| Astro-satpass documentation | Contained in the Astro-satpass distribution. |
Astro::Coord::ECI::Utils - Utility routines for astronomical calculations
use Astro::Coord::ECI::Utils qw{:all};
my $now = time ();
print "The current Julian day is ", julianday ($now);
This module was written to provide a home for all the constants and utility subroutines used by Astro::Coord::ECI and its descendents. What ended up here was anything that was essentially a subroutine, not a method.
Because figuring out how to convert to and from Perl time bids fair to
become complicated, this module is also responsible for figuring out how
that is done, and exporting whatever is needful to export. See :time
below for the gory details.
This package exports nothing by default. But all the constants, variables, and subroutines documented below are exportable, and the following export tags may be used:
This imports everything exportable into your name space.
This imports the time routines into your name space. If
Time::y2038 is available, it will be loaded, and both
this tag and :all will import gmtime, localtime, timegm, and
timelocal into your name space. Otherwise, Time::Local|Time::Local
will be loaded, and both this tag and :all will import timegm and
timelocal into your name space.
Under Perl 5.6 you may find that, if you use any of the above tags, you need to specify them first in your import list.
AU = number of kilometers in an astronomical unit JD_OF_EPOCH = the Julian Day of Perl epoch 0 LIGHTYEAR = number of kilometers in a light year PARSEC = number of kilometers in a parsec PERL2000 = January 1 2000, 12 noon universal, in Perl time PI = the circle ratio, computed as atan2 (0, -1) PIOVER2 = half the circle ratio SECSPERDAY = the number of seconds in a day SECS_PER_SIDERIAL_DAY = seconds in a siderial day SPEED_OF_LIGHT = speed of light in kilometers per second TWOPI = twice the circle ratio
This variable represents the POSIX::strftime format used to convert times to strings. The default value is '%a %b %d %Y %H:%M:%S' to be consistent with the behavior of gmtime (or, to be precise, the behavior of ctime as documented on my system).
This variable represents the Julian Day of the switch from Julian to Gregorian calendars. This is used by date2jd(), jd2date(), and the routines which depend on them, for deciding whether the date is to be interpreted as in the Julian or Gregorian calendar. Its initial setting is 2299160.5, which represents midnight October 15 1582 in the Gregorian calendar, which is the date that calendar was first adopted. This is slightly different than the value of 2299161 (noon of the same day) used by Jean Meeus.
If you are interested in historical calculations, you may wish to reset this appropriately. If you use date2jd to calculate the new value, be aware of the effect the current setting of $JD_GREGORIAN has on the interpretation of the date you give.
This subroutine calculates the arc in radians whose cosine is the given value.
This subroutine calculates the arc in radians whose sine is the given value.
This subroutine calculates the typical atmospheric extinction in magnitudes at the given elevation above the horizon in radians and the given height above sea level in kilometers.
The algorithm comes from Daniel W. E. Green's article "Magnitude Corrections for Atmospheric Extinction", which was published in the July 1992 issue of "International Comet Quarterly", and is available online at http://www.cfa.harvard.edu/icq/ICQExtinct.html. The text of this article makes it clear that the actual value of the atmospheric extinction can vary greatly from the typical values given even in the absence of cloud cover.
This subroutine converts the given date to the corresponding Julian day. The inputs are as for Time::Local::timegm; $mon is in the range 0 - 11, and $yr is from 1900, with earlier years being negative. The year 1 BC is represented as -1900.
If less than 6 arguments are provided, zeroes will be prepended to the argument list as needed.
The date is presumed to be in the Gregorian calendar. If the resultant Julian Day is before $JD_GREGORIAN, the date is reinterpreted as being from the Julian calendar.
The only validation is that the month be between 0 and 11 inclusive, and that the year be not less than -6612 (4713 BC). Fractional days are accepted.
The algorithm is from Jean Meeus' "Astronomical Algorithms", second edition, chapter 7 ("Julian Day"), pages 60ff, but the month is zero-based, not 1-based, and years are 1900-based.
