Initial import of version 2.10

main
Gergely Polonkai 2 years ago
commit ded7b26f78
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GPG Key ID: 2D2885533B869ED4

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all:
cd src && ${MAKE}
install:
cd src && ${MAKE} install
cd doc && ${MAKE} install
cd data && ${MAKE} install

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SE1_FILES = \
seas_00.se1 \
seas_06.se1 \
seas_12.se1 \
seas_18.se1 \
seas_24.se1 \
seas_30.se1 \
seas_36.se1 \
seas_42.se1 \
seas_48.se1 \
seasm06.se1 \
seasm12.se1 \
seasm18.se1 \
seasm24.se1 \
seasm30.se1 \
seasm36.se1 \
seasm42.se1 \
seasm48.se1 \
seasm54.se1 \
semo_00.se1 \
semo_06.se1 \
semo_12.se1 \
semo_18.se1 \
semo_24.se1 \
semo_30.se1 \
semo_36.se1 \
semo_42.se1 \
semo_48.se1 \
semom06.se1 \
semom12.se1 \
semom18.se1 \
semom24.se1 \
semom30.se1 \
semom36.se1 \
semom42.se1 \
semom48.se1 \
semom54.se1 \
sepl_00.se1 \
sepl_06.se1 \
sepl_12.se1 \
sepl_18.se1 \
sepl_24.se1 \
sepl_30.se1 \
sepl_36.se1 \
sepl_42.se1 \
sepl_48.se1 \
seplm06.se1 \
seplm12.se1 \
seplm18.se1 \
seplm24.se1 \
seplm30.se1 \
seplm36.se1 \
seplm42.se1 \
seplm48.se1 \
seplm54.se1 \
$(NULL)
OTHER_FILES = \
seorbel.txt \
seasnam.txt \
sefstars.txt \
seleapsec.txt \
$(NULL)
all:
install:
mkdir -p $(DESTDIR)/usr/share/libswe
install -m 0644 $(SE1_FILES) $(OTHER_FILES) $(DESTDIR)/usr/share/libswe

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# This file contains the dates of leap seconds to be taken into account
# by the Swiss Ephemeris.
# For each new leap second add the date of its insertion in the format
# yyyymmdd, e.g. "20081231" for 31 december 2008.
# The leap second is inserted at the end of the day.
20081231

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# Orbital elements of ficticious planets
# 27 Jan. 2000
#
# This file is part of the Swiss Ephemeris, from Version 1.52 on.
#
# Warning! These planets do not exist!
#
# The user can add his or her own elements.
# 960 is the maximum number of ficticious planets.
#
# The elements order is as follows:
# 1. epoch of elements (Julian day)
# 2. equinox (Julian day or "J1900" or "B1950" or "J2000")
# 3. mean anomaly at epoch
# 4. semi-axis
# 5. eccentricity
# 6. argument of perihelion (ang. distance of perihelion from node)
# 7. ascending node
# 8. inclination
# 9. name of planet
#
# use '#' for comments
# to compute a body with swe_calc(), use planet number
# ipl = SE_FICT_OFFSET_1 + number_of_elements_set,
# e.g. number of Kronos is ipl = 39 + 4 = 43
#
# Witte/Sieggruen planets, refined by James Neely
J1900, J1900, 163.7409, 40.99837, 0.00460, 171.4333, 129.8325, 1.0833, Cupido # 1
J1900, J1900, 27.6496, 50.66744, 0.00245, 148.1796, 161.3339, 1.0500, Hades # 2
J1900, J1900, 165.1232, 59.21436, 0.00120, 299.0440, 0.0000, 0.0000, Zeus # 3
J1900, J1900, 169.0193, 64.81690, 0.00305, 208.8801, 0.0000, 0.0000, Kronos # 4
J1900, J1900, 138.0533, 70.29949, 0.00000, 0.0000, 0.0000, 0.0000, Apollon # 5
J1900, J1900, 351.3350, 73.62765, 0.00000, 0.0000, 0.0000, 0.0000, Admetos # 6
J1900, J1900, 55.8983, 77.25568, 0.00000, 0.0000, 0.0000, 0.0000, Vulcanus # 7
J1900, J1900, 165.5163, 83.66907, 0.00000, 0.0000, 0.0000, 0.0000, Poseidon # 8
#
# Isis-Transpluto; elements from "Die Sterne" 3/1952, p. 70ff.
# Strubell does not give an equinox. 1945 is taken in order to
# reproduce the as best as ASTRON ephemeris. (This is a strange
# choice, though.)
# The epoch according to Strubell is 1772.76.
# 1772 is a leap year!
# The fraction is counted from 1 Jan. 1772
2368547.66, 2431456.5, 0.0, 77.775, 0.3, 0.7, 0, 0, Isis-Transpluto # 9
# Nibiru, elements from Christian Woeltge, Hannover
1856113.380954, 1856113.380954, 0.0, 234.8921, 0.981092, 103.966, -44.567, 158.708, Nibiru # 10
# Harrington, elements from Astronomical Journal 96(4), Oct. 1988
2374696.5, J2000, 0.0, 101.2, 0.411, 208.5, 275.4, 32.4, Harrington # 11
# according to W.G. Hoyt, "Planets X and Pluto", Tucson 1980, p. 63
2395662.5, 2395662.5, 34.05, 36.15, 0.10761, 284.75, 0, 0, Leverrier (Neptune) # 12
2395662.5, 2395662.5, 24.28, 37.25, 0.12062, 299.11, 0, 0, Adams (Neptune) # 13
2425977.5, 2425977.5, 281, 43.0, 0.202, 204.9, 0, 0, Lowell (Pluto) # 14
2425977.5, 2425977.5, 48.95, 55.1, 0.31, 280.1, 100, 15, Pickering (Pluto) # 15
# intramercurian hypothetical Vulcan acc. to L.H. Weston
J1900,JDATE, 252.8987988 + 707550.7341 * T, 0.13744, 0.019, 322.212069+1670.056*T, 47.787931-1670.056*T, 7.5, Vulcan # 16
# Selena/White Moon
J2000,JDATE, 242.2205555 + 5143.5418158 * T, 0.05280098949, 0.0, 0.0, 0.0, 0.0, Selena/White Moon, geo # 17
# Hypothetical planet Proserpina, according to http://www.geocities.com/Hollywood/Academy/7519/proserpina.html
# J1900, 170.73 + 51.05 * T
J1900,JDATE, 170.73, 79.225630, 0, 0, 0, 0, Proserpina #18
# Waldemath's Second Earth Moon
# Elements were derived by D.Koch from Waldemaths original elements as given in
# David Walters' book on Vulcan. They differ from Solar Fire (Graham Dawsons)
# elements, which are based on the assumption that the "mean longitude" given
# by Waldemath is an observation (a true longitude)
# Neither Swisseph nor Solar fire elements agree with Delphine Jay's ephemeris,
# which is obviously wrong.
2414290.95827875,2414290.95827875, 70.3407215 + 109023.2634989 * T, 0.0068400705250028, 0.1587, 8.14049594 + 2393.47417444 * T, 136.24878256 - 1131.71719709 * T, 2.5, Waldemath, geo # 19
# Colin R. Nicholl's Comet, according to "The Great Christ Comet", p. 223.
1719500.7, J2000, 0.0, 1190.0, 0.9999, 9.47, 200.08, 178.3, Christ Comet # 20
# Planet 9, according to: Fienga & alii, Constraints on the location of a
# possible 9th planet, Astronomy & Astrophysics no. FiengaLaskar2016R5. The
# authors provide true anomaly 117.8. Mean anomaly derived by D. Koch
2457388.5,J2000,45.5272966,700,0.6,150,113,30,Planet_9 # 21
# Comet Halley 12 BCE, only good near 12 BCE;
# Yeomans/Kiang, Mon. Not. R. astr. Soc. (1981), 197, p. 643
1717323.34852, B1950, 0.0, 17.99261849, 0.9673664, 92.54399, 35.19064, 163.58392, Comet Halley 12 BCE # 22
# 2015 RR245
2457600.5,J2000,322.50413,81.2891975,0.5852663,261.41753,211.67680,7.57643,2015 RR245 # 23
#
# The following elements are for test only
# (Selena without T)
J2000,JDATE, 242.2205555, 0.05279142865925, 0.0, 0.0, 0.0, 0.0, Selena/White Moon, geo # 17
# (Selena with T, gives exactly the same position)
J2000,JDATE, 242.2205555 + 5143.5418158 * T, 0.05279142865925, 0.0, 0.0, 0.0, 0.0, Selena/White Moon with T Terms, geo # 17
J2000, JDATE, 174.794787 + 149472.5157715 * T, 0.38709831, 0.20563175 + 0.000020406 * T, 29.125226 + 0.3702885 * T, 48.330893 + 1.186189 * T, 7.004986 + 0.0018215 * T, Mercury elem. for equ. of date # 18
J2000, J2000, 174.794787 + 149472.5157715 * T, 0.38709831, 0.20563175 + 0.000020406 * T, 29.125226 + 0.2842872 * T, 48.330893 - 0.1254229 * T, 7.004986 - 0.0059516 * T, Mercury Test J2000 Elements# 18

