NJOY 99.0                                                     31 Dec 99
 -----------------------------------------------------------------------

 This is version 99.0 of the NJOY nuclear data processing system.  It
 is a cleaned up version of NJOY 97 that moves further towards using
 modern block structures instead of statement numbers for flow control
 (but some routines still use statement numbers!).  Physical constants
 have been moved into a few global common blocks and standardized to
 the current NIST CODATA values.  The bulk of the changes are in the
 ACER module, where we support several new features scheduled to 
 appear early in the year 2000 in MCNP4c, and where we provide data
 for high-energy problems, incident charged particles, and photonuclear
 reactions for MCNPX.  We also fix the NJOY Y2K problem!  Note that 
 there are two new test problems:

  Problem 13 is to demonstrate the new MCNP formats
  and ACE plotting.

  Problem 14 is to demonstrate ACE incident proton
  data and MCNPX format.

 To help the user, the following sections start with specific key
 phrases; use your editor to search for the desired topics.

   << The NJOY Nuclear Data Processing System >>
   << NJOY documentation >>
   << distribution files >>
   << installation on unix machines >>
   << installation on DOS/Windows machines using Lahey LF95 >> 
   << installation on DOS/Windows machines using Absoft f90 >>
   << revision control with upd >>
   << notes on machine dependencies >>
   << test problems >>

 This version has been tested on a Sun Ultra using f77, on an SGI
 Origin 2000 using f90, on X86 machine using Absoft f90 and Lahey LF95,
 and on a linux machine using g77 and Portland Group f77.  Caution:
 problems were seen for some systems when optimization was used.
 Supporting files for other systems have to be updated from the NJOY97
 versions by analogy with the NJOY99 versions.  Users not supported 
 by the files in this distribution are requested to send back the 
 appropriate patches for their machines for further distribution.

 -----------------------------------------------------------------------

 << The NJOY Nuclear Data Processing System >>

 The NJOY Nuclear Data Processing System is a modular computer code
 used for converting evaluated nuclear data in the ENDF format into
 libraries useful for applications calculations.  Because the 
 Evaluated Nuclear Data File (ENDF) format is used all around the
 world (e.g., ENDF/B-VI in the US, JEF-2.2 in Europe, JENDL-3.2 in
 Japan, BROND-2.2 in Russia), NJOY gives its users access to a wide 
 variety of the most up-to-date nuclear data.  NJOY provides
 comprehensive capabilities for processing evaluated data, and it
 can serve applications ranging from continuous-energy Monte Carlo
 (MCNP), through deterministic transport codes (DANT, ANISN, DORT),
 to reactor lattice codes (WIMS, EPRI).  The modular nature of NJOY
 makes it easier to add output for other kinds of application
 libraries or to add new computational features.  NJOY handles a
 wide variety of nuclear effects, including resonances, Doppler
 broadening, heating (KERMA), radiation damage, thermal scattering
 (even cold moderators), gas production, neutrons and charged
 particles, photoatomic interactions, photonuclear reactions, self 
 shielding, probability tables, photon production, and high-energy 
 interactions (to 150 MeV).  Output can include printed listings, 
 special library files for applications, and Postscript graphics 
 (plus color).

 -----------------------------------------------------------------------

 << NJOY documentation >>

 New documentation for NJOY99 is not yet available.  In the meantime,
 use the NJOY91 documentation in the report "The NJOY Nuclear Data
 Processing System, Version 91," LA-12740-M (1994).  The differences
 in user input will be found in the Userinp file that comes with the
 distribution, or in the comments in the source code.  For more 
 information on LEAPR, see "New Thermal Neutron Scattering Files for
 ENDF/B-VI Release 2," LA-12639-MS (1994).  The reports are
 available by request or in Postscript form in the Publications area
 of http://t2.lanl.gov/.  In addition, there are tutorials on the
 ENDF system and NJOY97 available in http://t2.lanl.gov/endf and
 http://t2.lanl.gov/njoy.
 
