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Lunt B600 Calcium K Blocking Filter

SKU LSS-LS6CaKMDd
Original price CA$1,253.00 - Original price CA$1,253.00
Original price
CA$1,253.00
CA$1,253.00 - CA$1,253.00
Current price CA$1,253.00
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  • Isolates the 393.4 nm Calcium-K (Ca-K) emission line
  • 6mm internal blocking filter aperture
  • Narrow <2.4 Angstrom bandpass for high-contrast views
  • Available in 2-inch diagonal or straight-through housings
  • Optimized primarily for solar imaging
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  • Description
  • FAQ
  • Specifications
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  • Warranty
  • Lunt B600 Calcium K Blocking Filter

    The Lunt B600 Calcium K Blocking Filter is an imaging module designed to isolate the 393.4 nm emission line with a 6mm internal blocking filter. With a narrow <2.4 Angstrom bandpass, this 2-inch module reveals the intricate, high-contrast details of the Sun's lower chromosphere—a layer of solar activity just below what is visible in Hydrogen-alpha.

    The 393.4 nm Calcium-K Line: A Deeper Look at Solar Activity

    This filter targets the Calcium-K (Ca-K) line at 393.4 nm, an emission from ionized calcium at the edge of the visible spectrum. This reveals a cooler, lower layer of the chromosphere than H-alpha, showing areas of super-granulation cells that are brightest in regions of intense magnetic fields. By studying the sun in both Ca-K and H-alpha, you gain crucial insights into the structure, strength, and depth of active regions and sunspots.

    A <2.4 Angstrom Bandpass Optimized for Cameras

    With a bandpass of less than 2.4 Angstroms, the Lunt B600 delivers the high contrast needed to resolve fine chromospheric details. Because the 393.4 nm wavelength sits in the deep violet/UV part of the spectrum, it can be difficult for the human eye to perceive fully, as the cornea naturally yellows with age. For this reason, the Ca-K line is best studied with monochrome cameras, which are highly sensitive at this wavelength and can capture stunningly detailed images of the solar surface.

    2-inch Diagonal or Straight-Through Housings for Refractors

    The Lunt B600 Ca-K module is designed for versatility and can be integrated with most standard nighttime refractors or Lunt's Modular Telescopes. It is available in two 2-inch housings to suit your imaging train: a 2-inch star diagonal for a comfortable equipment angle, or a 2-inch straight-through tube for direct optical paths. Both versions include a T2 thread for secure camera attachment, with the straight-through model also offering a standard 2-inch eyepiece/accessory holder.

  • Why is the Lunt B600 Ca-K filter primarily for imaging?

    The filter isolates light at 393.4 nm, which is a deep violet color at the edge of the human visible spectrum. Many people, especially as they get older, have difficulty perceiving contrast at this wavelength due to natural yellowing of the eye's cornea. Cameras, particularly monochrome CMOS/CCD sensors, are very sensitive to this wavelength and can record far more detail than is typically visible by eye.

    What will I see with the Lunt B600 Ca-K filter that I can't see in H-alpha?

    The Lunt B600 Ca-K filter shows a different, slightly lower and cooler layer of the Sun's chromosphere. Key features visible in Ca-K include:

    • Supergranulation: A network of large-scale convection cells across the solar surface.
    • Plage: Bright regions around sunspots that indicate high magnetic activity, which appear with higher contrast in Ca-K.
    • Sunspot Structure: Details in the magnetic regions preceding and surrounding sunspots.

    Can I use the Lunt B600 Ca-K module with my existing non-Lunt refractor?

    Yes, the Lunt B600 Ca-K module is designed to work with most standard nighttime refractors. You simply insert the 2-inch blocking filter diagonal or straight-through tube into your focuser. No other filters are required on the front of the telescope.

    How would the Lunt B600 Ca-K filter reveal details in a complex sunspot group like AR3664?

    For a large active region like AR3664, the Lunt B600 Ca-K filter would excel at highlighting the bright, magnetically active plage surrounding the dark sunspot umbrae. It would clearly define the boundaries of the magnetic activity and show the underlying supergranulation network, providing a more complete picture of the region's structure than a white-light or H-alpha view alone.

    What is the difference between the diagonal and straight-through versions of the Lunt B600 Ca-K filter?

    Both versions contain the same 6mm Ca-K blocking filter. The choice depends on your setup preference:

    • The 2" Star Diagonal version provides a 90-degree angle, which can be more convenient for positioning equipment and avoiding clearance issues on some mounts.
    • The 2" Straight-Through version keeps your camera and accessories directly in the optical path, which some imagers prefer for simplicity. It also includes both T2 threads and a 2" eyepiece holder.

    I have an 80mm f/7 refractor; which camera type works best with the Lunt B600 Ca-K filter?

    For an 80mm refractor, a monochrome CMOS planetary camera with small pixels (around 2.9 to 3.75 microns) would be an excellent match for the Lunt B600 Ca-K filter. The monochrome sensor provides the necessary sensitivity at the 393.4 nm wavelength, and the small pixels will provide high-resolution sampling of the solar details delivered by your telescope.

  • Wavelength 393.4 nm (Calcium-K)
    Bandpass <2.4 Angstroms
    Blocking Filter Aperture 6mm
    Housing Format 2-inch
    Available Housings 2" Star Diagonal or 2" Straight-Through Tube
    Connections T2 and/or 2" depending on housing choice
    GTIN LS6CaKMD
    MPN LS12CaKMD
    • Lunt B600 Calcium K Blocking Filter Module (in selected housing)

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  • Lunt Solar Systems 5-Year Warranty