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all:
install:
mkdir -p $(DESTDIR)/usr/share/doc/libswe
install -m 0644 sweph.gif swephin.gif swephprg.htm swephprg.pdf swisseph.htm swisseph.pdf $(DESTDIR)/usr/share/doc/libswe

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Revision history for Perl extension SwissEph.
First created on 3 April 2009, with Swiss Ephemeris 1.76.
Updated on 27 January 2011:
- Function swe_utc_time_zone() added for Swiss Ephemeris 1.77
- Delta t updated
- Fixed stars: algorithm in swe_fixstar() was improved, new input file sefstars.txt was created
Updated on 7 September 2012:
- Precession algorithm was updated
- Function swe_rise_trans_true_hor() added for Swiss Ephemeris 1.78
- several minor bug fixes (see documentation swephprg.pdf)
Updated on 23 April 2013, Swiss Ephemeris 1.79
- Improved precision in eclipse calculations: 2nd and 3rd contact with solar eclipses, penumbral and partial phases with lunar eclipses.
- Bug fix in function swe_sol_eclipse_when_loc().If the local maximum eclipse occurs at sunset or sunrise, tret[0] now gives the moment when the lower limb of the Sun touches the horizon. This was not correctly implemented in former versions
- Bug fix in Perl functions swe_house() etc. These functions had crashed with a segmention violation if called with the house parameter G.
- Bug fix in Perl function swe_utc_to_jd(), where gregflag had been read from the 4th instead of the 6th parameter.
- Bug fix in Perl functions to do with date conversion. The default mechanism for gregflag was buggy.
- For Hindu astrologers, some more ayanamshas were added that are related to Suryasiddhanta and Aryabhata and are of historical interest.
Updated on 31 August 2012
- Function swe_house_name() added for Swiss Ephemeris 1.80
Updated on 11 February 2014, for Swiss Ephemeris 2.00:
- Major release, Swisseph can handle JPL ephemeris DE431
- The following functions were added:
swe_lun_eclipse_when_loc() searches locally visible lunar eclipse
swe_lmt_to_lat() conversion of LMT to LAT
swe_lat_to_lmt() conversion of LAT to LMT
Updated on 18 March 2015, Swiss Ephemeris 2.01:
- a few constants added to SwissEph.pm
Updated on 5 August 2015, Swiss Ephemeris 2.02:
- The following functions were added:
swe_deltat_ex() provides Delta T adjusted to ephemeris chosen
swe_get_ayanamsa_ex() provides ayanamsa depending on ephemeris chosen
swe_get_ayanamsa_ex_ut() provides ayanamsa depending on ephemeris chosen
Updated on 14 August 2015, Swiss Ephemeris 2.02.01:
- see documentation swephprg.pdf
Updated on 16 Oct 2015, Swiss Ephemeris 2.03:
- see documentation swephprg.pdf
Updated on 21 Oct 2015, Swiss Ephemeris 2.04:
- see documentation swephprg.pdf
Updated on 26 May 2016, Swiss Ephemeris 2.05:
- see documentation swephprg.pdf
Updated on 12 Jan 2018, Swiss Ephemeris 2.07:
- see documentation swephprg.pdf
Updated on 19 Jun 2019, Swiss Ephemeris 2.08:
- a few defines (constants) were added in SwissEph.pm
Updated on 9 Aug 2019, Swiss Ephemeris 2.08:
- eclipse functions return saros series and eclipse numbers
Updated on 23 Jul 2020, Swiss Ephemeris 2.09:
- see documentation swephprg.pdf
Updated on 18 Aug 2020, Swiss Ephemeris 2.09.02:
- see documentation swephprg.pdf
Updated on 10 Dec 2020, Swiss Ephemeris 2.10:
- see documentation swephprg.pdf

