- Moved non-critical dependencies out of main requirements.
RadialSolver: Fixed bug in Takeuchi starting conditions where y6 was pulling the incorrect value. Kamata starting conditions were not affected.
- The changes introduced in this release led to around 25% improvement in TidalPy's RadialSolver Love Number Calculator speed.
- TidalPy now works on Python 3.14.
- Bumped version of
ipymplto<=0.11.0. - Bumped version of
CyRKto>=0.17.1, <0.18.1. - Increased numpy's max pinnings to
<2.5.
- Changed
TidalPy.constants.d_PI_DBLtoTidalPy.constants.d_PIsince the "DBL" is redundant with the "d_".- Same for
d_INF,d_EPS_10,d_EPS_100,d_EPS,d_NAN
- Same for
Version 0.7.2 was skipped! It was never released!
- Fixed surface boundary condition bug where dynamic liquid layers were using too small of a struct and could cause crashes (and wrong results).
- Removes support for MacOS 13 builds.
- Fixed top-level directories and files being mistakenly installed.
- Updated
np.trapztoscipy.integrate.trapezoiddue to deprecation of the former. - Fixed bug in the henning melting model where shear modulus may not have had the correct value when fully melted.
- Fixed issues in some of the demo notebooks.
- Fixed notebooks to work with changes to Matplotlib.
- Added action to automatically update version numbers, dates, and commit hashs in
citation.cff,codemeta.json, andmeta.yaml.
- Added
fontsizekwarg to projection plotter in utilities.graphics. - Changed the default of
yplotso plotting imaginary parts of radial solution is by default off.
- Added JOSS paper draft to Papers/2025-JOSS.
- Added documentation interface with Sphinx and ReadTheDocs.
- Added and updated readme badges.
- Extensive changes to all documentation files and structure.
- Changed how CHANGES.md (main change log) is structured. Major versions will appear as top level headers.
- Change TidalPy's license to Apache 2.0.
- Added
CODE_OF_CONDUCT.mdwith TidalPy's code of conduct. - Added
CONTRIBUTING.mdwith information on how others can contribute to TidalPy. - Updated
citation.cffwith latest information. - Added
codemeta.jsonwith citation and metadata. - Removed MacOS-13 tests.
- Removed unused code, tests, and documentations.
- TidalPy now uses
ruffto check for code issues.- Added ruff lint check to ubuntu tests.
- Fixed many code issues found with ruff (these are not bug fixes, just syntax compliance and best practices).
- Moved more module/file level constants into TidalPy.constants and in the configuration file.
- Added TidalPy logo.
- Added more restrictive pinning for numpy's max version to work with latest CyRK.
- RadialSolver solution can now provide quality factors
rs_solution.Qand phase lag angles (in radians)rs_solution.lag.
- Fixed issue where RadialSolver would incorrectly say a result was successful when the application of surface boundary conditions failed.
- Fixed issue where RadialSolver solution's diagnostics would print the incorrect parameter for a planet's mass.
- RadialSolver solution returns nan's instead of None for Love numbers when a solution fails.
- RadialSolver solution Love number attributes now return lists of np.nan if the user requested multiple solution types (e.g., "tidal, loading") and the solution failed. This allows the user to still subscript
rs_solution.k[0], rs_solution.k[1]even if the solution was not successful.
- Added more tests to check RadialSolver Solution attributes.
- Fixed issue where
TidalPy.RadialSolver.shootingwould pick the incorrect starting index. If the starting layer (set by the starting radius) was not the first layer it could cause a int overflow and lead to access violation crashes.
- Updates some GitHub action dependencies.
- Added more tests to check
RadialSolverstarting radius conditions to try to catch bugs like this patch fixed!
TidalPy.tides.modes.collapse_multilayer_modesnow checks for ill-formedradius_arraysand will raise an error if it detects a problem.- Improved how
projection_mapdisplays colorbar numbers.
- Fixed issue where
TidalPy.tides.modes.collapse_multilayer_modeswas not treating macro-layer boundaries correctly.
TidalPy.tides.modes.collapse_multilayer_modesnow requires a tuple of rheology instances for both shear and bulk rheology. One for each macro layer. This allows different rheologies to be used for different layers.
- Fixed some warnings that were showing up in the multilayer demo notebook.
- Updated to work with CyRK v0.15.1
- This change results in about a 18% performance improvement for RadialSolver depending on the problem.
