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movement: add sunrise/sunset face

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Joey Castillo 2022-01-15 19:21:39 -05:00
parent 41eaa9c1c0
commit baf25aaa7a
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326
movement/lib/sunriset/sunriset.c Normal file
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/*
SUNRISET.C - computes Sun rise/set times, start/end of twilight, and
the length of the day at any date and latitude
Written as DAYLEN.C, 1989-08-16
Modified to SUNRISET.C, 1992-12-01
(c) Paul Schlyter, 1989, 1992
Released to the public domain by Paul Schlyter, December 1992
*/
#include <stdio.h>
#include <math.h>
#include "sunriset.h"
/* A macro to compute the number of days elapsed since 2000 Jan 0.0 */
/* (which is equal to 1999 Dec 31, 0h UT) */
#define days_since_2000_Jan_0(y,m,d) \
(367L*(y)-((7*((y)+(((m)+9)/12)))/4)+((275*(m))/9)+(d)-730530L)
/* Some conversion factors between radians and degrees */
#ifndef PI
#define PI 3.1415926535897932384
#endif
#define RADEG ( 180.0 / PI )
#define DEGRAD ( PI / 180.0 )
/* The trigonometric functions in degrees */
#define sind(x) sin((x)*DEGRAD)
#define cosd(x) cos((x)*DEGRAD)
#define tand(x) tan((x)*DEGRAD)
#define atand(x) (RADEG*atan(x))
#define asind(x) (RADEG*asin(x))
#define acosd(x) (RADEG*acos(x))
#define atan2d(y,x) (RADEG*atan2(y,x))
/* The "workhorse" function for sun rise/set times */
int __sunriset__( int year, int month, int day, double lon, double lat,
double altit, int upper_limb, double *trise, double *tset )
/***************************************************************************/
/* Note: year,month,date = calendar date, 1801-2099 only. */
/* Eastern longitude positive, Western longitude negative */
/* Northern latitude positive, Southern latitude negative */
/* The longitude value IS critical in this function! */
/* altit = the altitude which the Sun should cross */
/* Set to -35/60 degrees for rise/set, -6 degrees */
/* for civil, -12 degrees for nautical and -18 */
/* degrees for astronomical twilight. */
/* upper_limb: non-zero -> upper limb, zero -> center */
/* Set to non-zero (e.g. 1) when computing rise/set */
/* times, and to zero when computing start/end of */
/* twilight. */
/* *rise = where to store the rise time */
/* *set = where to store the set time */
/* Both times are relative to the specified altitude, */
/* and thus this function can be used to compute */
/* various twilight times, as well as rise/set times */
/* Return value: 0 = sun rises/sets this day, times stored at */
/* *trise and *tset. */
/* +1 = sun above the specified "horizon" 24 hours. */
/* *trise set to time when the sun is at south, */
/* minus 12 hours while *tset is set to the south */
/* time plus 12 hours. "Day" length = 24 hours */
/* -1 = sun is below the specified "horizon" 24 hours */
/* "Day" length = 0 hours, *trise and *tset are */
/* both set to the time when the sun is at south. */
/* */
/**********************************************************************/
{
double d, /* Days since 2000 Jan 0.0 (negative before) */
sr, /* Solar distance, astronomical units */
sRA, /* Sun's Right Ascension */
sdec, /* Sun's declination */
sradius, /* Sun's apparent radius */
t, /* Diurnal arc */
tsouth, /* Time when Sun is at south */
sidtime; /* Local sidereal time */
int rc = 0; /* Return cde from function - usually 0 */
/* Compute d of 12h local mean solar time */
d = days_since_2000_Jan_0(year,month,day) + 0.5 - lon/360.0;
/* Compute the local sidereal time of this moment */
sidtime = revolution( GMST0(d) + 180.0 + lon );
/* Compute Sun's RA, Decl and distance at this moment */
sun_RA_dec( d, &sRA, &sdec, &sr );
/* Compute time when Sun is at south - in hours UT */
