ON Semiconductor
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KAF-8300-AXC-CD-AA
צפה בפרטים DataSheets

KAF-8300-AXC-CD-AA

Introduction

The KAF-8300-AXC-CD-AA is a high-performance imaging sensor designed for use in astronomical and scientific applications. This entry provides an overview of the product, including its category, use, characteristics, package, specifications, pin configuration, functional features, advantages and disadvantages, working principles, application field plans, and alternative models.

Basic Information Overview

  • Category: Imaging Sensor
  • Use: Astronomical and Scientific Imaging
  • Characteristics: High sensitivity, low noise, large imaging area
  • Package: Ceramic Dual In-line Package (CDIP)
  • Essence: Advanced imaging technology for precise data capture
  • Packaging/Quantity: Single unit packaging

Specifications

  • Imaging Area: 17.96mm x 13.52mm
  • Pixel Size: 5.4μm x 5.4μm
  • Resolution: 3326 x 2504 pixels
  • Quantum Efficiency: >60% at 550nm
  • Read Noise: <10 electrons RMS
  • Dark Current: <0.1 electrons/sec at -15°C

Detailed Pin Configuration

The KAF-8300-AXC-CD-AA features a 40-pin ceramic dual in-line package with a detailed pin configuration for power supply, clocking, analog output, and control signals. The pinout ensures seamless integration into imaging systems and allows for efficient signal routing.

Functional Features

  • High Sensitivity: Enables precise detection of low-light astronomical objects
  • Low Noise: Provides clear and accurate imaging with minimal interference
  • Large Imaging Area: Allows for capturing expansive celestial scenes in high detail

Advantages and Disadvantages

Advantages

  • Exceptional sensitivity for low-light imaging
  • Low noise performance for high-quality data capture
  • Large imaging area for comprehensive scene coverage

Disadvantages

  • Higher cost compared to some alternative models
  • Requires careful handling and storage due to sensitive nature

Working Principles

The KAF-8300-AXC-CD-AA utilizes advanced semiconductor technology to convert incoming photons into electrical signals. These signals are then processed to generate high-resolution digital images, making it ideal for astronomical and scientific imaging applications.

Detailed Application Field Plans

The KAF-8300-AXC-CD-AA is well-suited for various applications, including: - Astronomical research and observation - Scientific imaging and analysis - Biomedical microscopy - Industrial inspection and metrology

Detailed and Complete Alternative Models

  • KAF-3200ME-CD-AA: Offers similar sensitivity and lower cost
  • KAI-11002-ABA-JD-BC: Larger imaging area and higher resolution
  • CCD-42-11-23: Cost-effective alternative with good performance

In conclusion, the KAF-8300-AXC-CD-AA stands as a high-performance imaging sensor catering to the specific needs of astronomical and scientific imaging applications. Its advanced features, coupled with its wide range of applications, make it a valuable component in various fields of research and industry.

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רשום 10 שאלות ותשובות נפוצות הקשורות ליישום של KAF-8300-AXC-CD-AA בפתרונות טכניים

  1. What is the KAF-8300-AXC-CD-AA?

    • The KAF-8300-AXC-CD-AA is a high-performance CCD image sensor commonly used in astronomical and scientific imaging applications.

  2. What are the key features of the KAF-8300-AXC-CD-AA?

    • The KAF-8300-AXC-CD-AA features a large imaging area, high sensitivity, low noise, and excellent quantum efficiency, making it suitable for demanding imaging requirements.

  3. How is the KAF-8300-AXC-CD-AA typically used in technical solutions?

    • The KAF-8300-AXC-CD-AA is often integrated into scientific cameras, telescopes, and other imaging systems to capture high-quality images for research and analysis.

  4. What are the advantages of using the KAF-8300-AXC-CD-AA in technical solutions?

    • The sensor's high sensitivity and low noise characteristics make it ideal for capturing faint signals and producing high-quality images in challenging imaging conditions.

  5. Are there any limitations or considerations when using the KAF-8300-AXC-CD-AA?

    • Users should be aware of potential issues related to dark current, read noise, and thermal management when integrating the sensor into their technical solutions.

  6. What are some common applications of the KAF-8300-AXC-CD-AA in technical solutions?

    • The sensor is frequently used in astronomy, microscopy, fluorescence imaging, and other scientific and industrial imaging applications that require high-quality, low-noise imaging.

  7. How does the KAF-8300-AXC-CD-AA compare to other image sensors in similar applications?

    • The KAF-8300-AXC-CD-AA is known for its combination of large imaging area, high sensitivity, and low noise, making it a popular choice for many technical solutions.

  8. What are the best practices for optimizing the performance of the KAF-8300-AXC-CD-AA in technical solutions?

    • Proper calibration, cooling, and exposure control are essential for maximizing the sensor's performance and achieving the best results in technical applications.

  9. Are there any specific software or drivers required to interface with the KAF-8300-AXC-CD-AA?

    • Depending on the imaging system, users may need to utilize specific software or drivers provided by the sensor manufacturer to interface with the KAF-8300-AXC-CD-AA.

  10. Where can I find additional resources and support for integrating the KAF-8300-AXC-CD-AA into my technical solution?

    • Users can refer to the sensor's datasheet, application notes, and contact the manufacturer's technical support for guidance on integrating the KAF-8300-AXC-CD-AA into their specific technical solutions.