--- /dev/null
+*
+* $Id$
+*
+* $Log$
+* Revision 1.1.1.2 1996/10/30 08:28:46 cernlib
+* Version 7.04
+*
+* Revision 1.1.1.1 1996/04/12 15:29:24 plothow
+* Version 7.01
+*
+*
+#include "pdf/pilot.h"
+C-----------------------------------------------------------------------
+ SUBROUTINE HMRS1EB(X,SCALE,MODE,UPV,DNV,SEA,STR,CHM,BOT,GL)
+C***************************************************************C
+C C
+C C
+C NEW VERSIONS !!!! JANUARY 1990 (AS DESCRIBED IN C
+C "PARTON DISTRIBUTIONS ... " P.N. HARRIMAN, A.D. MARTIN, C
+C R.G. ROBERTS AND W.J. STIRLING PREPRINT DTP-90-04 ) C
+C C
+C MODE 1 CORRESPONDS TO HARRIMAN, C
+C MARTIN, ROBERTS, STIRLING (EMC FIT) WITH LAMBDA= 100 MEV C
+C C
+C MODE 2 CORRESPONDS TO HARRIMAN, C
+C MARTIN, ROBERTS, STIRLING (BCDMS FIT) WITH LAMBDA= 190 MEV C
+C C
+C >>>>>>>> CROSS CHECK <<<<<<<< C
+C C
+C THE FIRST NUMBER IN THE "E" GRID IS 0.04096 C
+C THE FIRST NUMBER IN THE "B" GRID IS 0.04574 C
+C C
+C C
+C -*- C
+C C
+C (NOTE THAT X TIMES THE PARTON DISTRIBUTION FUNCTION C
+C IS RETURNED I.E. G(X) = GLU/X ETC, AND THAT "SEA" C
+C IS THE LIGHT QUARK SEA I.E. UBAR(X)=DBAR(X)= ... C
+C = SEA/X FOR A PROTON. IF IN DOUBT, CHECK THE C
+C MOMENTUM SUM RULE! NOTE ALSO THAT SCALE=Q IN GEV) C
+C C
+C -*- C
+C C
+C (THE RANGE OF APPLICABILITY IS CURRENTLY: C
+C 10**-4 < X < 1 AND 5 < Q**2 < 1.31 * 10**6 C
+C HIGHER Q**2 VALUES CAN BE SUPPLIED ON REQUEST C
+C - PROBLEMS, COMMENTS ETC TO WJS@UK.AC.DUR.HEP C
+C C
+C C
+C***************************************************************C
+#include "pdf/impdp.inc"
+ IF(MODE.EQ.1) CALL STRH1E(X,SCALE,UPV,DNV,SEA,STR,CHM,BOT,GL)
+ IF(MODE.EQ.2) CALL STRH1B(X,SCALE,UPV,DNV,SEA,STR,CHM,BOT,GL)
+ RETURN
+ END