Publications of O. Raukunen

A list of publications authored or co-authored by O. Raukunen, derived from the SAO/NASA Astrophysics Data System (ADS). The number in brackets after each title indicates the number of citations that the paper has received.

Orcid ID: 0000-0001-8346-5281

List of publications ordered by citations
Number of papers: 20 (refereed: 16)
No. of citations: 447
First author papers: 5 (refereed: 4)

2025

1. The High-Energy Protons of the Ground Level Enhancement (GLE74) Event on 11 May 2024 [6]
   Papaioannou, A., Mishev, A., Usoskin, I., Heber, B., Vainio, R., Larsen, N., Jarry, M., Rouillard, A. P., Talebpour Sheshvan, N., Laurenza, M., Dumbović, M., Vasalos, G., Gieseler, J., Koldobskiy, S., Raukunen, O., Palmroos, C., Hörlöck, M., Köberle, M., Wimmer-Schweingruber, R. F., Anastasiadis, A., Kühl, P. & Lavasa, E., Solar Physics, 300, 73

2024

1. Consistency of the average flux of solar energetic particles over different timescales up to mega-years [0]
   Usoskin, I., Koldobskiy, S., Poluianov, S., Raukunen, O., Vainio, R. & Kovaltsov, G., 38th International Cosmic Ray Conference, p. 1244
2. New reconstruction of annual integral solar proton fluences between 1984-2019 [0]
   Usoskin, I., Raukunen, O., Koldobskiy, S., Kovaltsov, G. & Vainio, R., 38th International Cosmic Ray Conference, p. 1242

2023

1. Magnetic connectivity and solar energetic proton event intensity profiles at deka-MeV energy [3]
   Paassilta, Miikka, Vainio, Rami, Papaioannou, Athanasios, Raukunen, Osku, Barcewicz, Suvi & Anastasiadis, Anastasios, Advances in Space Research, 71, 1840
2. Consistency of the average flux of solar energetic particles over timescales of years to megayears [8]
   Usoskin, I. G., Koldobskiy, S. A., Poluianov, S. V., Raukunen, O., Vainio, R. & Kovaltsov, G. A., A&A, 670, L22
3. High Energy Solar Particle Events and Their Relationship to Associated Flare, CME and GLE Parameters [20]
   Waterfall, C. O. G., Dalla, S., Raukunen, O., Heynderickx, D., Jiggens, P. & Vainio, R., Space Weather, 21, e2022SW003334

2022

1. The probabilistic solar particle event forecasting (PROSPER) model [17]
   Papaioannou, Athanasios, Vainio, Rami, Raukunen, Osku, Jiggens, Piers, Aran, Angels, Dierckxsens, Mark, Mallios, Sotirios A., Paassilta, Miikka & Anastasiadis, Anastasios, Journal of Space Weather and Space Climate, 12, 24
2. Annual integral solar proton fluences for 1984-2019 [6]
   Raukunen, O., Usoskin, I., Koldobskiy, S., Kovaltsov, G. & Vainio, R., A&A, 665, A65

2021

1. New reconstruction of event-integrated spectra (spectral fluences) for major solar energetic particle events [39]
   Koldobskiy, S., Raukunen, O., Vainio, R., Kovaltsov, G. A. & Usoskin, I., A&A, 647, A132

2020

1. Very high energy proton peak flux model [14]
   Raukunen, Osku, Paassilta, Miikka, Vainio, Rami, Rodriguez, Juan V., Eronen, Timo, Crosby, Norma, Dierckxsens, Mark, Jiggens, Piers, Heynderickx, Daniel & Sandberg, Ingmar, Journal of Space Weather and Space Climate, 10, 24

2019

1. GUMICS-4 analysis of interplanetary coronal mass ejection impact on Earth during low and typical Mach number solar winds [3]
   Lakka, Antti, Pulkkinen, Tuija I., Dimmock, Andrew P., Kilpua, Emilia, Ala-Lahti, Matti, Honkonen, Ilja, Palmroth, Minna & Raukunen, Osku, Annales Geophysicae, 37, 561