 -----------------------------------------------------------------------

 << distribution files >>
 
 The distribution files for NJOY 99 are as follows:
 
     Readme0       this information file
     Userinp       text file of NJOY input instructions
     src           upd source file (contains *deck cards)
     up0           upd directives input file for 99.0
     upsun         specialized updates for Sun workstations
     upsun8        specialized updates for Sun using -dbl option
     upcray        specialized updates for UNICOS at Los Alamos
     uprs6k        specialized updates for IBM RS/6000 machines
     updecau       specialized updates for DEC Alpha unix
     uplinux       specialized updates for linux using g77
     upabs         specialized updates for dos Absoft f90
     uplf95        specialized updates for dos Lahey LF95
     makef.sun     Sun make file for maintaining njoy
     makef.sun8    Sun make file for for -dbl option (see upsun8)
     makef.cray    UNICOS make file for maintaining njoy
     makef.rs6k    IBM RS/6000 make file for maintaining njoy
     makef.decau   DEC Alpha unix make file for f90
     makef.linux   make file for linux using the g77 compiler
     makef.abs     make file for dos Absoft f90
     install.bat   install script for Lahey LF95
     load.bat      load script for Lahey LF95
     in01          unix shell script to run test problem 1
     run01.bat     DOS batch file to run test problem 1
     in01.dat      input data for DOS run of test problem 1
     out01         test problem 1 output from Sun Ultra 60
     pend01        test problem 1 PENDF from Sun Ultra 60
     in02                        .
     run02.bat                   .
     in02.dat                    .
     out02                       .
     pend02                      .
     in03                        .
     run03.bat                   .
     in03.dat                    .
     out03                       .
     plot03.ps                   .
     in04                        .
     run04.bat                   .
     in04.dat                    .
     out04                       .
     in05                        .
     run05.bat                   .
     in05.dat                    .
     out05                       .
     plot05.ps                   .
     in06                        .
     run06.bat                   .
     in06.dat                    .
     plot06.ps                   .
     in07                        .
     run07.bat                   .
     in07.dat                    .
     out07                       .
     pend07                      .
     ace07                       .
     in08                        .
     run08.bat                   .
     in08.dat                    .
     out08                       .
     pend08                      .
     ace08                       .
     in09                        .
     run09.bat                   .
     in09.dat                    .
     out09                       .
     pend09                      .
     in10                        .
     run10.bat                   .
     in10.dat                    .
     out10                       .
     pend10                      .
     ace10                       .
     in11                        .
     run11.bat                   .
     in11.dat                    .
     out11                       .
     wims11                      .
     in12                        .
     run12.bat                   .
     in12.dat                    .
     out12                       .
     pend12                      .
     plot12.ps                   .
     in13                        .
     run13.bat                   .
     in13.dat                    .
     out13                       .
     pend13                      .
     ace13                       .
     plot13.ps                   .
     in14                        .
     run14.bat                   .
     in14.dat                    .
     out14                       .
     ace14                       .
     plot14.ps                   .
     gam23         input data for test problem
     gam27         input data for test problem
     t322          input data for test problem
     t404          input data for test problem
     t511          input data for test problem
     eni61         input data for test problem
     epn14         input data for test problem
     upd.f         version-control code for updating njoy
                     (this version writes module.f)

 -----------------------------------------------------------------------

 << installation on unix machines >>
 
 For the initial installation...
 
   Make sure the following files are in your working directory:

      makef.xxx for your system
      upd.f
      src
      up0
      upxxx for your system

   and do the following:

      cp makef.xxx Makefile
      f90 -o upd upd.f   (or cf90, f77, g77, ...)
      cat up0 upxxx > upn
      (check upn to make sure that "*set sw" is present, if needed)
      upd
      make

      xnjoy is your executable file
      module.f is a fortran compiler input file
      module.o is an object deck
 
   To make a change to NJOY 99.0 on unix ...
 
   Make sure the following files are available:

      upd (the executable version)
      upn (the expanded version)
      src
      Makefile
      module.f files
      module.o files
      previous xnjoy

   Edit upn to add the new upd "ident" and to list which
   modules need to be updated; for example,

      *cpl groupr
      *ident fixbug
      */ fix a hypothetical bug in groupr
      *d groupr.444,445
      *ident vers
      ...

   Then just do the following:

      upd
      make

   Versions of the test problem input files in unix script
   form are included in the distribution of NJOY 99.0.
   To run the test problems, move the input scripts to a
   test directory created in the directory that contains the
   xnjoy file, and then simple type

      sh in01

   and so on.  Compare the resulting files, such as out01
   and pend01, to the ones included in the distribution;
   e.g.,

      diff out01 ../out01 > difs-out1

 -----------------------------------------------------------------------

 << installation on DOS/Windows machines using Lahey LF95 >> 
 
 For the initial installation...

   Open DOS command window and change the active directory
   to the NJOY99 working directory.

   Make sure that your working directory for NJOY99 contains the
   following files:

      src
      up0
      uplf95
      upd.f
      install.bat
      load.bat

      (combine up0 and uplf95 into upn)
      copy up0+uplf95 upn

      (make sure that upn contains "*cmp all" and "*set sw")

      (compile upd)
      lf95 upd.f -out upd.exe

      (make the module.f files)
      upd

      (compile and load all the modules)
      install

   The final executable code will be njoy.exe.

 To run the test problems ...

   Create a subdirectory in your NJOY working directory called test.
   Move the in*.dat and run*.bat files into test.  Make sure the
   following data files are available in your working directory (that
   is, the directory that contains test):

      t322
      t404
      t511
      eni61
      epn14
      gam23
      gam27

   Using a DOS window, cd into test, and type "run01".  Continue
   for run02, run03, etc.  The result files, such as out01, out02,
   etc., will appear in the test directory.  Compare the result files
   in the test directory with the one from the original distribution.

 To make changes to NJOY99 in the Lahey LF95 environment ...

   Edit upn to add the new upd "ident" and to list which
   modules need to be updated; for example,

      *cpl groupr
      *ident fixbug
      */ fix a hypothetical bug in groupr
      *d groupr.444,445
      *ident vers
      ...

   Run upd from a DOS window. Run the compiler on the new deck
   or decks:

      lf95 -c deck.f 

   Run the load script to rebuild the binary njoy.exe:

      load

 -----------------------------------------------------------------------

 << installation on DOS/Windows machines using Absoft f90 >>
 
 For the initial installation...
 
   Make sure the following files are in your working directory:

      makef.abs 
      upd.f
      src
      up0
      upabs

   and do the following:

      copy makef.abs Makefile
      f90 -o upd.exe upd.f
      copy up0+upabs upn
      (check upn to make sure that the following lines are present
       at the start of the upn file: "*cpl all", "*lst all", 
       "*set sw", and "*noid")
      upd
      amake

      njoy.exe is your executable file
      module.f is a fortran compiler input file
      module.lst is a listing file
      module.obj is an object deck

   Note the Absoft f90 doesn't like to have text beyond column 72.
   Therefore, we provide the module.lst files to give an easy way to
   see the upd reference numbers for each line.  The module.f files
   do not have line identifiers.
 
   To make a change to NJOY 99.0 ...
 
   Make sure the following files are available:

      upd (the executable version)
      upn (the expanded version)
      src
      Makefile
      module.f files
      module.obj files
      previous njoy.exe

   Edit upn to add the new upd "ident" and to list which
   modules need to be updated; for example,

      *cpl groupr
      *lst groupr
      *noid
      *set sw
      *ident fixbug
      */ fix a hypothetical bug in groupr
      *d groupr.444,445
      *ident vers
      ...

