Technical Service Document 61 - 11/97
STARLITE 55 SOFTWARE UPGRADE VERSION ST31197
Starlite 55 Colorhead is supplied on a 32-Pin EPROM
chip. This version adds the following features to those
of the previous versions.
Improved Filtration-to-Density Correction:
Filtration-to-Density Correction automatically
increases or decreases the Starlite lamp power
to compensate for varying filtration. Previously,
this was left up to the operator of the Starlite.
This new version of this feature is designed
for use with BBS brand Video Analyzers and Translators.
Self Test Routine:
The Starlite can now perform most of the steps
described in the Technical Service Document
"Manual Control Test Diagnostic,"
automatically. This is useful in finding problems
with the Starlites mechanical and electronic
systems. This routine is accessed at the end
of the Starlite Diagnostics menu.
| NOTE: If you are upgrading from
an older version of Starlite Software, this version
may not function properly unless you perform a MASTER
RESET function to clear the Starlites memory.
This action may take place automatically upon installing
the new chip. A Master Reset will completely clear
all the memory items in the Starlite, including
your Master Color Balance, and any Job Memories
you may have saved. Please allow some "recovery
time" as part of installing this version of
software. |
Full Descriptions of the new Filtration to Density
Correction is described in the following pages. If you
have any questions or problems with the new software
version, please contact your local ZBE dealer or the
offices of ZBE, Inc, at the address and phone number
at bottom of page.
Filtration to Density Correction
The Starlites Filtration to Density Correction
is designed to make the colorhead automatically compensate
its amount of light output power (D) as you change
the filtration (C, M, and Y). This feature is convenient
for users who are used to working with "Visual
Density" instead of the "Neutral Density"
normally utilized by the Starlite.
Users of any analyzers or translators manufactured
by Bildsysteme Brugger & Schmerler GmbH (BBS), will
require this mode of operation for the Starlite to be
compatible with their analyzer or translator system.
Functional Description:
The Starlites Filtration to Density Correction
simply feeds a portion of each color filtration value
into the Density output. These ratios are defined by
the user, so that the Starlites light output can
be matched to the specific machine or system with which
it is being used. The ratio for each color is expressed
as a percentage (0% - 100%).
This system of correction uses the difference
between the current filtration on the keypad and the
standard filtration (set during the CALIBRATE MASTER
COLOR BALANCE) to calculate the density correction.
Thus, the Filtration to Density Correction uses two
sets of data for operation: The Standard Negative (Shirley)
Filtration as entered during the CALIBRATE MASTER COLOR
BALANCE routine, and the Filtration to Density Correction
Gains as entered in the Starlite Calibration Menu ("Edit
Filt to Dens Correction Gains") as percentage (%)
values.
An Example:
To demonstrate this system, consider an operator that
has calibrated his Starlite to make a perfect Standard
(Shirley) print at D:60, M:60, and Y:60,
to correspond with his BBS video analyzer. In addition,
he has entered his Filtration to Density Correction
Gains as C:0%, M:50%, Y:25%.
Now that the Starlite is ready for printing, the operator
analyzes a new negative, for which the BBS reads a filtration
of D:90 M:80 Y:76. When he enters this new current filtration
at the main screen of the Starlite, the Starlite computer
makes the following computations:
| |
D:
|
C:
|
M:
|
Y:
|
| Standard (Shirley)
Filtration (in CCs):
Set when the Starlite was originally calibrated
using the CALIBRATE MASTER COLOR BALANCE routine.
|
60
|
0
|
60
|
60
|
| Current Filtration:
Entered for printing the new negative.
|
90
|
0
|
80
|
76
|
| Difference from Standard
to Current Filtration:
Calculated by Starlite Filtration to Density
Correction
|
+30
|
0
|
+20
|
+16
|
| Filtration to Density Correction
Gains:
Entered in the Edit Filtration to Density Correction
Gains item in the Starlite Calibration Menu.
|
|
0%
|
50%
|
25%
|
| Calculated Correction
to Density of light output:
|
|
|
20cc x 50%=
+10cc
|
16cc x 25% =
+4cc
|
| |
|
|
|
|
Note that the Density value on the keypad will not
be changed (it will still be 90cc as entered by
the operator), but the amount of light that goes with
this value will be +14cc brighter than it would have
been without the Filtration to Density compensation.
This increase at the output of the Starlite will compensate
for the light lost through the filters, keeping the
total light energy (Visual Density) the same as it falls
onto the baseboard.
Setting it up:
In order to benefit from the new Filtration to Density
Correction, the Correction Gains must be set to the
proper percentage amounts. Since the effects of filtration
(M and Y) upon Density is different for different darkroom
setups, you must set these values yourself. Follow the
general process below as a starting point.
(f you already know what percentages of Magenta and
Yellow are part of Density, you can simply enter these
values in the Correction Gains screen of the Starlite
as described in step#11 below and in the users
manual.)
- Make a perfect Standard (Shirley) Print and calibrate
the Starlite using the CALIBRATE MASTER COLOR BALANCE
procedure as described in the Starlite manual. Use
the Standard filtration values that are used on
your analyzer. (BBS users usually use D:60 M:60
Y:60.)
- Analyze a different negative on the analyzer and
write down the filtration values. (The further the
color filtration is from the standard negative,
the better your setup will be.)
- Use the filtration values from the analyzer to
make a print with the Starlite. The resulting print
should be close in color balance, but in error in
Density.
- Be sure that you write down the Density on the
Starlite that you used to make this print.
- Change the Density at the Starlite and make more
test prints, until the print comes out correct in
density. Write down this new Density value.
- Subtract the Original analyzer Density (from Step#3)
from the Density that made the print correct (from
Step#5). Write down this Density Difference.
- Subtract the Shirley filtration value for Magenta
(Step#1) from the Analyzer Magenta value that the
analyzer gave for the new negative (Step#3). Write
down this Magenta Difference.
- Use a calculator to divide the Density Difference
by the Magenta Difference. The result will be a
number less than 1. (Example 0.42)
- Express this fractional number as a percentage
by multiplying by 100. (Example: 0.42 x 100= 42%)
- This value is your Correction Gain for Magenta.
Of this value (ex. 42), take approximately
one fifth of this number and call it he Correction
Gain for Yellow. (Example: 42 / 5 = 8. In this case,
Magenta Gain = 42% and Yellow Gain = 8%.)
- Enter these values in the Filtration to Density
Correction Gains in the Starlite Calibration Menu.
- In the Starlite Preferences Menu, find the item
titled FILTRATION TO DENSITY CORRECTION, and make
it ACTIVE. (See users manual for details.)
This procedure is designed as a starting point only.
As you analyze and make more prints from new negatives,
you will want to make fine adjustments to the Filtration
Correction gains.
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