Provided by: libdatetime-event-sunrise-perl_0.0505-1_all 
NAME
DateTime::Event::Sunrise - Perl DateTime extension for computing the sunrise/sunset on a
given day
SYNOPSIS
use DateTime;
use DateTime::Event::Sunrise;
# generating DateTime objects from a DateTime::Event::Sunrise object
my $sun_Kyiv = DateTime::Event::Sunrise->new(longitude => +30.85, # 30X51'E
latitude => +50.45); # 50X27'N
for (12, 13, 14) {
my $dt_yapc_eu = DateTime->new(year => 2013,
month => 8,
day => $_,
time_zone => 'Europe/Kiev');
say "In Kyiv (50X27'N, 30X51'E) on ", $dt_yapc_eu->ymd, " sunrise occurs at ", $sun_Kyiv->sunrise_datetime($dt_yapc_eu)->hms,
" and sunset occurs at ", $sun_Kyiv->sunset_datetime ($dt_yapc_eu)->hms;
}
# generating DateTime objects from DateTime::Set objects
my $sunrise_Austin = DateTime::Event::Sunrise->sunrise(longitude => -94.73, # 97X44'W
latitude => +30.3); # 30X18'N
my $sunset_Austin = DateTime::Event::Sunrise->sunset (longitude => -94.73,
latitude => +30.3);
my $dt_yapc_na_rise = DateTime->new(year => 2013,
month => 6,
day => 3,
time_zone => 'America/Chicago');
my $dt_yapc_na_set = $dt_yapc_na_rise->clone;
say "In Austin (30X18'N, 97X44'W), sunrises and sunsets are";
for (1..3) {
$dt_yapc_na_rise = $sunrise_Austin->next($dt_yapc_na_rise);
$dt_yapc_na_set = $sunset_Austin ->next($dt_yapc_na_set);
say $dt_yapc_na_rise, ' ', $dt_yapc_na_set;
}
# If you deal with a polar location
my $sun_in_Halley = DateTime::Event::Sunrise->new(
longitude => -26.65, # 26X39'W
latitude => -75.58, # 75X35'S
precise => 1,
);
my $Alex_arrival = DateTime->new(year => 2006, # approximate date, not necessarily the exact one
month => 1,
day => 15,
time_zone => 'Antarctica/Rothera');
say $Alex_arrival->strftime("Alex Gough (a Perl programmer) arrived at Halley Base on %Y-%m-%d.");
if ($sun_in_Halley->is_polar_day($Alex_arrival)) {
say "It would be days, maybe weeks, before the sun would set.";
}
elsif ($sun_in_Halley->is_polar_night($Alex_arrival)) {
say "It would be days, maybe weeks, before the sun would rise.";
}
else {
my $sunset = $sun_in_Halley->sunset_datetime($Alex_arrival);
say $sunset->strftime("And he saw his first antarctic sunset at %H:%M:%S.");
}
DESCRIPTION
This module will computes the time of sunrise and sunset for a given date and a given
location. The computation uses Paul Schlyter's algorithm.
Actually, the module creates a DateTime::Event::Sunrise object or a DateTime::Set object,
which are used to generate the sunrise or the sunset times for a given location and for
any date.
METHODS
new
This is the DateTime::Event::Sunrise constructor. It takes keyword parameters, which are:
longitude
This is the longitude of the location where the sunrises and sunsets are observed. It
is given as decimal degrees: no minutes, no seconds, but tenths and hundredths of
degrees. Another break with the normal usage is that Eastern longitude are positive,
Western longitudes are negative.
Default value is 0, that is Greenwich or any location on the eponymous meridian.
latitude
This is the latitude of the location where the sunrises and sunsets are observed. As
for the longitude, it is given as decimal degrees. Northern latitudes are positive
numbers, Southern latitudes are negative numbers.
Default value is 0, that is any location on the equator.
altitude
This is the height of the Sun at sunrise or sunset. In astronomical context, the
altitude or height is the angle between the Sun and the local horizon. It is expressed
as degrees, usually with a negative number, since the Sun is below the horizon.
Default value is -0.833, that is when the sun's upper limb touches the horizon, while
taking in account the light refraction.
