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Sandra Chapman
University of WarwickMeeting roles in:
The variation of high density region TEC maxima with daily F10.7 and its dependence upon season and solar cycle
Estimating the power carried by coherent structures in solar wind turbulence as seen by Solar Orbiter
Comparing the instantaneous energy transfer rates of plasmoid/flux rope and reconnection magnetic topologies in solar wind turbulence as seen by Cluster
Charting- a new paradigm to combine ‘hard data’ based risk quantification and ‘soft data’ anecdotal reports of hazard
Enter Note
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