   Then just do the following:

      upd
      amake

   Versions of the test problem input files in for dos are
   given in two parts, a runXX.bat file, and an inXX.dat file
   that is used by the batch file.  To run the test problems, 
   move the input scripts to a test directory created in the 
   directory that contains the njoy.exe file, and then simply
   type

      run01

   and so on.  Various output, pendf, ace, and Postscript files
   will be generated in the test directory.

 -----------------------------------------------------------------------

 << version control with upd >>
 
 Early versions of NJOY were maintained with CDC or Cray UPDATE,
 or with the UPEML update emulator from Sandia National Laboratory.
 This approach had the problems that not everybody had UPDATE and
 that UPEML wasn't exactly compatible with UPDATE for changes made
 upon earlier changes.  For these reasons, NJOY was provided with
 its own version control program called UPD.  This program performs 
 the same functions as UPDATE, but it is very simple in order to make
 it easier to transport the code to a variety of computer systems.
 UPD has evolved slightly from version to version of NJOY, and the
 version for NJOY 97 and NJOY99 works a little differently than the 
 preceding version.

 The original text of NJOY 99 is given in a file called "src",
 which contains "*deck module" cards at the start of each NJOY
 module (njoy, reconr, etc.).  No binary program library is used.
 UPD directives are given in the file "upn".  Each set of
 directives starts with the statement "*ident name" and contains
 additional statements like "*i address" or "*d address"
 followed by the text to be inserted or deleted.  The UPD
 addresses can have forms like the following:

    reconr.151
    groupr.522,533
    matxsr.111,up20.33

 The NJOY Quality Assurance program requires that idents be added
 to the upn file in strict sequence.   The first card after each
 "*ident name" card must be a comment card giving the module, date,
 and purpose for the change in the form

    */ groupr -- 30 Mar 95 -- fix problem with c.p. elastic
    */                          reported by NEA-DB

 An ident should contain changes for only one module.  Once an
 ident has been finished, dated, and released, it should never
 be changed directly.  It should only be changed by some subsequent
 ident using line numbers like "up20.33".   The conventional name
 for "official" idents are "up1", "up2", "up3", and so on.  The
 corresponding version names would be "99.1", "99.2", "99.3", and
 so on.  The last ident in upn is always "*ident vers", which
 has the following form:

    *ident vers
    */ update the version name and date
    */ to reflect the date of the latest modifications
    *d njoy.8,9
    c     *    version 99.0                                         *
    c     *    31 Dec 99                                            *
    *d njoy.279
          data vers/'99.0    '/

 This ident is changed as each ident is added to reflect the
 current version number and date.  The result of this procedure
 is that it is always possible to determine what version was
 used to run a particular problem, and knowing the version, it
 it possible to determine the exact configuration of the code
 for any run.

 Code changes for different computer systems are handled by UPD
 in two ways.  Generic changes are handled by "*if" constructs
 in the source file.  Currently, only one such option is implemented.
 Add the card "*set sw" at the start of upn for "short-word"
 machines (32-bit words). More specific system changes are included 
 in a machine ident that must be copied onto the end of the upn 
 file.  Examples are given in the distribution (see upsun, 
 upuni-la, upuni-sd, etc.).  These updates normally do things like 
 change the names of the local time and date routines and personalize 
 the NJOY "banner" for the specific laboratory.

 It is usually easy to transport UPD between different computer
 systems.  Unit 6 is intended for writing on the screen or
 an equivalent log file.  This is the default for many systems.

 UPD can put out two different kinds of files, a conventional
 compiler input file "module.f", and a special listing file
 "module.lst".  Beginning with UPD for NJOY 97, the code can 
 write out several updated modules during one pass for more 
 efficiency.  For example, "*cpl reconr,broadr" would write
 out compile files for the two modules RECONR and BROADR.  Then
 a simple "make" would recompile these two new decks and
 relink them into the NJOY executable.  Similarly, "*lst groupr"
 would make a new listing file for GROUPR.  For new installations,
 "*cpl all" and "*lst all" will make all the compile and listing
 files.  Just typing "make" will then finish the entire 
 installation.

