THE UNSOLVED PROBLEM OF SOLAR-WIND TURBULENCE

The solar wind forms the largest wind tunnel for plasma and magnetofluid turbulence that is accessible to Earth.It evolves from what is thought to be a turbulent source that continues to drive nonlinear turbulent dynamics as it q60 headers expands outward via large-scale, energy-containing wind shear and shocks.In the outer heliosphere, once the gr

Few-shot moen finney learning continues to pose a challenge as it is inherently difficult for visual recognition models to generalize with limited labeled examples.When the training data is limited, the process of training and fine-tuning the model will be unstable and inefficient due to overfitting.In this paper, we introduce NegCosIC: Negative Co