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Changes
Makefile.PL
MANIFEST
ppport.h
sweodef.h
swephexp.h
README
SwissEph.xs
t/SwissEph.t
lib/SwissEph.pm
blib/arch/auto/SwissEph/SwissEph.so
fix_selinux
/usr/local/lib64/swe/libswe.so.2.04
/usr/local/lib64/swe/libswe.so.2.05c
/usr/local/lib64/swe/libswe.so.2.05c
/usr/local/lib64/swe/libswe.so.2.05c
/usr/local/lib64/swe/libswe.so.2.05
/usr/local/lib64/swe/libswe.so.2.05.01
/usr/local/lib64/swe/libswe.so.2.05.02b02
/usr/local/lib64/swe/libswe.so.2.05.02b02
/usr/local/lib64/swe/libswe.so.2.05.02b03
/usr/local/lib64/swe/libswe.so.2.05.02b02
/usr/local/lib64/swe/libswe.so.2.05.02b04
/usr/local/lib64/swe/libswe.so.2.05.02b04
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/usr/local/lib64/swe/libswe.so.2.05.02b06
/usr/local/lib64/swe/libswe.so.2.06
/usr/local/lib64/swe/libswe.so.2.06.01b02
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/usr/local/lib64/swe/libswe.so.2.05c
/usr/local/lib64/swe/libswe.so.2.07.02
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/usr/local/lib64/swe/libswe.so.2.08
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/usr/local/lib64/swe/libswe.so.2.08.00a
/usr/local/lib64/swe/libswe.so.2.09
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/usr/local/lib64/swe/libswe.so.2.09.01
/usr/local/lib64/swe/libswe.so.2.09.02
/usr/local/lib64/swe/libswe.so.2.09.03
/usr/local/lib64/swe/libswe.so.2.10
META.yml Module YAML meta-data (added by MakeMaker)
META.json Module JSON meta-data (added by MakeMaker)

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{
"abstract" : "The Swiss Ephemeris made accessible for Perl \r",
"author" : [
"Dieter <dieter@astro.ch>"
],
"dynamic_config" : 1,
"generated_by" : "ExtUtils::MakeMaker version 6.68, CPAN::Meta::Converter version 2.120921",
"license" : [
"unknown"
],
"meta-spec" : {
"url" : "http://search.cpan.org/perldoc?CPAN::Meta::Spec",
"version" : "2"
},
"name" : "SwissEph",
"no_index" : {
"directory" : [
"t",
"inc"
]
},
"prereqs" : {
"build" : {
"requires" : {
"ExtUtils::MakeMaker" : "0"
}
},
"configure" : {
"requires" : {
"ExtUtils::MakeMaker" : "0"
}
},
"runtime" : {
"requires" : {}
}
},
"release_status" : "stable",
"version" : "2.10"
}

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---
abstract: "The Swiss Ephemeris made accessible for Perl \r"
author:
- 'Dieter <dieter@astro.ch>'
build_requires:
ExtUtils::MakeMaker: 0
configure_requires:
ExtUtils::MakeMaker: 0
dynamic_config: 1
generated_by: 'ExtUtils::MakeMaker version 6.68, CPAN::Meta::Converter version 2.120921'
license: unknown
meta-spec:
url: http://module-build.sourceforge.net/META-spec-v1.4.html
version: 1.4
name: SwissEph
no_index:
directory:
- t
- inc
requires: {}
version: 2.10

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#!/usr/local/bin/perl
use 5.008007;
use ExtUtils::MakeMaker;
# See lib/ExtUtils/MakeMaker.pm for details of how to influence
# the contents of the Makefile that is written.
WriteMakefile(
NAME => 'SwissEph',
VERSION_FROM => 'lib/SwissEph.pm', # finds $VERSION
PREREQ_PM => {}, # e.g., Module::Name => 1.1
($] >= 5.005 ? ## Add these new keywords supported since 5.005
(ABSTRACT_FROM => 'lib/SwissEph.pm', # retrieve abstract from module
AUTHOR => 'Dieter <dieter@astro.ch>') : ()),
#LIBS => ['-lC:\sweph\bin\swedll32'], # e.g., '-lm'
LIBS => ['-L/usr/local/lib64/swe -lswe'], # e.g., '-lm'
#LIBS => ['-lswe'], # e.g., '-lm'
DEFINE => '', # e.g., '-DHAVE_SOMETHING'
INC => '-I.', # e.g., '-I. -I/usr/include/other'
# DISTVNAME => 'perl_swisseph', #
# Un-comment this if you add C files to link with later:
# OBJECT => '$(O_FILES)', # link all the C files too
);

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SwissEph version 2.056
=====================
The README is used to introduce the module and provide instructions on
how to install the module, any machine dependencies it may have (for
example C compilers and installed libraries) and any other information
that should be provided before the module is installed.
INSTALLATION
On Linux:
=========
Before installing this module, you have to install a shared library of
the Swiss Ephemeris functions.
Unpack http://www.astro.com/ftp/swisseph/swe_unix_src_2.06.tar.gz
or whatever the latest version is, or the one you want to use.
There will be a src directory in the unpacked files. Go there
and run
make libswe.so to build the shared library. Copy this file to
/usr/local/lib64/swe
Usually, this will also require that you create a file (as root)
/etc/ld.so.conf.d/swisseph.conf
with the content line
/usr/local/lib64/swe
Now run ldconfig(8) (as root) in order to generate the
symbolic links required.
Now you can install the Perl module for the Swiss Ephemeris.
Type the following:
perl Makefile.PL
make
make test
make install (requires root)
On Windows:
===========
Before installing this module, you have to install the following things
on your computer:
- the Swiss Ephemeris DLL swedll32.dll. If haven't done this yet,
download the Swiss Ephemeris from the download area at
www.astro.com/swisseph and unpack it.
- Visual C++ Express Edition, which can be downloaded for free from the
http://www.microsoft.com/express/download/.
After that you can install the Perl module. In the current directory
(where you read this README file), open the file Makefile.PL and
fix the LIBS parameter. It must contain the directory to the Swiss Ephemeris
DLL. After that run:
perl Makefile.PL
nmake
nmake test
nmake install
COPYRIGHT AND LICENCE
Copyright (C) 2017 Astrodienst, Zurich, Switzerland.
This library is free software; you can redistribute it and/or modify
it under the same terms as Perl itself, either Perl version 5.8.7 or,
at your option, any later version of Perl 5 you may have available.
-----------------------
Update 23-march-2016, example how to use PerlSwissEph-2.04.tar.gz
download PerlSwissEph-2.04.tar.gz
unpack it with
tar xzvf PerlSwissEph-2.04.tar.gz
it creates a directory SwissEph-2.04
cd SwissEph-2.04
perl Makefile.PL (to create Makefile)
there is a warning:
Warning: the following files are missing in your kit:
/usr/local/lib64/swe/libswe.so.2.04
The tarball contains ./usr/local/lib64/swe/libswe.so.2.04
you must copy or move this to /usr/local/lib64/swe/libswe.so.2.04 by hand.
If your architecture is not 64-bit Linux, you may have to create libswe.so.2.04
from the Swisseph C source distribution yourself, and then place it properly.
Then you must tell the Linux system how to find the dynamic library.
On Redhat RHEL 6 this goes like this:
as root, cd /etc/ld.so.conf.d
edit or create a file swisseph.conf with this line in it
/usr/local/lib64/swe
now run as root: ldconfig
afterwards, you should find in /usr/local/lib64/swe/
something like this
lrwxrwxrwx. 1 root root 14 Mar 23 17:44 libswe.so -> libswe.so.2.04
lrwxrwxrwx. 1 root root 14 Mar 23 17:43 libswe.so.1 -> libswe.so.2.04
-rwxr-xr-x. 1 root root 847686 Mar 23 17:10 libswe.so.2.04
Now, as normal user, go back to
cd SwissEph-2.04
make
make test
as root, (unless you can write in the install target directories)
make install

