habile
发表于 2025-3-28 15:54:08
Interpreting Recent Observations of He I 10830 Ådepth, 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
发表于 2025-3-28 20:12:26
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Between
发表于 2025-3-29 02:05:05
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存在主义
发表于 2025-3-29 03:53:26
An Investigation of IR Triplet He I 10830 Å Profiles in Active Regions and the Quiet Chromosphere active-region spectra in the neighborhood of the He I 10830 Å 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
发表于 2025-3-29 07:42:50
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chassis
发表于 2025-3-29 12:44:26
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多嘴多舌
发表于 2025-3-29 18:59:15
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NICE
发表于 2025-3-29 21:47:41
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inhibit
发表于 2025-3-30 02:11:26
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MURAL
发表于 2025-3-30 04:28:12
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