Reserved for KB archivist: URL to suppl. info.halocmenitta@lmsal.com165035454582019-01-05T22:08:29.501Eruption of a polar crown filament502-690436.25293.32019-01-02T19:25:13.0002019-01-03T00:41:13.000
502.0-690.5
872.0587.0FEHEK0angstromshalocme2019-01-05T22:08:29.486ZtrueLMSALScott GreenMetaEventCreatorn/aFilamentEruptionFE: FilamentEruptionThis is best seen in intensity images in 304 A. Other low coronal signatures seem to be quite limited, implying that it is not a major event. The associated CME is not impressive (http://spaceweather.gmu.edu/seeds/mkmovie.php?cme=20190102.234807.w012.v0596.p251&frame=6&r_. Part of the reason may be that equatorial coronal holes prevent the eruption extending toward the equator. This event was predicted by a famous solar physicist shortly before the occurrence (https://twitter.com/cosmic_jet/status/1080578605271273472).