Positive altitude are allowed, in case the location is near a mountain range behind
which the sun rises or sets.
precise
Boolean to control which algorithm is used. A false value gives a simple algorithm,
but which can lead to inaccurate sunrise times and sunset times. A true value gives a
more elaborate algorithm, with a loop to refine the sunrise and sunset times and
obtain a better precision.
Default value is 0, to choose the simple algorithm.
This parameter replaces the "iteration" deprecated parameter.
upper_limb
Boolean to choose between checking the Sun's upper limb or its center. A true value
selects the upper limb, a false value selects the center.
This parameter is significant only when the altitude does not already deal with the
sun radius. When the altitude takes into account the sun radius, this parameter
should be false.
Default value is 0, since the upper limb correction is already taken in account with
the default -0.833 altitude.
silent
Boolean to control the output of some warning messages. With polar locations and
dates near the winter solstice or the summer solstice, it may happen that the sun
never rises above the horizon or never sets below. If this parameter is set to false,
the module will send warnings for these conditions. If this parameter is set to true,
the module will not pollute your STDERR stream.
Default value is 0, for backward compatibility.
sunrise, sunset
Although they come from the DateTime::Event::Sunrise module, these methods are
"DateTime::Set" constructors. They use the same parameters as the "new" constructor, but
they give objects from a different class.
sunrise_datetime, sunset_datetime
These two methods apply to "DateTime::Event::Sunrise" objects (that is, created with
"new", not "sunrise" or "sunset"). They receive one parameter in addition to $self, a
"DateTime" object. They return another "DateTime" object, for the same day, but with the
time of the sunrise or sunset, respectively.
sunrise_sunset_span
This method applies to "DateTime::Event::Sunrise" objects. It accepts a "DateTime" object
as the second parameter. It returns a "DateTime::Span" object, beginning at sunrise and
ending at sunset.
is_polar_night, is_polar_day, is_day_and_night
These methods apply to "DateTime::Event::Sunrise" objects. They accept a "DateTime" object
as the second parameter. They return a boolean indicating the following condutions:
• is_polar_night is true when the sun stays under the horizon. Or rather under the
altitude parameter used when the "DateTime::Event::Sunrise" object was created.
• is_polar_day is true when the sun stays above the horizon, resulting in a "Midnight
sun". Or rather when it stays above the altitude parameter used when the
"DateTime::Event::Sunrise" object was created.
• is_day_and_night is true when neither is_polar_day, nor is_polar_night are true.
next current previous contains as_list iterator
See DateTime::Set.
EXTENDED EXAMPLES
my $dt = DateTime->new( year => 2000,
month => 6,
day => 20,
);
my $sunrise = DateTime::Event::Sunrise ->sunrise (
longitude =>'-118',
latitude =>'33',
altitude => '-0.833',
precise => '1'
);
my $sunset = DateTime::Event::Sunrise ->sunset (
longitude =>'-118',
latitude =>'33',
altitude => '-0.833',
precise => '1'
);
my $tmp_rise = $sunrise->next( $dt );
my $dt2 = DateTime->new( year => 2000,
month => 12,
day => 31,
);
# iterator
my $dt_span = DateTime::Span->new( start =>$dt, end=>$dt2 );
my $set = $sunrise->intersection($dt_span);
my $iter = $set->iterator;
while ( my $dt = $iter->next ) {
print ' ',$dt->datetime;
}
# is it day or night?
my $day_set = DateTime::SpanSet->from_sets(
start_set => $sunrise, end_set => $sunset );
print $day_set->contains( $dt ) ? 'day' : 'night';
my $dt = DateTime->new( year => 2000,
month => 6,
day => 20,
time_zone => 'America/Los_Angeles',
);
my $sunrise = DateTime::Event::Sunrise ->new(
longitude =>'-118' ,
latitude => '33',
altitude => '-0.833',
precise => '1'
);
my $tmp = $sunrise->sunrise_sunset_span($dt);
print "Sunrise is:" , $tmp->start->datetime , "\n";
print "Sunset is:" , $tmp->end->datetime;
NOTES
Longitude Signs
Remember, contrary to the usual convention,
EASTERN longitudes are POSITIVE,
WESTERN longitudes are NEGATIVE.
