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Python Analysis Roadmap
Shane Maloney edited this page May 7, 2021
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- Processing raw TM to LB, L0, L1 fits files (L1 to L2 IDL for now)
- Packages: STIXcore
- Inputs: raw TM, spice kernels, SOC data, IDB
- Search, download and plot count-rate data for all products (expected inputs are L1/L2 fits)
- Combine data from requests and transform data from one product to another e.g. compressed pixel data to visibly or spectrogram
- Slice and combine time/energy bins
- Apply energy offsets and per detector energy channels corrections
- Packages: stixpy
- Inputs: ELUTS, Energy offsets, FITs files
- Fit observed count-rate spectra to to solar models to obtain photon spectrum
- Build spectrometer response matrix, detector response matrix, detector model (based on IDL code)
- For initial versions could use high res IDL generated DRMs
- Create model photon spectrum, pass through SRM to obtain count-rate for model and then fits to obtain parameters
- Direct inversion ?
- Packeges:
- stixpy - main interface
- rontogen? - possibly extend need to add versioned xcom data + detector model
- STIXcore - build per-detector SRM
- sunxpec - solar model and fitting?
- Inputs:
- Apply phase correction to
- Packages:
- stixpy - main interface will use STIXcore and xrayvsion
- STIXcore - non-visibility based imaging
- xrayvision - visibility imaging
- Inputs: