Evangelos Paouris
Affiliations: | 2017 | University of Athens, Greece, Zografou, Greece |
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"Evangelos Paouris"Mean distance: (not calculated yet)
Parents
Sign in to add mentor| Helen Mavromichalaki | grad student | 2017 | University of Athens, Greece | |
| (Space Weather Monitoring: Modulation of Cosmic Ray intensity due to large interplanetary Coronal Mass Ejections) | ||||
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Publications
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| Aminalragia-Giamini S, Jiggens P, Anastasiadis A, et al. (2020) Prediction of Solar Proton Event Fluence spectra from their Peak flux spectra Journal of Space Weather and Space Climate. 10: 1 |
| Mavromichalaki H, Gerontidou M, Paschalis P, et al. (2018) Real-time Detection of the Ground Level Enhancement on 10 September 2017 by A.Ne.Mo.S.: System report Social Work. 16: 1797-1805 |
| Mavromichalaki H, Preka-Papadema P, Theodoropoulou A, et al. (2017) A study of the possible relation of the cardiac arrhythmias occurrence to the polarity reversal of the solar magnetic field Advances in Space Research. 59: 366-378 |
| Paouris E, Mavromichalaki H. (2017) Effective Acceleration Model for the Arrival Time of Interplanetary Shocks driven by Coronal Mass Ejections Solar Physics. 292: 180 |
| Paouris E, Mavromichalaki H. (2017) Interplanetary Coronal Mass Ejections Resulting from Earth-Directed CMEs Using SOHO and ACE Combined Data During Solar Cycle 23 Solar Physics. 292: 30 |
| Gushchina RT, Belov AV, Eroshenko EA, et al. (2014) Cosmic ray modulation during the solar activity growth phase of cycle 24 Geomagnetism and Aeronomy. 54: 430-436 |
| Paouris E. (2013) Ineffectiveness of Narrow CMEs for Cosmic Ray Modulation Solar Physics. 284: 589-597 |
| Mavromichalaki H, Paouris E. (2012) Long-Term Cosmic Ray Variability and the CME-Index Advances in Astronomy. 2012: 1-8 |
| Paouris E, Mavromichalaki H, Belov A, et al. (2012) Galactic Cosmic Ray Modulation and the Last Solar Minimum Solar Physics. 280: 255-271 |
| Mavromichalaki H, Paouris E, Karalidi T. (2007) Cosmic-Ray Modulation: An Empirical Relation with Solar and Heliospheric Parameters Solar Physics. 245: 369-390 |