This is a convenience routine that converts the given date to seconds since the epoch, going through date2jd() to do so. The arguments are the same as those of date2jd().
If less than 6 arguments are provided, zeroes will be prepended to the argument list as needed.
The functionality is the same as Time::Local::timegm, but this function lacks timegm's limited date range. These days, though, Time::y2038::timegm may be preferred over this subroutine.
This subroutine converts degrees to radians.
This subroutine calculates the square of the distance between the two sets of Cartesian coordinates. We do not take the square root here because of cases (e.g. the law of cosines) where we would just have to square the result again.
Notice that the subroutine does not assume three-dimensional coordinates. If @coord1 and @coord2 have six entries, you will get a six-dimensional distance.
This method returns the difference between dynamical and universal time at the given universal time. That is,
$dynamical = $time + dynamical_delta ($time)
if $time is universal time.
The algorithm is from Jean Meeus' "Astronomical Algorithms", 2nd Edition, Chapter 10, page 78.
This subroutine represents a safe way to call the 'represents' method on $thingy. You get back true if and only if $thingy->can('represents') does not throw an exception and returns true, and $thingy->represents($class) returns true. Otherwise it returns false. Any exception is trapped and dismissed.
This subroutine is called 'embodies' because it was too confusing to call it 'represents', both for the author and for the Perl interpreter.
This convenience subroutine converts the given time in seconds from the system epoch to the corresponding date and time. It is implemented in terms of jd2date (), with the year and month returned from that subroutine. The day is a whole number, with the fractional part converted to hours, minutes, and seconds. The $wday is the day of the week, with Sunday being 0. The $yday is the day of the year, with January 1 being 0. The trailing 0 is the summer time (or daylight saving time) indicator which is always 0 to be consistent with gmtime.
If called in scalar context, it returns the date formatted by POSIX::strftime, using the format string in $DATETIMEFORMAT.
The functionality is similar to gmtime, but lacks gmtime's limited date range.
The input must convert to a non-negative Julian date. The exact lower limit depends on the system, but is computed by -(JD_OF_EPOCH * 86400). For Unix systems with an epoch of January 1 1970, this is -210866760000.
Additional algorithms for day of week and day of year come from Jean Meeus' "Astronomical Algorithms", 2nd Edition, Chapter 7 (Julian Day), page 65.
This method returns the equation of time at the given dynamical time.
The algorithm is from W. S. Smart's "Text-Book on Spherical Astronomy", as reported in Jean Meeus' "Astronomical Algorithms", 2nd Edition, Chapter 28, page 185.
This function finds the first time between $start and $end for which test ($time) is true. The resolution is $limit, which defaults to 1 if not specified. If the times are reversed (i.e. the start time is after the end time) the time returned is the last time test ($time) is true.
The test () function is assumed to be false for the first part of the interval, and true for the rest. If this assumption is violated, the result of this subroutine should be considered meaningless.
The calculation is done by, essentially, a binary search; the interval is repeatedly split, the function is evaluated at the midpoint, and a new interval selected based on whether the result is true or false.
Actually, nothing in this function says the independent variable has to be time.
This method converts a ratio of light intensities to a difference in stellar magnitudes. The algorithm comes from Jean Meeus' "Astronomical Algorithms", Second Edition, Chapter 56, Page 395.
Note that, because of the way magnitudes work (a more negative number represents a brighter star) you get back a positive result for an intensity ratio less than 1, and a negative result for an intensity ratio greater than 1.
This subroutine converts the given Julian day to the corresponding date. The returns are year - 1900, month (0 to 11), day (which may have a fractional part), a Gregorian calendar indicator which is true if the date is in the Gregorian calendar and false if it is in the Julian calendar, and a leap (or bissextile) year indicator which is true if the year is a leap year and false otherwise. The year 1 BC is returned as -1900 (i.e. as year 0), and so on. The date will probably have a fractional part (e.g. 2006 1 1.5 for noon January first 2006).
If the $jd is before $JD_GREGORIAN, the date will be in the Julian calendar; otherwise it will be in the Gregorian calendar.
The input may not be less than 0.
