Quiet-time low energy ion spectra observed on Solar Orbiter during solar minimum. Mason, G. M., Ho, G. C., Allen, R. C., Xu, Z. G., Janitzek, N. P., Freiherr von Forstner, J. L., Kohllhoff, A., Pacheco, D., Rodríguez-Pacheco, J., Wimmer-Schweingruber, R. F., Bruce Andrews, G., Schlemm, C. E., Seifert, H., Tyagi, K., Lees, W. J., Hayes, J., Gómez-Herrero, R., Prieto, M., Sánchez-Prieto, S., Espinosa Lara, F., Cernuda, I., Parra Espada, P., Rodríguez Polo, O., Martínez Hellín, A., Martin, C., Böttcher, S., Berger, L., Terasa, J. C., Boden, S., Kulkarni, S. R., Ravanbakhsh, A., Yedla, M., Eldrum, S., Elftmann, R., & Kühl, P. Astronomy & Astrophysics, 656:L5, December, 2021.
Quiet-time low energy ion spectra observed on Solar Orbiter during solar minimum [link]Paper  doi  abstract   bibtex   
Context. The Solar Orbiter spacecraft cruised in the inner heliosphere during Feb. 2020 – Jan. 2021, moving between ∼0.5–1.0 au radial distance. The Energetic Particle Detector suite operated continuously during this period. Aims. The Suprathermal Ion Spectrograph and High Energy Telescope observations made during intervals in between transient intensity increases were used to determine the low energy ion spectra and composition during quiet times. Methods. Energetic particle spectra and major ion components, including 3He, were measured over the range ∼0.1–100 MeV nucleon−1. The radial dependence of 4.4 MeV nucleon−1 4He and O was measured. A short interval of extremely low intensities (“super-quiet”) was also studied.
@article{mason_quiet-time_2021,
	title = {Quiet-time low energy ion spectra observed on {Solar} {Orbiter} during solar minimum},
	volume = {656},
	issn = {0004-6361, 1432-0746},
	url = {https://www.aanda.org/10.1051/0004-6361/202140540},
	doi = {10.1051/0004-6361/202140540},
	abstract = {Context. The Solar Orbiter spacecraft cruised in the inner heliosphere during Feb. 2020 – Jan. 2021, moving between ∼0.5–1.0 au radial distance. The Energetic Particle Detector suite operated continuously during this period. Aims. The Suprathermal Ion Spectrograph and High Energy Telescope observations made during intervals in between transient intensity increases were used to determine the low energy ion spectra and composition during quiet times. Methods. Energetic particle spectra and major ion components, including 3He, were measured over the range ∼0.1–100 MeV nucleon−1. The radial dependence of 4.4 MeV nucleon−1 4He and O was measured. A short interval of extremely low intensities (“super-quiet”) was also studied.},
	language = {en},
	urldate = {2022-07-12},
	journal = {Astronomy \& Astrophysics},
	author = {Mason, G. M. and Ho, G. C. and Allen, R. C. and Xu, Z. G. and Janitzek, N. P. and Freiherr von Forstner, J. L. and Kohllhoff, A. and Pacheco, D. and Rodríguez-Pacheco, J. and Wimmer-Schweingruber, R. F. and Bruce Andrews, G. and Schlemm, C. E. and Seifert, H. and Tyagi, K. and Lees, W. J. and Hayes, J. and Gómez-Herrero, R. and Prieto, M. and Sánchez-Prieto, S. and Espinosa Lara, F. and Cernuda, I. and Parra Espada, P. and Rodríguez Polo, O. and Martínez Hellín, A. and Martin, C. and Böttcher, S. and Berger, L. and Terasa, J. C. and Boden, S. and Kulkarni, S. R. and Ravanbakhsh, A. and Yedla, M. and Eldrum, S. and Elftmann, R. and Kühl, P.},
	month = dec,
	year = {2021},
	pages = {L5},
}

Downloads: 0