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authorFrederic Culot <calcurse@culot.org>2007-08-12 13:09:02 +0000
committerFrederic Culot <calcurse@culot.org>2007-08-12 13:09:02 +0000
commita9edab12b4f6ea33c478f89e00091a5817d25f9f (patch)
tree94f0795aa27234d549ba2e4edf5725e8c188f264 /src
parent73dce825b8f623f2b2ca3ddab1e4e10ab0c16977 (diff)
downloadcalcurse-a9edab12b4f6ea33c478f89e00091a5817d25f9f.tar.gz
calcurse-a9edab12b4f6ea33c478f89e00091a5817d25f9f.zip
calendar_get_pom(), pom(), potm() and adj360() added, based on the OpenBSD version of pom(6)
Diffstat (limited to 'src')
-rwxr-xr-xsrc/calendar.c180
1 files changed, 178 insertions, 2 deletions
diff --git a/src/calendar.c b/src/calendar.c
index 15c511c..9d75fbe 100755
--- a/src/calendar.c
+++ b/src/calendar.c
@@ -1,4 +1,4 @@
-/* $calcurse: calendar.c,v 1.9 2007/07/28 13:11:42 culot Exp $ */
+/* $calcurse: calendar.c,v 1.10 2007/08/12 13:09:02 culot Exp $ */
/*
* Calcurse - text-based organizer
@@ -29,6 +29,7 @@
#include <string.h>
#include <sys/types.h>
#include <time.h>
+#include <math.h>
#include "i18n.h"
#include "day.h"
@@ -39,6 +40,21 @@
#include "vars.h"
#include "utils.h"
+#ifndef M_PI
+#define M_PI 3.14159265358979323846
+#endif
+
+#define EPOCH 90
+#define EPSILONg 279.403303 /* solar ecliptic long at EPOCH */
+#define RHOg 282.768422 /* solar ecliptic long of perigee at EPOCH */
+#define ECCEN 0.016713 /* solar orbit eccentricity */
+#define lzero 318.351648 /* lunar mean long at EPOCH */
+#define Pzero 36.340410 /* lunar mean long of perigee at EPOCH */
+#define Nzero 318.510107 /* lunar mean long of node at EPOCH */
+#define TM_YEAR_BASE 1900
+
+#define isleap(y) ((((y) % 4) == 0 && ((y) % 100) != 0) || ((y) % 400) == 0)
+
static date_t today, slctd_day;
static bool week_begins_on_monday;
static pthread_mutex_t date_thread_mutex = PTHREAD_MUTEX_INITIALIZER;
@@ -100,7 +116,7 @@ calendar_set_current_date(void)
/* Needed to display sunday or monday as the first day of week in calendar. */
void
-calendar_set_first_day_of_week(wday_t first_day)
+calendar_set_first_day_of_week(wday_e first_day)
{
switch (first_day) {
case SUNDAY:
@@ -437,3 +453,163 @@ calendar_move_down(void)
} else
slctd_day.dd += 7;
}
+
+/*
+ * The pom, potm, dotr, adj360 are used to compute the current
+ * phase of the moon.
+ * The code is based on the OpenBSD version of pom(6).
+ * Below is reported the copyright notice.
+ */
+/*
+ * Copyright (c) 1989, 1993
+ * The Regents of the University of California. All rights reserved.
+ *
+ * This code is derived from software posted to USENET.
+ *
+ * Redistribution and use in source and binary forms, with or without
+ * modification, are permitted provided that the following conditions
+ * are met:
+ * 1. Redistributions of source code must retain the above copyright
+ * notice, this list of conditions and the following disclaimer.
+ * 2. Redistributions in binary form must reproduce the above copyright
+ * notice, this list of conditions and the following disclaimer in the
+ * documentation and/or other materials provided with the distribution.
+ * 3. Neither the name of the University nor the names of its contributors
+ * may be used to endorse or promote products derived from this software
+ * without specific prior written permission.
+ *
+ * THIS SOFTWARE IS PROVIDED BY THE REGENTS AND CONTRIBUTORS ``AS IS'' AND
+ * ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE
+ * IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE
+ * ARE DISCLAIMED. IN NO EVENT SHALL THE REGENTS OR CONTRIBUTORS BE LIABLE
+ * FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL
+ * DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS
+ * OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION)
+ * HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
+ * LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY
+ * OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF
+ * SUCH DAMAGE.