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/usr/sbin/semanage fcontext -a -t textrel_shlib_t /usr/lib/perl5/site_perl/5.8.8/i386-linux-thread-multi/auto/SwissEph/SwissEph.so
/sbin/restorecon -v /usr/lib/perl5/site_perl/5.8.8/i386-linux-thread-multi/auto/SwissEph/SwissEph.so
/usr/sbin/semanage fcontext -a -t textrel_shlib_t /usr/lib/libswe.so.1.76.00
/sbin/restorecon -v /usr/lib/libswe.so.1.76.00

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/************************************************************
definitions and constants for all Swiss Ephemeris source files,
only required for compiling the libraries, not for the external
interface of the libraries.
The definitions are a subset of Astrodienst's ourdef.h content
and must be kept compatible. Everything not used in SwissEph
has been deleted.
Does auto-detection of MSDOS (TURBO_C or MS_C), HPUNIX, Linux.
Must be extended for more portability; there should be a way
to detect byte order and file system type.
************************************************************/
/* Copyright (C) 1997 - 2008 Astrodienst AG, Switzerland. All rights reserved.
License conditions
------------------
This file is part of Swiss Ephemeris.
Swiss Ephemeris is distributed with NO WARRANTY OF ANY KIND. No author
or distributor accepts any responsibility for the consequences of using it,
or for whether it serves any particular purpose or works at all, unless he
or she says so in writing.
Swiss Ephemeris is made available by its authors under a dual licensing
system. The software developer, who uses any part of Swiss Ephemeris
in his or her software, must choose between one of the two license models,
which are
a) GNU public license version 2 or later
b) Swiss Ephemeris Professional License
The choice must be made before the software developer distributes software
containing parts of Swiss Ephemeris to others, and before any public
service using the developed software is activated.
If the developer choses the GNU GPL software license, he or she must fulfill
the conditions of that license, which includes the obligation to place his
or her whole software project under the GNU GPL or a compatible license.
See http://www.gnu.org/licenses/old-licenses/gpl-2.0.html
If the developer choses the Swiss Ephemeris Professional license,
he must follow the instructions as found in http://www.astro.com/swisseph/
and purchase the Swiss Ephemeris Professional Edition from Astrodienst
and sign the corresponding license contract.
The License grants you the right to use, copy, modify and redistribute
Swiss Ephemeris, but only under certain conditions described in the License.
Among other things, the License requires that the copyright notices and
this notice be preserved on all copies.
Authors of the Swiss Ephemeris: Dieter Koch and Alois Treindl
The authors of Swiss Ephemeris have no control or influence over any of
the derived works, i.e. over software or services created by other
programmers which use Swiss Ephemeris functions.
The names of the authors or of the copyright holder (Astrodienst) must not
be used for promoting any software, product or service which uses or contains
the Swiss Ephemeris. This copyright notice is the ONLY place where the
names of the authors can legally appear, except in cases where they have
given special permission in writing.
The trademarks 'Swiss Ephemeris' and 'Swiss Ephemeris inside' may be used
for promoting such software, products or services.
*/
#ifndef _OURDEF_INCLUDED /* ourdef.h is a superset of sweodef.h */
#ifndef _SWEODEF_INCLUDED /* allow multiple #includes */
#define _SWEODEF_INCLUDED
# define MY_TRUE 1 /* for use in other defines, before TRUE is defined */
# define MY_FALSE 0 /* for use in other defines, before TRUE is defined */
/* TLS support
*
* Sun Studio C/C++, IBM XL C/C++, GNU C and Intel C/C++ (Linux systems) -> __thread
* Borland, VC++ -> __declspec(thread)
*/
#if !defined(TLSOFF) && !defined( __APPLE__ ) && !defined(WIN32) && !defined(DOS32)
#if defined( __GNUC__ )
#define TLS __thread
#else
#define TLS __declspec(thread)
#endif
#else
#define TLS
#endif
#ifdef _WIN32 /* Microsoft VC 5.0 does not define MSDOS anymore */
# undef MSDOS
# define MSDOS MY_TRUE
#include <wtypes.h>
#include <objbase.h>
#include <wincon.h>
#include <winbase.h>
#include <io.h>
#include <windows.h>
# define sleep(x) Sleep((x) * 1000)
#endif
#ifdef _MSC_VER
# define MS_VC
#endif
#ifdef WIN32 /* Microsoft VC 5.0 does not define MSDOS anymore */
# define MSDOS MY_TRUE
#endif
#ifdef MSDOS /* already defined by some DOS compilers */
# undef MSDOS
# define MSDOS MY_TRUE
#endif
#ifdef __TURBOC__ /* defined by turboc */
# ifndef MSDOS
# define MSDOS MY_TRUE
# endif
# define TURBO_C
#endif
#ifdef __SC__ /* defined by Symantec C */
# ifndef MSDOS
# define MSDOS MY_TRUE
# endif
# define SYMANTEC_C
#endif
#ifdef __WATCOMC__ /* defined by WatcomC */
# ifndef MSDOS
# define MSDOS MY_TRUE
# endif
# define WATCOMC
#endif
#ifdef __MWERKS__ /* defined on Macintosh CodeWarrior */
# if macintosh && powerc
# define MACOS MY_TRUE /* let it undefined otherwise */
# define MSDOS MY_FALSE /* in case one above fired falsely */
# endif
#endif
#ifdef MSDOS
# define HPUNIX MY_FALSE
# define INTEL_BYTE_ORDER 1
# ifndef TURBO_C
# define MS_C /* assume Microsoft C compiler */
# endif
# define UNIX_FS MY_FALSE
#else
