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README.md
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@@ -53,7 +53,8 @@ The simulations follow realistic flux, duration, bandwidth, drift rate, and turb
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The simulated event amplitudes follow a **power-law distribution** consistent with solar radio burst statistics:
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This ensures realistic class imbalance and naturally high occurrence of weaker bursts.
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The simulated event amplitudes follow a **power-law distribution** consistent with solar radio burst statistics:
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<img src="https://cdn-uploads.huggingface.co/production/uploads/6914eb6cb0eda273f948014c/elaCFZyeG8zYymkiiDsKl.png" width="700"/>
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This ensures realistic class imbalance and naturally high occurrence of weaker bursts.
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