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Journal articles on the topic 'SEP events'

Author: Grafiati

Published: 10 March 2023

Last updated: 31 July 2025

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1

Bao, Baoleerqimuge, and Guoyu Ren. "Sea-Effect Precipitation over the Shandong Peninsula, Northern China." Journal of Applied Meteorology and Climatology 57, no. 6 (2018): 1291–308. http://dx.doi.org/10.1175/jamc-d-17-0200.1.

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AbstractSea-effect precipitation (SEP) over the Shandong Peninsula is a unique climatological phenomenon in mainland China, and it exerts a considerable impact on the southern shore of the Bohai Sea. From observed data from 123 stations for the period 1962–2012, the characteristics of cold-season (November–February) SEP in this area were analyzed. Results showed that SEP occurred throughout the late autumn and winter. In all, 1173 SEP days were identified during the 51 years, of which snow days accounted for 73.7% and rain and snow–rain days accounted for 16.1% and 10.1%, respectively. Decembe

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2

Kahler, Stephen W., and Alan G. Ling. "Forecasting Solar Energetic Particle (SEP) events with Flare X-ray peak ratios." Journal of Space Weather and Space Climate 8 (2018): A47. http://dx.doi.org/10.1051/swsc/2018033.

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Solar flare X-ray peak fluxes and fluences in the 0.1–0.8 nm band are often used in models to forecast solar energetic particle (SEP) events. Garcia (2004) [Forecasting methods for occurrence and magnitude of proton storms with solar soft X rays, Space Weather, 2, S02002, 2004] used ratios of the 0.05–0.4 and 0.1–0.8 nm bands of the X-ray instrument on the GOES spacecraft to plot inferred peak flare temperatures versus peak 0.1–0.8 nm fluxes for flares from 1988 to 2002. Flares associated with E > 10 MeV SEP events of >10 proton flux units (pfu) had statistically lower peak temperatures

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3

Verkhoglyadova, O. P., G. Li, G. P. Zank, et al. "Understanding large SEP events with the PATH code: Modeling of the 13 December 2006 SEP event." Journal of Geophysical Research: Space Physics 115, A12 (2010): n/a. http://dx.doi.org/10.1029/2010ja015615.

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4

Reinard, A. A., and M. A. Andrews. "Comparison of CME characteristics for SEP and non-SEP related events." Advances in Space Research 38, no. 3 (2006): 480–83. http://dx.doi.org/10.1016/j.asr.2005.01.028.

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5

Dmitriev, A. V., H. C. Yeh, J. K. Chao, I. S. Veselovsky, S. Y. Su, and C. C. Fu. "Top-side ionosphere response to extreme solar events." Annales Geophysicae 24, no. 5 (2006): 1469–77. http://dx.doi.org/10.5194/angeo-24-1469-2006.

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Abstract. Strong X-flares and solar energetic particle (SEP) fluxes are considered as sources of topside ionospheric disturbances observed by the ROCSAT-1/IPEI instrument during the Bastille Day event on 14 July 2000 and the Halloween event on 28 October–4 November 2003. It was found that within a prestorm period in the dayside ionosphere at altitudes of ~600 km the ion density increased up to ~80% in response to flare-associated enhancements of the solar X-ray emission. Ionospheric response to the SEP events was revealed both at sunlit and nightside hemispheres, where the ion density increase

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6

Kahler, S. W., A. G. Ling, and D. V. Reames. "Spatial Evolution of 20 MeV Solar Energetic Proton Events." Astrophysical Journal 942, no. 2 (2023): 68. http://dx.doi.org/10.3847/1538-4357/aca7c0.

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Abstract The longitudinal extents of solar energetic (E > 10 MeV) particle (SEP) events in the heliosphere are a characteristic important for understanding SEP acceleration and transport as well as their space weather effects. SEP detectors on the STEREO A and B spacecraft launched in 2008, combined with those on Earth-orbiting spacecraft, have enabled recent studies of this characteristic for many events. Each SEP event distribution has been characterized by a single central longitude, width, and amplitude derived from Gaussian fits to peak intensities or fluences at each spacecraft. To ca

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7

Georgoulis, Manolis K., Athanasios Papaioannou, Ingmar Sandberg, et al. "Analysis and interpretation of inner-heliospheric SEP events with the ESA Standard Radiation Environment Monitor (SREM) onboard the INTEGRAL and Rosetta Missions." Journal of Space Weather and Space Climate 8 (2018): A40. http://dx.doi.org/10.1051/swsc/2018027.