The algorithm is from Jean Meeus' "Astronomical Algorithms", second edition, chapter 7 ("Julian Day"), pages 63ff, but the month is zero-based, not 1-based, and the year is 1900-based.
This convenience subroutine converts the given Julian day to the corresponding date and time. All this really does is converts its argument to seconds since the system epoch, and pass off to epoch2datetime().
The input may not be less than 0.
Several of the algorithms in Jean Meeus' "Astronomical Algorithms" are expressed in terms of the number of Julian centuries from epoch J2000.0 (e.g equations 12.1, 22.1). This subroutine encapsulates that calculation.
This subroutine converts a Perl date to the number of Julian days (and fractions thereof) since Julian 2000.0. This quantity is used in a number of the algorithms in Jean Meeus' "Astronomical Algorithms".
The computation makes use of information from Jean Meeus' "Astronomical Algorithms", 2nd Edition, Chapter 7, page 62.
This subroutine converts a Perl date to a Julian day number.
The computation makes use of information from Jean Meeus' "Astronomical Algorithms", 2nd Edition, Chapter 7, page 62.
This convenience method loads the named module (using 'require'), throwing an exception if the load fails. If the load succeeds, it returns the result of the 'require' built-in, which is required to be true for a successful load. Results are cached, and subsequent attempts to load the same module simply give the cached results.
This subroutine returns true if the input looks like a number. It uses Scalar::Util::looks_like_number if that is available, otherwise it uses its own code, which is lifted verbatim from Scalar::Util 1.19, which in turn leans heavily on perlfaq4.
This subroutine returns the maximum of its arguments. If List::Util can be loaded and 'max' imported, that's what you get. Otherwise you get a pure Perl implementation.
This subroutine returns the minimum of its arguments. If List::Util can be loaded and 'min' imported, that's what you get. Otherwise you get a pure Perl implementation.
This subroutine reduces the given angle in radians to the range 0 <= $theta < TWOPI.
This subroutine calculates the nutation in longitude (delta psi) for the given dynamical time.
The algorithm comes from Jean Meeus' "Astronomical Algorithms", 2nd Edition, Chapter 22, pages 143ff. Meeus states that it is good to 0.5 seconds of arc.
This subroutine calculates the nutation in obliquity (delta epsilon) for the given dynamical time.
The algorithm comes from Jean Meeus' "Astronomical Algorithms", 2nd Edition, Chapter 22, pages 143ff. Meeus states that it is good to 0.1 seconds of arc.
This subroutine calculates the obliquity of the ecliptic in radians at the given dynamical time.
The algorithm comes from Jean Meeus' "Astronomical Algorithms", 2nd Edition, Chapter 22, pages 143ff. The conversion from universal to dynamical time comes from chapter 10, equation 10.2 on page 78.
This subroutine calculates the ecliptic longitude of the ascending node of the Moon's mean orbit at the given dynamical time.
The algorithm comes from Jean Meeus' "Astronomical Algorithms", 2nd Edition, Chapter 22, pages 143ff.
This subroutine converts the given angle in radians to its equivalent in degrees.
This subroutine computes the tangent of the given angle in radians.
This subroutine returns the Greenwich hour angle of the mean equinox at 0 hours universal on the day whose time is given (i.e. the argument is a standard Perl time).
This subroutine returns the Greenwich hour angle of the mean equinox at the given time.
The algorithm comes from Jean Meeus' "Astronomical Algorithms", 2nd Edition, equation 12.4, page 88.
This subroutine computes and returns the vector cross product of $b and $c. Vectors are represented by array references. The cross product is only defined if both arrays have 3 elements.
This subroutine computes and returns the vector dot product of $b and $c. Vectors are represented by array references. The dot product is only defined if both arrays have the same number of elements.
This subroutine computes and returns the magnitude of vector $b. The vector is represented by an array reference.
This subroutine computes and returns a unit vector pointing in the same direction as $b. The vectors are represented by array references.
The author wishes to acknowledge Jean Meeus, whose book "Astronomical Algorithms" (second edition) published by Willmann-Bell Inc (http://www.willbell.com/) provided several of the algorithms implemented herein.
