Roper Photometric manual Class 101 ICL Plexpstartscript101

Models: Photometric

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PVCAM

NAME

SYNOPSIS

DESCRIPTION

RETURN VALUE SEE ALSO

NOTES

Class 101: ICL

pl_exp_start_script(101)

pl_exp_start_script – begin exposing, return immediately.

boolean

pl_exp_start_script(int16 hcam, void_ptr pixel_stream)

hcam must specify a CCD camera that has been successfully opened by PVCAM.

This function is the companion function to pl_exp_setup_script. pl_exp_setup_script must be called first to define the exposure and program this information into the camera. After that, pl_exp_start_script may be called one or more times. Each time, it will trigger the script to begin executing from the start, and then immediately return. (Since a script may have been aborted in the middle, leaving the camera in an unknown state, well written scripts will usually force the camera to a known state at the start of the script.)

Exposure progress is monitored through pl_exp_check_status. The next script can be started as soon as the readout is finished or an abort is performed (pl_exp_abort).

The user must allocate pixel_stream, an appropriately sized memory buffer for data collection. The buffer must be at least stream_size bytes large, where stream_size is the value returned from pl_exp_setup_script. In addition, this memory needs to be page locked or similarly protected on virtual memory systems. These requirements are system specific.

There is a special case for users who want to use their own frame grabber (with an appropriately equipped camera). If a null pointer is passed in for pixel_stream, pl_exp_start_script will assume that the user is routing the data to a frame grabber or other device under user control. Under those conditions, pl_exp_start_script will initiate the exposure, but will not attempt to handle incoming data.

TRUE for success, FALSE for a failure. Failure sets pl_error_code.

pl_exp_setup_script(101), pl_exp_abort(0), pl_exp_check_status(0)

This is programmed as macro call pl_exp_start_seq. This script function exists to provide a complete and coherent conceptual model for the sequence style exposure functions. From the API level, it should always appear that an exposure style is self-contained and complete, and that each exposure style is completely independent from every other exposure style. Underneath the API, though, code will be reused as needed.

Chapter 2. ICL 25

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Roper Photometric manual Class 101 ICL Plexpstartscript101, Boolean Plexpstartscriptint16 hcam, voidptr pixelstream