CIRCUIT ANALYSIS EXAMPLES
1 GHz Feedback Amplifier
As before, when you choose "
(1) Sceptre" from the
Main
Menu. either by pressing "
1" or by using
the "
F1" function key, you'll enter the
Sceptre
Module. The screen display will look as follows:
Sceptre
Module
Filename
[<Enter>=Quit] ? _
For our second example, we'll analyze a
single-stage
feedback amplifier. This particular circuit was selected because it has
been analyzed by other software, and the results are given in the
literature for you to look at: See Pgs. 218-222 of Reference 4. Another
reason for selecting this circuit is because it will
give you valuable
experience on
how to
parallel connect two different two-port
networks.
We'll show you how to use the
TWO code to represent
a two-port device, the
SRL element, and the other
three
output formats:
S2,
IR, and
OR.
In response to the filename question
above, type in
"
AMPS1" and then press
<Enter>.
The circuit diagram for this amplifier is shown
below,
followed by the .CKT file listing.
CAP
|
AA
|
PA
|
3
|
|
|
|
|
IND
|
BB
|
SE
|
10
|
|
|
|
|
SRL
|
CC
|
SE
|
208
|
28
|
|
|
|
TWO
|
DD
|
S1
|
50
|
|
|
|
|
PAR
|
CC
|
DD
|
|
|
|
|
|
RES
|
DD
|
PA
|
300
|
|
|
|
|
CAP
|
EE
|
PA
|
3
|
|
|
|
|
IND
|
FF
|
SE
|
10
|
|
|
|
|
CAX
|
AA
|
FF
|
|
|
|
|
|
PRI
|
AA
|
S1
|
50
|
|
|
|
|
END
|
|
|
|
|
|
|
|
10
|
100
|
250
|
500
|
750
|
1000
|
1250
|
1500
|
.95
|
-2
|
7.35
|
174.6
|
.003
|
84.3
|
1.01
|
-1
|
.92
|
-11
|
7.15
|
168.0
|
.007
|
79.0
|
.99
|
-4
|
.87
|
-28
|
6.83
|
154.5
|
.015
|
69.2
|
.96
|
-10
|
.78
|
-54
|
6.28
|
135.0
|
.026
|
54.0
|
.90
|
-18
|
.69
|
-78
|
5.67
|
123.0
|
.033
|
41.4
|
.84
|
-26
|
.63
|
-09
|
5.04
|
113.0
|
.037
|
33.0
|
.79
|
-30
|
.60
|
-114
|
4.42
|
99.9
|
.038
|
29.3
|
.77
|
-33
|
.60
|
-127
|
3.88
|
87.0
|
.039
|
28.0
|
.76
|
-35
|
Carefully study the .CKT file listing shown
above. In the
fifth line above, the
SRL
and
TWO are parallel connected using the
PAR
CC DD command. See
Appendix
B if this is not clear. Also, note that, after using the
PAR
CC DD command, that
DD is
again
made available for use in the next line down Now, the first
eight
lines describe the circuit from left to right. All these two-port
networks are then
cascaded in line 9 using the
CAX
AA FF command.
Having created a
new two-port,
AA,
which represents the
entire amplifier circuit, we
now "finish up" the file. As when we created the
FILTER
file, we must specify the
output format, issue an
END
command, specify the
analysis frequencies, and,
since this is an
active circuit,
and not
passive one, as
FILTER
was, we must enter scattering parameter data for the
TWO,
the active two-port device.
The
convention within
Sceptre,
in what has become
standard format for s-data, thru
out the industry, is shown below:
S11M,S11A,S21M,S21A,S12M,S12A,S22M,S22A
The scattering parameters
S11,
S21,
S12, and
S22 are entered, in
that
order, and in Mag/Ang form, where "
M" is magnitude,
as "
A" is angle.
If you had
two (or more) active devices, you would
enter the s-data as follows:
TWO #1 S-Data at frequency F1
TWO #2 S-Data at frequency F1
TWO #1 S-Data at frequency F2
TWO #2 S-Data at frequency F2
etc.
After entering the filename as "
AMPS1," (several
lines up),
Sceptre then asks:
Analysis or Tweak
(A/T) [<Enter>=Quit] ? _
In
response, type "
A," press the
<Enter> key, and then choose
not
to print by pressing
<Enter> once
again.
Note: At this point, you'll be asked "
Print Logfile (Y/N) [<Enter>=No] ? _" Please press
<Enter>.
If you choose the option to 'Print Logfile,' the data will be directed
to 'Logfile.txt' within the \mwdata2 sub-directory,
and to the screen. Right-click on
'Logfile.txt' to print it, and then DELETE the file; it will re-create
when next needed.
Please please
<Enter> to choose "
N" in response to the above question.