# ifdef MACOS
# define HPUNIX MY_FALSE
# define UNIX_FS MY_FALSE
# else
# define MSDOS MY_FALSE
# define HPUNIX MY_TRUE
# ifndef _HPUX_SOURCE
# define _HPUX_SOURCE
# endif
# define UNIX_FS MY_TRUE
# endif
#endif
#include <math.h>
#include <stdlib.h>
#ifndef FILE
# include <stdio.h>
#endif
#if HPUNIX
# include <unistd.h>
#endif
/*
* if we have 16-bit ints, we define INT_16; we will need %ld to printf an int32
* if we have 64-bit long, we define LONG_64
* If none is defined, we have int = long = 32 bit, and use %d to printf an int32
*/
#include <limits.h>
#if INT_MAX < 40000
# define INT_16
#else
# if LONG_MAX > INT_MAX
# define LONG_64
# endif
#endif
#ifdef BYTE_ORDER
#ifdef LITTLE_ENDIAN
# if BYTE_ORDER == LITTLE_ENDIAN
# define INTEL_BYTE_ORDER
# endif
#endif
#endif
#ifdef INT_16
typedef long int32;
typedef unsigned long uint32;
typedef int int16;
typedef double REAL8; /* real with at least 64 bit precision */
typedef long INT4; /* signed integer with at least 32 bit precision */
typedef unsigned long UINT4;
/* unsigned integer with at least 32 bit precision */
typedef int AS_BOOL;
typedef unsigned int UINT2; /* unsigned 16 bits */
# define ABS4 labs /* abs function for long */
#else
typedef int int32;
typedef long long int64;
typedef unsigned int uint32;
typedef short int16;
typedef double REAL8; /* real with at least 64 bit precision */
typedef int INT4; /* signed integer with at least 32 bit precision */
typedef unsigned int UINT4;
/* unsigned integer with at least 32 bit precision */
typedef int AS_BOOL;
typedef unsigned short UINT2; /* unsigned 16 bits */
# define ABS4 abs /* abs function for long */
#endif
#if MSDOS
# ifdef TURBO_C
# include <alloc.h> /* MSC needs malloc ! */
# else
# include <malloc.h>
# endif
# define SIGALRM SIGINT
#endif
#ifndef TRUE
# define TRUE 1
# define FALSE 0
#endif
#ifndef OK
# define OK (0)
# define ERR (-1)
#endif
/* hack because UCHAR is already used by mingw gcc */
#ifdef __GNUC__
#ifdef _WIN32
#define UCHAR SWE_UCHAR
#endif
#endif
typedef unsigned char UCHAR;
#define UCP (UCHAR*)
#define SCP (char*)
# define ODEGREE_STRING "°" /* degree as string, utf8 encoding */
#ifndef HUGE
# define HUGE 1.7E+308 /* biggest value for REAL8 */
#endif
#ifndef M_PI
# define M_PI 3.14159265358979323846
#endif
/* #define forward static obsolete */
#define AS_MAXCH 256 /* used for string declarations, allowing 255 char+\0 */
/*
#define DEGTORAD 0.0174532925199433
#define RADTODEG 57.2957795130823
*/
#define RADTODEG (180.0 / M_PI)
#define DEGTORAD (M_PI / 180.0)
typedef int32 centisec; /* centiseconds used for angles and times */
#define CS (centisec) /* use for casting */
#define CSEC centisec /* use for typing */
#define DEG 360000 /* degree expressed in centiseconds */
#define DEG7_30 (2700000) /* 7.5 degrees */
#define DEG15 (15 * DEG)
#define DEG24 (24 * DEG)
#define DEG30 (30 * DEG)
#define DEG60 (60 * DEG)
#define DEG90 (90 * DEG)
#define DEG120 (120 * DEG)
#define DEG150 (150 * DEG)
#define DEG180 (180 * DEG)
#define DEG270 (270 * DEG)
#define DEG360 (360 * DEG)
/* #define CSTORAD 4.84813681109536E-08 centisec to rad: pi / 180 /3600/100 */
/* #define RADTOCS 2.06264806247096E+07 rad to centisec 180*3600*100/pi */
#define CSTORAD (DEGTORAD / 360000.0)
#define RADTOCS (RADTODEG * 360000.0)
#define CS2DEG (1.0/360000.0) /* centisec to degree */
/* control strings for fopen() */
#if UNIX_FS
# define BFILE_R_ACCESS "r" /* open binary file for reading */
# define BFILE_RW_ACCESS "r+" /* open binary file for writing and reading */
# define BFILE_W_CREATE "w" /* create/open binary file for write*/
# define BFILE_A_ACCESS "a+" /* create/open binary file for append*/
# define FILE_R_ACCESS "r" /* open text file for reading */
# define FILE_RW_ACCESS "r+" /* open text file for writing and reading */
# define FILE_W_CREATE "w" /* create/open text file for write*/
# define FILE_A_ACCESS "a+" /* create/open text file for append*/
# define O_BINARY 0 /* for open(), not defined in Unix */
# define OPEN_MODE 0666 /* default file creation mode */
# define DIR_GLUE "/" /* glue string for directory/file */
# define PATH_SEPARATOR ";:" /* semicolon or colon may be used */
#else
# define BFILE_R_ACCESS "rb" /* open binary file for reading */
# define BFILE_RW_ACCESS "r+b" /* open binary file for writing and reading */
# define BFILE_W_CREATE "wb" /* create/open binary file for write*/
# define BFILE_A_ACCESS "a+b" /* create/open binary file for append*/
# define PATH_SEPARATOR ";" /* semicolon as PATH separator */
# define OPEN_MODE 0666 /* default file creation mode */
# ifdef MACOS
# define FILE_R_ACCESS "r" /* open text file for reading */
# define FILE_RW_ACCESS "r+" /* open text file for writing and reading */
# define FILE_W_CREATE "w" /* create/open text file for write*/
# define FILE_A_ACCESS "a+" /* create/open text file for append*/
# define DIR_GLUE ":" /* glue string for directory/file */
# else
# define FILE_R_ACCESS "rt" /* open text file for reading */
# define FILE_RW_ACCESS "r+t" /* open text file for writing and reading */
# define FILE_W_CREATE "wt" /* create/open text file for write*/
# define FILE_A_ACCESS "a+t" /* create/open text file for append*/
/* attention, all backslashes for msdos directry names must be written as \\,
because it is the C escape character */
# define DIR_GLUE "\\" /* glue string for directory/file */
# endif
#endif
#include <string.h>
#include <ctype.h>
#endif /* _SWEODEF_INCLUDED */
#endif /* _OURDEF_INCLUDED */

