An Examination of Observed Coronal Structures through Automated Techniques Across Solar Cycle 24 | Daniel Gass
University of Central Lancashire, United Kingdom
Natural Sciences (Astrophysics and Astrononmy)
The Atmospheric Imaging Assembly (AIA) of NASA’s Solar Dynamics Observatory (SDO) has been providing near uninterrupted coverage of the solar atmosphere since its launch on February 11, 2010, with full coverage of Solar Cycle 24, and ongoing coverage of Cycle 25. With a pixel resolution of 0.6 arcsec and full sun field of view in a time cadence of 12s in multiple EUV bands, this extensive data catalogue has captured a wide array of solar atmospheric phenomenon and can provide information as to how these change with the solar magnetic cycle.
Link to the European Solar Physics Online Seminars (ESPOS) webpage:
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