Probability Distribution Functions of Solar and Stellar Flares
The paper studies the soft X-ray data of solar flares and found that the distribution functions of flare fluence are successfully modeled by tapered power law or gamma function distributions whose power exponent is slightly smaller than 2, indicating that the total energy of the flare populations is...
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| Format: | Article |
| Language: | English |
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MDPI AG
2022-12-01
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| Series: | Physics |
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| Online Access: | https://www.mdpi.com/2624-8174/5/1/2 |