STRPL
, SNGAM
, SFIS
, CHISO
,
SNALF
, SNP
, SN2N
, SND
, or
SNT
. The first and second must be present (TRD
and NG
, respectively), and SFIS
must be present
(if not zero) to allow nubar to be calculated from nu*sigmaf.
The others are optional. As an example,
$ IOUT=6, NED=9, NEDS=9 ... CHISO STRPL SNGAM SFIS SN2N SNALF SNP SND SNT/ 1 CHI/ 2 TRD/ 3 NG/ 4 NFTOT/ 5 N2N/ 6 NA/ 7 NP/ 8 ND/ 9 NT/ ....The ordering of the names is not important. Note that the edit specifications for
SND
could load HEAT
or
DAME
into the corresponding position rather than the
(n,d) cross section. This kind of trick must be used with care
because some SN codes may calculate their
particle-balance-absorption edit from SNGAM
+SNALF
+SNF
+SND
+SNT
-SN2N
.
A separate vector chi is computed for each isotope with fission,
but no set chi vector or matrix is provided.
The output coding produces a total scattering matrix only. It
uses the option in which a different ``block'' is used for each
Legendre order. Subblocking is not used, so the scattering
blocks each consist of a single record containing all source and
sink groups for that order. No attempt is made to take full
advantage of JBAND
and IJJ
to remove zeroes, but
the matrices are triangularized and truncated using MAXUP
and MAXDN
for some savings in output file size.
The parameters AMASS
through KBR
in the isotope
control record are set to zero.
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