Bugs can be reported to the author by mail, or through http://rt.cpan.org/.
Thomas R. Wyant, III (wyant at cpan dot org)
Copyright (C) 2005-2011 by Thomas R. Wyant, III
This program is free software; you can redistribute it and/or modify it under the same terms as Perl 5.10.0. For more details, see the full text of the licenses in the directory LICENSES.
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.
| Astro-satpass documentation | Contained in the Astro-satpass distribution. |
package Astro::Coord::ECI::Utils; use strict; use warnings; our $VERSION = '0.039'; our @ISA = qw{Exporter}; use Carp; ## use Config; use Data::Dumper; use POSIX qw{floor strftime}; use Scalar::Util qw{ blessed }; my @time_routines; BEGIN { # NOTE WELL # # The logic here should be consistent with the optional-module text # emitted by inc/Astro/Coord/ECI/Recommend.pm. # eval { ## $Config{use64bitint} and return 0; require Time::y2038; Time::y2038->import(); @time_routines = ( qw{ gmtime localtime timegm timelocal } ); 1; } or do { require Time::Local; Time::Local->import(); @time_routines = ( qw{ timegm timelocal } ); }; } our @EXPORT; our @EXPORT_OK = ( qw{ AU $DATETIMEFORMAT $JD_GREGORIAN JD_OF_EPOCH LIGHTYEAR PARSEC PERL2000 PI PIOVER2 SECSPERDAY SECS_PER_SIDERIAL_DAY SPEED_OF_LIGHT TWOPI acos asin atmospheric_extinction date2epoch date2jd deg2rad distsq dynamical_delta embodies epoch2datetime equation_of_time find_first_true intensity_to_magnitude jcent2000 jd2date jd2datetime jday2000 julianday load_module looks_like_number max min mod2pi nutation_in_longitude nutation_in_obliquity obliquity omega rad2deg tan theta0 thetag vector_cross_product vector_dot_product vector_magnitude vector_unitize _classisa _instance }, @time_routines ); our %EXPORT_TAGS = ( all => \@EXPORT_OK, params => [ qw{ _classisa _instance } ], time => \@time_routines, ); use constant AU => 149597870; # 1 astronomical unit, per # Meeus, Appendix I pg 407. use constant LIGHTYEAR => 9.4607e12; # 1 light-year, per Meeus, # Appendix I pg 407. use constant PARSEC => 30.8568e12; # 1 parsec, per Meeus, # Appendix I pg 407. use constant PERL2000 => timegm (0, 0, 12, 1, 0, 100); use constant PI => atan2 (0, -1); use constant PIOVER2 => PI / 2; use constant SECSPERDAY => 86400; use constant SECS_PER_SIDERIAL_DAY => 86164.0905; # Appendix I, page 408. use constant SPEED_OF_LIGHT => 299792.458; # KM/sec, per NIST. ### use constant SOLAR_RADIUS => 1392000 / 2; # Meeus, Appendix I, page 407. use constant TWOPI => PI * 2;
sub acos { abs ($_[0]) > 1 and confess <<eod; Programming error - Trying to take the arc cosine of a number greater than 1. eod return atan2 (sqrt (1 - $_[0] * $_[0]), $_[0]) }
sub asin {return atan2 ($_[0], sqrt (1 - $_[0] * $_[0]))}
