The invention discloses an Ia type super-novelty star spectral parameter rapid inversion method based on a KAN network, and the method comprises the following steps: S1, carrying out data preprocessing, generating
simulation spectral data, including spectral lines and parameters, and carrying out the normalization; s2, building a KAN (Kernel
Area Network)
network model by using a python framework and a pytorch framework; s3, designing a
loss function; s4, training the model, and testing the error of each parameter in the stage; s5, performing learning rate adjustment by using an Adam optimizer and a StepLR scheduler in the training process, and optimizing the model; s6, performing
Gaussian sampling on an actually measured spectrum, and inputting the actually measured spectrum into the trained KAN model for prediction; s7, analyzing the result, and calculating the standard deviation of the output parameter data; by using the
deep learning technology of the KAN network, key physical and chemical parameters are efficiently predicted from the
celestial body spectrum, the problems that in the prior art, the calculation amount is too large, and an accurate calculation result cannot be efficiently obtained are solved, and the method has remarkable advantages in the aspects of improving the calculation efficiency and the
processing capacity and is suitable for spectrum
data analysis in the field of astronomical observation.