- Converted RadialSolver and EOSSolver status message to C++ strings.
- Updated some documentation.
- Fixed potential issue where RadialSolver could use a very small or even negative maximum step size.
- Added test to check if structure arrays have been changed.
- Added debug flag to installation files to help with cython debugging.
- Fixed issue where TidalPy structures (layers, planets, etc.) would return editable arrays instead of copies of arrays. This could lead to subsequent functions (like planet paint) changing the arrays. This fixes GitHub Issue #74.
- Fixed issue where shooting method was corrupting data when starting radius was too large (which happened for higher orders of l) This fixes GitHub Issue #72.
- Fixed broken demo notebooks.
- Removed max version limit for platformdirs package
- Changes GitHub actions to avoid testing when not needed.
- Now supports Python 3.13
- Removed various files that were being included in the manifest
- Updated to work with CyRK 0.13.3
- Updated to work with Numpy 2.x
- Bumping version to integrate into conda-forge.
- Fixed some build processes that could cause both numpy 1.X and 2.X to be installed and inconsistent use (only affected MacOS)
- Added performance benchmark for
TidalPy.RadialSolver.helpers.
- Fixed memory leak that was occurring in the EOS Solver (therefore also RadialSolver) due to CyRK's CySolverSolution not being dereferenced (this is a problem with CyRK, but hack applied to TidalPy until a fix can be made to CyRK).
- Improved
TidalPy.RadialSolver.helpers.build_rs_input_from_dataperformance by factor of 10x to 150x depending on layer structure. - Improved
TidalPy.RadialSolver.helpers.build_rs_input_homogeneous_layersperformance by factor of 15% to 3.5x depending on layer structure. - Improved
TidalPy.RadialSolver.radial_solverperformance by around 10% depending on layer structure.
- Removed support for the older non-cythonized
TidalPy.radial_solvermodule in favor ofTidalPy.RadialSolver
- Moved RadialSolver's Boundary Condition finder to its own function in
TidalPy.RadialSolver.boundaries.surface_bc.pyxto allow it to be used by both the shooting and propagation matrix techniques. - Decoupled radial solver from shooting method.
- Moved the shooting method (formerly just called
cf_radial_solver) to a dedicated file to prep for a different dedicated file for the prop matrix solver. - Now
TidalPy.RadialSolver.solveronly contains driver functions and output structures.
- Moved the shooting method (formerly just called
- Added Propagation Matrix technique to RadialSolver
- This is simplified for now. Only planets with 1 solid, static, incompressible layer are allowed.
- Other assumptions can be approximated, e.g., liquid layers use a small shear modulus.
- Multiple layers should also work if you have discontinuities in density, shear, etc. within your "one layer".
- A cythonized solid fundamental matrix implementation can be found in
TidalPy.RadialSolver.PropMatrix.solid_matrix.
- This is simplified for now. Only planets with 1 solid, static, incompressible layer are allowed.
- New radial slicing scheme required:
- TidalPy now requires
radial_solverinput arrays to be defined in a precise manner:radius_arraymust start at 0.- Each layer's upper and lower radius must be in the
radius_array. That means if there is more than one layer there will be two identical radius values!- E.g., if a planet has a ICB at 1000km and a CMB at 3500km. Then
radius_arraymust be setup with 2 values of 1000km and 2 values of 3500km. - Other parameters should be defined on a "as layer" basis. So shear modulus at the 1st 1000km would be the shear of the inner core, at the 2nd 1000km it would be the shear modulus of the outer core. Likewise shear modulus at the 1st 3500km would be for the outer core and at the 2nd 3500km would be the shear modulus for the mantle. Same goes for density and bulk modulus.
- E.g., if a planet has a ICB at 1000km and a CMB at 3500km. Then
- TidalPy now requires
- Added warning to check for instabilities (based on large number of steps taken; requires
warnings=True). - Changes to
radial_solverarguments:- Many changes to the order as well as additions and removals of arguments to
radial_solverhighly suggest looking through the updated documentation. radial_solverno longer requiresgravity_array.- New with this update is a self-consistent equation of state solver (EOSS) that is called from
radial_solver. This EOSS is used to find gravity(r).
- New with this update is a self-consistent equation of state solver (EOSS) that is called from
- Bulk modulus must now be provided as a complex-valued array
- If a non-zero imaginary portion is provided (e.g., found via a rheology) then bulk dissipation is now tracked.
