Sonnenbeobachtung
Solar observation is a very interesting area of Astronomy. There is something new to see here practically every day. Our home star is constantly changing! Regardless of in white light or in the narrow-band hydrogen or calcium band, observations of the processes on the sun are very impressive!
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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
This pre-filter is used for heat reduction for H-alpha observation with H-alpha filters in the tube and in prominence attachments.
This pre-filter is used for heat reduction for H-alpha observation with H-alpha filters in the tube and in prominence attachments.
This pre-filter is used for heat reduction for H-alpha observation with H-alpha filters in the tube and in prominence attachments.
This pre-filter is used for heat reduction for H-alpha observation with H-alpha filters in the tube and in prominence attachments.
This pre-filter is used for heat reduction for H-alpha observation with H-alpha filters in the tube and in prominence attachments.
This pre-filter is used for heat reduction for H-alpha observation with H-alpha filters in the tube and in prominence attachments.
Die SB2 Blende wird mit Klettband amTeleskop befestigt; sie schattet das Okular großflächig ab und verhindert störenden Lichteinfall in das Okular.
For observing Solar Eclipses, Sun Spots, Planet Transits, crossing aircrafts and satellites.