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Player One Apollo-M MINI IMX429 Mono Solar Camera

UGC POA-Apollo-M-MINI
Prix d'origine CA$558.00 - Prix d'origine CA$558.00
Prix d'origine
CA$558.00
CA$558.00 - CA$558.00
Prix actuel CA$558.00
Égalisation de prix!
  • 2.8 Megapixel SONY IMX429 monochrome sensor
  • 4.5μm pixels for high-resolution solar and lunar imaging
  • Global shutter eliminates motion artifacts from atmospheric turbulence
  • Up to 84 FPS at full 1944×1472 resolution
  • Passive Cooling System designed for daytime thermal stability
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  • Description
  • FAQ
  • Specifications
  • In the Box
  • Downloads
  • Warranty
  • Player One Apollo-M MINI IMX429 Mono Solar Camera

    The Player One Apollo-M MINI camera centers its design on the Sony IMX429 monochrome sensor, delivering a 1944×1472 resolution across its 2.8 million 4.5μm pixels. A global shutter captures the entire frame instantly at up to 84 FPS, while the sensor's high sensitivity is defined by a ≈79% peak QE and a low read noise of 1.45e. This combination of speed and low-noise architecture, supported by a 25k e full well depth, makes the Apollo-M MINI a dedicated tool for high-resolution solar imaging.

    IMX429 Global Shutter: Capturing the Sun at 4.5μm Resolution

    The critical feature for any solar camera is its shutter, and the Apollo-M MINI's global shutter exposes every one of its 2.8 million pixels simultaneously. This completely eliminates the wobbly, distorted artifacts that rolling shutters produce when imaging through atmospheric turbulence, ensuring solar granulation and spicule details are captured without distortion. The 4.5μm pixel size provides a fine image scale, allowing you to resolve intricate details on the solar disk with shorter focal length telescopes.

    84 FPS Data Transfer: Stable High-Speed Capture with DDR3 Cache

    At its full 1944×1472 resolution, the Apollo-M MINI streams data over its USB 3.0 port at 84 frames per second. To ensure this high-speed data stream is stable and free of dropped frames, Player One includes a DDR3 cache. This buffer secures data transmission, reduces read noise, and ensures consistent performance even when connected to a less powerful computer or a USB 2.0 port.

    Low-Noise Signal: 1.45e Read Noise and 79% QE with HCG Mode

    Capturing the subtle contrast of solar features requires a clean signal. The Apollo-M MINI achieves a low read noise of just 1.45e by using an automatic High Conversion Gain (HCG) mode. This system engages at higher gain settings to suppress noise without sacrificing the camera's dynamic range. Combined with a peak Quantum Efficiency of ≈79% and a 25k e full well capacity, the camera effectively captures the faint structures within prominences and the bright, detailed photosphere in the same session.

    Passive Cooling System: Thermal Control for Daytime Solar Imaging

    Imaging during the day introduces significant thermal challenges that can increase sensor noise. The Apollo-M MINI incorporates a Passive Cooling System (PCS) that conducts heat away from the IMX429 sensor to the camera's exterior. For even more demanding conditions, an optional Active Cooling System (ACS) is available. The sensor is protected by a D32*2MM window with a multi-layer anti-reflection coating to maximize light transmission and protect against dust.

    Apollo-M MINI vs. Apollo-M (IMX174): A Pixel-Scale Advantage

    The Apollo-M MINI (IMX429) is often compared to its sibling, the Apollo-M (IMX174). The choice between them depends entirely on your telescope and imaging goals.

    • Player One Apollo-M (IMX174): With its larger 1/1.2" sensor and 5.86µm pixels, the Apollo-M offers a wider field of view and is well-suited for full-disk solar imaging with shorter focal length instruments.
    • Player One Apollo-M MINI (IMX429): The MINI's smaller 4.5μm pixels give it a distinct advantage in resolution. On the same telescope, the MINI will deliver a more detailed, higher-magnification image, making it the superior choice for focusing on active regions, sunspots, and fine filamentary detail.
  • Why is a global shutter critical for the Apollo-M MINI in solar imaging?

    A global shutter exposes the entire 1944×1472 sensor at once, freezing moments of steady seeing. This prevents the "jello" effect or distortion seen with rolling shutters, which read the sensor line by line. For the Sun, where atmospheric turbulence is constant, a global shutter is essential for sharp, artifact-free images of granulation and filaments.

    What is the benefit of the Apollo-M MINI's 4.5μm pixels?

    The relatively small 4.5μm pixels provide high sampling resolution. This means that for a given telescope, the Apollo-M MINI will produce a more magnified image and capture finer details compared to a camera with larger pixels. It's ideal for resolving small sunspots, spicules, and intricate prominence structures without needing an aggressive Barlow lens.

    Do I need special filters to use the Apollo-M MINI for solar photography?

    Yes, absolutely. You must use a certified solar filter, such as a white-light filter (like Baader film) over the front of your telescope or a Herschel wedge for refractors. For H-alpha imaging, it must be used with a dedicated solar telescope or H-alpha filter system. Pointing the camera at the Sun without proper energy rejection will permanently destroy the sensor and can cause severe eye injury.

    How does the Apollo-M MINI perform for imaging solar prominences with a Lunt H-alpha telescope?

    The Apollo-M MINI is an excellent match for a Lunt H-alpha telescope. Its high sensitivity (≈79% QE) and low read noise (1.45e) are ideal for capturing the faint, detailed structures in solar prominences. The global shutter and high frame rate allow you to "freeze" moments of good seeing for the sharpest possible results.

    Can I use the Apollo-M MINI to image the International Space Station (ISS) transiting the sun with an 80mm f/6 refractor?

    Yes, the Apollo-M MINI is perfect for this task. The global shutter is critical for capturing a sharp, undistorted image of the fast-moving ISS. The high frame rate (up to 238 FPS at 640x480) gives you more chances to capture the perfect moment of transit against the solar disk. Remember to use a certified white-light solar filter on your refractor.

    What is the HCG mode on the Apollo-M MINI camera?

    The HCG (High Conversion Gain) mode is a feature of the sensor that automatically activates at higher gain settings. It significantly reduces read noise while preserving the full dynamic range of the sensor. This allows you to increase the camera's sensitivity for fainter targets, like solar prominences, without introducing excessive noise into the image.

  • Sensor SONY IMX429 2/3" CMOS (mono)
    Max Resolution 1944×1472
    Total Pixels 2.8 Mega Pixels
    Pixel Size 4.5μm
    Sensor Diagonal 11mm
    Image Size 8.75mm × 6.6mm
    Frame Rate (Full Res) 84 FPS (12bit)
    Shutter Type Global shutter
    Exposure Range 32μs - 2000s
    Readout Noise 5.6e - 1.45e
    QE Peak ≈79%
    Full Well Capacity 25k e
    ADC 12 bit
    Data Port USB 3.0 / USB 2.0
    Adapter 1.25″ / M42x0.75
    Back Focal Length 12.5mm
    Protective Window D32*2MM AR Plus Multi-Layer Coating
    Diameter 66mm
    Weight 160g
    Resolution & FPS (USB 3.0) 1944×1472 @ 68FPS (RAW16)
    1920×1080 @ 111FPS (RAW8) / 94FPS (RAW16)
    1280×720 @ 163FPS (RAW8/RAW16)
    800×600 @ 194FPS (RAW8/RAW16)
    640×480 @ 238FPS (RAW8/RAW16)
    Purchase Option Camera only, or Camera + ACS
  • Player One 2-Year Warranty