@article{MTMT:3331054,
	title = {Quiet-time 0.04-2 MeV/nucleon Ions at 1 AU in Solar Cycles 23 and 24},
	url = {https://m2.mtmt.hu/api/publication/3331054},
	author = {Zeldovich, MA and Logachev, YI and Kecskeméty, Károly},
	doi = {10.1007/s11207-017-1170-8},
	journal-iso = {SOL PHYS},
	journal = {SOLAR PHYSICS},
	volume = {293},
	unique-id = {3331054},
	issn = {0038-0938},
	year = {2018},
	eissn = {1573-093X}
}

@article{MTMT:2702736,
	title = {Suprathermal ions in quiescent periods at 1 AU in the 23rd and 24th solar-activity cycles},
	url = {https://m2.mtmt.hu/api/publication/2702736},
	author = {Zel'dovich, MA and Logachev, YI and Surova, GM and Kecskeméty, Károly},
	doi = {10.1134/S1063772914050072},
	journal-iso = {ASTRON REP+},
	journal = {ASTRONOMY REPORTS},
	volume = {58},
	unique-id = {2702736},
	issn = {1063-7729},
	year = {2014},
	eissn = {1562-6881},
	pages = {399-405}
}

@article{MTMT:2364924,
	title = {Low-energy 3He and 4He ions in interplanetary space during quiet periods of the 23rd solar cycle},
	url = {https://m2.mtmt.hu/api/publication/2364924},
	author = {Zel'dovich, MA and Logachev, YI and Surova, GM and Kecskeméty, Károly},
	doi = {10.1134/S1063772913060073},
	journal-iso = {ASTRON REP+},
	journal = {ASTRONOMY REPORTS},
	volume = {57},
	unique-id = {2364924},
	issn = {1063-7729},
	year = {2013},
	eissn = {1562-6881},
	pages = {562-565}
}

@article{MTMT:2225611,
	title = {The energy dependence of relative ion abundances during quiet-time periods in the 23rd solar cycle},
	url = {https://m2.mtmt.hu/api/publication/2225611},
	author = {Zeldovich, MA and Kecskeméty, Károly and Logachev, YI},
	doi = {10.1088/1742-6596/409/1/012168},
	journal-iso = {J PHYS CONF SER},
	journal = {JOURNAL OF PHYSICS-CONFERENCE SERIES},
	volume = {409},
	unique-id = {2225611},
	issn = {1742-6588},
	year = {2013},
	eissn = {1742-6596}
}

@article{MTMT:1679324,
	title = {Relative ion Fe, C and O abundances in quiet time particle fluxes in the 23 SC},
	url = {https://m2.mtmt.hu/api/publication/1679324},
	author = {Ishkov, VN and Zeldovich, MA and Kecskeméty, Károly and Logachev, YuI},
	doi = {10.1016/j.asr.2011.06.034},
	journal-iso = {ADV SPACE RES},
	journal = {ADVANCES IN SPACE RESEARCH},
	volume = {50},
	unique-id = {1679324},
	issn = {0273-1177},
	abstract = {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.},
	year = {2012},
	eissn = {1879-1948},
	pages = {757-761}
}