Sceptre has
four different
output format options. They are:
S1,
S2,
IR, and
OR. You must use
one
of them in the
PRI line of every .CKT file.
For
best results, Windows Users, running
Sceptre
in a DOS window, should keep the
number of analysis
frequencies to (say) 10 maximum.
We have been
told that the following URL contains
links about console/screen capture utilities that
may
be of value to some Windows Users. We cannot
vouch
for them, as we've
not tried them. Use them at your
own risk:
http://garbo.uwasa.fi/pc/screen.html
Here is another comment we received
about the display
of large files: "In Windows XP you can set the size of the screen
buffer in the DOS Window's Properties. This lets you do exactly what
you want without having to pipe the program to the More
utility."
Ethan Winer - UseNet newsgroup: alt.msdos.programmer
S1
Output Format
The
S1 option is used in the form
PRI AA
S1 50. It tells
Sceptre to print the
s-parameters of two-port "
AA" referenced to a 50 ohm
system. Run the example file
AMPS1 to see it in
use.
If the .CKT file contains an
active
element, i.e., a "
TWO,"
Sceptre
will print the stability factor K and its related parameter, B1. If the
.CKT file is
passive, the
printing of stability information will be suppressed.
S2
Output Format
The
S2 option is used in the form
PRI AA
S2 50. It does the same thing as
S1,
except it adds the location of input and output plane stability
circles. Run the example file
AMPS2 to see how it
works.
Knowledge of stability circle location helps you to design amplifiers
for the case where K, the stability factor, is < 1.
Note: When using the
S2 option, the data output to
the screen doubles. This
may cause, depending on
the
number of analysis frequencies, screen
overflow
when running
Sceptre in a DOS window.
So, when this option is used, the program will
pause
after printing the initial circuit analysis data. When you "
Press
any Key" to continue, the remaining stability circle data
will be output to the screen.
For more information on K, B1, and stability circles, see
Appendix D, and the book by
Guillermo Gonzalez, listed as Reference 4, in
Appendix G. If you click on a
link to
visit these appendices, please
remember
to use the
BACK button on your browser to return
here.
IR
Output Format
The
IR option is used in the form
PRI AA
IR 50. It tells
Sceptre
to print the input reflection coefficient magnitude and angle, the VSWR
in a 50 ohm system, the return loss (R.L.), and the series impedance
equivalent of S11 in two-port "
AA." Run example file
AMPIR to see how it works.
If the return loss is actually a
loss,
such as you would expect in an amplifier with good VSWR, its sign will
be
negative. If, on the other
hand, the device input impedance has a negative
real
part, such as in an oscillator, its sign will be
positive.
This option will
also allow you to create a .IMP
file for use by our
SmithMatch program.
OR
Output Format
The
OR option is used in the form
PRI AA
OR 50, and is the same as
IR, except it
works with S22, the output reflection coefficient.
This option will
also
allow you to create a .IMP file for use by our
SmithMatch
program.
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