# Note that the "constant" 0.120 in Aaer (aerosol scattering) is # based on a compromise value A0 = 0.050 in Green's equation 3 # (not exhibited here), which can vary from 0.035 in the winter to # 0.065 in the summer. This makes a difference of a couple tenths # at 20 degrees elevation, but a couple magnitudes at the # horizon. Green also remarks that the 1.5 denominator in the # same equation (a.k.a. the scale height) can be up to twice # that. sub atmospheric_extinction { my ($elevation, $height) = @_; my $cosZ = cos (PIOVER2 - $elevation); my $X = 1/($cosZ + 0.025 * exp (-11 * $cosZ)); # Green 1 my $Aray = 0.1451 * exp (-$height / 7.996); # Green 2 my $Aaer = 0.120 * exp (-$height / 1.5); # Green 4 return ($Aray + $Aaer + 0.016) * $X; # Green 5, 6 }
our $DATETIMEFORMAT; our $JD_GREGORIAN; BEGIN { $DATETIMEFORMAT = '%a %b %d %Y %H:%M:%S'; $JD_GREGORIAN = 2299160.5; } sub date2jd { my @args = @_; unshift @args, 0 while @args < 6; my ($sec, $min, $hr, $day, $mon, $yr) = @args; $mon++; # Algorithm expects month 1-12. $yr += 1900; # Algorithm expects zero-based year. ($yr < -4712) and croak "Error - Invalid year $yr"; ($mon < 1 || $mon > 12) and croak "Error - Invalid month $mon"; if ($mon < 3) { --$yr; $mon += 12; } my $A = floor ($yr / 100); my $B = 2 - $A + floor ($A / 4); my $jd = floor (365.25 * ($yr + 4716)) + floor (30.6001 * ($mon + 1)) + $day + $B - 1524.5 + ((($sec || 0) / 60 + ($min || 0)) / 60 + ($hr || 0)) / 24; $jd < $JD_GREGORIAN and $jd = floor (365.25 * ($yr + 4716)) + floor (30.6001 * ($mon + 1)) + $day - 1524.5 + ((($sec || 0) / 60 + ($min || 0)) / 60 + ($hr || 0)) / 24; return $jd; } use constant JD_OF_EPOCH => date2jd (gmtime (0));
sub date2epoch { my @args = @_; unshift @args, 0 while @args < 6; my ($sec, $min, $hr, $day, $mon, $yr) = @args; return (date2jd ($day, $mon, $yr) - JD_OF_EPOCH) * SECSPERDAY + (($hr || 0) * 60 + ($min || 0)) * 60 + ($sec || 0); }
sub deg2rad {return $_[0] * PI / 180}
sub distsq { my ($a, $b) = @_; (ref $a eq 'ARRAY' && ref $b eq 'ARRAY' && @$a == @$b) or confess <<eod; Programming error - Both arguments to distsq must be references to arrays of the same length. eod my $sum = 0; my $size = @$a; for (my $inx = 0; $inx < $size; $inx++) { my $delta = $a->[$inx] - $b->[$inx]; $sum += $delta * $delta; } return $sum }
sub dynamical_delta { my ($time) = @_; my $year = (gmtime $time)[5] + 1900; my $t = ($year - 2000) / 100; my $correction = .37 * ($year - 2100); # Meeus' correction to (10.2) return (25.3 * $t + 102) * $t + 102 # Meeus (10.2) + $correction; # Meeus' correction. }
sub embodies { my ($thingy, $class) = @_; my $code = eval {$thingy->can('represents')}; return $code ? $code->($thingy, $class) : undef; }
sub epoch2datetime { my ($time) = @_; my $day = floor ($time / SECSPERDAY); my $sec = $time - $day * SECSPERDAY; ($day, my $mon, my $yr, my $greg, my $leap) = jd2date ( my $jd = $day + JD_OF_EPOCH); $day = floor ($day + .5); my $min = floor ($sec / 60); $sec = $sec - $min * 60; my $hr = floor ($min / 60); $min = $min - $hr * 60; my $wday = ($jd + 1.5) % 7; my $yd = floor (275 * ($mon + 1) / 9) - (2 - $leap) * floor (($mon + 10) / 12) + $day - 31; wantarray and return ($sec, $min, $hr, $day, $mon, $yr, $wday, $yd, 0); return strftime ($DATETIMEFORMAT, $sec, $min, $hr, $day, $mon, $yr, $wday, $yd, 0); }
