Aurora

Numerous changes including many for OSM, EIRENE, DIVIMP and FACIT

Release including oedge parsing routines, A&M data reading routines using AMJUEL + HYDHEL, corrected particle conservation in particle transport forward model.

Release to trigger publish on pypi+conda

What's Changed

• Add option to not load selected atomic data files by @odstrcilt in https://github.com/fsciortino/Aurora/pull/50
• Prevent error when somebody set zero source by @odstrcilt in https://github.com/fsciortino/Aurora/pull/39
• Provide parsed ADF15 files in the form of pandas DataFrames by @fsciortino in https://github.com/fsciortino/Aurora/pull/51
• small bug in dimensions of rcl_rad_prof fixed by @TGleiter in https://github.com/fsciortino/Aurora/pull/52

New Contributors

• @TGleiter made their first contribution in https://github.com/fsciortino/Aurora/pull/52

Full Changelog: https://github.com/fsciortino/Aurora/compare/v2.0.7-beta1...v2.0.8-beta1

Allow reading of ADF15 with ISEL indices

Release multiple python versions

Updates mostly resulting from PR #37 and #38 and #41 .
This is a new release after a PyPi issue was fixed in pypa/warehouse#10501

Releasing of v.2.0.0. The code is still under active development, but sufficiently stable to motivate jumping above v0. We skip v1 since was initially used on PyPI and to avoid issues it is simplest to go above v1.

Timely update to allow use of spectroscopic line identification from ADF15 files within OMFIT. Other miscellaneous updates.

Simplified treatment of NBI CXR + calculation of tau_imp from steady state runs

New methods/functions added to run the AURORA forward model until steady state and to read ADAS ADF12, ADF21 and ADF22 files. Refer to https://open.adas.ac.uk/ for details.

Improvements for superstage unstaging, time-dept D and V, code efficiency.

Minor update.

Validation of the forward model based on work done with @odstrcilt within OMFIT. A couple of small issues were corrected and the process of unstaging superstages was improved. A few error messages were also added for cases where a user requests a ADAS file that cannot be found, making error interpretation easier.

Inclusion of superstage modeling in AURORA's forward model. This can significantly speed up simulations of ion transport and offer a way to explore the superstage approximation for edge codes.

Other minor changes include modification of functions to get fractional abundances at ionization equilibrium.

Used to simplify conda-forge installation.

Hide a few packages from direct import

Features to permit use of time-dependent sources with standard aurora definitions of the radial grid for forward modeling.