A new double passband mode for a birefringent filter used for solar vector video magnetographs and video Dopplergraphs.

Details A new double passband mode for a birefringent filter used for solar vector video magnetographs and video Dopplergraphs. A new double passband mode for a birefringent filter used for solar vector video magnetographs and video Dopplergraphs.

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990acaps..10..180a&link_type=abstract

Acta Astrophys. Sin., Vol. 10, No. 2, p. 180 - 187

Statistics

Computation

3

Sun: Magnetographs

Scientific paper

After the analysis of the Ramsey double passband mode applied to the solar video magnetograph and video Dopplergraph, a new double passband mode have been suggested. The only difference between the new mode and the Ramsey mode is that the thickest element is placed in the middle of the filter so that the second thickest element is placed in the front of the filter. The computation shows that the new mode is the best one. The total S/N are 0.963, -0.8, and 0.578 for the three modes, respectively. The new mode may be valuable to a space vectormagnetograph or a new groud based system, and also can be contributed to the improvement of the systems in operation.

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