sub equation_of_time { my $time = shift; my $epsilon = obliquity ($time); my $y = tan($epsilon / 2); $y *= $y; # The following algorithm is from Meeus, chapter 25, page, 163 ff. my $T = jcent2000($time); # Meeus (25.1) my $L0 = mod2pi(deg2rad((.0003032 * $T + 36000.76983) * $T # Meeus (25.2) + 280.46646)); my $M = mod2pi(deg2rad(((-.0001537) * $T + 35999.05029) # Meeus (25.3) * $T + 357.52911)); my $e = (-0.0000001267 * $T - 0.000042037) * $T + 0.016708634;# Meeus (25.4) my $E = $y * sin (2 * $L0) - 2 * $e * sin ($M) + 4 * $e * $y * sin ($M) * cos (2 * $L0) - $y * $y * .5 * sin (4 * $L0) - 1.25 * $e * $e * sin (2 * $M); # Meeus (28.3) return $E * SECSPERDAY / TWOPI; # The formula gives radians. }
sub find_first_true { my ($begin, $end, $test, $limit) = @_; $limit ||= 1; if ($limit >= 1) { if ($begin <= $end) { $begin = floor ($begin); $end = floor ($end) == $end ? $end : floor ($end) + 1; } else { $end = floor ($end); $begin = floor ($begin) == $begin ? $begin : floor ($begin) + 1; } } my $iterator = ( $end > $begin ? sub {$end - $begin > $limit} : sub {$begin - $end > $limit} ); while ($iterator->()) { my $mid = $limit >= 1 ? floor (($begin + $end) / 2) : ($begin + $end) / 2; ($begin, $end) = ($test->($mid)) ? ($begin, $mid) : ($mid, $end); } return $end; }
{ # Begin local symbol block my $intensity_to_mag_factor; # Calculate only if needed. sub intensity_to_magnitude { return - ($intensity_to_mag_factor ||= 2.5 / log (10)) * log ($_[0]); } }
sub jd2date { my ($time) = @_; my $mod_jd = $time + 0.5; my $Z = floor ($mod_jd); my $F = $mod_jd - $Z; my $A = (my $julian = $Z < $JD_GREGORIAN) ? $Z : do { my $alpha = floor (($Z - 1867216.25)/36524.25); $Z + 1 + $alpha - floor ($alpha / 4); }; my $B = $A + 1524; my $C = floor (($B - 122.1) / 365.25); my $D = floor (365.25 * $C); my $E = floor (($B - $D) / 30.6001); my $day = $B - $D - floor (30.6001 * $E) + $F; my $mon = $E < 14 ? $E - 1 : $E - 13; my $yr = $mon > 2 ? $C - 4716 : $C - 4715; return ($day, $mon - 1, $yr - 1900, !$julian, ($julian ? !($yr % 4) : ( $yr % 400 ? $yr % 100 ? !($yr % 4) : 0 : 1))); ## % 400 ? 1 : $yr % 100 ? 0 : !($yr % 4)))); }
sub jd2datetime { my ($time) = @_; return epoch2datetime(($time - JD_OF_EPOCH) * SECSPERDAY); }
sub jcent2000 {return jday2000 ($_[0]) / 36525}
sub jday2000 {return ($_[0] - PERL2000) / SECSPERDAY}
sub julianday {return jday2000($_[0]) + 2_451_545.0}
{ # Local symbol block. Oh, for 5.10 and state variables. my %error; my %rslt; sub load_module { my ($module) = @_; exists $error{$module} and croak $error{$module}; exists $rslt{$module} and return $rslt{$module}; # I considered Module::Load here, but it appears not to support # .pmc files. No, it's not an issue at the moment, but it may be # if Perl 6 becomes a reality. $rslt{$module} = eval "require $module"; $@ and croak ($error{$module} = $@); return $rslt{$module}; } } # End local symbol block.