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Using two heliospheric vantage points, we study 22 solar energetic particle (SEP) events, 14 of which were detected at both locations. SEP proton events were detected during the declining phase of solar cycle 23 (November 2003–December 2006) by means of two nearly identical Standard Radiation Environment Monitor (SREM) units in energies ranging between 12.6 MeV and 166.3 MeV. In this work we combine SREM data with diverse solar and interplanetary measurements, aiming to backtrace solar eruptions from their impact in geospace (i.e., from L1 Lagrangian point to Earth’s magnetosphere) to their pa

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8

Koldobskiy, S., O. Raukunen, R. Vainio, G. A. Kovaltsov, and I. Usoskin. "New reconstruction of event-integrated spectra (spectral fluences) for major solar energetic particle events." Astronomy & Astrophysics 647 (March 2021): A132. http://dx.doi.org/10.1051/0004-6361/202040058.

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Aims. Fluences of solar energetic particles (SEPs) are not easy to evaluate, especially for high-energy events (i.e. ground-level enhancements, GLEs). Earlier estimates of event-integrated SEP fluences for GLEs were based on partly outdated assumptions and data, and they required revisions. Here, we present the results of a full revision of the spectral fluences for most major SEP events (GLEs) for the period from 1956 to 2017 using updated low-energy flux estimates along with greatly revisited high-energy flux data and applying the newly invented reconstruction method including an improved ne

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9

Gopalswamy, N., S. Yashiro, S. Akiyama, et al. "Coronal mass ejections, type II radio bursts, and solar energetic particle events in the SOHO era." Annales Geophysicae 26, no. 10 (2008): 3033–47. http://dx.doi.org/10.5194/angeo-26-3033-2008.

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Abstract. Using the extensive and uniform data on coronal mass ejections (CMEs), solar energetic particle (SEP) events, and type II radio bursts during the SOHO era, we discuss how the CME properties such as speed, width and solar-source longitude decide whether CMEs are associated with type II radio bursts and SEP events. We discuss why some radio-quiet CMEs are associated with small SEP events while some radio-loud CMEs are not associated with SEP events. We conclude that either some fast and wide CMEs do not drive shocks or they drive weak shocks that do not produce significant levels of pa

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10

Wiedenbeck, M. E., G. M. Mason, and B. Klecker. "Isotopic Fractionation in 3He-rich SEP Events." Journal of Physics: Conference Series 1332 (November 2019): 012017. http://dx.doi.org/10.1088/1742-6596/1332/1/012017.

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11

Hosseinzadeh, Pouya, Soukaina Filali Boubrahimi, and Shah Muhammad Hamdi. "Improving Solar Energetic Particle Event Prediction through Multivariate Time Series Data Augmentation." Astrophysical Journal Supplement Series 270, no. 2 (2024): 31. http://dx.doi.org/10.3847/1538-4365/ad1de0.

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Abstract Solar energetic particles (SEPs) are associated with extreme solar events that can cause major damage to space- and ground-based life and infrastructure. High-intensity SEP events, particularly ∼100 MeV SEP events, can pose severe health risks for astronauts owing to radiation exposure and affect Earth’s orbiting satellites (e.g., Landsat and the International Space Station). A major challenge in the SEP event prediction task is the lack of adequate SEP data because of the rarity of these events. In this work, we aim to improve the prediction of ∼30, ∼60, and ∼100 MeV SEP events by sy

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12

Swalwell, Bill, Silvia Dalla, and Robert Walsh. "Forecasting Solar Energetic Particle Events and Associated False Alarms." Proceedings of the International Astronomical Union 13, S335 (2017): 324–27. http://dx.doi.org/10.1017/s1743921317011036.

