Merge branch 'master' into enable-ruff-RUF002-rule

Author: cclauss

.pre-commit-config.yaml

@@ -16,7 +16,7 @@ repos:
       - id: auto-walrus
 
   - repo: https://github.com/astral-sh/ruff-pre-commit
-    rev: v0.3.7
+    rev: v0.4.1
     hooks:
       - id: ruff
       - id: ruff-format
@@ -29,7 +29,7 @@ repos:
           - tomli
 
   - repo: https://github.com/tox-dev/pyproject-fmt
-    rev: "1.7.0"
+    rev: "1.8.0"
     hooks:
       - id: pyproject-fmt
 

computer_vision/cnn_classification.py

@@ -25,7 +25,7 @@
 
 # Importing the Keras libraries and packages
 import tensorflow as tf
-from tensorflow.keras import layers, models
+from keras import layers, models
 
 if __name__ == "__main__":
     # Initialising the CNN

machine_learning/lstm/lstm_prediction.py

@@ -7,9 +7,9 @@
 
 import numpy as np
 import pandas as pd
+from keras.layers import LSTM, Dense
+from keras.models import Sequential
 from sklearn.preprocessing import MinMaxScaler
-from tensorflow.keras.layers import LSTM, Dense
-from tensorflow.keras.models import Sequential
 
 if __name__ == "__main__":
     """

physics/basic_orbital_capture.py

@@ -4,14 +4,14 @@
 
 """
 These two functions will return the radii of impact for a target object
-of mass M and radius R as well as it's effective cross sectional area σ(sigma).
-That is to say any projectile with velocity v passing within σ, will impact the
+of mass M and radius R as well as it's effective cross sectional area sigma.
+That is to say any projectile with velocity v passing within sigma, will impact the
 target object with mass M. The derivation of which is given at the bottom
 of this file.
 
 The derivation shows that a projectile does not need to aim directly at the target
 body in order to hit it, as  R_capture>R_target. Astronomers refer to the effective
-cross section for capture as σ=π*R_capture**2.
+cross section for capture as sigma=π*R_capture**2.
 
 This algorithm does not account for an N-body problem.
 

physics/malus_law.py

@@ -31,7 +31,7 @@
 Real polarizers are also not perfect blockers of the polarization orthogonal to
 their polarization axis; the ratio of the transmission of the unwanted component
 to the wanted component is called the extinction ratio, and varies from around
-1:500 for Polaroid to about 1:106 for Glan–Taylor prism polarizers.
+1:500 for Polaroid to about 1:106 for Glan-Taylor prism polarizers.
 
 Reference : "https://en.wikipedia.org/wiki/Polarizer#Malus's_law_and_other_properties"
 """

pyproject.toml

@@ -11,6 +11,7 @@ lint.ignore = [    # `ruff rule S101` for a description of that rule
   "PT011",    # `pytest.raises(Exception)` is too broad, set the `match` parameter or use a more specific exception
   "PT018",    # Assertion should be broken down into multiple parts
   "RUF001",   # String contains ambiguous {}. Did you mean {}?
+  "RUF002",   # Docstring contains ambiguous {}. Did you mean {}?
   "RUF003",   # Comment contains ambiguous {}. Did you mean {}?
   "S101",     # Use of `assert` detected -- DO NOT FIX
   "S311",     # Standard pseudo-random generators are not suitable for cryptographic purposes -- FIX ME