Manual for KP-F145WCL

Manual for KP-F145WCL

Brand: HITACHI

Category: Digital Camera

Document Type: Manual

Language: EN

Available Languages: EN , ES

Uploaded: Nov. 21, 2025, 6:02 p.m.

Manual Publish Date: 2011-04-25

Warranty Information

Refer to the "Declaration of Conformity" for compliance with directives, not for specific warranty periods.

Overview

The KP-F145WCL is a CameraLink output type black and white camera utilizing a 2/3-inch progressive scan CCD image sensor with square pixels. It provides high-quality images at 30 frames per second with non-interlaced output, suitable for image processing.

Features

  • High resolution with a 2/3-inch 1,450,000 pixels CCD.
  • Small and lightweight (44(W) x 44(H) x 41(D) mm / approx. 110g) due to the SDR connector.
  • Automatic power supply change via CameraLink (PoCL) or DCIN/SYNC connector.

System Example

The KP-F145WCL connects to a frame grabber board using a CameraLink cable. Power can be supplied via the CameraLink cable or a DC adapter.

Section Names and Functions

Key sections include Camera/Tripod adaptor mounting screw holes, Lens mount (C mount), CameraLink connectors for video output and control, and DC IN/SYNC connector for power and external trigger/VD signal input.

Camera Mounting

Mount the camera using the optional tripod adaptor "TA-F500" to a tripod or mounting bracket. Ensure screws are of appropriate length (4 to 5.5mm) to avoid damage.

Lens

Observe the lens mounting dimensions to prevent camera and lens damage.

Troubleshooting and error codes

Phenomena Description
Smear and blooming Vertical bands visible when strong light enters the scene. Adjust camera aiming direction.
Fixed pattern noise High ambient temperature can cause noise throughout the scene.
Moire Interaction between patterns can produce a phantom pattern. Consider scene elements carefully.
Ghosting Strong direct or reflected light near an object can cause ghosting. Select scene layout and camera pointing direction carefully.
White spot Rarely appear on screen due to cosmic rays; more common at high sensitivity and temperature.
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