 ----------------------------------------------------------------------

 << notes on machine dependencies >>

 We have tried to keep all routines that depend on the particular
 machine, operating system, or compiler being used in the NJOY
 module.  We have provided "upxxx" files and special "makef.xxx" files
 that will incorporate machine dependencies into NJOY for system that
 we are able to test ourselves.  Other files have sometimes been
 contributed by users with access to other systems.  If you have to
 bring the code up on a new system, these existing files may help to
 guide you.

 One of the machine dependencies that has always been around is the
 differences in time and date calls on different system.  With the
 advent of Fortran-90, this has been partly alleviated.  However, 
 Fortran-90 doesn't have an intrinsic routine to return the amount
 of system time that has been used by a job.  Some of our upxxx files
 just return a run time based on the system clock, which would not be
 accurate in a multi-processing environment.  The LANL Cray system
 provides the "second" call, which works fine.  You'll just have to
 try to provide the best option available on your own local system.
 
 Starting late in the NJOY94 series, we changed over to using the
 SLATEC libraries for fundamental math routines, because they are
 very accurate, and they can be used without restrictions.  These
 routines require some basic parameters to describe the real number
 system used by your computer.  The source code gives some options for
 mostly obsolete systems.  Most modern machines use IEEE arithmetic,
 and one of the sets of constants included in our upxxx file should
 be OK.  However, you would be well advised to check your system's
 documentation to more specific values for these parameters.  Note
 that different sets of parameters are used on 32-bit (real*8)
 systems and 64-bit systems (like the Cray).

 There are still some problems with number systems and word length
 on the machines in wide use today.  Classical 32-bit machines
 work fairly well in NJOY99 using real*8 variables.  As a rule, these
 machines and compilers do not support integer*8 variables.  This
 can create word-alignment problems, and we have tried to fix them.
 However, some cases require binary records with mixed real and
 binary elements (CCCC-type files).  In these cases, we have had to
 limit ourselves to 32-bit accuracy using real*4 and integer*4
 values.

 In some cases, the compilers have "-r8", "-i8", or "-dbl"
 options that automatically promote code written to 64-bit standards
 to run on 32-bit machines.  This seems to work OK for NJOY on
 some systems.  However, you have to be sure that the set of compiler
 options that you use promotes both reals and integers to 64-bit
 size in order to prevent word-alignment problems.  Unfortunately,
 neither linux g77 nor Sun f90 support such an autodoubling option, 
 which is one of the reasons that we provided explicit doubling in 
 NJOY99.

 The new generation of machines with 64-bit chips, such as the Sun
 Ultra, promise to eliminate this problem.  However, the current
 compilers are not always completely 64-bit capable, and their
 abilities to use mixed real*8 and integer*8 data may be limited.
 Therefore, we are currently treating them just like 32-bit systems.

 Cray machines have always used 64-bit variables for both reals and
 integers, and there are no problems with mixed data.  However, note
 that Cray arithmetic uses more bits in the exponents or real numbers
 and fewer in the fraction part.  Therefore, numbers on the Cray
 have slightly less precision than those on the IEEE-type machines.

 ----------------------------------------------------------------------

   << test problems >>

 An extensive set of test problems is provided with NJOY99, both to
 check an installation, and to provide examples of how to use NJOY.
 In order to provide continuity to earlier versions, we still use
 fairly old ENDF/B-III, -IV, and -V files for these tests.  They also
 tend to have less detail than the new ENDF/B-VI files, which make
 the test problems run faster.  Simple unix scripts or DOS batch
 files make it fairly easy to run the test problems.

