Titlebook: Infrared Solar Physics; Proceedings of the 1 D. M. Rabin,J. T. Jefferies,C. Lindsey Conference proceedings 1994 Springer Science+Business M

habile

Interpreting Recent Observations of He I 10830 ?depth, velocity, and continuum intensity. These and other images imply that if large-scale deficits in coronal irradiation induce weakening of the 10830 line, the ionizing radiation must be produced in close enough spatial proximity to the region of formation for 10830 to allow sharply defined spati

Ringworm

Between

存在主義

An Investigation of IR Triplet He I 10830 ? Profiles in Active Regions and the Quiet Chromosphere active-region spectra in the neighborhood of the He I 10830 ? line confirm that the the line is enhanced in sunspot umbrae. The line profiles of umbrae and faculae differ qualitatively. Flares show a decrease in the line depth in comparison to faculae, and in flare kernels the line undergoes an emi

Corporeal

chassis

多嘴多舌

NICE

inhibit

MURAL

Interferometry of Solar Flares at 3-mm Wavelengthaign of the Max’91 Program. We show evidence that millimeter emission probes the most energetic (MeV) electrons in solar flares; we also find that in the same flare there can be both impulsive nonthermal and gradual thermal millimeter emission. Millimeter emission usually occurs at the steep rise ph