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# Before `make install' is performed this script should be runnable with
# `make test'. After `make install' it should work as `perl SwissEph.t'
use Test::More tests => 248;
BEGIN { use_ok("SwissEph") };
#------------------------------------------------------------------------
# Sun for 2451544.5 ET : Longitude should be 279.858461
#------------------------------------------------------------------------
my $ref;
my $i;
my @xx;
my $serr="";
#------------------------------------------------------------------------
# Coordinate transformation
#------------------------------------------------------------------------
# ecliptic -> equator
my @rade = SwissEph::swe_cotrans([80, 5, 0], -23);
is(round_4($rade[0]), 78.7418, "swe_cotrans([80, 5, 0], -23) -> ra");
is(round_4($rade[1]), 27.6169, "swe_cotrans([80, 5, 0], -23) -> de");
# with speed
@rade = SwissEph::swe_cotrans_sp([80, 5, 0, 1, 0, 0], -23);
is(round_4($rade[0]), 78.7418, "swe_cotrans([80, 5, 0], -23) -> ra");
is(round_4($rade[1]), 27.6169, "swe_cotrans([80, 5, 0], -23) -> de");
is(round_4($rade[3]), 1.1210, "swe_cotrans([80, 5, 0], -23) -> ra_speed");
is(round_4($rade[4]), 0.0763, "swe_cotrans([80, 5, 0], -23) -> de_speed");
#------------------------------------------------------------------------
# Function Delta T - values may change, but the seconds for 2000-1-1 are sure
#------------------------------------------------------------------------
is( round_4(SwissEph::swe_deltat( 2451545 )* 86400), 63.8289, "swe_deltat(1 jan 2000)");
$ref = SwissEph::swe_deltat_ex(2451545, SwissEph::SEFLG_MOSEPH);
is(round_4($ref->{dt} *86400.0), 63.8289, "swe_deltat_ex(1 jan 2000)");
#------------------------------------------------------------------------
# Sidereal Time
#------------------------------------------------------------------------
is(round_4( SwissEph::swe_sidtime( 2451544.5 )), 6.6643, "swe_sidtime(1 jan 2000)");
is(round_4( SwissEph::swe_sidtime0( 2451544.5, 23.5, 0)), 6.6645, "swe_sidtime0(1 jan 2000,23.5,0)");
$ref = SwissEph::swe_time_equ(2415020.5);
is($ref->{retval}, 0, "swe_time_equ(1 jan 1900)->retval");
if (exists($ref->{serr})) {
print STDERR "swe_time_equ(1 jan 1900)->serr = $ref->{serr}\n";
}
is(round_4($ref->{time_equ}), -0.0023, "swe_time_equ(1 jan 1900)->time_equ");
$ref = SwissEph::swe_lat_to_lmt(-146780.0, 82.2);
if (exists($ref->{serr})) {
print STDERR "swe_time_equ(1 jan 1900)->serr = $ref->{serr}\n";
}
is(round_4($ref->{tjd_lmt}), -146779.9898, "swe_lat_to_lmt(-146780.0, 82.2)->tjd_lmt");
$ref = SwissEph::swe_lmt_to_lat(-146779.9898, 82.2);
if (exists($ref->{serr})) {
print STDERR "swe_time_equ(1 jan 1900)->serr = $ref->{serr}\n";
}
is(round_4($ref->{tjd_lat}), -146779.9998, "swe_lmt_to_lat(-146779.986742931, 82.2)->tjd_lat");
#------------------------------------------------------------------------
# Calendar conversion
#------------------------------------------------------------------------
is( SwissEph::swe_julday(2000,1,1,0.), 2451544.5, "swe_julday() 1 jan 2000");
is( SwissEph::swe_julday(2000,1,1,0.,1), 2451544.5, "swe_julday() 1 jan 2000, explicit greg flag");
is( SwissEph::swe_julday(2000,1,1,0.,0), 2451557.5, "swe_julday() 1 jan 2000, explicit jul flag");
$ref = SwissEph::swe_revjul(2436723.5888888889,1);
is($ref->{iyar}, 1959, "swe_revjul(2436723.5888888889), year");
is($ref->{imon}, 6, "swe_revjul(2436723.5888888889), month");
is($ref->{iday}, 4, "swe_revjul(2436723.5888888889), day");
is($ref->{ihou}, 2, "swe_revjul(2436723.5888888889), hour");
is($ref->{imin}, 8, "swe_revjul(2436723.5888888889), minute");
is($ref->{isec}, 0, "swe_revjul(2436723.5888888889), second");
is(round_4($ref->{dhou}), 2.1333, "swe_revjul(2436723.5888888889), hour/decimal");
#------------------------------------------------------------------------
# Wrapper for swe_houses
#------------------------------------------------------------------------
$ref = SwissEph::swe_houses( 2451544.5, 52., 7., "P");
is( round_4( $ref->{cusps}->[1] ), 191.8825, "swe_houses()->{1}");
is( round_4( $ref->{cusps}->[2] ), 217.0327, "swe_houses()->{2}");
is( round_4( $ref->{cusps}->[3] ), 248.4837, "swe_houses()->{3}");
is( round_4( $ref->{cusps}->[4] ), 285.6359, "swe_houses()->{4}");
is( round_4( $ref->{cusps}->[5] ), 321.0151, "swe_houses()->{5}");
is( round_4( $ref->{cusps}->[6] ), 349.6374, "swe_houses()->{6}");
is( round_4( $ref->{cusps}->[7] ), 11.8825, "swe_houses()->{7}");
is( round_4( $ref->{cusps}->[8] ), 37.0327, "swe_houses()->{8}");
is( round_4( $ref->{cusps}->[9] ), 68.4837, "swe_houses()->{9}");
is( round_4( $ref->{cusps}->[10] ), 105.6359, "swe_houses()->{10}");
is( round_4( $ref->{cusps}->[11] ), 141.0151, "swe_houses()->{11}");
is( round_4( $ref->{cusps}->[12] ), 169.6374, "swe_houses()->{12}");
