Pl_exp_start_script(101) – Roper Photometric User Manual
Page 31

Chapter 2. ICL
25
PVCAM
Class 101: ICL
pl_exp_start_script(101)
NAME
pl_exp_start_script
– begin exposing, return immediately.
SYNOPSIS
boolean
pl_exp_start_script(int16 hcam, void_ptr pixel_stream)
DESCRIPTION
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.
RETURN VALUE
TRUE for success, FALSE for a failure. Failure sets pl_error_code.
SEE ALSO
pl_exp_setup_script(101), pl_exp_abort(0),
pl_exp_check_status(0)
NOTES
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.