- If imaginary portions are zero, then bulk dissipation is ignored as in TidalPy v0.5.x and earlier. (this is actually dependent on your bulk rheology; it could also cause infinities...)
- Several arguments have had slight name refactors which will break calls that used keyword arguments. Review the RadialSolver documentation or "TidalPy/RadialSolver/solver.pyx" for the new argument names.
upper_radius_bylayer_arraymust now be provided as a numpy array (previously a tuple of floats was acceptable).- Added new optional argument
surface_pressure(default=0.0) used with EOSS to find pressure convergence. - Added new optional argument
core_model(default=0) used to set the lower boundary condition when the propagation matrix technique is used. - Added new optional argument
starting_radius(default=0.0) to allow the user to set the initial radius for the radial solution.- Setting the solution radius higher in the planet can improve solution stability when using the shooting method. Particularly if looking at higher harmonic
degree_ls. There is a trade off with accuracy so advise testing. - The starting radius must be >= 0.0, if 0.0 is provided (the default) then TidalPy will use the Martens technique to find a suitable starting radius (function of
degree_l, planet radius, and the new optional argumentstart_radius_tolerancewhich defaults to 1.0e-5).
- Setting the solution radius higher in the planet can improve solution stability when using the shooting method. Particularly if looking at higher harmonic
- Removed
limit_solution_to_radiusargument. - Added new optional argument
use_prop_matrix(default=False) to use the propagation matrix technique over the shooting method. - Equation of State Solver arguments:
eos_method_bylayer- EOSS method to use for each layer (currently only "interpolate" is supported).eos_integration_methodRunge-Kutta method to use for EOSS (default="RK45").eos_rtolandeos_atolcan also be provided to control integration error.eos_pressure_tol(default=1.0e-3) andeos_max_iters(default=40) control the pressure convergence of the EOSS.
- Added optional argument
perform_checks(default=True) that performs many checks on the user input before running the solution (small performance penalty, but highly recommend leaving on until your inputs are tested). - Added optional argument
log_info(default=False) that will log key physical and diagnostic information to TidalPy's log (which can be set to be consol print, log file, or both via TidalPy's configurations).- Note there is a performance hit when using this, particularly if logging to file is enabled.
- Many changes to the order as well as additions and removals of arguments to
New RadialSolver Helpers
- To assist with the generation of valid inputs to
radial_solver, TidalPy now provides two helper functions:- For planets with homogeneous layers:
from TidalPy.RadialSolver import build_rs_input_homogeneous_layerstakes in attributes for a planet made of layers with constant physical properties and then provides the arrays and other requiredradial_solverinputs that conform to the newradius_arrayscheme. - For planets with inhomogeneous layers:
from TidalPy.RadialSolver import build_rs_input_from_datawhich parses data arrays (loaded from a file or built elsewhere like using a more robust EOS than TidalPy offers) and makes changes to ensure they will work withradial_solver.
- For planets with homogeneous layers:
Expanded RadialSolverSolution Attributes and Methods
- The output of
radial_solver, an instance of theRadialSolverSolution, has been greatly expanded to provide much more data and functionality to the user. Full details can be found in the new RadialSolver documentation. Highlights include:- EOSS results like
<solution>.mass,<solution>.moi,<solution>.moi_factor,<solution>.central_pressure,<solution>.surface_gravity. - Diagnostic data like number of integration steps required per layer to find a solutions
<solution>.steps_taken, or EOSS diagnostics:<solution>.eos_iterations,<solution>.eos_pressure_error,<solution>.eos_success,<solution>.eos_message,<solution>.eos_steps_taken.- Much of the new diagnostic data as well as key results can now be quickly printed using
<solution>.print_diagnostics().
- Much of the new diagnostic data as well as key results can now be quickly printed using
- Method to quickly plot the viscoelastic-gravitational solution y's
<solution>.plot_ys(). - Method to quickly plot the EOS results
<solution>.plot_interior(). - In addition to the previously provided attributes like
<solution>.love,<solution>.k,<solution>.h,<solution>.l,<solution>.result.
- EOSS results like
- Shifted away from
PyMem_FreetoCyRK.utils.mem_freeto allow for consistency in future development.- Avoiding using these manual heap allocations whenever possible. Many new uses of smart pointers and C++ vectors.
- Updated GitHub actions.
