Facebook Instagram Twitter RSS Feed PodBean Back to top on side

Some features in the time series of energetic protons measured at L1 during November 2001

In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 55, no. 2
N. Veselinović - M. Savić - D. Maričić - F. Šterc - R. Banjanac - D. Joković - A. Dragić

Details:

Pages: 106 - 113
Language: eng
Keywords:
solar energetic particles, solar activity, fluence spectra
About article:
Extreme events originating on the Sun induce various processes in the heliosphere, such as shock waves and particle acceleration. In this work, we studied the impact of extreme solar events on the flux of energetic particles measured at Lagrange point L1. In many cases, the enhanced flux of energetic particles can be clearly associated with a specific source and involves a well-known acceleration mechanism. However, in some instances, this connection is not as easily established. We examined and compared structures in energetic proton time series where a clear source is not immediately obvious, with structures clearly related to the concurrent passage of an ICME by analyzing the event-integrated fluence of energetic protons during November 2001 to potentially gain insight into the origin of such events.
How to cite:
ISO 690:
Veselinović, N., Savić, M., Maričić, D., Šterc, F., Banjanac, R., Joković, D., Dragić, A. 2025. Some features in the time series of energetic protons measured at L1 during November 2001. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 55, no.2, pp. 106-113. 1335-1842. DOI: https://doi.org/10.31577/caosp.2025.55.2.106

APA:
Veselinović, N., Savić, M., Maričić, D., Šterc, F., Banjanac, R., Joković, D., Dragić, A. (2025). Some features in the time series of energetic protons measured at L1 during November 2001. Contributions of the Astronomical Observatory Skalnaté Pleso, 55(2), 106-113. 1335-1842. DOI: https://doi.org/10.31577/caosp.2025.55.2.106
About edition:
Publisher: Astronomical Institute, Slovak Academy of Sciences
Published: 1. 2. 2025
Rights:
Creative Commons License
This work is licensed under a Creative Commons Attribution 4.0 International License.