unless (eval {require Scalar::Util; Scalar::Util->import ('looks_like_number'); 1}) { no warnings qw{once}; *looks_like_number = sub { local $_ = shift; # checks from perlfaq4 return 0 if !defined($_) || ref($_); return 1 if (/^[+-]?\d+$/); # is a +/- integer return 1 if (/^([+-]?)(?=\d|\.\d)\d*(\.\d*)?([Ee]([+-]?\d+))?$/); # a C float return 1 if ($] >= 5.008 and /^(Inf(inity)?|NaN)$/i) or ($] >= 5.006001 and /^Inf$/i); return 0; }; }
unless (eval {require List::Util; List::Util->import ('max'); 1}) { no warnings qw{once}; *max = sub { my $rslt; foreach (@_) { defined $_ or next; if (!defined $rslt || $_ > $rslt) { $rslt = $_; } } $rslt; }; }
unless (eval {require List::Util; List::Util->import ('min'); 1}) { no warnings qw{once}; *min = sub { my $rslt; foreach (@_) { defined $_ or next; if (!defined $rslt || $_ < $rslt) { $rslt = $_; } } $rslt; }; }
sub mod2pi {return $_[0] - floor ($_[0] / TWOPI) * TWOPI}
sub nutation_in_longitude { my $time = shift; my $T = jcent2000 ($time); # Meeus (22.1) my $omega = mod2pi (deg2rad ((($T / 450000 + .0020708) * $T - 1934.136261) * $T + 125.04452)); my $L = mod2pi (deg2rad (36000.7698 * $T + 280.4665)); my $Lprime = mod2pi (deg2rad (481267.8813 * $T + 218.3165)); my $delta_psi = deg2rad ((-17.20 * sin ($omega) - 1.32 * sin (2 * $L) - 0.23 * sin (2 * $Lprime) + 0.21 * sin (2 * $omega))/3600); return $delta_psi; }
sub nutation_in_obliquity { my $time = shift; my $T = jcent2000 ($time); # Meeus (22.1) my $omega = mod2pi (deg2rad ((($T / 450000 + .0020708) * $T - 1934.136261) * $T + 125.04452)); my $L = mod2pi (deg2rad (36000.7698 * $T + 280.4665)); my $Lprime = mod2pi (deg2rad (481267.8813 * $T + 218.3165)); my $delta_epsilon = deg2rad ((9.20 * cos ($omega) + 0.57 * cos (2 * $L) + 0.10 * cos (2 * $Lprime) - 0.09 * cos (2 * $omega))/3600); return $delta_epsilon; }
use constant E0BASE => (21.446 / 60 + 26) / 60 + 23; sub obliquity { my $time = shift; my $T = jcent2000 ($time); # Meeus (22.1) my $delta_epsilon = nutation_in_obliquity ($time); my $epsilon0 = deg2rad (((0.001813 * $T - 0.00059) * $T - 46.8150) * $T / 3600 + E0BASE); return $epsilon0 + $delta_epsilon; }
sub omega { my $T = jcent2000 (shift); # Meeus (22.1) return mod2pi (deg2rad ((($T / 450000 + .0020708) * $T - 1934.136261) * $T + 125.04452)); }
sub rad2deg {return $_[0] / PI * 180}
sub tan {return sin ($_[0]) / cos ($_[0])}
sub theta0 { my ($time) = @_; return thetag (timegm (0, 0, 0, (gmtime $time)[3 .. 5])); }
# Meeus, pg 88, equation 12.4, converted to radians and Perl dates. sub thetag { my ($time) = @_; my $T = jcent2000 ($time); return mod2pi (4.89496121273579 + 6.30038809898496 * jday2000 ($time)) + (6.77070812713916e-06 - 4.5087296615715e-10 * $T) * $T * $T; }
sub vector_cross_product { my ( $b, $c ) = @_; @{ $b } == 3 and @{ $c } == 3 or confess 'Programming error - vector_cross_product arguments', ' must be references to arrays of length 3'; return [ $b->[1] * $c->[2] - $b->[2] * $c->[1], $b->[2] * $c->[0] - $b->[0] * $c->[2], $b->[0] * $c->[1] - $b->[1] * $c->[0], ]; }
sub vector_dot_product { my ( $b, $c ) = @_; @{ $b } == @{ $c } or confess 'Programming error - vector_dot_product arguments ', 'must be references to arrays of the same length'; my $prod = 0; my $size = @{ $b } - 1; foreach my $inx ( 0 .. $size ) { $prod += $b->[$inx] * $c->[$inx]; } return $prod; }