- Moved to more consistent and robust types (e.g., int for degree_l vs. prior unsigned-char; unsigned-int).
- Added inverse function
cinvinTidalPy.utilities.math.complex. - New "TidalPy/constants.pyx" isolates all TidalPy constants. Available to both Python and Cython. Refactored all files to use the constants in this file.
- New numerics module
TidalPy.math.numericsfor low-level floating point functions.- New cythonized
isclosefunction that matches functionality of python'smath.isclose
- New cythonized
- Cythonized radial sensitivity to shear/bulk functions in
TidalPy.tides.multilayer.sensitivity(based on Tobie+2005) - Cythonized radial heating functions that use the sensitivity to shear/bulk functions in
TidalPy.tides.multilayer.heating(based on Tobie+2005) - Improved logging so it is less spammy.
- Logger now logs all exceptions raised.
- Moved TidalPy's default config and world config dir to user's "Documents" folder (from system appdata folder).
- If upgrading from previous version of TidalPy, you can safely delete the old config directory.
- On Windows the old dir was: "'C:\Users\\AppData\Local\TidalPy'"; The new dir is "'C:\Users\\Documents\TidalPy'"
- On Mac the old dir was: "'/Users//Library/Application Support/TidalPy'"; The new dir is "'/Users//Documents/TidalPy'"
- On Linux the old dir was: "'/Users//.local/share/TidalPy'"; The new dir is "'/home//Documents/TidalPy'"
- If upgrading from previous version of TidalPy, you can safely delete the old config directory.
- New switch
TidalPy.log_to_file()to quickly turn on saving log to file (this can also be adjusted in the TidalPy configurations). - TidalPy now looks for an environment variable "TIDALPY_TEST_MODE" to turn on test mode during first initialization (can later be changed using the
TidalPy.test_mode()command or settingTidalPy._test_mode = False; TidalPy.reinit()). - Made use of more TidalPy-specific exceptions.
- Tweaked the
TidalPy.utilities.graphics -> yplot. - User can now override TidalPy.config using
TidalPy.reinit(<new config toml file path; or dictionary of configs>). - Refactored and made improvements to
TidalPy.utilities.graphics.planet_plot.
- Added support for CyRK v0.12.x
- Added support for Burnman v0.2.x
- Reworked TidalPy's documentation structure in prep for a shift to Sphinx in the future.
- Greatly expanded and improved RadialSolver documentation which can be found in "TidalPy/Documentation/RadialSolver"
- Fixed issue where
radial_solverarrays could dealloc while references still pointed to them (hanging pointers). - Missing Cython compile arguments in TidalPy's utilities,
nondimensional.pyx. - Fixed incorrect type in dynamic liquid layers that may have been causing some errors to propagate.
- Fixed issue where
TidalPy._config_pathwas not being updated. - Fixed issue where log files could not be created.
- Fixed dependency compatibility issues.
- Fixed incorrect function signature type for scipy's
spherical_jn. SciPy v.1.14.X uses a new signature which is breaking on MacOS. Limiting to "SciPy<1.14" for now. See GitHub Issue #65
- Fixed RadialSolver frequency warning message for dynamic liquid layers not displaying for correct layer types.
- Added way to suppress warning messages in RadialSolver.
- To turn this suppression on, pass
warnings=FalsetoRadialSolver.radial_solver.
- To turn this suppression on, pass
- RadialSolver: Fixed bug where solutions between liquid and solid layers were not propagating correctly.
- New Love number benchmarks for Earth provided by Nick Wagner in
Benchmarks & Performance\RadialSolver\Earth Love Numbers.ipynb(Jupyter Notebook).
- Pre-allocated several cythonized arrays to nans to help with debugging.
- Provided more error messages to improve user experience.
- Cythonized non-dim function now takes in the planet's density and radius as variables to change.
- Improved the Tobie and Roberts benchmarks for radial solver.
- Updated to work with CyRK 0.8.7
- Improved RadialSolver documentation regarding higher degree-l.
- Added info about issues that can arise from using non C-continguous arrays in cythonized functions.
- Added error message to
RadialSolver.radial_solverif length of provided assumption tuples is not the same. - Fixed issue where non C-continguous arrays were allowed in cythonized functions that required them.
- Removed Python 3.8 support due to issues with building SciPy.
