Suprathermal ions from coronal holes at 1 au in solar cycles 23 and 24: dependence of ion abundances on solar wind speed

ABSTRACT The relative abundances of thermal and suprathermal C, O, and Fe ions are analysed and compared in solar wind streams from near-equatorial coronal holes (CHs) during quiet periods of nearly two solar cycle minima. Ion fluxes with energies of ∼0.04–2 MeV per nucleon are studied using data fr...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2021-04, Vol.502 (2), p.2961-2969
Hauptverfasser:	Zeldovich, M A, Kecskeméty, K, Logachev, Yu I
Format:	Artikel
Sprache:	eng
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