The Fine Structure Fast Solar Wind Near the Sun - Discrete Velocity Microstreams Suggest Energization at the Base of the Corona by Interchange Reconnection Within the Network Magnetic Field

The Fine Structure Fast Solar Wind Near the Sun - Discrete Velocity Microstreams Suggest Energization at the Base of the Corona by Interchange Reconnection Within the Network Magnetic Field

Kavli Institute for Theoretical Physics via YouTube Direct link

The fine structure fast solar wind near the Sun: discrete velocity... | Stuart Bale (UCB)

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The fine structure fast solar wind near the Sun: discrete velocity... | Stuart Bale (UCB)

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The Fine Structure Fast Solar Wind Near the Sun - Discrete Velocity Microstreams Suggest Energization at the Base of the Corona by Interchange Reconnection Within the Network Magnetic Field

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  1. 1 The fine structure fast solar wind near the Sun: discrete velocity... | Stuart Bale (UCB)

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