High resolution spectroscopy of the disk chromosphere

Details High resolution spectroscopy of the disk chromosphere High resolution spectroscopy of the disk chromosphere

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...37..309b&link_type=abstract

Solar Physics, vol. 37, Aug. 1974, p. 309-315.

Physics

20

Chromosphere, Emission Spectra, Fine Structure, K Lines, Solar Spectra, Chronophotography, Photographic Recording, Shock Heating, Solar Atmosphere, Spectral Resolution, Time Response, Wavelengths

Scientific paper

Description of the dark structures observed in the K-line wings and seeming to propagate inward into the K-line core or upward in the solar atmosphere. These so-called dark whiskers appear to be related to the bright disturbances (or bright whiskers) described by Liu (1974). It is argued that both may be related to the shocks which heat the atmosphere and the corona.

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