tsouth = 12.0 - rev180(sidtime - sRA)/15.0;
/* Compute the Sun's apparent radius in degrees */
sradius = 0.2666 / sr;
/* Do correction to upper limb, if necessary */
if ( upper_limb )
altit -= sradius;
/* Compute the diurnal arc that the Sun traverses to reach */
/* the specified altitude altit: */
{
double cost;
cost = ( sind(altit) - sind(lat) * sind(sdec) ) /
( cosd(lat) * cosd(sdec) );
if ( cost >= 1.0 )
rc = -1, t = 0.0; /* Sun always below altit */
else if ( cost <= -1.0 )
rc = +1, t = 12.0; /* Sun always above altit */
else
t = acosd(cost)/15.0; /* The diurnal arc, hours */
}
/* Store rise and set times - in hours UT */
*trise = tsouth - t;
*tset = tsouth + t;
return rc;
} /* __sunriset__ */
/* The "workhorse" function */
double __daylen__( int year, int month, int day, double lon, double lat,
double altit, int upper_limb )
/**********************************************************************/
/* Note: year,month,date = calendar date, 1801-2099 only. */
/* Eastern longitude positive, Western longitude negative */
/* Northern latitude positive, Southern latitude negative */
/* The longitude value is not critical. Set it to the correct */
/* longitude if you're picky, otherwise set to to, say, 0.0 */
/* The latitude however IS critical - be sure to get it correct */
/* altit = the altitude which the Sun should cross */
/* Set to -35/60 degrees for rise/set, -6 degrees */
/* for civil, -12 degrees for nautical and -18 */
/* degrees for astronomical twilight. */
/* upper_limb: non-zero -> upper limb, zero -> center */
/* Set to non-zero (e.g. 1) when computing day length */
/* and to zero when computing day+twilight length. */
/**********************************************************************/
{
double d, /* Days since 2000 Jan 0.0 (negative before) */
obl_ecl, /* Obliquity (inclination) of Earth's axis */
sr, /* Solar distance, astronomical units */
slon, /* True solar longitude */
sin_sdecl, /* Sine of Sun's declination */
cos_sdecl, /* Cosine of Sun's declination */
sradius, /* Sun's apparent radius */
t; /* Diurnal arc */
/* Compute d of 12h local mean solar time */
d = days_since_2000_Jan_0(year,month,day) + 0.5 - lon/360.0;
/* Compute obliquity of ecliptic (inclination of Earth's axis) */
obl_ecl = 23.4393 - 3.563E-7 * d;
/* Compute Sun's ecliptic longitude and distance */
sunpos( d, &slon, &sr );
/* Compute sine and cosine of Sun's declination */
sin_sdecl = sind(obl_ecl) * sind(slon);
cos_sdecl = sqrt( 1.0 - sin_sdecl * sin_sdecl );
/* Compute the Sun's apparent radius, degrees */
sradius = 0.2666 / sr;
/* Do correction to upper limb, if necessary */
if ( upper_limb )
altit -= sradius;
/* Compute the diurnal arc that the Sun traverses to reach */
/* the specified altitude altit: */
{
double cost;
cost = ( sind(altit) - sind(lat) * sin_sdecl ) /
( cosd(lat) * cos_sdecl );
if ( cost >= 1.0 )
t = 0.0; /* Sun always below altit */
else if ( cost <= -1.0 )
t = 24.0; /* Sun always above altit */
else t = (2.0/15.0) * acosd(cost); /* The diurnal arc, hours */
}
return t;
} /* __daylen__ */
/* This function computes the Sun's position at any instant */
void sunpos( double d, double *lon, double *r )
/******************************************************/
/* Computes the Sun's ecliptic longitude and distance */
/* at an instant given in d, number of days since */
/* 2000 Jan 0.0. The Sun's ecliptic latitude is not */
/* computed, since it's always very near 0. */
/******************************************************/
{
double M, /* Mean anomaly of the Sun */
w, /* Mean longitude of perihelion */
/* Note: Sun's mean longitude = M + w */
e, /* Eccentricity of Earth's orbit */
E, /* Eccentric anomaly */
x, y, /* x, y coordinates in orbit */
v; /* True anomaly */
/* Compute mean elements */
