mikew@wyse.wyse.com (Mike Wexler) (09/27/88)
Submitted-by: jef@helios.ee.lbl.gov Posting-number: Volume 1, Issue 53 Archive-name: xphoon/part01 [As you noticed this file is for X10. In the future all X10 programs will be noted. If it doesn't say X10 it is for X11. Also I don't have X10 so I haven't tested it.] #! /bin/sh # This is a shell archive. Remove anything before this line, then unpack # it by saving it into a file and typing "sh file". To overwrite existing # files, type "sh file -c". You can also feed this as standard input via # unshar, or by typing "sh <file", e.g.. If this archive is complete, you # will see the following message at the end: # "End of archive 1 (of 3)." # Contents: README cheapmoon.bitmap.Z.uuab phase.c tws.h # Wrapped by mikew@wyse on Tue Sep 27 08:19:08 1988 PATH=/bin:/usr/bin:/usr/ucb ; export PATH if test -f 'README' -a "${1}" != "-c" ; then echo shar: Will not clobber existing file \"'README'\" else echo shar: Extracting \"'README'\" \(1901 characters\) sed "s/^X//" >'README' <<'END_OF_FILE' X xphoon, X10 version X Distribution of 15aug88 X XFiles in this distribution: X X README this X Makefile guess X main.c main routine X cheapmoon.c wrapper for standard-sized moon bitmap X bigcheapmoon.c wrapper for big moon bitmap X phase.c phase of moon calculations, from phoon and moontool X dtime.c extracted from the libtws date/time library X tws.h include file from libtws X xphoon.man manual entry X cheapmoon.bitmap.Z.uu?? standard-sized moon bitmap X XTo compile: unpack the shar files, and do a 'make unshar' to get Xcheapmoon.bitmap. Then: X XDisplay size: if your display is a standard Sun low-res 1152x900 screen, Xyou can use cheapmoon.bitmap. If you have a Sun high-res 1600x1280 screen, Xand you can FTP, you can fetch bigcheapmoon from expo.lcs.mit.edu, in Xcontrib/poskbitmaptars/poskbitmaps.b.tar - the Makefile is already set Xup to make xbigphoon out of bigcheapmoon. If you have some other size Xdisplay, you will have to HACK. I suggest using the "pbm" portable Xbitmap package to cut and paste. Pbm is available for FTP in the same Xplace as above, and it has also been distributed over comp.sources.misc Xso it will be in the various archives. Then: X XOnce you have the display size figured out, do a make. If things don't Xwork quite right, you may have to mess with the compiler flags in the XMakefile. For instance, we like to add -fswitch because some of our XSuns have floating point chips and others don't. Also, we use the -temp Xflag to specify a different temporary area because many of our Suns have Xsmall /tmp's. X X XFeedback is welcome - send bug reports, enhancements, checks, money orders, Xgold bullion, drugs, etc. to the addresses below. X X Jef Poskanzer X jef@rtsg.ee.lbl.gov X {ucbvax, lll-crg, sun!pacbell, apple, hplabs}!well!pokey X X Craig Leres X leres@helios.ee.lbl.gov X ucbvax!leres END_OF_FILE if test 1901 -ne `wc -c <'README'`; then echo shar: \"'README'\" unpacked with wrong size! fi # end of 'README' fi if test -f 'cheapmoon.bitmap.Z.uuab' -a "${1}" != "-c" ; then echo shar: Will not clobber existing file \"'cheapmoon.bitmap.Z.uuab'\" else echo shar: Extracting \"'cheapmoon.bitmap.Z.uuab'\" \(34100 characters\) sed "s/^X//" >'cheapmoon.bitmap.Z.uuab' <<'END_OF_FILE' XMCAIPT@,\CN ?DXKO4/7!@1./HH'#&I0#&;5M<Y#+LA4F<]M4>D%-J?D^:9#O XMQXQ?[=G'#$I[-:Q59?