Titlebook: Hot Thin Plasmas in Astrophysics; Roberto Pallavicini (Director of the ASI) Book 1988 Kluwer Academic Publishers 1988 Galaxy.LOPES.Librati

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1389-2185 s they are revealed by X-ray observations from space. The X-ray and UV emission from optically thin thermal plasmas is a common feature of many astrophysical sy978-94-010-7878-8978-94-009-3065-0Series ISSN 1389-2185

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F. Bely-Dubauproposed investigation. The SMOTE method is used for addressing the issue of imbalanced datasets. The utilization of imbalance techniques is highly effective. It may effectively rectify the uneven distribution of classes, hence enhancing the accuracy of a machine learning model in identifying the un

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Martin V. Zombeckomparative results between simulation and experiments, the simulation flame lengths were 30 mm for residual fuel fractions of 1%. In contrast, the flame visualization showed a flame length of 14 mm. Therefore, there was about twice the length difference between the actual flame visualization and the

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