M = revolution( 356.0470 + 0.9856002585 * d );
w = 282.9404 + 4.70935E-5 * d;
e = 0.016709 - 1.151E-9 * d;
/* Compute true longitude and radius vector */
E = M + e * RADEG * sind(M) * ( 1.0 + e * cosd(M) );
x = cosd(E) - e;
y = sqrt( 1.0 - e*e ) * sind(E);
*r = sqrt( x*x + y*y ); /* Solar distance */
v = atan2d( y, x ); /* True anomaly */
*lon = v + w; /* True solar longitude */
if ( *lon >= 360.0 )
*lon -= 360.0; /* Make it 0..360 degrees */
}
void sun_RA_dec( double d, double *RA, double *dec, double *r )
/******************************************************/
/* Computes the Sun's equatorial coordinates RA, Decl */
/* and also its distance, at an instant given in d, */
/* the number of days since 2000 Jan 0.0. */
/******************************************************/
{
double lon, obl_ecl, x, y, z;
/* Compute Sun's ecliptical coordinates */
sunpos( d, &lon, r );
/* Compute ecliptic rectangular coordinates (z=0) */
x = *r * cosd(lon);
y = *r * sind(lon);
/* Compute obliquity of ecliptic (inclination of Earth's axis) */
obl_ecl = 23.4393 - 3.563E-7 * d;
/* Convert to equatorial rectangular coordinates - x is unchanged */
z = y * sind(obl_ecl);
y = y * cosd(obl_ecl);
/* Convert to spherical coordinates */
*RA = atan2d( y, x );
*dec = atan2d( z, sqrt(x*x + y*y) );
} /* sun_RA_dec */
/******************************************************************/
/* This function reduces any angle to within the first revolution */
/* by subtracting or adding even multiples of 360.0 until the */
/* result is >= 0.0 and < 360.0 */
/******************************************************************/
#define INV360 ( 1.0 / 360.0 )
double revolution( double x )
/*****************************************/
/* Reduce angle to within 0..360 degrees */
/*****************************************/
{
return( x - 360.0 * floor( x * INV360 ) );
} /* revolution */
double rev180( double x )
/*********************************************/
/* Reduce angle to within +180..+180 degrees */
/*********************************************/
{
return( x - 360.0 * floor( x * INV360 + 0.5 ) );
} /* revolution */
/*******************************************************************/
/* This function computes GMST0, the Greenwich Mean Sidereal Time */
/* at 0h UT (i.e. the sidereal time at the Greenwhich meridian at */
/* 0h UT). GMST is then the sidereal time at Greenwich at any */
/* time of the day. I've generalized GMST0 as well, and define it */
/* as: GMST0 = GMST - UT -- this allows GMST0 to be computed at */
/* other times than 0h UT as well. While this sounds somewhat */
/* contradictory, it is very practical: instead of computing */
/* GMST like: */
/* */
/* GMST = (GMST0) + UT * (366.2422/365.2422) */
/* */
/* where (GMST0) is the GMST last time UT was 0 hours, one simply */
/* computes: */
/* */
/* GMST = GMST0 + UT */
/* */
/* where GMST0 is the GMST "at 0h UT" but at the current moment! */
/* Defined in this way, GMST0 will increase with about 4 min a */
/* day. It also happens that GMST0 (in degrees, 1 hr = 15 degr) */
/* is equal to the Sun's mean longitude plus/minus 180 degrees! */
/* (if we neglect aberration, which amounts to 20 seconds of arc */
/* or 1.33 seconds of time) */
/* */
/*******************************************************************/
double GMST0( double d )
{
double sidtim0;
/* Sidtime at 0h UT = L (Sun's mean longitude) + 180.0 degr */
/* L = M + w, as defined in sunpos(). Since I'm too lazy to */
/* add these numbers, I'll let the C compiler do it for me. */
/* Any decent C compiler will add the constants at compile */
/* time, imposing no runtime or code overhead. */
sidtim0 = revolution( ( 180.0 + 356.0470 + 282.9404 ) +
( 0.9856002585 + 4.70935E-5 ) * d );
return sidtim0;
} /* GMST0 */

