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Solar Summer Intern Project Descriptions:
2013
Coronal heating by Alfven wave turbulence and the observational signatures of Alfven waves
Jets in the Solar Atmosphere
Finding the source of ion beams in the solar wind
Tracing out the Solar Magnetic Field
Spectroscopic observations of coronal mass ejections
What Makes the Solar Cycle Tick? Improving prediction through a better Understanding the Evolution of the Polar Magnetic Flux
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