Daystar Quantum Calcium II H-Line Solar Filter - 5Å PE Grade
- Targets the Calcium II H-Line Emission
- Optimized for Visual and Imaging Use
- Reveals Lower Chromospheric Detail
- Produces a High-Contrast Violet Image
- Professional (PE) Grade Optical System
Measure how tall a prominence stands and how long a filament runs on your own solar images.
Open Solar RulerThe Daystar Quantum Calcium II H-Line Solar Filter is engineered for observers who want to visually experience the sun's lower chromosphere. By specifically targeting the Calcium H-line, this filter produces a higher contrast and more easily visible violet image than traditional K-line filters, making it a superior choice for direct observation and advanced imaging.
While most academic solar research has focused on the Calcium K-line, that wavelength (393.3nm) sits below the approximately 400nm end of the visual spectrum and is difficult for the human eye to perceive. Daystar's H-Line filter targets a different emission line of Calcium that is significantly closer to the visible spectrum, resulting in a bright, high-contrast violet view that is far easier to focus and observe directly through the eyepiece.
This filter opens a window into the dynamic lower layers of the solar atmosphere, revealing details invisible in white light or Hydrogen-alpha. You can observe the bright, complex magnetic regions known as plage that surround sunspot groups, track the boundaries of supergranulation cells across the solar disk, and witness the energetic brightening that precedes a solar flare.
The choice between a Calcium H-line and K-line filter comes down to your primary application: research or visual astronomy.
The Daystar Quantum Calcium II H-Line filter reveals features in the sun's lower chromosphere. You will be able to see bright plage (active regions around sunspots), the network pattern of supergranulation cells, and pre-flare brightening in magnetically complex areas.
You should choose the H-Line filter if you have any interest in visual observation. The K-line wavelength sits below the approximately 400nm end of the visual spectrum, so it is harder for the human eye to see. The H-line is much closer to the visible spectrum, producing a distinct violet image that is significantly easier to see and focus through an eyepiece.
It is designed to excel at both. However, its primary advantage over traditional K-line filters is its superior performance for visual observation. For imagers, the more visible wavelength can also make achieving sharp focus easier before starting a capture sequence.
While the sunspots themselves will appear as dark umbra (similar to white light), the Daystar Quantum Calcium II H-Line filter will reveal the extensive, bright, and detailed plage surrounding the spot group. This highlights the intense magnetic activity below the surface, which is completely invisible without a specialized filter like this one.
It can be, set up to Daystar's requirements. Calcium H and K filters do not require F/30 but are used at F/15, F/20 or greater, so an SCT must be configured to deliver at least F/15. Instead of a red or yellow glass energy rejection filter, use a dielectric "hot mirror" UV/IR cut filter ahead of focus, plus an additional neutral density solar film on apertures above 150mm or for long-term dedicated use. The brighter, more visible image produced by the H-line can be an advantage on long focal-ratio instruments like SCTs, potentially allowing for shorter exposure times during imaging compared to K-line systems.
The sun will appear as a high-contrast, deep violet image. This color is the natural result of isolating the specific Calcium H-line emission. While deep, this particular shade of violet is much easier for the human eye to perceive than the light from a K-line filter.
| Wavelength | 396.9 nm (3969 Å) |
| Bandpass | 5 Å |
| Tuning | Red/blue wing shift buttons with LCD wavelength readout (0.1 Å) |
Quantum filter
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100-240V power supply with US, European, UK and Australian wall plates
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