Remove phase of moon feature
The computation never really worked before and it seems like the feature is not very helpful, sometimes even confusing (see GitHub issue #21). The macro ISLEAP is moved to calcurse.h. Signed-off-by: Lars Henriksen <LarsHenriksen@get2net.dk> Signed-off-by: Lukas Fleischer <lfleischer@calcurse.org>
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@ -302,6 +302,8 @@ struct date {
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unsigned yyyy;
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unsigned yyyy;
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};
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};
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#define ISLEAP(y) ((((y) % 4) == 0 && ((y) % 100) != 0) || ((y) % 400) == 0)
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/* Appointment definition. */
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/* Appointment definition. */
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struct apoint {
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struct apoint {
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long start; /* seconds since 1 jan 1970 */
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long start; /* seconds since 1 jan 1970 */
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@ -740,7 +742,6 @@ void ui_calendar_change_day(int);
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void ui_calendar_move(enum move, int);
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void ui_calendar_move(enum move, int);
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long ui_calendar_start_of_year(void);
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long ui_calendar_start_of_year(void);
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long ui_calendar_end_of_year(void);
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long ui_calendar_end_of_year(void);
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const char *ui_calendar_get_pom(time_t);
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/* config.c */
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/* config.c */
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void config_load(void);
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void config_load(void);
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@ -44,29 +44,6 @@
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#include "calcurse.h"
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#include "calcurse.h"
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#ifndef M_PI
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#define M_PI 3.14159265358979323846
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#endif
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#define EPOCH 90
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#define EPSILONg 279.403303 /* solar ecliptic long at EPOCH */
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#define RHOg 282.768422 /* solar ecliptic long of perigee at EPOCH */
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#define ECCEN 0.016713 /* solar orbit eccentricity */
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#define lzero 318.351648 /* lunar mean long at EPOCH */
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#define Pzero 36.340410 /* lunar mean long of perigee at EPOCH */
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#define Nzero 318.510107 /* lunar mean long of node at EPOCH */
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#define ISLEAP(y) ((((y) % 4) == 0 && ((y) % 100) != 0) || ((y) % 400) == 0)
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enum pom {
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NO_POM,
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FIRST_QUARTER,
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FULL_MOON,
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LAST_QUARTER,
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NEW_MOON,
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MOON_PHASES
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};
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static struct date today, slctd_day;
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static struct date today, slctd_day;
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static unsigned ui_calendar_view, week_begins_on_monday;
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static unsigned ui_calendar_view, week_begins_on_monday;
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static pthread_mutex_t date_thread_mutex = PTHREAD_MUTEX_INITIALIZER;
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static pthread_mutex_t date_thread_mutex = PTHREAD_MUTEX_INITIALIZER;
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@ -780,161 +757,3 @@ long ui_calendar_end_of_year(void)
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return (long)(timer - 1);
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return (long)(timer - 1);
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}
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}
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/*
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* The pom, potm, dotr, adj360 are used to compute the current
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* phase of the moon.
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* The code is based on the OpenBSD version of pom(6).
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* Below is reported the copyright notice.
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*/
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/*
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* Copyright (c) 1989, 1993
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* The Regents of the University of California. All rights reserved.
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*
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* This code is derived from software posted to USENET.
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*
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* Redistribution and use in source and binary forms, with or without
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* modification, are permitted provided that the following conditions
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* are met:
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* 1. Redistributions of source code must retain the above copyright
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* notice, this list of conditions and the following disclaimer.
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* 2. Redistributions in binary form must reproduce the above copyright
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* notice, this list of conditions and the following disclaimer in the
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* documentation and/or other materials provided with the distribution.
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* 3. Neither the name of the University nor the names of its contributors
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* may be used to endorse or promote products derived from this software
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* without specific prior written permission.
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*
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* THIS SOFTWARE IS PROVIDED BY THE REGENTS AND CONTRIBUTORS ``AS IS'' AND
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* ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE
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* IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE
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* ARE DISCLAIMED. IN NO EVENT SHALL THE REGENTS OR CONTRIBUTORS BE LIABLE
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* FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL
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* DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS
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* OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION)
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* HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
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* LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY
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* OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF
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* SUCH DAMAGE.
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*/
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/*
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* dtor --
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* convert degrees to radians
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*/
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static double dtor(double deg)
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{
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return deg * M_PI / 180;
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}
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/*
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* adj360 --
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* adjust value so 0 <= deg <= 360
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*/
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static void adj360(double *deg)
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{
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for (;;)
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if (*deg < 0.0)
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*deg += 360.0;
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else if (*deg > 360.0)
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*deg -= 360.0;
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else
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break;
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}
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/*
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* Phase of the Moon. Calculates the current phase of the moon.
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* Based on routines from `Practical Astronomy with Your Calculator',
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* by Duffett-Smith. Comments give the section from the book that
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* particular piece of code was adapted from.