This version is likely to break code based on TidalPy v0.4.X and earlier
- A major change starting with v0.5.0 is the switch from numba.njited functions to cython precompiled functions and extension classes. The reasons for doing this are numerous. This transition will be completed in stages with minor versions (v0.X.0) each bringing a new set of cythonized updates until all njited functions are retired.
- For this version:
- Converted
TidalPy.radial_solver.radial_solverto cythonizedTidalPy.RadialSolver.radial_solver.- The old radial solver method will be removed in TidalPy version 0.6.0.
- Added new cython-based
TidalPy.utilities.classes.base_xbase cython extension class that other classes are built off of. - Converted
TidalPy.rheology.complex_compliances.compliance_modelsto cythonizedTidalPy.rheology.models.- Improved the new rheology methods to better handle extreme values of frequency and modulus.
- The old rheology solvers will be removed in a future release of python.
- Added several new cython-based helper functions in the utilities package.
- Converted
- Added support for Python 3.11 and 3.12. TidalPy now runs on Python 3.8--3.12.
- Note that currently the Burnman package does not support 3.12 so that functionality is limited to python 3.8-3.11.
- Removed support for
solver_numbain theradial_solvermodule. - Removed some imports from main package and sub modules'
__init__to avoid slow load times. - Moved conversion tools from
TidalPy.toolbox.conversionstoTidalPy.utilities.conversions. - Changed setup files so that cython code can be compiled.
special- for high-performance, general, scientific functions.
- Moved TidalPy configs to a standard user directory by default. The specific location will depend on the OS.
- Default configs will be installed on the first
import TidalPycall after installation.- These defaults are stored in the
TidalPy.defaultc.pyas a string which is copy and pasted to the newTidalPy_Configs.toml.
- These defaults are stored in the
- There is a new
TidalPy.clear_data()function to delete all data stored in these locations. Data will be rebuilt the next time TidalPy is imported. - New
TidalPy.set_config(config_path)to change the active configuration file used by TidalPy.- Note that
TidalPy.reinit()should be called after changing the configurations.
- Note that
- New
TidalPy.set_world_dir(world_dir_path)to change which directory to pull world configs from. - Moved away from the system of
default.pyconfigurations for sub modules. All default configs are stored in the sameTidalPy_Config.toml
- Default configs will be installed on the first
- Shifted from
jsontotomlfiles for world configs.- Store all world configs to a zip file for easier distribution.
- TidalPy now requires:
- CyRK>=0.8.6
- Cython>=3.0.0
- Moved
BurnMan3rd party dependence to a more dedicatedExtendingfolder for future development. - To make TidalPy lighter weight we are starting to remove a lot of 3rd party packages.
complex_complianceconfigurations are now stored in the top levelrheologyin all configs.- For example, in prior TidalPy versions you would need to change the complex compliance model by editing
config['layers']['mantle']['rheology']['complex_compliance']['model'] = 'andrade'. Now this would be:config['layers']['mantle']['rheology']['model'] = 'andrade'.
- For example, in prior TidalPy versions you would need to change the complex compliance model by editing
- Added unique frequency finder functions to the
modesmodule. - Moved most of the type hints behind the
typing.TYPE_CHECKINGflag. - Moved non-critical files out of repository.
- Created a new
tides.heatingmodule and moved the volumetric heating calculations there. - Expanded the performance suite to better track the
radial_solvermodule. - Moved
cache.pyto top-level. - Turned off numba cacheing on several functions that may be used in the radial solver.
- rheology
- complex compliance functions
- radial_solver.numerical
- initial guess functions
- interface functions
- rheology
- Converted radial_solver.numerical initial guess and interface functions output to np.ndarrays rather than numba lists.
- Removed
config_helper.pyand the functions defined within. - New RadialSolver class now supports more than just boolean inputs.
- Future proofing to allow for a greater variety of layer types.
- Added exoplanet archive download functionality in
TidalPy.utilities.exoplanets.
- Fixed floating point comparison bug in
multilayer_modessolver. - Fixed obliquity not being used issue in quick tides calculator.
- Fixed issue in incorrect TidalPy version being loaded into the package.
- Improved the performance of the stress and strain calculator by ~20%.
- Cythonize Performance Increases:
- New
RadialSolver.radial_solverleads to a ~50x performance boost. - New cythonized rheology models are 500% faster for arrays; 40,000% faster for scalars (not a typo!)
