; Some Sun based astronomical times and data for locations in Germany for Gcal-2.20 or newer ; ; $Id: de-sdata.rc 0.06 2000/06/30 00:00:06 tom Exp $ ; ; Copyright (c) 2000 Thomas Esken ; Im Hagenfeld 84 ; D-48147 M"unster ; GERMANY ; ; This software doesn't claim completeness, correctness or usability. ; On principle I will not be liable for ANY damages or losses (implicit ; or explicit), which result from using or handling my software. ; If you use this software, you agree without any exception to this ; agreement, which binds you LEGALLY !! ; ; This program is free software; you can redistribute it and/or modify ; it under the terms of the `GNU General Public License' as published by ; the `Free Software Foundation'; either version 2, or (at your option) ; any later version. ; ; You should have received a copy of the `GNU General Public License' ; along with this program; if not, write to the: ; ; Free Software Foundation, Inc. ; 59 Temple Place - Suite 330 ; Boston, MA 02111-1307, USA ; ; ; Try this resource file by using the `-QUx' option of Gcal. ; Try `--time-offset=ARG' to calculate some data for a definite time! ; Try `--precise' to display data and times more precise! ; ; *** If you modify this file you have to rename the modified version. ; *** If you make any improvements I would like to hear from you. ; *** But I do not promise any support. ; ; ; Name of location and geographical co-ordinate $l=%3%1Münster%2 $c=+5158+00738+61 ; ; Line templates $p=0*d1#999 ; ; Definitions for winter time $a=%e0@a#0@b-1 ; ; Winter time in Germany == CEWT/GMT-1 (+60 minutes) $w=+60 ; ; Start of winter time in Germany b=10sun9 ; ; Definitions for summer time $b=%i0@a#0@b-1 ; ; Summer time in Germany == CEST/GMT-2 (+120 minutes) $s=+120 ; ; Start of summer time in Germany a=03sun9 ; ; Data $t=A00 calculations for geographic co-ordinate $c $p $a $t,$w/$l $p $b $t,$s/$l $p A01 gmt time and date %@ $p A02 local time and date %t /%n $p A03 given time-offset %ot$c $t=A04 local julian date at %<9*ot$c %ou$c $p $a $t,$w $p $b $t,$s $t=A05 local julian ephemeris date at %<9*ot$c %ov$c $p $a $t,$w $p $b $t,$s $t=A06 local sidereal time at %<9*ot$c %os$c $p $a $t,$w $p $b $t,$s $t=A07 equation-of-time at %<9*ot$c %ow$c $p $a $t,$w $p $b $t,$s $t=A08 delta-t in ss.fract at %<9*ot$c %or$c $p $a $t,$w $p $b $t,$s ; $t=B00 T sun/earth distance in au at %<9*ot$c %of$c $p $a $t,$w $p $b $t,$s $t=B01 T sun/earth distance in km at %<9*ot$c %o*f$c $p $a $t,$w $p $b $t,$s $t=B02 T sun's ecliptic longitude at %<9*ot$c %od$c $p $a $t,$w $p $b $t,$s $t=B03 T sun's right ascension at %<9*ot$c %oe$c $p $a $t,$w $p $b $t,$s $t=B04 T sun's declination angle at %<9*ot$c %oc$c $p $a $t,$w $p $b $t,$s $t=B05 T sun's azimuth angle at %<9*ot$c %ob$c $p $a $t,$w $p $b $t,$s $t=B06 T sun's elevation angle at %<9*ot$c %oa$c $p $a $t,$w $p $b $t,$s $t=B07 T sun's horizontal parallax at %<9*ot$c %o*g$c $p $a $t,$w $p $b $t,$s $t=B08 T sun's semidiameter at %<9*ot$c %o*h$c $p $a $t,$w $p $b $t,$s $t=B09 T sun/moon azimuth delta at %<9*ot$c %oy$c $p $a $t,$w $p $b $t,$s $t=B10 T sun/moon elevation delta at %<9*ot$c %ox$c $p $a $t,$w $p $b $t,$s $t=B11 T atmospheric refraction at %<9*ot$c %o*i$c $p $a $t,$w $p $b $t,$s ; $t=C00 G sun/earth distance in au at %<9*ot$c %oo$c $p $a $t,$w $p $b $t,$s $t=C01 G sun/earth distance in km at %<9*ot$c %o*o$c $p $a $t,$w $p $b $t,$s $t=C02 G sun's ecliptic longitude at %<9*ot$c %om$c $p $a $t,$w $p $b $t,$s $t=C03 G sun's right ascension at %<9*ot$c %on$c $p $a $t,$w $p $b $t,$s $t=C04 G sun's declination angle at %<9*ot$c %ol$c $p $a $t,$w $p $b $t,$s $t=C05 G sun's azimuth angle at %<9*ot$c %ok$c $p $a $t,$w $p $b $t,$s $t=C06 G sun's elevation angle at %<9*ot$c %oj$c $p $a $t,$w $p $b $t,$s $t=C07 G sun's horizontal parallax at %<9*ot$c %o*p$c $p $a $t,$w $p $b $t,$s $t=C08 G sun's semidiameter at %<9*ot$c %o*q$c $p $a $t,$w $p $b $t,$s $t=C09 G sun/moon azimuth delta at %<9*ot$c %oA$c $p $a $t,$w $p $b $t,$s $t=C10 G sun/moon elevation delta at %<9*ot$c %oz$c $p $a $t,$w $p $b $t,$s ; $t=DM0 sun's midnight (near lowest culmination) at %o0$c $p $a $t,$w $p $b $t,$s $t=DM2 T sun's elevation angle at sun's midnight %oI$c $p $a $t,$w $p $b $t,$s $t=DM3 G sun's elevation angle at sun's midnight %oM$c $p $a $t,$w $p $b $t,$s $t=DM4 sun/moon midnight delta %oF$c $p $a $t,$w $p $b $t,$s $t=DN1 sun's noon (near highest culmination) at %s1$c $p $a $t,$w $p $b $t,$s $t=DN2 T sun's elevation angle at sun's noon %sJ$c $p $a $t,$w $p $b $t,$s $t=DN3 G sun's elevation angle at sun's noon %sN$c $p $a $t,$w $p $b $t,$s $t=DN4 sun/moon noon delta %sG$c $p $a $t,$w $p $b $t,$s ; $t=ER0 astronomical twilight starts at %o9$c $p $a $t,$w $p $b $t,$s $t=FR0 amateur-astronomers twilight starts at %o8$c $p $a $t,$w $p $b $t,$s $t=GR0 nautical twilight starts at %o7$c $p $a $t,$w $p $b $t,$s $t=HR0 civil twilight starts at %o6$c $p $a $t,$w $p $b $t,$s $t=IR0 sun's upper limb (standard rise) rises at %o5$c $p $a $t,$w $p $b $t,$s $t=IR3 T sun's azimuth angle at sun's rise %oL$c $p $a $t,$w $p $b $t,$s $t=IR4 T sun's elevation angle at sun's rise %oK$c $p $a $t,$w $p $b $t,$s $t=IR5 G sun's azimuth angle at sun's rise %oP$c $p $a $t,$w $p $b $t,$s $t=IR6 G sun's elevation angle at sun's rise %oO$c $p $a $t,$w $p $b $t,$s $t=IR7 T sun/moon azimuth delta at sun's rise %oC$c $p $a $t,$w $p $b $t,$s $t=IR8 T sun/moon elevation delta at sun's rise %oB$c $p $a $t,$w $p $b $t,$s $t=IR9 G sun/moon azimuth delta at sun's rise %oE$c $p $a $t,$w $p $b $t,$s $t=IRA G sun/moon elevation delta at sun's rise %oD$c $p $a $t,$w $p $b $t,$s $t=IRB sun/moon standard rise delta %oH$c $p $a $t,$w $p $b $t,$s $t=JR0 sun's center rises at %o4$c $p $a $t,$w $p $b $t,$s $t=KR0 sun's upper limb at math-horizon rises at %o3$c $p $a $t,$w $p $b $t,$s $t=LR0 sun's center at math-horizon rises at %o2$c $p $a $t,$w $p $b $t,$s $t=MR0 shadow