 Problem 1: This one runs on carbon to check RECONR for materials
   with no resonance parameters, to do Doppler broadening to 300K,
   to calculate heating KERMA and radiation damage, and to calculate
   the thermal scattering from graphite.  The pointwise (PENDF)
   results are converted into multigroup form.  The important things
   to look at are the various counts in RECONR and the multigroup
   values from GROUPR on the file "out01".  To see even more detail, 
   check the PENDF file "pend01".

 Problem 2: This is a demonstration of preparing a library for LMFBR
   applications using methods active in the 80's.  It is still useful
   for check RECONR resonance reconstruction, Doppler broadening to
   more than one temperature, the generation of unresolved resonance
   data, and multigroup averaging with self shielding.  The CCCC
   output provides an alternative look at the cross sections and
   group-to-group matrices.  Pay attention to the output from RECONR
   to see if the same number of resonance points are produced.  Note
   the number of points at each temperature and the thermal quantities
   printed by BROADR.  The unresolved self shielding shows up in the
   UNRESR output and again in GROUPR and CCCCR.  The multigroup
   constants printed on "out02" provide plenty of opportunities to
   check your installation.  For even more detail, check the PENDF
   file on "pend02".

 Problem 3: This one demonstrates processing photoatomic data and the
   use of MATXS output files.  Newer versions of the photoatomic data
   are all on one file, rather than the two shown here.  Note that
   two materials are processed to show the limiting behaviors.  The
   multigroup constants printed by GAMINR on "out03" can be checked.
   Two different output formats are generated: the DTF format and
   the MATXS format.  The DTFR numbers are given on the listing, and
   you can check the details of the MATXS results on "matxs03".
   DTFR also generates Postscript plots of its results; you can
   view them from "plot03" using ghostview or any Postscript printer.

 Problem 4: This test problem computes cross section covariances
   using the ERRORR module for U-235 from ENDF/B-V.  The performance
   of ERRORR can be tested by looking at the values on "out04".

 Problem 5: This one demonstrates formatting covariance data using our
   "boxer" format, and it generates detailed Postscript plots (in
   color) of the variances and correlations.  Look at "plot05" with
   ghostview or a color Postscript printer.

 Problem 6: This case demonstrates and tests some of the features of
   the PLOTR and VIEWR modules.  The output file is not very interesting,
   and we don't provide it.  Look at "plot06" using ghostview or a
   Postscript printer.

 Problem 7: This example demonstrates the production of a library for
   the MCNP continuous-energy Monte Carlo code for Pu-238 from ENDF/B-IV.
   Older versions of MCNP required a set of multigroup photon production
   tables to construct the 30x20 grid of photon emission bins used in
   those days.  This problem demonstrates how that was done, but the
   method is rarely needed these days.  Still, these results provide
   another useful set of tests for your installation.  The most 
   interesting numbers are those in the ACER output on "out07".  It
   is difficult to use tools like "diff" to compare such outputs
   unless the energy grids are exactly the same.  Some of the changes
   made to NJOY99 were designed to try to achieve identical energy
   grids between different machines, and diff may work for you.  If
   not, you can still spot check the results.  We provide both the
   PENDF on "pend07" and the ACE file on "ace07" to allow for very
   detailed checks.

 Problem 8: This case was added to check the processing of a typical
   ENDF/B-VI material using Reich-Moore resonances and File 6 for
   energy-angle distributions.  Pay special attention to the
   resonance results as shown by the counts on the RECONR listing
   and the values on the PENDF and ACE files (pend08 and ace08).
   In addition, check the energy-angle distributions as printed out
   by ACER on "out08".

 Problem 9: This one demonstrates the use of LEAPR to generate a 
   scattering kernel for water.  We have used the ENDF physics model, 
   but we reduced the alpha and beta ranges to make the case run 
   faster with less output.  Note that RECONR and BROADR are run to 
   prepare a base for the thermal data at 296K.  THERMR was run with 
   its long printout option to provide plenty of numbers on "out09" 
   for comparisons.  For additional details, look at the actual 
   LEAPR output on "pend09".

