A New Magnetic Parameter of Active Regions Distinguishing Large Eruptive and Confined Solar Flares
Ting Li
This database includes a total of 106 flares (43 eruptive and 63 confined) of Geostationary Operational Environmental Satellite (GOES) class C5.0 and larger that occurred within 45 degree from the central meridian, from June 2010 until June 2019. For each event in the database, we measured the magnetic nonpotential parameters of active regions producing solar flares.
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FlareM1.0Para.csv
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readme_FlareM1.0Para.txt
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Paper Information
Paper Title:
A New Magnetic Parameter of Active Regions Distinguishing Large Eruptive and Confined Solar Flares
Publication:
The Astrophysical Journal
Bibcode:
2022ApJ...926L..14L
DOI:
10.3847/2041-8213/ac5251
Identifiers
DOI:
10.12149/101088
VO Identifier:
ivo://China-VO/paperdata/101088
Publication Date:
2022-01-04
Citation Guidelines
Ting Li et al. 2022. A New Magnetic Parameter of Active Regions Distinguishing Large Eruptive and Confined Solar Flares. Version 1.0. https://doi.org/10.12149/101088
@misc{10.12149/101088,
doi = {10.12149/101088},
url = {https://doi.org/10.12149/101088},
author = {Ting Li},
title = {A New Magnetic Parameter of Active Regions Distinguishing Large Eruptive and Confined Solar Flares},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2022}
}
doi = {10.12149/101088},
url = {https://doi.org/10.12149/101088},
author = {Ting Li},
title = {A New Magnetic Parameter of Active Regions Distinguishing Large Eruptive and Confined Solar Flares},
version = {1.0},
publisher = {Nataional Astronomical Data Center of China},
year= {2022}
}
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This DOI represents all versions, and will always resolve to the latest one.
2022-01-04