Suprathermal particles from corotating interaction regions during the first perihelion pass of Solar Orbiter

The first orbit of Solar Orbiter provided comprehensive measurements of six corotating interaction regions (CIRs) within 1 au. Five of these CIRs were also observed by ACE at 1 au, allowing for comparisons of the suprathermal ion intensities and spectra at different radial distances. Only subtle mod...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2021-12, Vol.656, p.L2
Hauptverfasser: Allen, R. C., Mason, G. M., Ho, G. C., Rodríguez-Pacheco, J., Wimmer-Schweingruber, R. F., Andrews, G. B., Berger, L., Boden, S., Cernuda, I., Espinosa Lara, F., Freiherr von Forstner, J. L., Gómez-Herrero, R., Hayes, J. R., Kulkarni, S. R., Lees, W. J., Martin, C., Pacheco, D., Polo, O. R., Prieto, M., Ravanbakhsh, A., Sánchez-Prieto, S., Schlemm, C. E., Seifert, H., Terasa, J. C., Tyagi, K., Xu, Z., Yedla, M.
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Sprache:eng
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Zusammenfassung:The first orbit of Solar Orbiter provided comprehensive measurements of six corotating interaction regions (CIRs) within 1 au. Five of these CIRs were also observed by ACE at 1 au, allowing for comparisons of the suprathermal ion intensities and spectra at different radial distances. Only subtle modulations of the 4 He spectral slopes are observed between Solar Orbiter and ACE. Additionally, the radial gradients of 226−320 keV/nuc 4 He ion intensities between Solar Orbiter and ACE are similar to that of 1.53 MeV H reported by Van Hollebeke et al. (1978, J. Geophys. Res., 83, A10). These observations provide a new addition to the study of the radial dependence of CIR-associated suprathermal ions in the inner heliosphere.
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361/202039870