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AbstractBecause of the significant dangers they pose, accurate forecasting of Solar Energetic Particle (SEP) events is vital. Whilst it has long been known that SEP-production is associated with high-energy solar events, forecasting algorithms based upon the observation of these types of solar event suffer from high false alarm rates. Here we analyse the parameters of 4 very high energy solar events which were false alarms, with a view to reaching an understanding as to why SEPs were not detected at Earth. We find that in each case at least two factors were present which have been shown to be

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13

Kahler, S. W., and A. G. Ling. "Solar–Stellar Connection: X-Ray Flares to Energetic (E > 10 MeV) Particle Events." Astrophysical Journal 956, no. 1 (2023): 24. http://dx.doi.org/10.3847/1538-4357/acf1ff.

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Abstract Energetic particle environments are an important factor for the viability of life on exoplanets surrounding flare stars. In the heliosphere, large gradual solar energetic (E > 10 MeV) particle (SEP) events are produced by shocks from fast coronal mass ejections (CMEs). Extensive observations of solar X-ray flares, CMEs, and SEP events can provide guidance for flare star models of stellar energetic particle (StEP) events, for which stellar flares, but only rarely the associated CMEs, are observed. Comparing an extensive list of peak fluxes, timescales, and peak temperatures of 585 ≥

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14

Hosseinzadeh, Pouya, Soukaina Filali Boubrahimi, and Shah Muhammad Hamdi. "An End-to-end Ensemble Machine Learning Approach for Predicting High-impact Solar Energetic Particle Events Using Multimodal Data." Astrophysical Journal Supplement Series 277, no. 2 (2025): 34. https://doi.org/10.3847/1538-4365/adb1c4.

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Abstract Solar energetic particle (SEP) events, in particular high-energy-range SEP events, pose significant risks to space missions, astronauts, and technological infrastructure. Accurate prediction of these high-impact events is crucial for mitigating potential hazards. In this study, we present an end-to-end ensemble machine learning (ML) framework for the prediction of high-impact ∼100 MeV SEP events. Our approach leverages diverse data modalities sourced from the Solar and Heliospheric Observatory and the Geostationary Operational Environmental Satellite integrating extracted active regio

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15

Bahri, Omar, Peiyu Li, Soukaïna Filali Boubrahimi, and Shah Muhammad Hamdi. "Predicting Solar Energetic Particle Events with Time Series Shapelets." Astrophysical Journal 980, no. 1 (2025): 128. https://doi.org/10.3847/1538-4357/ada601.

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Abstract Solar energetic particle (SEP) events pose significant risks to both space and ground-level infrastructure, as well as to human health in space. Understanding and predicting these events are critical for mitigating their potential impacts. In this paper, we address the challenge of predicting SEP events using proton flux data. We leverage some of the most recent advances in time series data mining, such as shapelets and the matrix profile, to propose a simple and easily understandable prediction approach. Our objective is to mitigate the interpretability challenges inherent to most ma

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16

Parent, P.-Y., D. Verscharen, G. Nicolaou, and C. J. Owen. "Microchannel plate response to solar energetic particles and consequences for solar-wind measurements on ESA’s Vigil mission." RAS Techniques and Instruments 3, no. 1 (2024): 844–52. https://doi.org/10.1093/rasti/rzae053.

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ABSTRACT Space weather forecasting aims at predicting the impacts of the Sun, interplanetary space, and the planetary environment on biological and technological systems. To monitor space weather, the European Space Agency is developing the Vigil mission. Vigil will carry the Plasma Analyser (PLA) instrument. We investigate the expected impact of Solar Energetic Particles (SEPs) on PLA. We analyse previous measurements from Solar Orbiter’s Solar Wind Analyser (SWA) Electron Analyser System (EAS) that, like PLA, uses a microchannel plate (MCP) as its detector. Using a fitting algorithm, we extr

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17

Vainio, Rami. "Particle acceleration and turbulence transport in heliospheric plasmas." Proceedings of the International Astronomical Union 4, S257 (2008): 413–23. http://dx.doi.org/10.1017/s1743921309029640.

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AbstractPlasma turbulence at various length scales affects practically all mechanisms proposed to be responsible for particle acceleration in the heliosphere. In this paper, we concentrate on providing a synthesis of some recent efforts to understand particle acceleration in the solar corona and inner heliosphere. Acceleration at coronal and interplanetary shock waves driven by coronal mass ejections (CMEs) is the most viable mechanism for producing large gradual solar energetic particle (SEP) events, whereas particle acceleration in impulsive flares is assumed to be responsible for the genera

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18

Klein, Karl-Ludwig. "Radio Astronomical Tools for the Study of Solar Energetic Particles II.Time-Extended Acceleration at Subrelativistic and Relativistic Energies." Frontiers in Astronomy and Space Sciences 7 (March 11, 2021). http://dx.doi.org/10.3389/fspas.2020.580445.

