/usr/share/gcal/sdata.rc is in gcal-common 3.6.3-3.
This file is owned by root:root, with mode 0o644.
The actual contents of the file can be viewed below.
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 | ; Some Sun based astronomical times and data for Gcal-2.20 or newer
;
; $Id: sdata.rc 0.07 2000/06/30 00:00:07 tom Exp $
;
; Copyright (c) 2000 Thomas Esken <esken@gmx.net>
; 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:
;
;
;
; 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!
;
; Either set your preferred geographical base location here
; or comment the proper next lines and run Gcal with the `--text-variable=ARG'
; option for passing the geographical base location in a flexible manner like:
;
; gcal -f./sdata.rc -QUx --text-var='$l=Münster:$c=+5158+00738+61:$z=60' --time-offset=t
;
; *** 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
; $l=%3%1Münster%2
; Geographical co-ordinate of location
; $c=+5158+00738+61
; Timezone of location
; $z=60
;
; Line templates
$p=0*d1#999
;
$l=
$c=
$z=
;
; Data.
$p A00 calculations for geographic co-ordinate $c,$z/$l
$p A01 gmt time and date %@
$p A02 local time and date %t /%n
$p A03 given time-offset %ot$c
$p A04 local julian date at %<9*ot$c %ou$c,$z
$p A05 local julian ephemeris date at %<9*ot$c %ov$c,$z
$p A06 local sidereal time at %<9*ot$c %os$c,$z
$p A07 equation-of-time at %<9*ot$c %ow$c,$z
$p A08 delta-t in ss.fract at %<9*ot$c %or$c,$z
;
$p B00 T sun/earth distance in au at %<9*ot$c %of$c,$z
$p B01 T sun/earth distance in km at %<9*ot$c %o*f$c,$z
$p B02 T sun's ecliptic longitude at %<9*ot$c %od$c,$z
$p B03 T sun's right ascension at %<9*ot$c %oe$c,$z
$p B04 T sun's declination angle at %<9*ot$c %oc$c,$z
$p B05 T sun's azimuth angle at %<9*ot$c %ob$c,$z
$p B06 T sun's elevation angle at %<9*ot$c %oa$c,$z
$p B07 T sun's horizontal parallax at %<9*ot$c %o*g$c,$z
$p B08 T sun's semidiameter at %<9*ot$c %o*h$c,$z
$p B09 T sun/moon azimuth delta at %<9*ot$c %oy$c,$z
$p B10 T sun/moon elevation delta at %<9*ot$c %ox$c,$z
$p B11 T atmospheric refraction at %<9*ot$c %o*i$c,$z
;
$p C00 G sun/earth distance in au at %<9*ot$c %oo$c,$z
$p C01 G sun/earth distance in km at %<9*ot$c %o*o$c,$z
$p C02 G sun's ecliptic longitude at %<9*ot$c %om$c,$z
$p C03 G sun's right ascension at %<9*ot$c %on$c,$z
$p C04 G sun's declination angle at %<9*ot$c %ol$c,$z
$p C05 G sun's azimuth angle at %<9*ot$c %ok$c,$z
$p C06 G sun's elevation angle at %<9*ot$c %oj$c,$z
$p C07 G sun's horizontal parallax at %<9*ot$c %o*p$c,$z
$p C08 G sun's semidiameter at %<9*ot$c %o*q$c,$z
$p C09 G sun/moon azimuth delta at %<9*ot$c %oA$c,$z
$p C10 G sun/moon elevation delta at %<9*ot$c %oz$c,$z
;
$p DM0 sun's midnight (near lowest culmination) at %o0$c,$z
$p DM2 T sun's elevation angle at sun's midnight %oI$c,$z
$p DM3 G sun's elevation angle at sun's midnight %oM$c,$z
$p DM4 sun/moon midnight delta %oF$c,$z
$p DN1 sun's noon (near highest culmination) at %s1$c,$z
$p DN2 T sun's elevation angle at sun's noon %sJ$c,$z
$p DN3 G sun's elevation angle at sun's noon %sN$c,$z
