Quiet-time 0.04–2 MeV/nucleon Ions at 1 AU in Solar Cycles 23 and 24

M. A. Zeldovich, Y. I. Logachev, K. Kecskeméty

Research output: Contribution to journalArticle

1 Citation (Scopus)

Abstract

The fluxes of 3He, 4He, C, O, and Fe ions at low energies (about 0.04–2MeV/nucleon) are studied during quiet periods in Solar Cycles (SC) 23 and 24 using data from the ULEIS/ACE instrument. In selecting quiet periods (the definition is given in Section 2.1), additional data from EPHIN/SOHO and EPAM/ACE were also used. The analysis of the ion energy spectra and their relative abundances shows that their behavior is governed by their first-ionization potential. Substantial differences in the ion energy spectra in two consecutive solar cycles are observed during the quiet periods selected. Quiet-time fluxes are divided into three distinct types according to the ∼80–320keV/nucleon Fe/O ratio. Our results confirm the earlier observation that these types of suprathermal particles have different origins, that is, they represent different seed populations that are accelerated by different processes. Except for the solar activity minimum, the Fe/O ratio during quiet-time periods correspond either to the abundances of ions in particle fluxes accelerated in impulsive solar flares or to the mean abundances of elements in the solar corona. At the activity minimum, this ratio takes on values that are characteristic for the solar wind. These results indicate that the background fluxes of low-energy particles in the ascending, maximum, and decay phases of the solar cycle include significant contributions from both coronal particles accelerated to suprathermal energies and ions accelerated in small impulsive solar flares rich in Fe, while the contribution of remnants from earlier SEP events cannot be excluded. The comparison of suprathermal ion abundances during the first five years of SC 23 and SC 24 suggests that the quiet-time and non-quiet fluxes of Fe and 3He were lower in SC 24.

Original languageEnglish
Article number3
JournalSolar Physics
Volume293
Issue number1
DOIs
Publication statusPublished - Jan 1 2018

Fingerprint

solar cycles
solar cycle
ion
ions
energy
solar flares
energy spectra
solar corona
flux (rate)
solar activity
particle energy
ionization potentials
solar wind
corona
seeds
relative abundance
ionization
seed
particle
decay

Keywords

  • Ion abundances
  • Particle emission
  • Solar activity
  • Solar wind

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Quiet-time 0.04–2 MeV/nucleon Ions at 1 AU in Solar Cycles 23 and 24. / Zeldovich, M. A.; Logachev, Y. I.; Kecskeméty, K.

In: Solar Physics, Vol. 293, No. 1, 3, 01.01.2018.

Research output: Contribution to journalArticle

Zeldovich, M. A. ; Logachev, Y. I. ; Kecskeméty, K. / Quiet-time 0.04–2 MeV/nucleon Ions at 1 AU in Solar Cycles 23 and 24. In: Solar Physics. 2018 ; Vol. 293, No. 1.
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