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Solar energetic particle (SEP) events are commonly separated in two categories: numerous “impulsive” events of relatively short duration, and a few “gradual” events, where SEP-intensities may stay enhanced over several days at energies up to several tens of MeV. In some gradual events the SEP spectrum extends to relativistic energies (>1 GeV), over shorter durations. The two categories are strongly related to an idea developed in the 1960s based on radio observations: Type III bursts, which were addressed in a companion chapter, outline impulsive acceleration of electrons to subrelativistic

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19

Kahler, Stephen. "Second-Class Citizen in the Heliophysics Community." Frontiers in Astronomy and Space Sciences 9 (April 13, 2022). http://dx.doi.org/10.3389/fspas.2022.892965.

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The study of solar energetic particles (SEPs) is an important area of solar research and space weather. An SEP event extends over large regions of the heliosphere, involves energy ranges varying by decades, and evolves over various time and spatial scales and with ion composition, but with SEP observations limited to in situ detections on a few spacecraft for any given event, we are unable to observe these properties synoptically. Solar studies in general are the beneficiaries of imaging and remote sensing observations over practically all wavelengths and timescales from ground and space based

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20

Farwa, G. U., N. Dresing, J. Gieseler, et al. "Electron and proton peak intensities as observed by a five-spacecraft fleet in solar cycle 25." Astronomy & Astrophysics, December 9, 2024. https://doi.org/10.1051/0004-6361/202450945.

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Solar energetic particle (SEP) events are related to solar flares and fast coronal mass ejections (CMEs). In the case of large events, which are typically associated with both a strong flare and a fast CME driving a shock front, identification of the dominant SEP acceleration mechanism is challenging. Using novel spacecraft observations of strong SEP events detected in solar cycle 25, we aim to identify the parent acceleration region of the observed electron and proton events. We analysed 45 SEP events in November 2020 -- May 2023 including $>25$ MeV protons using data from multiple spacecr

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21

Miyake, Fusa, Masataka Hakozaki, Hisashi Hayakawa, Naruki Nakano, and Lukas Wacker. "No signature of extreme solar energetic particle events in high-precision 14C data from the Alaskan tree for 1844–1876 CE." Journal of Space Weather and Space Climate, November 29, 2023. http://dx.doi.org/10.1051/swsc/2023030.

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Cosmogenic nuclides—14C from tree rings and 10Be & 36Cl from ice cores serve as an effective proxy for past extreme solar energetic particle (SEP) events. After identifying the first signature of an extreme SEP event in 774 CE, several candidates have been found in these proxy archives, such as 993 CE, 660 BCE, and 7176 BCE. Their magnitudes have been estimated to be tens of times larger than that of the largest SEP event ever observed since 1950s. Although a detailed survey of such extreme SEP events is ongoing, the detection of intermediate-sized SEP events that bridge the gap between mo

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22

Löwe, Jan Leo, Salman Khaksarighiri, Robert F. Wimmer‐Schweingruber, et al. "Nowcasting Solar Energetic Particle Events for Mars Missions." Space Weather 23, no. 4 (2025). https://doi.org/10.1029/2025sw004372.

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AbstractIn addition to the omnipresent Galactic Cosmic Rays, sudden Solar Energetic Particle (SEP) events present considerable health hazards for manned space missions. These events not only contribute to an increased long‐term cancer risk, but can, in extreme cases, cause acute radiation syndromes. Forecasting their imminent occurrence could significantly reduce radiation exposure by warning astronauts to move to shelter. However, all currently available tools are primarily designed for the Earth or Earth‐Moon system, which limits their applicability to future Mars missions. To address this,

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23

Reames, Donald V. "Excess H, Suppressed He, and the Abundances of Elements in Solar Energetic Particles." Solar Physics 294, no. 10 (2019). http://dx.doi.org/10.1007/s11207-019-1533-4.