+ */
+
+/*
+ * dtor --
+ * convert degrees to radians
+ */
+static double
+dtor(double deg)
+{
+ return(deg * M_PI / 180);
+}
+
+/*
+ * adj360 --
+ * adjust value so 0 <= deg <= 360
+ */
+static void
+adj360(double *deg)
+{
+ for (;;)
+ if (*deg < 0.0)
+ *deg += 360.0;
+ else if (*deg > 360.0)
+ *deg -= 360.0;
+ else
+ break;
+}
+
+/*
+ * potm --
+ * return phase of the moon
+ */
+static double
+potm(double days)
+{
+ double N, Msol, Ec, LambdaSol, l, Mm, Ev, Ac, A3, Mmprime;
+ double A4, lprime, V, ldprime, D, Nm;
+
+ N = 360.0 * days / 365.242191; /* sec 46 #3 */
+ adj360(&N);
+ Msol = N + EPSILONg - RHOg; /* sec 46 #4 */
+ adj360(&Msol);
+ Ec = 360 / M_PI * ECCEN * sin(dtor(Msol)); /* sec 46 #5 */
+ LambdaSol = N + Ec + EPSILONg; /* sec 46 #6 */
+ adj360(&LambdaSol);
+ l = 13.1763966 * days + lzero; /* sec 65 #4 */
+ adj360(&l);
+ Mm = l - (0.1114041 * days) - Pzero; /* sec 65 #5 */
+ adj360(&Mm);
+ Nm = Nzero - (0.0529539 * days); /* sec 65 #6 */
+ adj360(&Nm);
+ Ev = 1.2739 * sin(dtor(2*(l - LambdaSol) - Mm)); /* sec 65 #7 */
+ Ac = 0.1858 * sin(dtor(Msol)); /* sec 65 #8 */
+ A3 = 0.37 * sin(dtor(Msol));
+ Mmprime = Mm + Ev - Ac - A3; /* sec 65 #9 */
+ Ec = 6.2886 * sin(dtor(Mmprime)); /* sec 65 #10 */
+ A4 = 0.214 * sin(dtor(2 * Mmprime)); /* sec 65 #11 */
+ lprime = l + Ev + Ec - Ac + A4; /* sec 65 #12 */
+ V = 0.6583 * sin(dtor(2 * (lprime - LambdaSol))); /* sec 65 #13 */
+ ldprime = lprime + V; /* sec 65 #14 */
+ D = ldprime - LambdaSol; /* sec 67 #2 */
+ return(50.0 * (1 - cos(dtor(D)))); /* sec 67 #3 */
+}
+
+/*
+ * Phase of the Moon. Calculates the current phase of the moon.
+ * Based on routines from `Practical Astronomy with Your Calculator',
+ * by Duffett-Smith. Comments give the section from the book that
+ * particular piece of code was adapted from.
+ *
+ * -- Keith E. Brandt VIII 1984
+ *
+ * Updated to the Third Edition of Duffett-Smith's book, IX 1998
+ *
+ */
+static double
+pom(time_t tmpt)
+{
+ struct tm *GMT;
+ double days;
+ int cnt;
+ pom_e pom;
+
+ pom = NO_POM;
+ GMT = gmtime(&tmpt);
+ days = (GMT->tm_yday + 1) + ((GMT->tm_hour +
+ (GMT->tm_min / 60.0) + (GMT->tm_sec / 3600.0)) / 24.0);
+ for (cnt = EPOCH; cnt < GMT->tm_year; ++cnt)
+ days += isleap(cnt + TM_YEAR_BASE) ? 366 : 365;
+ /* Selected time could be before EPOCH */
+ for (cnt = GMT->tm_year; cnt < EPOCH; ++cnt)
+ days -= isleap(cnt + TM_YEAR_BASE) ? 366 : 365;
+
+ return (potm(days));
+}
+
+/*
+ * Return a pictogram representing the current phase of the moon.
+ * Careful: date is the selected day in calendar at 00:00, so it represents
+ * the phase of the moon for previous day.
+ */
+char *
+calendar_get_pom(time_t date)
+{
+ char *pom_pict[MOON_PHASES] = {" ", "|) ", "(|)", "(| ", " | "};
+ pom_e phase = NO_POM;
+ double pom_today, relative_pom, pom_yesterday, pom_tomorrow;
+ const double half = 50.0;
+
+ pom_yesterday = pom(date);
+ pom_today = pom(date + DAYINSEC);
+ relative_pom = abs(pom_today - half);
+ pom_tomorrow = pom(date + 2 * DAYINSEC);
+ if (pom_today > pom_yesterday && pom_today > pom_tomorrow)
+ phase = FULL_MOON;
+ else if (pom_today < pom_yesterday && pom_today < pom_tomorrow)
+ phase = NEW_MOON;
+ else if (relative_pom < abs(pom_yesterday - half) &&
+ relative_pom < abs(pom_tomorrow - half))
+ phase = (pom_tomorrow > pom_today) ?
+ FIRST_QUARTER : LAST_QUARTER;
+
+ return (pom_pict[phase]);
+}