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The spectra of near-vertical structures on the solar disk (1972)

White, O. R.

Springer

Solar physics 27 (1972), S. 27-33

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ISSN: 1573-093X

Source: Springer Online Journal Archives 1860-2000

Topics: Physics

Notes: Abstract Bright emission arches in the spectra of Hα and the Ca II (H and K lines) are identified as the spectroscopic picture of the chromospheric network as it appears near the solar limb. Analysis of the geometrical properties of these spectroscopic arches indicates that the average network is a diverging sheet with a divergence angle of ∼ 50°. This sheet extends to 2600 km and 2000 km as an opaque emission feature in Hα and the Ca II (H and K) lines, respectively.

Type of Medium: Electronic Resource

URL: http://dx.doi.org/10.1007/BF00151766

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