=RU![JLR"%(?%']B00&#KFSM/]QU[J>^0WUW^>U,9! 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F;V(2L&C5PP12'5O\AJRF END_OF_FILE if test 34100 -ne `wc -c <'cheapmoon.bitmap.Z.uuab'`; then echo shar: \"'cheapmoon.bitmap.Z.uuab'\" unpacked with wrong size! fi # end of 'cheapmoon.bitmap.Z.uuab' fi if test -f 'phase.c' -a "${1}" != "-c" ; then echo shar: Will not clobber existing file \"'phase.c'\" else echo shar: Extracting \"'phase.c'\" \(13799 characters\) sed "s/^X//" >'phase.c' <<'END_OF_FILE' X/* phase.c - routines to calculate the phase of the moon X** X** ver date who remarks X** --- ------- --- ------------------------------------------------------------- X** 01A 07jun88 JP Adapted from "moontool.c" by John Walker, Release 2.0. X*/ X X X#include <stdio.h> X#include <math.h> X#include "tws.h" X X/* Astronomical constants. */ X X#define epoch 2444238.5 /* 1980 January 0.0 */ X X/* Constants defining the Sun's apparent orbit. */ X X#define elonge 278.833540 /* ecliptic longitude of the Sun X at epoch 1980.0 */ X#define elongp 282.596403 /* ecliptic longitude of the Sun at X perigee */ X#define eccent 0.016718 /* eccentricity of Earth's orbit */ X#define sunsmax 1.495985e8 /* semi-major axis of Earth's orbit, km */ X#define sunangsiz 0.533128 /* sun's angular size, degrees, at X semi-major axis distance */ X X/* Elements of the Moon's orbit, epoch 1980.0. */ X X#define mmlong 64.975464 /* moon's mean lonigitude at the epoch */ X#define mmlongp 349.383063 /* mean longitude of the perigee at the X epoch */ X#define mlnode 151.950429 /* mean longitude of the node at the X epoch */ X#define minc 5.145396 /* inclination of the Moon's orbit */ X#define mecc 0.054900 /* eccentricity of the Moon's orbit */ X#define mangsiz 0.5181 /* moon's angular size at distance a X from Earth */ X#define msmax 384401.0 /* semi-major axis of Moon's orbit in km */ X#define mparallax 0.9507 /* parallax at distance a from Earth */ X#define synmonth 29.53058868 /* synodic month (new Moon to new Moon) */ X#define lunatbase 2423436.0 /* base date for E. W. Brown's numbered X series of lunations (1923 January 16) */ X X/* Properties of the Earth. */ X X#define earthrad 6378.16 /* radius of Earth in kilometres */ X X X#define PI 3.14159265358979323846 /* assume not near black hole nor in X Tennessee */ X X/* Handy mathematical functions. */ X X#define sgn(x) (((x) < 0) ? -1 : ((x) > 0 ? 1 : 0)) /* extract sign */ X#define abs(x) ((x) < 0 ? (-(x)) : (x)) /* absolute val */ X#define fixangle(a) ((a) - 360.0 * (floor((a) / 360.0))) /* fix angle */ X#define torad(d) ((d) * (PI / 180.0)) /* deg->rad */ X#define todeg(d) ((d) * (180.0 / PI)) /* rad->deg */ X#define dsin(x) (sin(torad((x)))) /* sin from deg */ X#define dcos(x) (cos(torad((x)))) /* cos from deg */ X X X/* jdate - convert internal GMT date and time to Julian day and fraction */ X Xstatic long jdate(t) Xstruct tws *t; X{ X long c, m, y; X X y = t->tw_year + 1900; X m = t->tw_mon + 1; X if (m > 2) X m = m - 3; X else { X m = m + 9; X y--; X } X c = y / 100L; /* compute century */ X y -= 100L * c; X return t->tw_mday + (c * 146097L) / 4 + (y * 1461L) / 4 + X (m * 153L + 2) / 5 + 1721119L; X} X X/* jtime - convert internal date and time to astronomical Julian X** time (i.e. Julian date plus day fraction, expressed as X** a double) X*/ X Xdouble jtime(t) Xstruct tws *t; X{ X int