A brief
Analysis in progress
message will flash on-screen, followed by data output to the screen.
Your screen display should look
similar to the
following:
Sceptre Circuit Analysis on 07-18-2006 at
16:23:32
Filename: AMPS1
Freq
|
S11 Mag/Ang
|
S21 Mag/Ang
|
S12 Mag/Ang
|
S22 Mag/Ang
|
S21(dB)
K B1
|
|
|
|
|
|
|
10
|
0.075/
16.8
|
2.684/ 175.4
|
0.184/
-0.2
|
0.043/ 138.2
|
8.57
1.25 0.76
|
100
|
0.077/
10.9
|
2.665/ 163.0
|
0.182/ -15.5
|
0.080/ 103.2
|
8.52
1.26 0.77
|
250
|
0.095/
5.2
|
2.711/ 140.1
|
0.178/ -41.0
|
0.145/
78.4
|
8.66
1.23 0.77
|
500
|
0.218/
-6.0
|
2.954/ 100.4
|
0.168/ -83.7
|
0.191/
63.3
|
9.41
1.14 0.80
|
750
|
0.436/
-34.0
|
3.200/
58.7
|
0.146/-130.5
|
0.230/
83.4
|
10.10
1.11 0.86
|
1000
|
0.628/
-71.0
|
3.260/
11.7
|
0.119/-178.1
|
0.366/
83.4
|
10.26
1.10 0.88
|
1250
|
0.489/-108.6
|
3.528/
-51.7
|
0.104/ 125.0
|
0.364/
94.0
|
10.95
1.08 0.95
|
1500
|
0.632/
-66.6
|
1.999/-144.1
|
0.047/
42.3
|
0.872/
89.4
|
6.02
1.12 0.27
|
Task Completed
Follow the on-screen instruction to "
Press any Key"
to return to the opening prompt. It would be a good idea for you to
now
run AMPS2, it
adds
stability circles to the display, and is the
second
of four different
Sceptre output formats.
The only difference between the
AMPS1 and the
AMP2
.CKT files,
both of which are in the \mwdata2\
sub-directory, is line 10. In
AMPS1, you see
PRI
AA S1 50, while in
AMPS2 its been changed
to
PRI AA S2 50.
If you
do choose to run
AMPS2,
here is what will happen: The amplifier circuit will
first
be analyzed as it was above, and data output to the screen,
again
as above,
then, at the bottom of the
screen, you'll see "
Press any Key." This is a
pause,
because the 25-line DOS window is
full, and without
it, you would not see the first
half of the output data. When you do "
Press any Key,"
stability circle data will be output to the screen.
There are two
other output data formats: they are
IR
and
OR. The two amplifier data files in the
\mwdata2 sub-directory containing them are named,
respectively,
AMPIR and
AMPOR.
Let's
try the
IR print option
to see what the output format
looks like, O.K.?
First, return to the opening prompt, where you'll be asked:
Sceptre
Module
Filename
[<Enter>=Quit] ? _
Enter the filename as "
AMPIR"
and then press
<Enter>. Choose the
analysis
option, and choose
not to print, or create a Logfile.
Here is what the
IR output format looks like:
Sceptre
Circuit Analysis on 07-18-2006 at 16:40:10
Filename: AMPIR
Input Reflection Coefficient and VSWR in a 50 ohm system
Freq
|
Rho Mag/Ang
|
VSWR
|
R.L. (dB)
|
Z(R+jX) ohm
|
|
|
|
|
|
10
|
0.075/
16.8
|
1.163
|
-22.443
|
57.730+j 2.530
|
100
|
0.077/
10.9
|
1.166
|
-22.318
|
58.105+j 1.691
|
250
|
0.095/
5.2
|
1.211
|
-20.408
|
60.489+j 1.061
|
500
|
0.218/
-6.0
|
1.559
|
-13.217
|
77.631-j 3.728
|
750
|
0.436/ -34.0
|
2.546
|
-7.210
|
86.728-j52.177
|
1000
|
0.628/ -71.0
|
4.378
|
-4.040
|
30.740-j60.286
|
1250
|
0.489/-108.6
|
2.914
|
-6.215
|
24.542-j29.902
|
1500
|
0.632/ -66.6
|
4.436
|
-3.984
|
33.472-j64.664
|
Create SmithMatch .IMP
File (Y/N) [<Enter>=No] ? _
Task Completed
CAUTION: Do not
answer "Y" to the "Create SmithMatch .IMP
File" question above if you do not
have our SmithMatch software installed. If you do,
you will generate an error
message.
If you were to run "
AMPOR,"
you would see what the output impedance and VSWR look like.
Please answer "
No" to the "
Create
SmithMatch .IMP File" question above and return to the
opening prompt. From there, you can press
<Enter>
and exit
Sceptre,
or,
you can go on to the
next example.
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