Observing solar phenomenas with the large solar vacuum telescope |
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| Authors: | N M Firstova V I Polyakov |
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| Institution: | 1.Institute of Solar-Terrestrial Physics, Siberian Branch,Russian Academy of Sciences,Irkutsk,Russia |
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| Abstract: | The large solar vacuum telescope (LSVT) was designed to study solar phenomenas with high spatial and spectral resolution.
Due to the large size of the telescope, its real spatial resolution may be as high as ≈0.4 arcsec, which makes it possible
to observe fine-structure solar phenomenas like Ellerman bombs and pores. At present, the main subjects of investigation are
solar flares. The LSVT research methods—spectral, spectropolarimetric, and filter—provide valuable information on the physical
parameters in the phenomenas under study. Spectra and images of the Sun are recorded through an birefringent filter by two
CCD cameras. |
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