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wtbarnes / mocksipipeline

Pipeline for producing synthetic images from the Multi-Order Spectral Imager (MOXSI)
MIT License
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Function for computing response functions for different abundance models #3

Closed wtbarnes closed 9 months ago

wtbarnes commented 2 years ago

When computing the instrument temperature response functions, a particular abundance model is assumed. In general, when computing the DEM through inversion, we don't want to assume a particular abundance model as we are trying to determine which abundance model best matches the observations.

We should have a function that computes the temperature response of both AIA and XRT for different abundances. This involves folding the emissivity through the wavelength response functions of the instrument.

wtbarnes commented 9 months ago

This is closed by the fact that the compute_temperature_response function just takes in a spectra (which can have any abundance applied to it).