length equal 2x object height at %oQ$c $p $a $t,$w $p $b $t,$s $t=NR0 shadow length equal 1x object height at %oR$c $p $a $t,$w $p $b $t,$s ; $t=NS1 shadow length equal 1x object height at %sR$c $p $a $t,$w $p $b $t,$s $t=MS1 shadow length equal 2x object height at %sQ$c $p $a $t,$w $p $b $t,$s $t=LS1 sun's center at math-horizon sets at %s2$c $p $a $t,$w $p $b $t,$s $t=KS1 sun's upper limb at math-horizon sets at %s3$c $p $a $t,$w $p $b $t,$s $t=JS1 sun's center sets at %s4$c $p $a $t,$w $p $b $t,$s $t=IS1 sun's upper limb (standard set) sets at %s5$c $p $a $t,$w $p $b $t,$s $t=IS3 T sun's azimuth angle at sun's set %sL$c $p $a $t,$w $p $b $t,$s $t=IS4 T sun's elevation angle at sun's set %sK$c $p $a $t,$w $p $b $t,$s $t=IS5 G sun's azimuth angle at sun's set %sP$c $p $a $t,$w $p $b $t,$s $t=IS6 G sun's elevation angle at sun's set %sO$c $p $a $t,$w $p $b $t,$s $t=IS7 T sun/moon azimuth delta at sun's set %sC$c $p $a $t,$w $p $b $t,$s $t=IS8 T sun/moon elevation delta at sun's set %sB$c $p $a $t,$w $p $b $t,$s $t=IS9 G sun/moon azimuth delta at sun's set %sE$c $p $a $t,$w $p $b $t,$s $t=ISA G sun/moon elevation delta at sun's set %sD$c $p $a $t,$w $p $b $t,$s $t=ISB sun/moon standard set delta %sH$c $p $a $t,$w $p $b $t,$s $t=HS1 civil twilight ends at %s6$c $p $a $t,$w $p $b $t,$s $t=GS1 nautical twilight ends at %s7$c $p $a $t,$w $p $b $t,$s $t=FS1 amateur-astronomers twilight ends at %s8$c $p $a $t,$w $p $b $t,$s $t=ES1 astronomical twilight ends at %s9$c $p $a $t,$w $p $b $t,$s ; $t=QE5 astronomical twilight visible %u9$c $p $a $t,$w $p $b $t,$s $t=QE6 astronomical twilight non-visible %z9$c $p $a $t,$w $p $b $t,$s $t=QF5 amateur-astronomers twilight visible %u8$c $p $a $t,$w $p $b $t,$s $t=QF6 amateur-astronomers twilight non-visible %z8$c $p $a $t,$w $p $b $t,$s $t=QG5 nautical twilight visible %u7$c $p $a $t,$w $p $b $t,$s $t=QG6 nautical twilight non-visible %z7$c $p $a $t,$w $p $b $t,$s $t=QH5 civil twilight visible %u6$c $p $a $t,$w $p $b $t,$s $t=QH6 civil twilight non-visible %z6$c $p $a $t,$w $p $b $t,$s $t=QI5 sun's upper limb (standard r/s) visible %u5$c $p $a $t,$w $p $b $t,$s $t=QI6 sun's upper limb (standard r/s) non-visible %z5$c $p $a $t,$w $p $b $t,$s $t=QJ5 sun's center visible %u4$c $p $a $t,$w $p $b $t,$s $t=QJ6 sun's center non-visible %z4$c $p $a $t,$w $p $b $t,$s $t=QK5 math-horizon sun's upper limb visible %u3$c $p $a $t,$w $p $b $t,$s $t=QK6 math-horizon sun's upper limb non-visible %z3$c $p $a $t,$w $p $b $t,$s $t=QL5 math-horizon sun's center visible %u2$c $p $a $t,$w $p $b $t,$s $t=QL6 math-horizon sun's center non-visible %z2$c $p $a $t,$w $p $b $t,$s $t=QM5 shadow length 2x object height visible %uQ$c $p $a $t,$w $p $b $t,$s $t=QM6 shadow length 2x object height non-visible %zQ$c $p $a $t,$w $p $b $t,$s $t=QN5 shadow length 1x object height visible %uR$c $p $a $t,$w $p $b $t,$s $t=QN6 shadow length 1x object height non-visible %zR$c $p $a $t,$w $p $b $t,$s