H-alpha Solar Filters
The central part of the H-alpha filtering is the Fabry-Pérot interferometer. Unlike the Etalon, this filter is adjustable and can be variably set to a ZWL. This gives more flexibility for different object and detail observations.
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Filters with 0.3Å ångström bandwidths will reveal superior surface contrast above any other filter.
Filters with 0.4 ångström bandwidths will reveal excellent surface contrast as well as fine chromosphere detail.
Filters with 0.5 ångström bandwidths will reveal better surface contrast as well as great prominences.
Filters with 0.6 ångström bandwidths will reveal some surface contrast as well as prominences.
Filters with 0.7 ångström bandwidths will reveal prominences in high contrast and occasionally, surface texture.
PE Filters with 0.8 ångström bandwidths will reveal prominences in high contrast.
Filters with 0.7~0.9 ångström bandwidths will reveal prominences in high contrast.
Daystar Quantum SE 0.4Ä H-alpha filters show chromospheric apparitions with high contrast
Transforms a normal telescope up to 3060mm focal length into an H-alpha solar telescope showing prominences & more
50mm special filter for the observation of the sun For telescopes up to 3060mm focal length & 2" focuser Additional adapter plate required for mounting Shows protuberances & more details on the sun Bandwidth less than 0.75 Angstrom Filter system with H-Alpha Etalon & Blocking Filter For visual sun observation & photography Absolutely safe, no danger to the eyes Introducing the LS100 Hydrogen-alpha system. We are offering the 100mm aperture integrally tuned etalon for use on any customer supplied refractor.