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Abstract Recent studies of the abundances of H and He relative to those of heavier ions in solar energetic particle (SEP) events suggest new features in the underlying physics. Impulsive SEP events, defined by uniquely large enhancements of Fe/O, emerge from magnetic reconnection in solar jets. In small, “pure,” shock-free, impulsive SEP events, protons with mass-to-charge ratio $A/Q = 1$A/Q=1 fit the power-law dependence of element abundance enhancements versus$A/Q$A/Q extrapolated from the heavier elements $6 \leq Z \leq 56$6≤Z≤56. Sometimes these events have order-of-magnitude suppressions

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24

Nitta, Nariaki V., Radoslav Bučík, Glenn M. Mason, et al. "Solar activities associated with 3He-rich solar energetic particle events observed by Solar Orbiter." Frontiers in Astronomy and Space Sciences 10 (March 14, 2023). http://dx.doi.org/10.3389/fspas.2023.1148467.

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A series of 3He-rich solar energetic particle (SEP) events was observed by Solar Orbiter in May 2021 at a radial distance of 0.95 AU. An isolated active region AR 12824 was likely the ultimate source of these SEP events. The period of the enhanced flux of 3He was also a period of frequent type III bursts in the decametric-hectometric range, confirming their close relationship. As in past studies, we try to find the solar activities possibly responsible for 3He-rich SEP events, using the type III bursts close to the particle injection times estimated from the velocity dispersion. But this exerc

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25

Yan Hao, Ding Liu-Guan, Li Feng, and Bin Gu. "A Study on the Relationship between Solar Energetic Particle Intensity and Coronal Mass Ejections and its Associated Type II Radio Bursts." Acta Physica Sinica, 2024, 0. http://dx.doi.org/10.7498/aps.73.20231855.

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Based on the multiple-vantage observations of STEREO, SOHO, Wind and other spacecraft, the fast and wide coronal mass ejections (CME) during the 24th solar cycle from January 2010 to September 2014 were selected in this paper. Using the outputs of Richardson's (2014) empirical model of solar energetic particle (SEP) intensity under different conditions, the effects of its associations such as CME, pre-CME, type II radio bursts, and so on, on SEP intensity were analyzed, and the relationship between SEP event and these characteristics was also discussed. The major conclusions are as follows: 1.

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AUSTRALO. "REPO4EU News - Sep 2023." September 4, 2023. https://doi.org/10.5281/zenodo.8334585.

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Reames, Donald V. "On the Correlation between Energy Spectra and Element Abundances in Solar Energetic Particles." Solar Physics 296, no. 1 (2021). http://dx.doi.org/10.1007/s11207-021-01762-z.

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AbstractIn solar energetic particle (SEP) events, the physical processes of both shock acceleration and scattering during transport can cause energy-spectral indices to be correlated with enhancement or suppression of element abundances versus mass-to-charge ratios $A/Q$ A / Q . We observe correlations for those “gradual” SEP events where shock waves accelerate ions from the ambient coronal plasma, but there are no such correlations for “impulsive” SEP events produced by magnetic reconnection in solar jets, where abundance enhancement in different events vary from $(A/Q)^{+2}$ ( A / Q ) + 2 to

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Ho, G. C., G. M. Mason, R. C. Allen, R. F. Wimmer-Schweingruber, J. Rodríguez-Pacheco, and R. Gómez-Herrero. "Interplanetary Ion Flux Dropouts Across Multiple 3He-Rich Events." Frontiers in Astronomy and Space Sciences 9 (July 14, 2022). http://dx.doi.org/10.3389/fspas.2022.939799.

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Solar Orbiter, a joint ESA/NASA mission, is studying the Sun and inner heliosphere in greater detail than ever before. Launched in February 2020, Solar Orbiter has already completed its first three orbits, reaching perihelia of 0.5 au from the Sun in June 2020, February and August 2021. During the first 2 years in orbit, Solar Orbiter observed multiple 3He-rich Solar Energetic Particle (SEP) events inside 1 au. Even though these events were small, their spectral forms, 3He content, and association with energetic electrons and type III bursts convincingly identifies them as 3He-rich SEP events

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29

"Healthcare fallout following events of Sep 11 2001." PharmacoEconomics & Outcomes News 353, no. 1 (2002): 12. http://dx.doi.org/10.1007/bf03278806.