 Problem 10: This sample problem demonstrates the production of 
   unresolved resonance probability tables for MCNP.  We run both 
   UNRESR and PURR using the same sigma0 grid to allow additional 
   checks of both modules and to allow for comparisons between the 
   deterministic and probabilistic approaches to computing Bondarenko 
   cross sections.  We provide the output listing on "out10", the 
   PENDF file on "pend10", and the ACE file on "ace10".  Lots of 
   results to check.

 Problem 11: This one demonstrates the production of a library for 
   the WIMS reactor lattice code using Pu-238 from ENDF/B-IV.  Check 
   both GROUPR output and WIMSR output on "out11".  The WIMS library 
   file produced is provided on "wims11".

 Problem 12:  This one shows how the new gas production capability 
   works with Ni-61 from ENDF/B-VI.  To see the detailed results for 
   gas production, look for MT=203 and 207 in File 3 of the PENDF 
   tape "pend12".  Also, check out the color Postscript plots of 
   resonance cross sections and gas production cross sections 
   on "plot12".

 Problem 13:  This case demonstrates the new MCNP formats and ACE 
   plotting.  These formats will be needed for MCNP4c and MCNPX.

 Problem 14:  This problem is to demonstrate ACE incident proton
  data and the MCNPX charged-particle format.

  For NJOY99, the test problems were run on a number of different
  machine/compiler combinations, and the differences between the
  resulting files are tallied.  The result are given in the
  following table:

   1 Sun Solaris f77 with -g option running on an Ultra 60
   2 SGI Origin 2000 f90 with -g
   3 Windows 98 and Lahey LF95 with default optimization
   4 Windows 98 and Absoft f90 with -g
   5 Linux with g77 and -O optimization
   6 Linux with Portland Group pgf77 with -g option

   Number of different numbers found using diff:

   file tested    1-2    1-3    1-4    1-5    5-6   
   --------------------------------------------------
    out01          0      0      0     11      0
    pend01         0      0      0      0      0
    out02          0      0      0     97     23
    pend02         0      0      0      0      0
    out03          0      0      2     22      9
    out04          0      0      0      0      0
    out07          0      0      0      6      0
    pend07         0      0      0      0      0
    ace07          0      0      0      7      0
    out08          0      0      0     38      0
    pend08         0      0      0      7      0
    out09          0      0      0      0      0
    pend09         0      0      0      0      0
    out11          3      1      1     11      3
    wims11         5      6      6      8      0
    pend12         0      0      0      2      0
    out13          0      0     44      5     56
    pend13         0      0      0      7      0
    ace13          0      0      0      6      0
    out14          6      0     63      0     81
    ace14          5      0      0      0     15
   --------------------------------------------------
   Notes:
    1.  The large count in "1-5" for out02, out03, and out08
       is for small Legendre components smaller than 1e-6
       computed from differences.  There seems to be a 
       small difference in the arithmetic between the Linux 
       machines and all the others.  The "5-6" column 
       demonstrates that both Linux compilers show many of 
       the same differences.
    2.  The large difference in "1-4" and "5-6" for out13
       and out14 seem to result from different behavior in
       rounding numbers for printing.  This is demonstrated
       by having identical ace files.

     Some interesting timing numbers for the test problems:

      test    Sun Ultra    Pentium III   Pentium III     
       no      360 MHz       450 MHz       500 MHz    
               f77 -g        lf95       Linux g77 -O 
     -------------------------------------------------
       01       65.6         16.2          20.2    
       02       45.7         18.6          20.8   
       03       14.3          6.8           7.3
       04        4.4          2.5           3.5       
       05       39.3         20.8          27.6      
       07       29.3         12.5          16.4     
       08       46.8         23.5          23.9    
       09       36.3         16.1          22.0   
       10       52.2         15.9        
       11      104.3         28.3          32.5   
       12        8.9          6.1           6.5  
       13       37.0         22.9          31.1
       14       27.1          9.9          22.1
     ------------------------------------------------