is( round_4( $ref->{asc} ), 191.8825, "swe_houses()->{asc}");
is( round_4( $ref->{mc} ), 105.6359, "swe_houses()->{mc}");
is( round_4( $ref->{armc} ), 106.9642, "swe_houses()->{armc}");
is( round_4( $ref->{vertex} ), 27.2378, "swe_houses()->{vertex}");
is( round_4( $ref->{equasc} ), 198.3910, "swe_houses()->{equasc}");
is( round_4( $ref->{coasc1} ), 218.3740, "swe_houses()->{coasc1}");
is( round_4( $ref->{coasc2} ), 193.7952, "swe_houses()->{coasc2}");
is( round_4( $ref->{polasc} ), 38.3740, "swe_houses()->{polasc}");
$ref = SwissEph::swe_houses_armc( 106.96424825, 52., 23.4376796111111, "P");
is( round_4( $ref->{cusps}->[1] ), 191.8825, "swe_houses_armc()->{1}");
is( round_4( $ref->{cusps}->[2] ), 217.0327, "swe_houses_armc()->{2}");
is( round_4( $ref->{cusps}->[3] ), 248.4837, "swe_houses_armc()->{3}");
is( round_4( $ref->{cusps}->[4] ), 285.6359, "swe_houses_armc()->{4}");
is( round_4( $ref->{cusps}->[5] ), 321.0151, "swe_houses_armc()->{5}");
is( round_4( $ref->{cusps}->[6] ), 349.6374, "swe_houses_armc()->{6}");
is( round_4( $ref->{cusps}->[7] ), 11.8825, "swe_houses_armc()->{7}");
is( round_4( $ref->{cusps}->[8] ), 37.0327, "swe_houses_armc()->{8}");
is( round_4( $ref->{cusps}->[9] ), 68.4837, "swe_houses_armc()->{9}");
is( round_4( $ref->{cusps}->[10] ), 105.6359, "swe_houses_armc()->{10}");
is( round_4( $ref->{cusps}->[11] ), 141.0151, "swe_houses_armc()->{11}");
is( round_4( $ref->{cusps}->[12] ), 169.6374, "swe_houses_armc()->{12}");
is( round_4( $ref->{asc} ), 191.8825, "swe_houses_armc()->{asc}");
is( round_4( $ref->{mc} ), 105.6359, "swe_houses_armc()->{mc}");
is( round_4( $ref->{armc} ), 106.9642, "swe_houses_armc()->{armc}");
is( round_4( $ref->{vertex} ), 27.2378, "swe_houses_armc()->{vertex}");
is( round_4( $ref->{equasc} ), 198.3910, "swe_houses_armc()->{equasc}");
is( round_4( $ref->{coasc1} ), 218.3740, "swe_houses_armc()->{coasc1}");
is( round_4( $ref->{coasc2} ), 193.7952, "swe_houses_armc()->{coasc2}");
is( round_4( $ref->{polasc} ), 38.3740, "swe_houses_armc()->{polasc}");
$ref = SwissEph::swe_houses_ex( 2451544.5, 0, 52., 7., "P");
is( round_4( $ref->{cusps}->[1] ), 191.8825, "swe_houses_ex()->{1}");
is( round_4( $ref->{cusps}->[2] ), 217.0327, "swe_houses_ex()->{2}");
is( round_4( $ref->{cusps}->[3] ), 248.4837, "swe_houses_ex()->{3}");
is( round_4( $ref->{cusps}->[4] ), 285.6359, "swe_houses_ex()->{4}");
is( round_4( $ref->{cusps}->[5] ), 321.0151, "swe_houses_ex()->{5}");
is( round_4( $ref->{cusps}->[6] ), 349.6374, "swe_houses_ex()->{6}");
is( round_4( $ref->{cusps}->[7] ), 11.8825, "swe_houses_ex()->{7}");
is( round_4( $ref->{cusps}->[8] ), 37.0327, "swe_houses_ex()->{8}");
is( round_4( $ref->{cusps}->[9] ), 68.4837, "swe_houses_ex()->{9}");
is( round_4( $ref->{cusps}->[10] ), 105.6359, "swe_houses_ex()->{10}");
is( round_4( $ref->{cusps}->[11] ), 141.0151, "swe_houses_ex()->{11}");
is( round_4( $ref->{cusps}->[12] ), 169.6374, "swe_houses_ex()->{12}");
is( round_4( $ref->{asc} ), 191.8825, "swe_houses_ex()->{asc}");
is( round_4( $ref->{mc} ), 105.6359, "swe_houses_ex()->{mc}");
is( round_4( $ref->{armc} ), 106.9642, "swe_houses_ex()->{armc}");
is( round_4( $ref->{vertex} ), 27.2378, "swe_houses_ex()->{vertex}");
is( round_4( $ref->{equasc} ), 198.3910, "swe_houses_ex()->{equasc}");
is( round_4( $ref->{coasc1} ), 218.3740, "swe_houses_ex()->{coasc1}");
is( round_4( $ref->{coasc2} ), 193.7952, "swe_houses_ex()->{coasc2}");
is( round_4( $ref->{polasc} ), 38.3740, "swe_houses_ex()->{polasc}");
$ref = SwissEph::swe_house_pos(290,47,23.5,"P",72,0);
is($ref->{retval}, 0, "swe_house_pos()->retval");
if (exists($ref->{serr})) {
print STDERR "swe_house_pos()->serr = $ref->{serr}\n";
}
is($ref->{ihno}, 2, "swe_house_pos()->ihno");
is(round_4($ref->{dhpos}), 2.1459, "swe_house_pos()->dhpos");
is(round_4($ref->{dhpos_deg}), 34.3767, "swe_house_pos()->dhpos_deg");
$ref = SwissEph::swe_gauquelin_sector(2436723.5888888889,SwissEph::SE_MOON,"",0,0,[8.6,47.35,400],1013,15);
is($ref->{retval}, 0, "swe_gauquelin_sector()->retval");
if (exists($ref->{serr})) {
print STDERR "swe_gauquelin_sector(1 jan 1900)->serr = $ref->{serr}\n";
}
is(round_4($ref->{dsector}), 36.1724, "swe_gauquelin_sector()->dsector");
#------------------------------------------------------------------------
# Wrapper for swe_calc
#------------------------------------------------------------------------
$ref = SwissEph::swe_calc(2415020.5, 3, 260);
is($ref->{retval}, 260, "swe_calc(1900, Venus)->retval");
if (exists($ref->{serr})) {
print STDERR "swe_calc(1900, Venus)->serr = $ref->{serr}\n";
}
is(round_4($ref->{xx}->[0]), 306.3745, "swe_calc(1900, Venus)->xx[0]");
is(round_4($ref->{xx}->[1]), -1.6830, "swe_calc(1900, Venus)->xx[1]");
is(round_4($ref->{xx}->[2]), 1.4646, "swe_calc(1900, Venus)->xx[2]");
is(round_4($ref->{xx}->[3]), 1.2435, "swe_calc(1900, Venus)->xx[3]");
