The helioseismic and magnetic imager (

Hayashi K, Hoeksema JT, Liu Y , Bobra MG, Sun XD, Norton AA · 2015 · DOI 10.1007/s11207-015-0686-z

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it

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astro-ph.SR · 2026-05-25 · unverdicted · novelty 5.0

Sulphur abundances decrease above 150 G in coronal loops, indicating FIP fractionation is modulated by mean magnetic field strength.

astro-ph.SR · 2026-04-21 · unverdicted · novelty 4.0

Statistical analysis shows solar energetic electrons rarely cross the heliospheric current sheet unless the source or spacecraft is close to it.

Showing 2 of 2 citing papers.

Signs of Sulphur fractionation under high magnetic field strength astro-ph.SR · 2026-05-25 · unverdicted · none · ref 48
Sulphur abundances decrease above 150 G in coronal loops, indicating FIP fractionation is modulated by mean magnetic field strength.
Do Solar Energetic Electrons cross the Heliospheric Current Sheet? - A Statistical Study astro-ph.SR · 2026-04-21 · unverdicted · none · ref 222
Statistical analysis shows solar energetic electrons rarely cross the heliospheric current sheet unless the source or spacecraft is close to it.