- New
- Moved
radial_solverto a top-level module of TidalPy.- Added
find_lovefunction to theradial_solvermodule for the calculation of Love and Shida numbers. - Added
sensitivity_to_shearfunction to theradial_solvermodule based on Tobie et al. (2005). - Added
sensitivity_to_bulkfunction to theradial_solvermodule based on Tobie et al. (2005).
- Added
- Added
newtonandelasticcomplex compliances to rheology module for ALMA comparisons.
- Updated and added to
radial_solvertest suite. - Changed
radial_solver.interfacesfunctions to only require the top most value of the radial solutions rather than the whole array.
- Fixed bug in
radial_solverwhere interfaces between a dynamic and static liquid were not correctly handled.
- Added a multilayer tidal potential that allows for arbitrary obliquity.
- Added in load Love number calculations to the multilayer code.
- Removed a lot of 3rd-party dependencies to make TidalPy's install more lean.
- Switched over to using the integrators from the new
CyRKpackage- Changed the signature of the numerical-int multilayer solver.
- Breaks Old Code
- Changed the signature of the numerical-int multilayer solver.
- Issue with Numba 0.55 and dictionary updates. This restricts TidalPy to Python version 3.9 or lower.
- Started a lot of prep work for a move to sphinx or similar for documentation (this will be a 0.5.0 feature).
- Created a generalized multi-layer collapse function in
TidalPy.tides.multilayer.numerical_int.collapse.- This will likely break old code. It was introduced in v0.4.0.dev10.
- Arbitrary layer structures can now be fed into the y-solver. e.g., liquid-solid, solid-liquid, liquid-solid-liquid-solid, etc.
- Note: Multiple dynamic liquid layers will likely lead to stability problems.
- y-solver no longer requires a
model_namevariable. The function will automatically utilize the correct model based on theis_layer_solidandis_layer_staticlists. - Removed the old code that handled individual cases.
- Interfaces between multiple liquid layers are now supported (but not well tested).
- Two liquid layers of different types can be next to one another (dynamic-static; static-dynamic).
- y-solvers functional argument signature has changed (both regular and numba versions)
- Breaks Old Code
- Numerical integrator declaration has changed.
- Planet_bulk_density is now a required argument.
- Modified several other TidalPy functions to match this new call signature for the y-solver.
- Removed the y-derivative return from the propagation matrix (to match the output format of the numerical int)
- Breaks Old Code
- Refactored
tidal_y_solvertoradial_solversince non-tidal calculations can be made with it.- Breaks Old Code (pre v0.4.0.dev11)
- Switched from
setup.pyto a streamlinedpyproject.tomlinstallation process. - Changes to radial ODE's
- Input arguments and output diffeqs are now passed as numpy arrays rather than tuples.
- Input and outputs are now passed as floats not complex (doubling the number of terms)
- Added
numba-scipydependence to allow the use of scipy's special functions.- Removed the pre-calculated factorial method. Using scipy's gamma now.
- TODO: Note the numba-scipy package on github is not updated to the newest version of scipy. Packaging numba-scipy with TidalPy for now.
- Improved the performance of the pure-numba radial solve by ~10%
- Added newer functions to the performance recording suite.
- Improved performance of eccentricity and inclination functions for non-multilayer tidal calculations.
- Added TidalPy to Zenodo. DOI added to readme.
- Removed Gitter account for now.
- Added files and functions to quickly install additional 3rd party applications
- Improvements to GitHub workflows
- Switched over to using the 3rd party
cmcramericolormap package rather than trying to maintain it within tidalpy - Added a delta time to HH:MM:SS converter to utilities.string_helper
- Made improvements to multiprocessing user info
- Cleaned up & added some docstrings and type hints
- Tidal y solver for the prop matrix method no longer returns the y-derivatives.
- dy1/dr is now calculated directly in the
decompose()function.
- dy1/dr is now calculated directly in the
- Created a config helper function
TidalPy.test_mode()to quickly setup TidalPy configs for pytest'ing - Cleaned up comments and reordered items in
multilayer.numerical_int.collapse. - Fixed a bug when using SciPy's Radau integrator method.
- The version number is now checked with importlib in TidalPy.init. Version number should only be changed in the pyproject.toml.
- Updated the pure-numba version of the radial solver's argument signature to better match the python implementation.
- Updated Github Actions
- Fixed bug in GridPlot related to number of subplots.
- Fixed bug in global variable for world config loader.
