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Mapping solar magnetic fields from the photosphere to the base of the corona
DOI: 10.1126/sciadv.abe8406 Bibcode: 2021SciA....7.8406I

Hara, Hirohisa; De Pontieu, Bart; Carlsson, Mats +25 more

Routine ultraviolet imaging of the Sun's upper atmosphere shows the spectacular manifestation of solar activity; yet we remain blind to its main driver, the magnetic field. Here we report unprecedented spectropolarimetric observations of an active region plage and its surrounding enhanced network, showing circular polarization in ultraviolet (Mg I…

2021 Science Advances
Hinode IRIS 50
The source of the major solar energetic particle events from super active region 11944
DOI: 10.1126/sciadv.abf0068 Bibcode: 2021SciA....7...68B

Brooks, David H.; Yardley, Stephanie L.

Shock waves associated with fast coronal mass ejections (CMEs) accelerate solar energetic particles (SEPs) in the long duration, gradual events that pose hazards to crewed spaceflight and near-Earth technological assets, but the source of the CME shock-accelerated plasma is still debated. Here, we use multi-messenger observations from the Heliophy…

2021 Science Advances
Hinode 29