Nonthermal line broadening at solar flare footpoints is primarily field-aligned, demonstrated by systematic decrease in line widths from disk center to limb across 4,593 Hinode/EIS spectra from 407 flares.
(1949).Extrapolation, Interpolation, and Smoothing of Stationary Time Series: With Engineering Applications(The MIT Press)
2 Pith papers cite this work. Polarity classification is still indexing.
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Hinode/EIS full-disk mosaics show coronal intensity tracks solar cycle via active region coverage while velocity properties in log T~6.2 plasma remain stable across cycles 24-25.
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Nonthermal line broadening at solar flare footpoints is primarily field-aligned
Nonthermal line broadening at solar flare footpoints is primarily field-aligned, demonstrated by systematic decrease in line widths from disk center to limb across 4,593 Hinode/EIS spectra from 407 flares.
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Full-Disk Spectroscopy of the Solar Corona Across a Solar Cycle with Hinode/EIS
Hinode/EIS full-disk mosaics show coronal intensity tracks solar cycle via active region coverage while velocity properties in log T~6.2 plasma remain stable across cycles 24-25.