On the other hand, the latitude signs follow the usual convention:
Northen latitudes are positive,
Southern latitudes are negative.
Sun Height
There are a number of sun heights to choose from. The default is -0.833 because this is
what most countries use. Feel free to specify it if you need to. Here is the list of
values to specify the sun height with:
• 0 degrees
Center of Sun's disk touches a mathematical horizon
• -0.25 degrees
Sun's upper limb touches a mathematical horizon
• -0.583 degrees
Center of Sun's disk touches the horizon; atmospheric refraction accounted for
• -0.833 degrees
Sun's supper limb touches the horizon; atmospheric refraction accounted for
• -6 degrees
Civil twilight (one can no longer read outside without artificial illumination)
• -12 degrees
Nautical twilight (navigation using a sea horizon no longer possible)
• -15 degrees
Amateur astronomical twilight (the sky is dark enough for most astronomical
observations)
• -18 degrees
Astronomical twilight (the sky is completely dark)
Notes on the Precise Algorithm
The original method only gives an approximate value of the Sun's rise/set times. The
error rarely exceeds one or two minutes, but at high latitudes, when the Midnight Sun soon
will start or just has ended, the errors may be much larger. If you want higher accuracy,
you must then select the precise variant of the algorithm. This feature is new as of
version 0.7. Here is what I have tried to accomplish with this.
a) Compute sunrise or sunset as always, with one exception: to convert LHA from degrees
to hours, divide by 15.04107 instead of 15.0 (this accounts for the difference between
the solar day and the sidereal day.
b) Re-do the computation but compute the Sun's RA and Decl, and also GMST0, for the
moment of sunrise or sunset last computed.
c) Iterate b) until the computed sunrise or sunset no longer changes significantly.
Usually 2 iterations are enough, in rare cases 3 or 4 iterations may be needed.
Notes on polar locations
If the location is beyond either polar circle, and if the date is near either solstice,
there can be midnight sun or polar night. In this case, there is neither sunrise nor
sunset, and the module "carp"s that the sun never rises or never sets. Then, it returns
the time at which the sun is at its highest or lowest point.
DEPENDENCIES
This module requires:
• DateTime
• DateTime::Set
• DateTime::Span
• Params::Validate
• Set::Infinite
• POSIX
• Math::Trig
BUGS AND CAVEATS
Using a latitude of 90 degrees (North Pole or South Pole) gives curious results. I guess
that it is linked with a ambiguous value resulting from a 0/0 computation.
Using a longitude of 177 degrees, or any longitude near the 180 meridian, may also give
curious results, especially with the precise algorithm.
The precise algorithm should be overhauled.
AUTHORS
Original author: Ron Hill <rkhill@firstlight.net>
Co-maintainer: Jean Forget <JFORGET@cpan.org>
SPECIAL THANKS
Robert Creager [Astro-Sunrise@LogicalChaos.org]
for providing help with converting Paul's C code to perl.
Flavio S. Glock [fglock@pucrs.br]
for providing the the interface to the DateTime::Set module.
CREDITS
Paul Schlyter, Stockholm, Sweden
for his excellent web page on the subject.
Rich Bowen (rbowen@rbowen.com)
for suggestions.
People at <http://geocoder.opencagedata.com/>
for noticing an endless loop condition in Astro::Sunrise and for fixing it.
COPYRIGHT and LICENSE
Perl Module
This program is distributed under the same terms as Perl 5.16.3: GNU Public License
version 1 or later and Perl Artistic License
You can find the text of the licenses in the LICENSE file or at
<http://www.perlfoundation.org/artistic_license_1_0> and
<http://www.gnu.org/licenses/gpl-1.0.html>.
Here is the summary of GPL:
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 1, or (at your option) any later version.
This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY;
without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.
See the GNU General Public License for more details.
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.
Original C program
Here is the copyright information provided by Paul Schlyter for the original C program:
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
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 AUTHOR 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.
SEE ALSO
perl(1).
DateTime Web page at http://datetime.perl.org/
DateTime::Set
DateTime::SpanSet
Astro::Sunrise
DateTime::Event::Jewish::Sunrise
Paul Schlyter's homepage at http://stjarnhimlen.se/english.html