- Fixed type hint bug in the numba-based tidal y solver.
- Fixed bug that caused numba-based tidal y solver to not compile.
- Fixed bug that was causing full TidalPy log to print while in a Jupyter Notebook environment.
- If you would like the log to print in a notebook then use
TidalPy.toggle_log_print_in_jupyter()or set theprint_log_in_jupytertoTruein the "configurations.py" file.
- If you would like the log to print in a notebook then use
- Fixed an error in the multimode volumetric heating calculation where "_rr", "_thth", "_phiphi" were being double counted
- Fixed an error in the stress/strain calculations where the static, instead of complex, shear was being used.
- Removed the soon-to-be deprecated np.float, np.complex, np.int references.
- Added a check to see if cartopy is installed before functions that depend on it are imported.
- Fixed coverage problem with github actions.
- Fixed issue importing nbTuple.
- Fixed issues with GitHub actions and coverage.
Multilayer scripts based on 0.3.3 or earlier will likely break with this version!
- Added
TidalPy.modes.multilayer_modes.pymodule to offer simplified calculation of multilayer tidal heating. - Added
GridPlotclass to quickly make grid-like matplotlib figures. CheckoutTidalPy.utilities.graphics.grid_plot.py - Added
Cartopydependence.- Can now make cool projection maps! Added basic functionality to
TidalPy.utilities.graphics.global_map.py. - New jupyter notebooks to showcase map projects and GridPlot functionality.
- Can now make cool projection maps! Added basic functionality to
- Improved performance on both mode and non-mode tidal potential functions by at least a factor of 3. If used correctly these can be nearly 100x faster.
- Added a new obliquity version of the mode version tidal potential.
- Stress and strain relationship for multi-layer tides now allows for arbitrary rheology.
- Created a single multilayer solver to handle an arbitrary layer structure.
See
TidalPy.tides.multilayer.numerical_int.solver.py - Stress & Strain relationship now accounts for arbitrary rheology.
- Created a single multi-mode solver for multilayer problems. See
TidalPy.tides.modes.multilayer_modes.py - TidalPy now defaults to using the frequency dependent zeta versions of Andrade and Sundberg rheologies.
- This was done to avoid issues with real(complex_comp) at zero frequency which happens in multi mode calculations.
- Added numba-safe version of multilayer calc
- Added a helper function to quickly calculate masses, volumes, and gravity for spherical shells provided a radius
and density array:
TidalPy.utilities.spherical_helper.calculate_mass_gravity_arrays. - Added more colormaps, updated how reserved versions are constructed, updated old maps.
- Better support for post-multiprocessing function inputs.
- Refactored tidal mode calculation functions into a new TidalPy.tides.modes module.
- Added a voxel calculator to TidalPy.utilities.spherical_helper. Also, added related tests & benchmarking tools.
- Added a dictionary to track known color maps. It can be imported at
TidalPy.utilities.cmaps.KNOWN_CMAPS - Made some improvements to the unique_path function in io_helper.py
- Rearranged the tidal potential argument order.
- Added some sanity checks on the various kinds on both mode and non-mode tidal potentials to compare with one another.
- Updated stress, strain, and displacement calculations to account for new low-memory calculation method.
- Greatly increased performance of multilayer stress, strain, and potential calculations.
- Refactored much of the multilayer functions from TidalPy.toolbox to TidalPy.tides.multilayer.numerical_int and sub modules
- Reworked numba-safe RK integrator. Does not reproduce scipy exactly for chaotic functions when numba is on.
- Fixed issue that was causing some multilayer boundary calculations to be 10x slower.
- Fixed issue where 2D arrays would not work on njited
neg_array_for_log_plotfunction. - Fixed issue where there could be negative love numbers with frequency is zero in multi-mode calculator
- Updated to work with BurnMan v1.0 release.
- Updated the NSR tidal potential for multilayer code to a multi-modal version
- Improvements to the multilayer module
- Added more tests
- Removed the remaining
_arrayfunctions
- Changes to setup to use released version of BurnMan.
- Added a simplistic (not modal version) NSR tidal potential for use in the multilayer code.
- Added multiprocessor toolkit to
TidalPy.utilities.multiprocessing
- Did large scale code reformatting (just style, no refactoring) on nearly all files.
- Cleaned up some doc strings.
Scripts based on 0.2.x will likely break with this version!