c; X X c = - t->tw_zone; X if ( t->tw_flags & TW_DST ) X c += 60; X X return (jdate(t) - 0.5) + X (t->tw_sec + 60 * (t->tw_min + c + 60 * t->tw_hour)) / 86400.0; X} X X/* jyear - convert Julian date to year, month, day, which are X** returned via integer pointers to integers X*/ X Xstatic void jyear(td, yy, mm, dd) Xdouble td; Xint *yy, *mm, *dd; X{ X double j, d, y, m; X X td += 0.5; /* astronomical to civil */ X j = floor(td); X j = j - 1721119.0; X y = floor(((4 * j) - 1) / 146097.0); X j = (j * 4.0) - (1.0 + (146097.0 * y)); X d = floor(j / 4.0); X j = floor(((4.0 * d) + 3.0) / 1461.0); X d = ((4.0 * d) + 3.0) - (1461.0 * j); X d = floor((d + 4.0) / 4.0); X m = floor(((5.0 * d) - 3) / 153.0); X d = (5.0 * d) - (3.0 + (153.0 * m)); X d = floor((d + 5.0) / 5.0); X y = (100.0 * y) + j; X if (m < 10.0) X m = m + 3; X else { X m = m - 9; X y = y + 1; X } X *yy = y; X *mm = m; X *dd = d; X} X X/* jhms - convert Julian time to hour, minutes, and seconds */ X Xstatic void jhms(j, h, m, s) Xdouble j; Xint *h, *m, *s; X{ X long ij; X X j += 0.5; /* astronomical to civil */ X ij = (j - floor(j)) * 86400.0; X *h = ij / 3600L; X *m = (ij / 60L) % 60L; X *s = ij % 60L; X} X X/* meanphase - calculates mean phase of the Moon for a given base date X** and desired phase: X** 0.0 New Moon X** 0.25 First quarter X** 0.5 Full moon X** 0.75 Last quarter X** Beware!!! This routine returns meaningless X** results for any other phase arguments. Don't X** attempt to generalise it without understanding X** that the motion of the moon is far more complicated X** that this calculation reveals. X*/ X Xstatic double meanphase(sdate, phase, usek) Xdouble sdate, phase; Xdouble *usek; X{ X int yy, mm, dd; X double k, t, t2, t3, nt1; X X jyear(sdate, &yy, &mm, &dd); X X k = (yy + ((mm - 1) * (1.0 / 12.0)) - 1900) * 12.3685; X X /* Time in Julian centuries from 1900 January 0.5. */ X t = (sdate - 2415020.0) / 36525; X t2 = t * t; /* square for frequent use */ X t3 = t2 * t; /* cube for frequent use */ X X *usek = k = floor(k) + phase; X nt1 = 2415020.75933 + synmonth * k X + 0.0001178 * t2 X - 0.000000155 * t3 X + 0.00033 * dsin(166.56 + 132.87 * t - 0.009173 * t2); X X return nt1; X} X X/* truephase - given a K value used to determine the mean phase of the X** new moon, and a phase selector (0.0, 0.25, 0.5, 0.75), X** obtain the true, corrected phase time X*/ X Xstatic double truephase(k, phase) Xdouble k, phase; X{ X double t, t2, t3, pt, m, mprime, f; X int apcor = 0; X X k += phase; /* add phase to new moon time */ X t = k / 1236.85; /* time in Julian centuries from X 1900 January 0.5 */ X t2 = t * t; /* square for frequent use */ X t3 = t2 * t; /* cube for frequent use */ X pt = 2415020.75933 /* mean time of phase */ X + synmonth * k X + 0.0001178 * t2 X - 0.000000155 * t3 X + 0.00033 * dsin(166.56 + 132.87 * t - 0.009173 * t2); X X m = 359.2242 /* Sun's mean anomaly */ X + 29.10535608 * k X - 0.0000333 * t2 X - 0.00000347 * t3; X mprime = 306.0253 /* Moon's mean anomaly */ X + 385.81691806 * k X + 0.0107306 * t2 X + 0.00001236 * t3; X f = 21.2964 /* Moon's argument of latitude */ X + 390.67050646 * k X - 0.0016528 * t2 X - 0.00000239 * t3; X if ((phase < 0.01) || (abs(phase - 0.5) < 0.01)) { X X /* Corrections for New and Full Moon. */ X X pt += (0.1734 - 0.000393 * t) * dsin(m) X + 0.0021 * dsin(2 * m) X - 0.4068 * dsin(mprime) X + 0.0161 * dsin(2 * mprime) X - 0.0004 * dsin(3 * mprime) X + 0.0104 * dsin(2 * f) X - 0.0051 * dsin(m + mprime) X - 0.0074 * dsin(m - mprime) X + 0.0004 * dsin(2 * f + m) X - 0.0004 * dsin(2 * f - m) X - 0.0006 * dsin(2 * f + mprime) X + 0.0010 * dsin(2 * f - mprime) X + 0.0005 * dsin(m + 2 * mprime); X apcor = 1; X } else if ((abs(phase - 0.25) < 0.01 || (abs(phase - 0.75) < 0.01))) { X pt += (0.1721 - 0.0004 * t) * dsin(m) X + 0.0021 * dsin(2 * m) X - 0.6280 * dsin(mprime) X + 0.0089 * dsin(2 * mprime) X - 0.0004 * dsin(3 * mprime) X + 0.0079 * dsin(2 * f) X - 0.0119 * dsin(m + mprime) X - 0.0047 * dsin(m - mprime) X + 0.0003 * dsin(2 * f + m) X - 0.0004 * dsin(2 * f - m) X - 0.0006 * dsin(2 * f + mprime) X + 0.0021 * dsin(2 * f - mprime) X + 0.0003 * dsin(m + 2 * mprime) X + 0.0004 * dsin(m - 2 * mprime) X - 0.0003 * dsin(2 * m + mprime); X if (phase < 0.5) X /* First quarter correction. */ X pt += 0.0028 - 0.0004 * dcos(m) + 0.0003 * dcos(mprime); X else X /* Last quarter correction. */ X pt += -0.0028 + 0.0004 * dcos(m) - 0.0003 * dcos(mprime); X apcor = 1; X } X if (!apcor) { X fprintf(stderr, "truephase() called with invalid phase selector.\n"); X abort(); X } X return pt; X} X X/* phasehunt5 - find time of phases of the moon which surround the current X** date. Five phases are found, starting and ending with the X** new moons which bound the current lunation X*/ X Xvoid phasehunt5(sdate, phases) Xdouble sdate; Xdouble phases[5]; X{ X double adate, k1, k2, nt1, nt2; X X adate = sdate - 45; X nt1 = meanphase(adate, 0.0, &k1); X for ( ; ; ) { X adate += synmonth; X nt2 = meanphase(adate, 0.0, &k2); X if (nt1 <= sdate && nt2 > sdate) X break; X nt1 = nt2; X k1 = k2; X } X phases[0] = truephase(k1, 0.0); X phases[1] = truephase(k1, 0.25); X phases[2] = truephase(k1, 0.5); X phases[3] = truephase(k1, 0.75); X phases[4] = truephase(k2, 0.0); X} X X X/* phasehunt2 - find time of phases of the moon which surround the current X** date. Two phases are found. X*/ X Xvoid phasehunt2(sdate, phases, which) Xdouble sdate; Xdouble phases[2]; Xdouble which[2]; X{ X double adate, k1, k2, nt1, nt2; X X adate = sdate - 45; X nt1 = meanphase(adate, 0.0, &k1); X for ( ; ; ) { X adate += synmonth; X nt2 = meanphase(adate, 0.0, &k2); X if (nt1 <= sdate && nt2 > sdate) X break; X nt1 = nt2; X k1 = k2; X } X phases[0] = truephase(k1, 0.0); X which[0] = 0.0; X phases[1] = truephase(k1, 0.25); X which[1] = 0.25; X if ( phases[1] <= sdate ) { X phases[0] = phases[1]; X which[0] = which[1]; X phases[1] = truephase(k1, 0.5); X which[1] = 0.5; X if ( phases[1] <= sdate ) { X phases[0] = phases[1]; X which[0] = which[1]; X phases[1] = truephase(k1, 0.75); X which[1] = 0.75; X if ( phases[1] <= sdate ) { X phases[0] = phases[1]; X which[0] = which[1]; X phases[1] = truephase(k2, 0.0); X which[1] = 0.0; X } X } X } X} X X X/* kepler - solve the equation of Kepler */ X Xstatic double kepler(m, ecc) Xdouble m, ecc; X{ X double e, delta; X#define EPSILON 1E-6 X X e = m = torad(m); X do { X delta = e - ecc * sin(e) - m; X e -= delta / (1 - ecc * cos(e)); X } while (abs(delta) > EPSILON); X return e; X} X X/* phase - calculate phase of moon as a fraction: X** X** The argument is the time for which the phase is requested, X** expressed as a Julian date and fraction. Returns the terminator X** phase angle as a percentage of a full