Published June 12, 2024 | Version v1
Computational notebook Open

Cool304: Decomposing the AIA 304 channel into its cool and hot components

Authors/Creators

  • 1. ROR icon Northumbria University

Contributors

  • 1. ROR icon Université Paris-Saclay
  • 2. ROR icon Armagh Observatory & Planetarium
  • 3. ROR icon Universitat de les Illes Balears

Description

Cool and Hot decomposition of the SDO/AIA 304 solar instrument passband.

Three methods are presented for this purpose:

  • RFit method
  • DEM method
  • BSS method

These methods are explained in detail in the publication:
"Decomposing the AIA 304 channel into its cool and hot components"
Patrick Antolin, Frédéric Auchère, Ethan Winch, Elie Soubrié, Ramon Oliver
Solar Physics (2024, accepted)
DOI: 10.1007/s11207-024-02337-4

Files

Solar-Cool-Hot.zip

Files (83.4 MB)

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Additional details

Identifiers

DOI
10.1007/s11207-024-02337-4

Funding

Science and Technology Facilities Council
The Cool Alter-Ego of the Hot Solar Corona ST/R004285/2
Ministerio de Ciencia, Innovación y Universidades
Procesos dinámicos en la atmósfera solar (DynSun) PID2020-112791GB-I00

Software

Repository URL
https://github.com/patrickantolin/Solar-Cool-Hot
Programming language
Jupyter Notebook , Python