- Added the first iteration of a multilayer tidal calculator module in
TidalPy.tides.multilayerthis module provides basic functionality to calculate tidal dissipation in a semi-homogeneous, shell-based approach. This is more accurate than the pure homogeneous model used throughout the rest of TidalPy. The downside with the current version is that it does not allow for NSR or high eccentricity / obliquity. A future version will attempt to add in a more robust Tidal Potential equation which will allow for additional physics. - Setup.py has been revamped as has the installation process. This is in prep to allow for TidalPy to become available on PyPI.
- Did away with most of the
_arrayfunctions. Found a way for njit to compile a function to handle either arrays or floats.- Left the
self._func_array(in addition toself._func) in themodel.pyclasses just in case we ever ** do** need to define array functions in the future: all the infrastructure is still in place.
- Left the
- Added a numba-safe Explicit Runge-Kutta integrator. This is fully wrapped in njit'd functions.
- On its own this can be 5--20 times faster than
scipy.solve_ivp. - This also allows the integration function to be used from within another njit'd function(s).
- This is still very experimental so please use caution and testing when using it.
- On its own this can be 5--20 times faster than
- Numerous bug fixes.
- Removed the array versions of the dynamic functions.
use_arrayis still tracked in OOP and some quick calculation functions. These may all be not necessary now.
- New cookbook to showcase the multilayer calculations.
- Added surface area slices to base physical class.
- Fixed some issues with how radius slices are tracked within layers and worlds.
<world/layer>.radii[0]is never the radius at the bottom of the object, it is always one dx up.- An interpolation had to be added to Burnman layers since Burnman radii starts at 0.
- Improved various docstrings.
- Refactored the
TidalPy.toolstoTidalPy.toolbox. - Refactored
CookbookstoDemos. - conversions.semi_a2orbital_motion and orbital_motion2semi_a now always return np.nan where they used to return complex numbers.
Will break studies based on previous versions
Note: TidalPy version of "0.2.0" was never made publicly available. This is the next version after 0.1.0.
- Major refactoring all over.
- Replaced the custom logging system with one based on Python's logging package.
- Logger will not print to console if using a Jupyter notebook.
- User can decide if the log is saved to disk or not.
- Modified OOP Backend
- Models are now free to access the state properties of layers and planets. This eliminates the need to pass arguments into model classes for calculations. All the user has to do is change the layer and/or planet's state properties and then those changes will automatically propagate.
- New Rheology Scheme
- To better follow real physics, all strength-based models have been moved under the redesigned
Rheologyclass. - This includes: liquid and solid viscosity calculations, partial melting, and complex compliance
- Love numbers are now calculated by a new
Tidesclass instead of theRheology(see next bullet point).
- To better follow real physics, all strength-based models have been moved under the redesigned
- New Tides Module
- New
Tidesclass and child classes have been implemented which handle all Love number and tidal calculations for both a rheology-based approach or for the CPL/CTL model. - This module contains functionality to calculate tidal heating and tidal potential derivatives based on a complex compliance function and the various thermal and orbital parameters.
- The functions to calculate the Love numbers are also stored here.
- New eccentricity functions have been added including terms up to and including e^20 and tidal order l=7.
- New inclination functions have been added (with arbitrary accuracy) up to tidal order l=7.
- New
- Other
- Various functions and classes have been reworked or removed to simplify the code base.
- Removed ".pyname" from classes.
- Utilities package has been reorganized.
- Changed the setup pipeline to only require one command.
- Many new docstrings, type hints, and overall clean up of functions and classes. All docstrings should now follow the numpy format.
- Many new tests for both the functional and OOP versions of TidalPy.
- setup.py no longer requires a separate command line call to install the Burnman package.
- More comments and spelling/typo fixes everywhere.
- Added CVD-friendly color maps made by Crameri (2018; http://doi.org/10.5281/zenodo.1243862) to the utilities.graphics module
- More log.debug() calls all over. This should hopefully help bugfixes in the future (especially OOP bugs).
- Fixed bug in world_builder.py : build_from_world where nested dicts were not being overwritten as expected.
- Fixed bug in melt fraction checks for the float version of the Henning model.
- Fixed bug in the Henning melting model where viscosity and shear was not being calculated correctly during the breakdown band (critical melt fraction + ~5%). This only affected a phase space that was rarely important for tidal calculations (planets would pass through it very quickly).
Initial Release - Changes not tracked