circle (i.e., 0 to 1), X** and stores into pointer arguments the illuminated fraction of X** the Moon's disc, the Moon's age in days and fraction, the X** distance of the Moon from the centre of the Earth, and the X** angular diameter subtended by the Moon as seen by an observer X** at the centre of the Earth. X*/ X Xdouble phase(pdate, pphase, mage, dist, angdia, sudist, suangdia) Xdouble pdate; Xdouble *pphase; /* illuminated fraction */ Xdouble *mage; /* age of moon in days */ Xdouble *dist; /* distance in kilometres */ Xdouble *angdia; /* angular diameter in degrees */ Xdouble *sudist; /* distance to Sun */ Xdouble *suangdia; /* sun's angular diameter */ X{ X X double Day, N, M, Ec, Lambdasun, ml, MM, MN, Ev, Ae, A3, MmP, X mEc, A4, lP, V, lPP, NP, y, x, Lambdamoon, BetaM, X MoonAge, MoonPhase, X MoonDist, MoonDFrac, MoonAng, MoonPar, X F, SunDist, SunAng; X X /* Calculation of the Sun's position. */ X X Day = pdate - epoch; /* date within epoch */ X N = fixangle((360 / 365.2422) * Day); /* mean anomaly of the Sun */ X M = fixangle(N + elonge - elongp); /* convert from perigee X co-ordinates to epoch 1980.0 */ X Ec = kepler(M, eccent); /* solve equation of Kepler */ X Ec = sqrt((1 + eccent) / (1 - eccent)) * tan(Ec / 2); X Ec = 2 * todeg(atan(Ec)); /* true anomaly */ X Lambdasun = fixangle(Ec + elongp); /* Sun's geocentric ecliptic X longitude */ X /* Orbital distance factor. */ X F = ((1 + eccent * cos(torad(Ec))) / (1 - eccent * eccent)); X SunDist = sunsmax / F; /* distance to Sun in km */ X SunAng = F * sunangsiz; /* Sun's angular size in degrees */ X X X /* Calculation of the Moon's position. */ X X /* Moon's mean longitude. */ X ml = fixangle(13.1763966 * Day + mmlong); X X /* Moon's mean anomaly. */ X MM = fixangle(ml - 0.1114041 * Day - mmlongp); X X /* Moon's ascending node mean longitude. */ X MN = fixangle(mlnode - 0.0529539 * Day); X X /* Evection. */ X Ev = 1.2739 * sin(torad(2 * (ml - Lambdasun) - MM)); X X /* Annual equation. */ X Ae = 0.1858 * sin(torad(M)); X X /* Correction term. */ X A3 = 0.37 * sin(torad(M)); X X /* Corrected anomaly. */ X MmP = MM + Ev - Ae - A3; X X /* Correction for the equation of the centre. */ X mEc = 6.2886 * sin(torad(MmP)); X X /* Another correction term. */ X A4 = 0.214 * sin(torad(2 * MmP)); X X /* Corrected longitude. */ X lP = ml + Ev + mEc - Ae + A4; X X /* Variation. */ X V = 0.6583 * sin(torad(2 * (lP - Lambdasun))); X X /* True longitude. */ X lPP = lP + V; X X /* Corrected longitude of the node. */ X NP = MN - 0.16 * sin(torad(M)); X X /* Y inclination coordinate. */ X y = sin(torad(lPP - NP)) * cos(torad(minc)); X X /* X inclination coordinate. */ X x = cos(torad(lPP - NP)); X X /* Ecliptic longitude. */ X Lambdamoon = todeg(atan2(y, x)); X Lambdamoon += NP; X X /* Ecliptic latitude. */ X BetaM = todeg(asin(sin(torad(lPP - NP)) * sin(torad(minc)))); X X /* Calculation of the phase of the Moon. */ X X /* Age of the Moon in degrees. */ X MoonAge = lPP - Lambdasun; X X /* Phase of the Moon. */ X MoonPhase = (1 - cos(torad(MoonAge))) / 2; X X /* Calculate distance of moon from the centre of the Earth. */ X X MoonDist = (msmax * (1 - mecc * mecc)) / X (1 + mecc * cos(torad(MmP + mEc))); X X /* Calculate Moon's angular diameter. */ X X MoonDFrac = MoonDist / msmax; X MoonAng = mangsiz / MoonDFrac; X X /* Calculate Moon's parallax. */ X X MoonPar = mparallax / MoonDFrac; X X *pphase = MoonPhase; X *mage = synmonth * (fixangle(MoonAge) / 360.0); X *dist = MoonDist; X *angdia = MoonAng; X *sudist = SunDist; X *suangdia = SunAng; X return torad(fixangle(MoonAge)); X} END_OF_FILE if test 13799 -ne `wc -c <'phase.c'`; then echo shar: \"'phase.c'\" unpacked with wrong size! fi # end of 'phase.c' fi if test -f 'tws.h' -a "${1}" != "-c" ; then echo shar: Will not clobber existing file \"'tws.h'\" else echo shar: Extracting \"'tws.h'\" \(2290 characters\) sed "s/^X//" >'tws.h' <<'END_OF_FILE' X/* tws.h - header file for libtws date/time library */ X X X/* Definition of the tws data structure. */ X Xstruct tws { X int tw_sec; X int tw_min; X int tw_hour; X X int tw_mday; X int tw_mon; X int tw_year; X X int tw_wday; X int tw_yday; X X int tw_zone; X X long tw_clock; X X int tw_flags; X#define TW_NULL 0x0000 X#define TW_SDAY 0x0007 /* how day-of-week was determined */ X#define TW_SNIL 0x0000 /* not given */ X#define TW_SEXP 0x0001 /* explicitly given */ X#define TW_SIMP 0x0002 /* implicitly given */ X#define TW_DST 0x0010 /* daylight savings time */ X#define TW_ZONE 0x0020 /* use numeric timezones only */ X#define TW_JUNK 0x0040 /* date string contained junk */ X}; X X X/* Declarations of routines. */ X Xvoid twscopy( ); X /* twscopy( &totws, &fromtws ) copies a tws */ Xint twsort( ); X /* twsort( &tws1, &tws2 ) compares two tws's: 1 means tws1 is X later; -1 means tws1 is earlier; 0 means they are equal */ Xlong twclock( ); X /* twclock( &tws ) turns a tws into a time(3)-style clock value */ Xlong twjuliandate( ); X /* twjuliandate( &tws ) returns the Julian day number of a tws */ Xlong twsubtract( ); X /* twsubtract( &tws1, &tws2 ) returns seconds of difference */ X X/* These routines are functionally similar to the ctime(3) routines X in the standard Unix library. */ Xchar *dctime( ); X /* dctime( &tws ) returns a string for the date/time passed in */ Xstruct tws *dlocaltime( ); X /* dlocaltime( &clock ) turns a time(3) clock value into a tws */ Xstruct tws *dgmtime( ); X /* dgmtime( &clock ) turns a time(3) clock value into a tws */ Xchar *dasctime( ); X /* dasctime( &tws, flags ) turns a tws into a string */ Xchar *dtimezone( ); X /* dtimezone( offset, flags ) returns the name of the time zone */ X Xchar *dtimenow( ); X /* dtimenow( ) returns a string for the current date/time */ X Xstruct tws *dparsetime( ); X /* dparsetime( &str ) turns a string into a tws */ X Xstruct tws *dtwstime( ); X /* dtwstime( ) returns a tws for the current date/time */ X X#ifdef ATZ X#define dtime(cl) dasctime( dlocaltime( cl ), TW_NULL ) X#else ATZ X#define dtime(cl) dasctime( dlocaltime( cl ), TW_ZONE ) X#endif ATZ X X#define dtwszone(tw) dtimezone( tw -> tw_zone, tw -> tw_flags ) X X Xextern char *tw_dotw[], *tw_ldotw[], *tw_moty[]; END_OF_FILE if test 2290 -ne `wc -c <'tws.h'`; then echo shar: \"'tws.h'\" unpacked with wrong size! fi # end of 'tws.h' fi echo shar: End of archive 1 \(of 3\). cp /dev/null ark1isdone MISSING="" for I in 1 2 3 ; do if test ! -f ark${I}isdone ; then MISSING="${MISSING} ${I}" fi done if test "${MISSING}" = "" ; then echo You have unpacked all 3 archives. rm -f ark[1-9]isdone else echo You still need to unpack the following archives: echo " " ${MISSING} fi ## End of shell archive. exit 0 -- Mike Wexler(wyse!mikew) Phone: (408)433-1000 x1330