* **************************************************************************************
* Becareful power pow(x, y)

* In spectre and LTSpice, y can be a float
* In hspice (and spectre include files in spice format) - y is truncated to an integer



* **************************************************************************************
tran tran stop=GTFINAL errpreset=moderate \
  write=SEED.icc writefinal=SEED.fcc annotate=status maxiters=5 \
  noisefmax=100e6 noiseseed=1


real gregclip( real x, real a) {

  return ((1.0+a+x)/2.0 * (1.0-sqrt(1.0 - 4.0*x/((1.0+a+x)*(1.0+a+x)))));

}

gregsweep.scs:MJCK (JCK   PSS) bsource i=(10e-6 * gregclip(max(0.0, V(JCK, PSS)/0.1), 0.05))
gregsweep.scs:MSNK (IDN  PSS) bsource i=(10e-6 * gregclip(max(0.0, V(IDN, PSS)/0.1), 0.05))
gregsweep.scs:MSNC (PCC  IUP) bsource i=(10e-6 * gregclip(max(0.0, V(PCC, IUP)/0.1), 0.05))
gy_top.scs:real gregclip( real x, real a) {
gy_top.scs:MSNK (IDN  PSS) bsource i=(30e-6 * gregclip(max(0.0, V(IDN, PSS)/0.1), 0.05))
gy_top.scs:MSNC (PCC  IUP) bsource i=(30e-6 * gregclip(max(0.0, V(PCC, IUP)/0.1), 0.05))


//****************************************************************************************
//* save options
//****************************************************************************************
fileOptions options rawfmt=nutascii rawfile=SEED.nta

saveOptions options save=lvlpub nestlvl=0

// save RCK CK80 CK160 CK800 vkp vkn \
//  CKDDR D\<19\> D\<1\> D\<0\> \
//  xs.xser.bdp xs.xser.bdp.bdn \
//  LOCK QMP\<0\> \
//  xp.fsti xp.fsto xp.pccv

save vkp vkn TXP TXN \
  xp.fsti xp.fsto xp.pccv \
  VVDPLLA:p VVDPLLD:p VVDSERA:p VVDSERD:p VVDSERT:p \
  xs.Xxser\/s19p   xs.Xxser\/s19n \
  xs.Xxser\/s15p   xs.Xxser\/s15n \
  xs.Xxser\/s11p   xs.Xxser\/s11n \
  xs.Xxser\/s7p    xs.Xxser\/s7n \
  xs.Xxser\/s3p    xs.Xxser\/s3n


//****************************************************************************************

//****************************************************************************************
//* analysis
//****************************************************************************************
simuOptions options reltol=1e-3 vabstol=1e-6 iabstol=1e-12 \
  temp=27 tnom=27 gmin=1e-12 rforce=1 \
  maxnotes=5 maxwarns=5 digits=10 cols=80 pivrel=1e-3 \
  sensfile=SEED.sns checklimitdest=file checklimitfile=SEED.chk \
  dochecklimit=no checklimitdetails=no \
  vabsshort=-1 rabsshort=-1 redefinedparams=error

dcOp dc write=SEED.dcc maxiters=150 maxsteps=10000 annotate=status

dcOpInfo info what=oppoint where=file file=SEED.opp nestlvl=2

tran tran stop=GTFINAL errpreset=moderate \
  write=SEED.icc writefinal=SEED.fcc annotate=status maxiters=5 \
  noisefmax=100e6 noiseseed=1


//****************************************************************************************





Saving Data

Documentation

  spectreref-->Other_Simulation_Topics-->Output_Selections_(save)  [p. 450]


    save X[:param] ... [depth=num] [sigtype=node|dev|subckt|all] 
      [devtype=component_type] [subckt=subckt_master] 
      [exclude=[wildcard_patterns_list]] [compression=no|yes] [ports=yes|no] 
      [filter=none|rc] [probelvl=num]

    save 7 out OpAmp1.comp M1:currents D3:oppoint L1:1 R4:pwr

    save x*.*1 depth=3

    save x*.*1 sigtype=subckt

    save *:c devtype=bjt

    save * subckt=inv

    save * exclude=[X1* X2*]

    save X1:A probelvl=3

    save nA:currents probelvl=2



  spectreuser-->Specifying_Output_for_Viewing-->Preparing_Out_for_Viewing

    how to set output format for nutascii ...
    how to set which file name









Hello Dave,

What kind of Nutmeg format do you mean? Ngspice uses SPICE3f5-raw output 
dataset format. XYCE simulator by Sandia also this format. It's 
described it XYCE reference manual in the Section 8 You can download 
this manual here: 
https://xyce.sandia.gov/downloads/_assets/documents/Reference_Guide.pdf

I have also started development of command-line utility and Octave 
package that will allow to read SPICE-3f5 raw-ASCII and raw-Binary 
datasets. My tools are available here: https://github.com/ra3xdh/convraw 
It is based on It consists of two parts:

1. Convraw command-line utitluty. It allows to convert SPICE dataset 
into other file formats. CSV is available now. HDF5 will be added soon.
2. Spiceraw Octave package. It allows to read SPICE dataset directly 
into Octave. It will read the whole dataset into a matrix structure.

My toolkit is licensed under GPL. All is written in C++. It allows to 
increase performance on running datasets reading in loops.

---
Regards,
Vadim Kuznetsov