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movement/lib/sunriset/sunriset.h Normal file
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/*
SUNRISET.H - computes Sun rise/set times, start/end of twilight, and
the length of the day at any date and latitude
Written as DAYLEN.C, 1989-08-16
Modified to SUNRISET.C, 1992-12-01
(c) Paul Schlyter, 1989, 1992
Released to the public domain by Paul Schlyter, December 1992
*/
#ifndef SUNRISET_H_
#define SUNRISET_H_
/* Function prototypes */
double __daylen__( int year, int month, int day, double lon, double lat,
double altit, int upper_limb );
int __sunriset__( int year, int month, int day, double lon, double lat,
double altit, int upper_limb, double *rise, double *set );
void sunpos( double d, double *lon, double *r );
void sun_RA_dec( double d, double *RA, double *dec, double *r );
double revolution( double x );
double rev180( double x );
double GMST0( double d );
/* Following are some macros around the "workhorse" function __daylen__ */
/* They mainly fill in the desired values for the reference altitude */
/* below the horizon, and also selects whether this altitude should */
/* refer to the Sun's center or its upper limb. */
/* This macro computes the length of the day, from sunrise to sunset. */
/* Sunrise/set is considered to occur when the Sun's upper limb is */
/* 35 arc minutes below the horizon (this accounts for the refraction */
/* of the Earth's atmosphere). */
#define day_length(year,month,day,lon,lat) \
__daylen__( year, month, day, lon, lat, -35.0/60.0, 1 )
/* This macro computes the length of the day, including civil twilight. */
/* Civil twilight starts/ends when the Sun's center is 6 degrees below */
/* the horizon. */
#define day_civil_twilight_length(year,month,day,lon,lat) \
__daylen__( year, month, day, lon, lat, -6.0, 0 )
/* This macro computes the length of the day, incl. nautical twilight. */
/* Nautical twilight starts/ends when the Sun's center is 12 degrees */
/* below the horizon. */
#define day_nautical_twilight_length(year,month,day,lon,lat) \
__daylen__( year, month, day, lon, lat, -12.0, 0 )
/* This macro computes the length of the day, incl. astronomical twilight. */
/* Astronomical twilight starts/ends when the Sun's center is 18 degrees */
/* below the horizon. */
#define day_astronomical_twilight_length(year,month,day,lon,lat) \
__daylen__( year, month, day, lon, lat, -18.0, 0 )
/* This macro computes times for sunrise/sunset. */
/* Sunrise/set is considered to occur when the Sun's upper limb is */
/* 35 arc minutes below the horizon (this accounts for the refraction */
/* of the Earth's atmosphere). */
#define sun_rise_set(year,month,day,lon,lat,rise,set) \
__sunriset__( year, month, day, lon, lat, -35.0/60.0, 1, rise, set )
/* This macro computes the start and end times of civil twilight. */
/* Civil twilight starts/ends when the Sun's center is 6 degrees below */
/* the horizon. */
#define civil_twilight(year,month,day,lon,lat,start,end) \
__sunriset__( year, month, day, lon, lat, -6.0, 0, start, end )
/* This macro computes the start and end times of nautical twilight. */
/* Nautical twilight starts/ends when the Sun's center is 12 degrees */
/* below the horizon. */
#define nautical_twilight(year,month,day,lon,lat,start,end) \
__sunriset__( year, month, day, lon, lat, -12.0, 0, start, end )
/* This macro computes the start and end times of astronomical twilight. */
/* Astronomical twilight starts/ends when the Sun's center is 18 degrees */
/* below the horizon. */
#define astronomical_twilight(year,month,day,lon,lat,start,end) \
__sunriset__( year, month, day, lon, lat, -18.0, 0, start, end )
#endif // SUNRISET_H_

3
movement/make/Makefile
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@ -17,6 +17,7 @@ INCLUDES += \
