TY  - JOUR
AU  - Zeldovich, MA
AU  - Logachev, YI
AU  - Kecskeméty, Károly
TI  - Quiet-time 0.04-2 MeV/nucleon Ions at 1 AU in Solar Cycles 23 and 24
JF  - SOLAR PHYSICS
J2  - SOL PHYS
VL  - 293
PY  - 2018
IS  - 1
PG  - 21
SN  - 0038-0938
DO  - 10.1007/s11207-017-1170-8
UR  - https://m2.mtmt.hu/api/publication/3331054
ID  - 3331054
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Zel'dovich, MA
AU  - Logachev, YI
AU  - Surova, GM
AU  - Kecskeméty, Károly
TI  - Suprathermal ions in quiescent periods at 1 AU in the 23rd and 24th solar-activity cycles
JF  - ASTRONOMY REPORTS
J2  - ASTRON REP+
VL  - 58
PY  - 2014
IS  - 6
SP  - 399
EP  - 405
PG  - 7
SN  - 1063-7729
DO  - 10.1134/S1063772914050072
UR  - https://m2.mtmt.hu/api/publication/2702736
ID  - 2702736
N1  - Original Russian Text © M.A.Zel’dovich, Yu.I. Logachev, G.M. 
Surova, K. Kecskeméty, 2014, published in Astronomicheskii 
Zhurnal, 2014, Vol. 91, No. 6, pp. 474–480.
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Zel'dovich, MA
AU  - Logachev, YI
AU  - Surova, GM
AU  - Kecskeméty, Károly
TI  - Low-energy 3He and 4He ions in interplanetary space during quiet periods of the 23rd solar cycle
JF  - ASTRONOMY REPORTS
J2  - ASTRON REP+
VL  - 57
PY  - 2013
IS  - 7
SP  - 562
EP  - 565
PG  - 4
SN  - 1063-7729
DO  - 10.1134/S1063772913060073
UR  - https://m2.mtmt.hu/api/publication/2364924
ID  - 2364924
N1  - WoS:hiba:000321760700007 2019-03-09 00:41 cím nem egyezik
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Zeldovich, MA
AU  - Kecskeméty, Károly
AU  - Logachev, YI
TI  - The energy dependence of relative ion abundances during quiet-time periods in the 23rd solar cycle
JF  - JOURNAL OF PHYSICS-CONFERENCE SERIES
J2  - J PHYS CONF SER
VL  - 409
PY  - 2013
IS  - 1
PG  - 4
SN  - 1742-6588
DO  - 10.1088/1742-6596/409/1/012168
UR  - https://m2.mtmt.hu/api/publication/2225611
ID  - 2225611
LA  - English
DB  - MTMT
ER  - 

TY  - JOUR
AU  - Ishkov, VN
AU  - Zeldovich, MA
AU  - Kecskeméty, Károly
AU  - Logachev, YuI
TI  - Relative ion Fe, C and O abundances in quiet time particle fluxes in the 23 SC
JF  - ADVANCES IN SPACE RESEARCH
J2  - ADV SPACE RES
VL  - 50
PY  - 2012
IS  - 6
SP  - 757
EP  - 761
PG  - 5
SN  - 0273-1177
DO  - 10.1016/j.asr.2011.06.034
UR  - https://m2.mtmt.hu/api/publication/1679324
ID  - 1679324
AB  - Using ACE and SOHO data the origin of quiet-time low-energy particle fluxes at 1 AU is studied in the 23rd solar cycle. One of the selection criteria of quiet-time periods is to demand that H/He < 10 provided that periods with noticeable contribution of remnants of gradual events have been excluded from consideration. Our results suggest different origin of 0.03-3 MeV/nucleon particles - different seed populations accelerated and different acceleration processes. During the ascending, maximum and descending phases of solar activity quiet-time ions consist of coronal particles accelerated to suprathermal energies in about a half of the quiet periods, the rest of quiet-time fluxes originates from particle acceleration in processes similar to those in small impulsive solar flares rich in Fe. At solar minimum the bulk solar wind particles serve as seed population. © 2011 COSPAR.
LA  - English
DB  - MTMT
ER  -