Investigations of Flaring Plasma Parameters during an M-class Flare Using the Differential Evolution Method and XSM/Chandrayaan-2 Observations

Investigations of Flaring Plasma Parameters during an M-class Flare Using the Differential Evolution Method and XSM/Chandrayaan-2 Observations

We employ the differential evolution (DE) method to analyze observations from the Solar X-Ray Monitor on board the Chandrayaan-2 spacecraft. DE belongs to the family of evolutionary algorithms that find solutions using mechanisms inspired by biological processes. This approach enables us to simultan...

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Bibliographic Details
Main Authors: Anna Kępa, Marek Siarkowski, Arun Kumar Awasthi, Janusz Sylwester, Barbara Sylwester
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal Letters
Subjects:
The Sun
Solar x-ray flares
Solar abundances
Solar corona
Online Access:https://doi.org/10.3847/2041-8213/ad0f23

Internet

https://doi.org/10.3847/2041-8213/ad0f23

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