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"Calendar of Events: J. Sep. Science 4/2002." Journal of Separation Science 25, no. 4 (2002): 265–66. http://dx.doi.org/10.1002/1615-9314(20020301)25:4<265::aid-jssc265>3.0.co;2-8.

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"Calendar of Events: J. Sep. Science 7/2002." Journal of Separation Science 25, no. 7 (2002): 469–70. http://dx.doi.org/10.1002/1615-9314(20020501)25:7<469::aid-jssc469>3.0.co;2-c.

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"Calendar of Events: J. Sep. Science 8/2002." Journal of Separation Science 25, no. 8 (2002): 549–50. http://dx.doi.org/10.1002/1615-9314(20020601)25:8<549::aid-jssc549>3.0.co;2-c.

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"Calendar of Events: J. Sep. Science 9/2002." Journal of Separation Science 25, no. 9 (2002): 629–30. http://dx.doi.org/10.1002/1615-9314(20020601)25:9<629::aid-jssc629>3.0.co;2-f.

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"Calendar of Events: J. Sep. Science 12/2002." Journal of Separation Science 25, no. 12 (2002): 780–82. http://dx.doi.org/10.1002/1615-9314(20020801)25:12<780::aid-jssc780>3.0.co;2-k.

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"Calendar of Events: J. Sep. Science 13/2002." Journal of Separation Science 25, no. 13 (2002): 856–58. http://dx.doi.org/10.1002/1615-9314(20020901)25:13<856::aid-jssc856>3.0.co;2-2.

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"Calendar of Events: J. Sep. Science 14/2002." Journal of Separation Science 25, no. 14 (2002): 925–26. http://dx.doi.org/10.1002/1615-9314(20021001)25:14<925::aid-jssc925>3.0.co;2-j.

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"Calendar of Events: J. Sep. Science 18/2002." Journal of Separation Science 25, no. 18 (2002): 1365–66. http://dx.doi.org/10.1002/jssc.200290009.

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"Calendar of Events: J. Sep. Science 5/2003." Journal of Separation Science 26, no. 5 (2003): 443–44. http://dx.doi.org/10.1002/jssc.200390059.

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"Calendar of Events: J. Sep. Science 8/2003." Journal of Separation Science 26, no. 8 (2003): 743–44. http://dx.doi.org/10.1002/jssc.200390092.

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"Calendar of Events: J. Sep. Science 11/2003." Journal of Separation Science 26, no. 11 (2003): 1075–76. http://dx.doi.org/10.1002/jssc.200390103.

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"Calendar of Events: J. Sep. Science 14/2003." Journal of Separation Science 26, no. 14 (2003): 1295–96. http://dx.doi.org/10.1002/jssc.200390109.

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"Calendar of Events: J. Sep. Science 17/2003." Journal of Separation Science 26, no. 17 (2003): 1599–600. http://dx.doi.org/10.1002/jssc.200390116.

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"Calendar of Events: J. Sep. Science 18/2003." Journal of Separation Science 26, no. 18 (2003): 1717–18. http://dx.doi.org/10.1002/jssc.200390119.

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"Calendar of Events: J. Sep. Science 3/2004." Journal of Separation Science 27, no. 3 (2004): 255–56. http://dx.doi.org/10.1002/jssc.200490008.

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"Calendar of Events: J. Sep. Science 4/2004." Journal of Separation Science 27, no. 4 (2004): 347–48. http://dx.doi.org/10.1002/jssc.200490013.

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"Calendar of Events: J. Sep. Science 9/2004." Journal of Separation Science 27, no. 9 (2004): 735–36. http://dx.doi.org/10.1002/jssc.200490032.

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"Calendar of Events: J. Sep. Science 12/2004." Journal of Separation Science 27, no. 12 (2004): 1051–52. http://dx.doi.org/10.1002/jssc.200490042.

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"Calendar of Events: J. Sep. Science 13/2004." Journal of Separation Science 27, no. 13 (2004): 1139–40. http://dx.doi.org/10.1002/jssc.200490049.

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"Calendar of Events: J. Sep. Science 14/2004." Journal of Separation Science 27, no. 14 (2004): 1235–36. http://dx.doi.org/10.1002/jssc.200490053.

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"Calendar of Events: J. Sep. Science 1/2005." Journal of Separation Science 28, no. 1 (2005): 111–12. http://dx.doi.org/10.1002/jssc.200590002.

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