$p DN4 sun/moon noon delta %sG$c,$z
;
$p ER0 astronomical twilight starts at %o9$c,$z
$p FR0 amateur-astronomers twilight starts at %o8$c,$z
$p GR0 nautical twilight starts at %o7$c,$z
$p HR0 civil twilight starts at %o6$c,$z
$p IR0 sun's upper limb (standard rise) rises at %o5$c,$z
$p IR3 T sun's azimuth angle at sun's rise %oL$c,$z
$p IR4 T sun's elevation angle at sun's rise %oK$c,$z
$p IR5 G sun's azimuth angle at sun's rise %oP$c,$z
$p IR6 G sun's elevation angle at sun's rise %oO$c,$z
$p IR7 T sun/moon azimuth delta at sun's rise %oC$c,$z
$p IR8 T sun/moon elevation delta at sun's rise %oB$c,$z
$p IR9 G sun/moon azimuth delta at sun's rise %oE$c,$z
$p IRA G sun/moon elevation delta at sun's rise %oD$c,$z
$p IRB sun/moon standard rise delta %oH$c,$z
$p JR0 sun's center rises at %o4$c,$z
$p KR0 sun's upper limb at math-horizon rises at %o3$c,$z
$p LR0 sun's center at math-horizon rises at %o2$c,$z
$p MR0 shadow length equal 2x object height at %oQ$c,$z
$p NR0 shadow length equal 1x object height at %oR$c,$z
;
$p NS1 shadow length equal 1x object height at %sR$c,$z
$p MS1 shadow length equal 2x object height at %sQ$c,$z
$p LS1 sun's center at math-horizon sets at %s2$c,$z
$p KS1 sun's upper limb at math-horizon sets at %s3$c,$z
$p JS1 sun's center sets at %s4$c,$z
$p IS1 sun's upper limb (standard set) sets at %s5$c,$z
$p IS3 T sun's azimuth angle at sun's set %sL$c,$z
$p IS4 T sun's elevation angle at sun's set %sK$c,$z
$p IS5 G sun's azimuth angle at sun's set %sP$c,$z
$p IS6 G sun's elevation angle at sun's set %sO$c,$z
$p IS7 T sun/moon azimuth delta at sun's set %sC$c,$z
$p IS8 T sun/moon elevation delta at sun's set %sB$c,$z
$p IS9 G sun/moon azimuth delta at sun's set %sE$c,$z
$p ISA G sun/moon elevation delta at sun's set %sD$c,$z
$p ISB sun/moon standard set delta %sH$c,$z
$p HS1 civil twilight ends at %s6$c,$z
$p GS1 nautical twilight ends at %s7$c,$z
$p FS1 amateur-astronomers twilight ends at %s8$c,$z
$p ES1 astronomical twilight ends at %s9$c,$z
;
$p QE5 astronomical twilight visible %u9$c,$z
$p QE6 astronomical twilight non-visible %z9$c,$z
$p QF5 amateur-astronomers twilight visible %u8$c,$z
$p QF6 amateur-astronomers twilight non-visible %z8$c,$z
$p QG5 nautical twilight visible %u7$c,$z
$p QG6 nautical twilight non-visible %z7$c,$z
$p QH5 civil twilight visible %u6$c,$z
$p QH6 civil twilight non-visible %z6$c,$z
$p QI5 sun's upper limb (standard r/s) visible %u5$c,$z
$p QI6 sun's upper limb (standard r/s) non-visible %z5$c,$z
$p QJ5 sun's center visible %u4$c,$z
$p QJ6 sun's center non-visible %z4$c,$z
$p QK5 math-horizon sun's upper limb visible %u3$c,$z
$p QK6 math-horizon sun's upper limb non-visible %z3$c,$z
$p QL5 math-horizon sun's center visible %u2$c,$z
$p QL6 math-horizon sun's center non-visible %z2$c,$z
$p QM5 shadow length 2x object height visible %uQ$c,$z
$p QM6 shadow length 2x object height non-visible %zQ$c,$z
$p QN5 shadow length 1x object height visible %uR$c,$z
$p QN6 shadow length 1x object height non-visible %zR$c,$z
|