-I../watch_faces/thermistor/ \
-I../watch_faces/demos/ \
-I../lib/TOTP-MCU/ \
-I../lib/sunriset/ \
# If you add any other source files you wish to compile, add them after ../app.c
# Note that you will need to add a backslash at the end of any line you wish to continue, i.e.
@ -27,6 +28,7 @@ INCLUDES += \
SRCS += \
../lib/TOTP-MCU/sha1.c \
../lib/TOTP-MCU/TOTP.c \
../lib/sunriset/sunriset.c \
../movement.c \
../watch_faces/clock/simple_clock_face.c \
../watch_faces/clock/world_clock_face.c \
@ -45,6 +47,7 @@ SRCS += \
../watch_faces/complications/day_one_face.c \
../watch_faces/complications/stopwatch_face.c \
../watch_faces/complications/totp_face.c \
../watch_faces/complications/sunrise_sunset_face.c \
# Leave this line at the bottom of the file; it has all the targets for making your project.
include $(TOP)/rules.mk

1
movement/movement_config.h
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@ -41,6 +41,7 @@
#include "lis2dh_logging_face.h"
#include "demo_face.h"
#include "hello_there_face.h"
#include "sunrise_sunset_face.h"
const watch_face_t watch_faces[] = {
simple_clock_face,

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movement/watch_faces/complications/sunrise_sunset_face.c Normal file
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/*
* MIT License
*
* Copyright (c) 2022 Joey Castillo
*
* Permission is hereby granted, free of charge, to any person obtaining a copy
* of this software and associated documentation files (the "Software"), to deal
* in the Software without restriction, including without limitation the rights
* to use, copy, modify, merge, publish, distribute, sublicense, and/or sell
* copies of the Software, and to permit persons to whom the Software is
* furnished to do so, subject to the following conditions:
*
* The above copyright notice and this permission notice shall be included in all
* copies or substantial portions of the Software.
*
* THE SOFTWARE IS PROVIDED "AS IS", WITHOUT WARRANTY OF ANY KIND, EXPRESS OR
* IMPLIED, INCLUDING BUT NOT LIMITED TO THE WARRANTIES OF MERCHANTABILITY,
* FITNESS FOR A PARTICULAR PURPOSE AND NONINFRINGEMENT. IN NO EVENT SHALL THE
* AUTHORS OR COPYRIGHT HOLDERS BE LIABLE FOR ANY CLAIM, DAMAGES OR OTHER
* LIABILITY, WHETHER IN AN ACTION OF CONTRACT, TORT OR OTHERWISE, ARISING FROM,
* OUT OF OR IN CONNECTION WITH THE SOFTWARE OR THE USE OR OTHER DEALINGS IN THE
* SOFTWARE.
*
* Sunrise/sunset calculations are public domain code by Paul Schlyter, December 1992
*
*/
#include <stdlib.h>
#include <string.h>
#include <math.h>
#include "sunrise_sunset_face.h"
#include "watch.h"
#include "watch_utility.h"
#include "sunriset.h"
static void _sunrise_sunset_face_update() {
char buf[14];
double rise, set, minutes;
// TODO: allow user to set location, using London for now.
double lat = 51.509865;
double lon = -0.118092;
// TODO: account for time zone, currently only operates in GMT.
watch_date_time date_time = watch_rtc_get_date_time(); // the current date / time
watch_date_time scratch_time; // scratchpad, contains different values at different times
scratch_time.reg = date_time.reg;
for(int i = 0; i < 2; i++) {
uint8_t result = sun_rise_set(scratch_time.unit.year + WATCH_RTC_REFERENCE_YEAR, scratch_time.unit.month, scratch_time.unit.day, lon, lat, &rise, &set);
if (result != 0) {
watch_clear_colon();
watch_clear_indicator(WATCH_INDICATOR_PM);
watch_clear_indicator(WATCH_INDICATOR_24H);
sprintf(buf, "%s%d none ", (result == 1) ? "SE" : "rI", scratch_time.unit.day);
watch_display_string(buf, 0);
return;
}
watch_set_colon();
// TODO: account for user's 12H/24H preference
watch_set_indicator(WATCH_INDICATOR_24H);
minutes = 60.0 * fmod(rise, 1);
scratch_time.unit.hour = floor(rise);
scratch_time.unit.minute = floor(minutes);
scratch_time.unit.second = 60.0 * fmod(minutes, 1);
if (date_time.reg < scratch_time.reg) {
// display today's sunrise, it hasn't happened yet
sprintf(buf, "rI%2d%2d%02d%02d", scratch_time.unit.day, scratch_time.unit.hour, scratch_time.unit.minute, scratch_time.unit.second);
watch_display_string(buf, 0);
return;
}
minutes = 60.0 * fmod(set, 1);
scratch_time.unit.hour = floor(set);
scratch_time.unit.minute = floor(minutes);
scratch_time.unit.second = 60.0 * fmod(minutes, 1);
if (date_time.reg < scratch_time.reg) {
// display today's sunset, it hasn't happened yet
sprintf(buf, "SE%2d%02d%02d%02d", scratch_time.unit.day, scratch_time.unit.hour, scratch_time.unit.minute, scratch_time.unit.second);
watch_display_string(buf, 0);
return;
}
// it's after sunset. we need to display sunrise for tomorrow.