sub vector_magnitude { my ( $b ) = @_; 'ARRAY' eq ref $b or confess 'Programming error - vector_magnitude argument ', 'must be a reference to an array'; my $mag = 0; my $size = @{ $b } - 1; foreach my $inx ( 0 .. $size ) { $mag += $b->[$inx] * $b->[$inx]; } return sqrt $mag; }
sub vector_unitize { my ( $b ) = @_; 'ARRAY' eq ref $b or confess 'Programming error - vector_unitize argument ', 'must be a reference to an array'; my $mag = vector_magnitude( $b ); return [ map { $_ / $mag } @{ $b } ]; } # _classisa( 'Foo', 'Bar' ); # # Returns true if Foo->isa( 'Bar' ) is true, and false otherwise. # In particular, returns false if the first argument is a # reference. sub _classisa { my ( $invocant, $class ) = @_; ref $invocant and return; defined $invocant or return; return $invocant->isa( $class ); } # _instance( $foo, 'Bar' ); # # Returns true if $foo is an instance of 'Bar', and false # otherwise. In particular, returns false if $foo is not a # reference, or if it is not blessed. sub _instance { my ( $object, $class ) = @_; ref $object or return; blessed( $object ) or return; return $object->isa( $class ); } # $epoch_time = _parse_time_iso_8601 # # Parse ISO 8601 date/time. I do not intend to expose this, since # it will probably go away when the satpass script is dropped. It # would actually be in that script except for the fact that it can # be more easily tested here, and because of the possibility that # it will be used in App::Satpass2. { my %special_day_offset = ( yesterday => -SECSPERDAY(), today => 0, tomorrow => SECSPERDAY(), ); sub _parse_time_iso_8601 { my ( $string ) = @_; my @zone; $string =~ s/ \s* (?: ( Z ) | ( [+-] ) ( \d{2} ) :? ( \d{2} )? ) \z //smx and @zone = ( $1, $2, $3, $4 ); my @date; # ISO 8601 date if ( $string =~ m{ \A ( \d{4} \D? | \d{2} \D ) # year: $1 (?: ( \d{1,2} ) \D? # month: $2 (?: ( \d{1,2} ) (?: \s* | \D? ) # day: $3 (?: ( \d{1,2} ) \D? # hour: $4 (?: ( \d{1,2} ) \D? # minute: $5 (?: ( \d{1,2} ) \D? # second: $6 ( \d* ) # fract: $7 )? )? )? )? )? \z }smx ) { @date = ( $1, $2, $3, $4, $5, $6, $7, undef ); # special-case 'yesterday', 'today', and 'tomorrow'. } elsif ( $string =~ m{ \A ( yesterday | today | tomorrow ) # day: $1 (?: \D* ( \d{1,2} ) \D? # hour: $2 (?: ( \d{1,2} ) \D? # minute: $3 (?: ( \d{1,2} ) \D? # second: $4 ( \d* ) # fract: $5 )? )? )? \z }smx ) { my @today = @zone ? gmtime : localtime; @date = ( $today[5] + 1900, $today[4] + 1, $today[3], $2, $3, $4, $5, $special_day_offset{$1} ); } else { return; } my $offset = pop @date || 0; if ( @zone && !$zone[0] ) { my ( undef, $sign, $hr, $min ) = @zone; $offset -= $sign . ( ( $hr * 60 + ( $min || 0 ) ) * 60 ) } foreach ( @date ) { defined $_ and s/ \D+ //smxg; } if ( $date[0] < 70 ) { $date[0] += 100; } elsif ( $date[0] >= 100 ) { $date[0] -= 1900; } defined $date[1] and --$date[1]; defined $date[2] or $date[2] = 1; my $frc = pop @date; foreach ( @date ) { defined $_ or $_ = 0; } my $time; if ( @zone ) { $time = timegm( reverse @date ); } else { $time = timelocal( reverse @date ); } if ( defined $frc && $frc ne '') { my $denom = 1 . ( 0 x length $frc ); $time += $frc / $denom; } return $time + $offset; } } 1; __END__
# ex: set textwidth=72 :