Up: Fabry-Perot filter based solar
A video magnetograph using a voltage tunable LiNbO3
Fabry-Perot etalon has been designed and constructed and is operational
at Udaipur Solar Observatory. The instrument is used in f/40 beam
of the telescope with an objective aperture of 15 cm and an imaging relay lens in telecentric mode.
The comparison of USO magnetograms with SOHO/MDI data shows the consistency
of our measurements. The preliminary data show the capability of the
instrument to take high spatial and temporal resolution observations
which can be used to undertake study of various problems related to
the magnetic field and flare productivity in active regions.
This instrument is the first such facility in the Indian
longitudes and fills an important gap for continuous coverage of observations of solar
active regions.
Acknowledgements
Our thanks are due to Prof. F. Kneer for
his valuable comments. The financial support for the present work comes
from the Department of Space (DOS), Government of India and Indo-US scientific collaboration
(NSF Grant INT - 9710279). The SOHO/MDI magnetogram used for the comparison
is kindly provided by SOI-MDI group. The high voltage switchable power
supply for KD*P modulator was designed and fabricated at the Space
Application Center (SAC), Ahmedabad, for which we acknowledge the
contribution of Dr. S.S. Rana, Mr. R.K. Arora and his group members.
Dr. D. Balasubramaniam and Dr. Vyas from SAC are acknowledged for their
help in optical coating. The mechanical components were fabricated by
Mr. B.L. Paneri of USO.
Up: Fabry-Perot filter based solar
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