2018

1. Updated Model of the Solar Energetic Proton Environment in Space [41]
   Jiggens, Piers, Heynderickx, Daniel, Sandberg, Ingmar, Truscott, Pete, Raukunen, Osku & Vainio, Rami, Journal of Space Weather and Space Climate, 8, A31
2. First Analysis of Ground-Level Enhancement (GLE) 72 on 10 September 2017: Spectral and Anisotropy Characteristics [56]
   Mishev, A., Usoskin, I., Raukunen, O., Paassilta, M., Valtonen, E., Kocharov, L. & Vainio, R., Solar Physics, 293, 136
3. Two solar proton fluence models based on ground level enhancement observations [64]
   Raukunen, Osku, Vainio, Rami, Tylka, Allan J., Dietrich, William F., Jiggens, Piers, Heynderickx, Daniel, Dierckxsens, Mark, Crosby, Norma, Ganse, Urs & Siipola, Robert, Journal of Space Weather and Space Climate, 8, A04

2017

1. Catalogue of 55-80 MeV solar proton events extending through solar cycles 23 and 24 [47]
   Paassilta, Miikka, Raukunen, Osku, Vainio, Rami, Valtonen, Eino, Papaioannou, Athanasios, Siipola, Robert, Riihonen, Esa, Dierckxsens, Mark, Crosby, Norma, Malandraki, Olga, Heber, Bernd & Klein, Karl-Ludwig, Journal of Space Weather and Space Climate, 7, A14
2. Why is solar cycle 24 an inefficient producer of high-energy particle events? [25]
   Vainio, Rami, Raukunen, Osku, Tylka, Allan J., Dietrich, William F. & Afanasiev, Alexandr, A&A, 604, A47

2016

1. Defining the SEP environment for specifications using the SAPPHIRE model [0]
   Jiggens, Piers, Heynderickx, Daniel, Truscott, Pete, Sandberg, Ingmar, Lei, Fan, Varotsou, Athina, Vainio, Rami & Raukunen, Osku, 2016 16th European Conference on Radiation and Its Effects on Components and Systems (RADECS), p. 47
2. Iron-rich solar particle events measured by SOHO/ERNE during two solar cycles [3]
   Raukunen, O., Valtonen, E. & Vainio, R., A&A, 589, A138

2015

1. Iron-rich solar particle events measured by SOHO/ERNE [1]
   Raukunen, O., Valtonen, E. & Vainio, R., 34th International Cosmic Ray Conference (ICRC2015), International Cosmic Ray Conference, 34, p. 124

2013

1. The first SEPServer event catalogue ~68-MeV solar proton events observed at 1 AU in 1996-2010 [94]
   Vainio, Rami, Valtonen, Eino, Heber, Bernd, Malandraki, Olga E., Papaioannou, Athanasios, Klein, Karl-Ludwig, Afanasiev, Alexander, Agueda, Neus, Aurass, Henry, Battarbee, Markus, Braune, Stephan, Dröge, Wolfgang, Ganse, Urs, Hamadache, Clarisse, Heynderickx, Daniel, Huttunen-Heikinmaa, Kalle, Kiener, Jürgen, Kilian, Patrick, Kopp, Andreas, Kouloumvakos, Athanasios, Maisala, Sami, Mishev, Alexander, Miteva, Rositsa, Nindos, Alexander, Oittinen, Tero, Raukunen, Osku, Riihonen, Esa, Rodríguez-Gasén, Rosa, Saloniemi, Oskari, Sanahuja, Blai, Scherer, Renate, Spanier, Felix, Tatischeff, Vincent, Tziotziou, Kostas, Usoskin, Ilya G. & Vilmer, Nicole, Journal of Space Weather and Space Climate, 3, A12