their phase of decline) is formed to a large extent by the structure of the interplanetary magnetic field and its irregularities that move away from the Sun with the solar wind velocity. When propagation is a pure diffusion, the solar particle fluxes decay after the maximum in a power-law manner. At the same time in many cases this decay is exponential, which is indicative of a considerable role played by the convective sweep of particles and their adiabatic deceleration in the expanding solar wind. In this paper we consider the events with long exponential decays and newly discovered series of successive events with identical exponential decays lasting for one to two weeks or more. They allow us to assume that the interplanetary space is stable and homogeneous during this period.
LA  - English
DB  - MTMT
ER  -