Changelog#

0.1.0 (unreleased)#

First pre-alpha release of muse, a Python library to read, analyze, and reduce data from the Multi-slit Solar Explorer (MUSE) mission.

muse.synthesis.vdem_synthesis — synthesize observables from a VDEM raster and one or more response functions via a tensor product, with NumPy, PyTorch, or JAX backends (optional GPU).
muse.synthesis.create_simple_vdem — build a velocity differential emission measure (DEM as a function of temperature and line-of-sight velocity) from a simulation box.
muse.synthesis.calculate_moments — compute the zeroth, first, and second spectral moments of a spectrum, with optional velocity masking. Flux and Doppler coordinate names are configurable.
muse.synthesis.wavelength_to_doppler / doppler_to_wavelength — convert between wavelength and Doppler-velocity coordinates.

muse.instrument.read_response — read a response function into an xarray.Dataset, interpolating over temperature (logT) and velocity (vdop) as needed.
muse.instrument.load_and_concat_responses — load multiple response functions and concatenate them along the line axis.

muse.transforms.match_fov — match data to the MUSE field of view by resampling to the instrument resolution and tiling along the raster axis.
muse.transforms.reshape_x_to_slit_step / reshape_slit_step_to_x — convert between a single x spatial axis and the slit / raster-step layout.

muse.variables.DEFAULTS_MUSE — frozen MUSE instrument constants (pixel sizes, slit geometry, diffraction parameters) with units attached.

Previous muse PyPI package which existed before LMSAL took over the namespace on PyPI.