3D rMHD simulations show coronal nanojets originate in cool dense plasma during reconnection, explaining their collimation and visibility across wavelengths.
arXiv preprint arXiv:2505.02733 (2025)
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On the cool nature of coronal nanojets
3D rMHD simulations show coronal nanojets originate in cool dense plasma during reconnection, explaining their collimation and visibility across wavelengths.