uint32_t timestamp = watch_utility_date_time_to_unix_time(date_time, 0);
timestamp += 86400;
scratch_time = watch_utility_date_time_from_unix_time(timestamp, 0);
}
}
void sunrise_sunset_face_setup(movement_settings_t *settings, uint8_t watch_face_index, void ** context_ptr) {
(void) settings;
(void) watch_face_index;
if (*context_ptr == NULL) {
*context_ptr = malloc(sizeof(sunrise_sunset_state_t));
memset(*context_ptr, 0, sizeof(sunrise_sunset_state_t));
}
}
void sunrise_sunset_face_activate(movement_settings_t *settings, void *context) {
(void) settings;
sunrise_sunset_state_t *state = (sunrise_sunset_state_t *)context;
movement_location_t movement_location = (movement_location_t) watch_get_backup_data(1);
state->latitude = movement_location.bit.latitude;
state->longitude = movement_location.bit.longitude;
}
bool sunrise_sunset_face_loop(movement_event_t event, movement_settings_t *settings, void *context) {
(void) settings;
(void) context;
switch (event.event_type) {
case EVENT_ACTIVATE:
break;
case EVENT_LOW_ENERGY_UPDATE:
case EVENT_TICK:
_sunrise_sunset_face_update();
break;
case EVENT_MODE_BUTTON_UP:
movement_move_to_next_face();
break;
case EVENT_LIGHT_BUTTON_DOWN:
movement_illuminate_led();
break;
case EVENT_LIGHT_BUTTON_UP:
break;
case EVENT_ALARM_BUTTON_UP:
break;
case EVENT_ALARM_LONG_PRESS:
// TODO: settings mode, to set the user's location.
break;
case EVENT_TIMEOUT:
// TODO: return home if we're on a settings page.
default:
break;
}
return true;
}
void sunrise_sunset_face_resign(movement_settings_t *settings, void *context) {
(void) settings;
(void) context;
movement_request_tick_frequency(1);
}

51
movement/watch_faces/complications/sunrise_sunset_face.h Normal file
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@ -0,0 +1,51 @@
/*
* MIT License
*
* Copyright (c) 2022 Joey Castillo
*
* Permission is hereby granted, free of charge, to any person obtaining a copy
* of this software and associated documentation files (the "Software"), to deal
* in the Software without restriction, including without limitation the rights
* to use, copy, modify, merge, publish, distribute, sublicense, and/or sell
* copies of the Software, and to permit persons to whom the Software is
* furnished to do so, subject to the following conditions:
*
* The above copyright notice and this permission notice shall be included in all
* copies or substantial portions of the Software.
*
* THE SOFTWARE IS PROVIDED "AS IS", WITHOUT WARRANTY OF ANY KIND, EXPRESS OR
* IMPLIED, INCLUDING BUT NOT LIMITED TO THE WARRANTIES OF MERCHANTABILITY,
* FITNESS FOR A PARTICULAR PURPOSE AND NONINFRINGEMENT. IN NO EVENT SHALL THE
* AUTHORS OR COPYRIGHT HOLDERS BE LIABLE FOR ANY CLAIM, DAMAGES OR OTHER
* LIABILITY, WHETHER IN AN ACTION OF CONTRACT, TORT OR OTHERWISE, ARISING FROM,
* OUT OF OR IN CONNECTION WITH THE SOFTWARE OR THE USE OR OTHER DEALINGS IN THE
* SOFTWARE.
*/
#ifndef SUNRISE_SUNSET_FACE_H_
#define SUNRISE_SUNSET_FACE_H_
#include "movement.h"
// The Day One face is designed to count upwards from the wearer's date of birth. It also functions as an
// interface for setting the birth date register, which other watch faces can use for various purposes.
typedef struct {
uint16_t latitude;
uint16_t longitude;
} sunrise_sunset_state_t;
void sunrise_sunset_face_setup(movement_settings_t *settings, uint8_t watch_face_index, void ** context_ptr);
void sunrise_sunset_face_activate(movement_settings_t *settings, void *context);
bool sunrise_sunset_face_loop(movement_event_t event, movement_settings_t *settings, void *context);
void sunrise_sunset_face_resign(movement_settings_t *settings, void *context);
static const watch_face_t sunrise_sunset_face = {
sunrise_sunset_face_setup,
sunrise_sunset_face_activate,
sunrise_sunset_face_loop,
sunrise_sunset_face_resign,
NULL
};
#endif // SUNRISE_SUNSET_FACE_H_