Hyperspectral solar observation based onthe sodium atomic filter
2016
This paper introduces the principle of hyperspectral solar imaging
observations based on atomic filters and their transmission properties.
The full disk solar images of the upper photosphere and the lower
chromosphere are obtained. Compared with the conventional interference
filters, the transmission peak of sodium atomic filters just corresponds
to the center of solar Fraunhofer D 2 line,
which is in favor of long-term and stable solar observations with
a high spectral resolution; its ultra-narrow bandwidth is more beneficial
to the detailed observation of the solar atmosphere, such as the plages
and bright network structures. The details of the observed solar structures
using our atomic filter (at 589 nm) in Wuhan are very similar to those
obtained by SDO satellite (at 160 nm), since the two wavelengths are
formed at similar heights. Our experiments demonstrate that the atomic
filters can provide an effective method for hyperspectral solar imaging
observations.
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