WHILE SOLAR ENERGETIC PARTICLES (SEPS) ARE BELIEVED TO ESCAPE THE SUN THROUGH OPEN MAGNETIC FIELD LINES, THE IDENTIFICATION OF THE PRECISE ESCAPE ROUTE HAS NOT BEEN POSSIBLE UNTIL NOW. EUV JETS AND TYPE III RADIO BURST IMAGING PROVIDE UNAMBIGUOUS DIRECT S
|Effective start/end date||1/11/13 → 1/10/16|
- National Aeronautics and Space Administration
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