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*
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* -- Keith E. Brandt VIII 1984
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*
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* Updated to the Third Edition of Duffett-Smith's book, IX 1998
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*
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*/
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/*
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* potm --
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* given number of days since January 1st 1990, 00:00
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* (incl. hours and minutes as a fraction of a day),
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* return phase of the moon as a percentage.
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*/
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static double potm(double days)
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{
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double N, Msol, Ec, LambdaSol, l, Mm, Ev, Ac, A3, Mmprime;
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double A4, lprime, V, ldprime, D, Nm;
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N = 360.0 * days / 365.242191; /* sec 46 #3 */
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adj360(&N);
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Msol = N + EPSILONg - RHOg; /* sec 46 #4 */
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adj360(&Msol);
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Ec = 360 / M_PI * ECCEN * sin(dtor(Msol)); /* sec 46 #5 */
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LambdaSol = N + Ec + EPSILONg; /* sec 46 #6 */
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adj360(&LambdaSol);
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l = 13.1763966 * days + lzero; /* sec 65 #4 */
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adj360(&l);
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Mm = l - (0.1114041 * days) - Pzero; /* sec 65 #5 */
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adj360(&Mm);
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Nm = Nzero - (0.0529539 * days); /* sec 65 #6 */
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adj360(&Nm);
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Ev = 1.2739 * sin(dtor(2 * (l - LambdaSol) - Mm)); /* sec 65 #7 */
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Ac = 0.1858 * sin(dtor(Msol)); /* sec 65 #8 */
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A3 = 0.37 * sin(dtor(Msol));
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Mmprime = Mm + Ev - Ac - A3; /* sec 65 #9 */
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Ec = 6.2886 * sin(dtor(Mmprime)); /* sec 65 #10 */
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A4 = 0.214 * sin(dtor(2 * Mmprime)); /* sec 65 #11 */
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lprime = l + Ev + Ec - Ac + A4; /* sec 65 #12 */
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V = 0.6583 * sin(dtor(2 * (lprime - LambdaSol))); /* sec 65 #13 */
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ldprime = lprime + V; /* sec 65 #14 */
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D = ldprime - LambdaSol; /* sec 67 #2 */
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return 50.0 * (1 - cos(dtor(D))); /* sec 67 #3 */
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}
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static double pom(time_t tmpt)
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{
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struct tm *GMT;
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double days;
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int cnt;
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GMT = gmtime(&tmpt);
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days = (GMT->tm_yday + 1) + ((GMT->tm_hour + (GMT->tm_min / 60.0) +
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(GMT->tm_sec / 3600.0)) / 24.0);
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for (cnt = EPOCH; cnt < GMT->tm_year; ++cnt)
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days += ISLEAP(cnt + TM_YEAR_BASE) ? 366 : 365;
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/* Selected time could be before EPOCH */
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for (cnt = GMT->tm_year; cnt < EPOCH; ++cnt)
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days -= ISLEAP(cnt + TM_YEAR_BASE) ? 366 : 365;
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return potm(days);
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}
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/*
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* Return a pictogram representing the current phase of the moon.
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* Careful: date is the selected day in calendar at 00:00,
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* and so represents the phase of the moon at midnight.
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*/
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const char *ui_calendar_get_pom(time_t date)
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{
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const char *pom_pict[MOON_PHASES] =
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{ " ", "|) ", "(|)", "(| ", " | " };
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enum pom phase = NO_POM;
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const double half = 50.0;
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date += DAYINSEC / 2; /* adjust to noon */
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double pom_n_b = pom(date - DAYINSEC); /* noon before */
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double pom_m_b = pom(date - DAYINSEC / 2); /* midnight before */
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double pom_n = pom(date); /* noon */
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double pom_m_a = pom(date + DAYINSEC / 2); /* midnight after */
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double pom_n_a = pom(date + DAYINSEC); /* noon after */
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if (pom_n > pom_n_b && pom_n > pom_n_a)
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phase = FULL_MOON;
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else if (pom_n < pom_n_b && pom_n < pom_n_a)
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phase = NEW_MOON;
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else if (pom_m_b < half && half < pom_m_a)
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phase = FIRST_QUARTER;
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else if (pom_m_b > half && half > pom_m_a)
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phase = LAST_QUARTER;
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return pom_pict[phase];
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}
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@ -916,7 +916,6 @@ static char *fmt_day_heading(time_t date)
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localtime_r(&date, &tm);
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localtime_r(&date, &tm);
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string_init(&s);
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string_init(&s);
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string_printf(&s, "%s ", ui_calendar_get_pom(date));
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string_catftime(&s, conf.day_heading, &tm);
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string_catftime(&s, conf.day_heading, &tm);
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return string_buf(&s);
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return string_buf(&s);
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}
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}
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@ -51,8 +51,6 @@
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#include "calcurse.h"
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#include "calcurse.h"
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#include "sha1.h"
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#include "sha1.h"
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#define ISLEAP(y) ((((y) % 4) == 0 && ((y) % 100) != 0) || ((y) % 400) == 0)
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#define FS_EXT_MAXLEN 64
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#define FS_EXT_MAXLEN 64
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enum format_specifier {
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enum format_specifier {
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