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Record W6948884069 · doi:10.5281/zenodo.13710527

SERPENTINE catalog of solar cycle 25 multi-spacecraft solar energetic particle events

2024· dataset· en· W6948884069 on OpenAlexaboutno aff

Bibliographic record

VenueZenodo (CERN European Organization for Nuclear Research) · 2024
Typedataset
Languageen
FieldAgricultural and Biological Sciences
TopicDiptera species taxonomy and behavior
Canadian institutionsnot available
FundersEuropean Commission
KeywordsSolar energetic particlesEvent (particle physics)Solar cycleSpacecraftProtonParticle (ecology)Solar maximumSolar wind

Abstract

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This catalog contains multi-spacecraft solar energetic particle (SEP) events, which were observed with the new heliospheric spacecraft fleet in solar cycle 25. It has been created within the European Union’s Horizon 2020 project SERPENTINE (Solar energetic particle analysis platform for the inner heliosphere). The catalog comprises key SEP characteristics observed by five different observer locations as provided by Solar Orbiter, Parker Solar Probe, STEREO A, Wind and SOHO (at the Lagrangian point 1), and BepiColombo. It focuses on large events, which show energetic proton increases above 25 MeV observed at least at two spacecraft. The catalog provides not only key parameters of the proton event but also the same parameters for 1 MeV and 100 keV electrons, respectively. For more information, and if you use this catalog, please refer to the corresponding publication: The solar cycle 25 multi-spacecraft solar energetic particle event catalog of the SERPENTINE projectN. Dresing, A. Yli-Laurila, S. Valkila, J. Gieseler, D. E. Morosan, G. U. Farwa, Y. Kartavykh, C. Palmroos, I. Jebaraj, S. Jensen, P. Kühl, B. Heber, F. Espinosa, R. Gómez-Herrero, E. Kilpua, V.-V. Linho, P. Oleynik, L. A. Hayes, A. Warmuth, F. Schuller, H. Collier, H. Xiao, E. Asvestari, D. Trotta, J. G. Mitchell, C. M. S. Cohen, A. W. Labrador, M. E. Hill and R. VainioA&A, 687 (2024) A72DOI: 10.1051/0004-6361/202449831, arXiv:2403.00658. The csv files provided here are archived versions of the dynamic catalog available at https://data.serpentine-h2020.eu/catalogs/sep-sc25/ Provided are two semicolon-separated csv files containing the same data. The only difference is that the file sep-sc25_extended_header.csv includes an extensive header. Field descriptions id: ID science_case: Science case date: Event date [UTC] flare_time: Flare time [UTC] flare_lat: Flare Carrington latitude [deg] flare_lon: Flare Carrington longitude [deg] flare_class: Flare class (GOES) flare_comments: Flare Comments radio_type2: Radio type II bursts decametric_type2_start: Decametric type II burst start time [UT] decametric_type2_stop: Decametric type II burst end time [UT] decametric_type2_freq_range: Decametric type II frequency range [MHz] radio_type2_start: Metric radio type II burst start time [UT] radio_type2_stop: Metric radio type II burst end time [UT] radio_type2_freq_range: Frequency range of metric type II burst [MHz] radio_imaging_available: Metric radio imaging available radio_comments: Radio comments cme_id: Associated CMEs solar_mach_link: Solar-Mach link S/C codes BepiC: BepiColombo L1: L1 (SOHO/Wind) PSP: Parker Solar Probe STA: STEREO A SolO: Solar Orbiter S/C related field descriptions {sc}_sc_lat: S/C Carrington latitude [deg] {sc}_sc_lon: S/C Carrington longitude [deg] {sc}_dist: S/C radial distance [au] {sc}_ip_shock_id: Associated IP shocks {sc}_p25MeV_onset_date: S/C protons 25 MeV onset date [UTC] {sc}_p25MeV_onset_time: S/C protons 25 MeV onset time [UTC] {sc}_p25MeV_onset_time_formatted: S/C protons 25 MeV onset time [UTC] (Formatted) {sc}_p25MeV_onset_averaging: S/C protons 25 MeV averaging used for onset [min] {sc}_p25MeV_onset_sector: S/C protons 25 MeV sector used for onset {sc}_p25MeV_peak_date: S/C protons 25 MeV peak date [UTC] {sc}_p25MeV_peak_time: S/C protons 25 MeV peak time [UTC] {sc}_p25MeV_peak_time_formatted: S/C protons 25 MeV peak time [UTC] (Formatted) {sc}_p25MeV_peak_flux: S/C protons 25 MeV peak flux [cm^-2 s^-1 sr^-1 MeV^-1] {sc}_p25MeV_peak_flux_formatted: S/C protons 25 MeV peak flux [cm^-2 s^-1 sr^-1 MeV^-1] (Formatted) {sc}_p25MeV_peak_averaging: S/C protons 25 MeV averaging used for peak [min] {sc}_p25MeV_peak_sector: S/C protons 25 MeV sector used for peak {sc}_p25MeV_injection_date: S/C protons 25 MeV inferred injection date [UTC] {sc}_p25MeV_injection_time: S/C protons 25 MeV inferred injection time [UTC] {sc}_p25MeV_pathlength: S/C protons 25 MeV path length used for inferred injection time [au] {sc}_p25MeV_sw_speed: S/C protons 25 MeV onset solar wind speed [km/s] {sc}_p25MeV_comments: S/C protons 25 MeV comments {sc}_e100keV_onset_date: S/C electrons 100 keV onset date [UTC] {sc}_e100keV_onset_time: S/C electrons 100 keV onset time [UTC] {sc}_e100keV_onset_time_formatted: S/C electrons 100 keV onset time [UTC] (Formatted) {sc}_e100keV_onset_averaging: S/C electrons 100 keV averaging used for onset [min] {sc}_e100keV_onset_sector: S/C electrons 100 keV sector used for onset {sc}_e100keV_peak_date: S/C electrons 100 keV peak date [UTC] {sc}_e100keV_peak_time: S/C electrons 100 keV peak time [UTC] {sc}_e100keV_peak_time_formatted: S/C electrons 100 keV peak time [UTC] (Formatted) {sc}_e100keV_peak_flux: S/C electrons 100 keV peak flux [cm^-2 s^-1 sr^-1 MeV^-1] {sc}_e100keV_peak_flux_formatted: S/C electrons 100 keV peak flux [cm^-2 s^-1 sr^-1 MeV^-1] (Formatted) {sc}_e100keV_peak_averaging: S/C electrons 100 keV averaging used for peak [min] {sc}_e100keV_peak_sector: S/C electrons 100 keV sector used for peak {sc}_e100keV_injection_date: S/C electrons 100 keV inferred injection date [UTC] {sc}_e100keV_injection_time: S/C electrons 100 keV inferred injection time [UTC] {sc}_e100keV_pathlength: S/C electrons 100 keV path length used for inferred injection time [au] {sc}_e100keV_sw_speed: S/C electrons 100 keV onset solar wind speed [km/s] {sc}_e100keV_comments: S/C electrons 100 keV comments {sc}_e1MeV_onset_date: S/C electrons 1 MeV onset date [UTC] {sc}_e1MeV_onset_time: S/C electrons 1 MeV onset time [UTC] {sc}_e1MeV_onset_time_formatted: S/C electrons 1 MeV onset time [UTC] (Formatted) {sc}_e1MeV_onset_averaging: S/C electrons 1 MeV averaging used for onset [min] {sc}_e1MeV_onset_sector: S/C electrons 1 MeV sector used for onset {sc}_e1MeV_peak_date: S/C electrons 1 MeV peak date [UTC] {sc}_e1MeV_peak_time: S/C electrons 1 MeV peak time [UTC] {sc}_e1MeV_peak_time_formatted: S/C electrons 1 MeV peak time [UTC] (Formatted) {sc}_e1MeV_peak_flux: S/C electrons 1 MeV peak flux [cm^-2 s^-1 sr^-1 MeV^-1] {sc}_e1MeV_peak_flux_formatted: S/C electrons 1 MeV peak flux [cm^-2 s^-1 sr^-1 MeV^-1] (Formatted) {sc}_e1MeV_peak_averaging: S/C electrons 1 MeV averaging used for peak [min] {sc}_e1MeV_peak_sector: S/C electrons 1 MeV sector used for peak {sc}_e1MeV_injection_date: S/C electrons 1 MeV inferred injection date [UTC] {sc}_e1MeV_injection_time: S/C electrons 1 MeV inferred injection time [UTC] {sc}_e1MeV_pathlength: S/C electrons 1 MeV path length used for inferred injection time [au] {sc}_e1MeV_sw_speed: S/C electrons 1 MeV onset solar wind speed [km/s] {sc}_e1MeV_comments: S/C electrons 1 MeV comments {sc}_ep_ratio: Ratio of Electrons (~1MeV) / Protons (25-40 MeV) CHANGELOG: 2024-09-06 Flare information has been updated Updated cme_id info corresponding to updated CME catalog (Zenodo version only: change file format from "semicolon separated" to "comma separated, with fields containing commas surrounded by quotes") 2024-05-24 Events 35, 36: flare times (GOES) were incorrectly provided as peak times. They have been changed to start times (like for all flares). All 8 events where SOLO/STIX has been used for flare determination had been time shifted to the Sun. Now they are shifted to 1 AU to be consistent with the GOES times.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.001
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: Not applicable
GenreCandidate signal: Dataset · Consensus signal: Dataset
Teacher disagreement score0.034
Threshold uncertainty score0.115

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0070.007
Science and technology studies0.0010.000
Scholarly communication0.0020.001
Open science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0340.024

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.038
GPT teacher head0.241
Teacher spread0.203 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designNot applicable
Domainnot available
GenreDataset

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

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Citations1
Published2024
Admission routes1
Has abstractyes

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