my $dt = SwissEph::swe_deltat(2415020.5);
$ref = SwissEph::swe_calc_ut(2415020.5-$dt, 3, 260);
is($ref->{retval}, 260, "swe_calc_ut(1900, Venus)->retval");
if (exists($ref->{serr})) {
print STDERR "swe_calc_ut(1900, Venus)->serr = $ref->{serr}\n";
}
is(round_4($ref->{xx}->[0]), 306.3745, "swe_calc_ut(1900, Venus)->xx[0]");
is(round_4($ref->{xx}->[1]), -1.6830, "swe_calc_ut(1900, Venus)->xx[1]");
is(round_4($ref->{xx}->[2]), 1.4646, "swe_calc_ut(1900, Venus)->xx[2]");
is(round_4($ref->{xx}->[3]), 1.2435, "swe_calc_ut(1900, Venus)->xx[3]");
#print STDERR "swe_calc_ut $ref->{xx}->[0] $ref->{xx}->[1]\n";
#------------------------------------------------------------------------
# Wrapper for swe_fixstar
#------------------------------------------------------------------------
$ref = SwissEph::swe_fixstar_mag("alcyone");
is($ref->{retval}, 0, "swe_fixstar_mag(Alcyone)->retval");
if (exists($ref->{serr})) {
print STDERR "swe_fixstar_mag(Alcyone)->serr = $ref->{serr}\n";
}
is($ref->{starname}, "Alcyone,etTau", "swe_fixstar_mag(Alcyone)->starname");
is(round_4($ref->{dmag}), 2.87, "swe_fixstar_mag(Alcyone)->dmag");
$ref = SwissEph::swe_fixstar("alcyone", 2415020.5, 4);
is($ref->{retval}, 4, "swe_fixstar(1900, Alcyone)->retval");
if (exists($ref->{serr})) {
print STDERR "swe_fixstar(1900, Alcyone)->serr = $ref->{serr}\n";
}
is($ref->{starname}, "Alcyone,etTau", "swe_fixstar(1900, Alcyone)->starname");
is(round_4($ref->{xx}->[0]), 58.6052, "swe_fixstar(1900, Alcyone)->xx[0]");
is(round_4($ref->{xx}->[2]), 25496153.13, "swe_fixstar(1900, Alcyone)->xx[2]");
$ref = SwissEph::swe_fixstar_ut("alcyone", 2415020.5-SwissEph::swe_deltat(2415020.5), 4);
is($ref->{retval}, 4, "swe_fixstar_ut(1900, Alcyone)->retval");
if (exists($ref->{serr})) {
print STDERR "swe_fixstar_ut(1900, Alcyone)->serr = $ref->{serr}\n";
}
is($ref->{starname}, "Alcyone,etTau", "swe_fixstar_ut(1900, Alcyone)->starname");
is(round_4($ref->{xx}->[0]), 58.6052, "swe_fixstar_ut(1900, Alcyone)->xx[0]");
is(round_4($ref->{xx}->[2]), 25496153.13, "swe_fixstar_ut(1900, Alcyone)->xx[2]");
$ref = SwissEph::swe_fixstar2("alcyone", 2415020.5, 4);
is($ref->{retval}, 4, "swe_fixstar2(1900, Alcyone)->retval");
if (exists($ref->{serr})) {
print STDERR "swe_fixstar2(1900, Alcyone)->serr = $ref->{serr}\n";
}
is($ref->{starname}, "Alcyone,etTau", "swe_fixstar2(1900, Alcyone)->starname");
is(round_4($ref->{xx}->[0]), 58.6052, "swe_fixstar2(1900, Alcyone)->xx[0]");
is(round_4($ref->{xx}->[2]), 25496153.13, "swe_fixstar2(1900, Alcyone)->xx[2]");
$ref = SwissEph::swe_fixstar2_ut("alcyone", 2415020.5-SwissEph::swe_deltat(2415020.5), 4);
is($ref->{retval}, 4, "swe_fixstar2_ut(1900, Alcyone)->retval");
if (exists($ref->{serr})) {
print STDERR "swe_fixstar2_ut(1900, Alcyone)->serr = $ref->{serr}\n";
}
is($ref->{starname}, "Alcyone,etTau", "swe_fixstar2_ut(1900, Alcyone)->starname");
is(round_4($ref->{xx}->[0]), 58.6052, "swe_fixstar2_ut(1900, Alcyone)->xx[0]");
is(round_4($ref->{xx}->[2]), 25496153.13, "swe_fixstar2_ut(1900, Alcyone)->xx[2]");
$ref = SwissEph::swe_fixstar2_mag("alcyone");
is($ref->{retval}, 0, "swe_fixstar2_mag(Alcyone)->retval");
if (exists($ref->{serr})) {
print STDERR "swe_fixstar2_mag(Alcyone)->serr = $ref->{serr}\n";
}
is($ref->{starname}, "Alcyone,etTau", "swe_fixstar2_mag(Alcyone)->starname");
is(round_4($ref->{dmag}), 2.87, "swe_fixstar2_mag(Alcyone)->dmag");
$ref = SwissEph::swe_pheno(2415020.5, 3, 4);
is($ref->{retval}, 4, "swe_pheno(1900, Venus)->retval");
if (exists($ref->{serr})) {
print STDERR "swe_pheno(1900, Venus)->serr = $ref->{serr}\n";
}
is(round_4($ref->{phase_angle}), 36.7449, "swe_pheno(1900, Venus)->phase_angle");
is(round_4($ref->{phase}), 0.9007, "swe_pheno(1900, Venus)->phase");
is(round_4($ref->{elongation}), 26.2712, "swe_pheno(1900, Venus)->elongation");
is(round_4($ref->{disc_diameter}), 0.0032, "swe_pheno(1900, Venus)->disc_diameter");
is(round_4($ref->{magnitude}), -3.9102, "swe_pheno(1900, Venus)->magnitude");
is(round_4($ref->{hor_parallax}), 0, "swe_pheno(1900, Venus)->hor_parallax");
is(round_4($ref->{attr}->[0]), 36.7449, "swe_pheno(1900, Venus)->attr[0]");
$ref = SwissEph::swe_pheno_ut(2415020.5 - SwissEph::swe_deltat(2415020.5), 3, 4);
is($ref->{retval}, 4, "swe_pheno_ut(1900, Venus)->retval");
if (exists($ref->{serr})) {
print STDERR "swe_pheno_ut(1900, Venus)->serr = $ref->{serr}\n";
}
is(round_4($ref->{phase_angle}), 36.7449, "swe_pheno_ut(1900, Venus)->phase_angle");
is(round_4($ref->{phase}), 0.9007, "swe_pheno_ut(1900, Venus)->phase");
is(round_4($ref->{elongation}), 26.2712, "swe_pheno_ut(1900, Venus)->elongation");
is(round_4($ref->{disc_diameter}), 0.0032, "swe_pheno_ut(1900, Venus)->disc_diameter");
is(round_4($ref->{magnitude}), -3.9102, "swe_pheno_ut(1900, Venus)->magnitude");
is(round_4($ref->{hor_parallax}), 0, "swe_pheno_ut(1900, Venus)->hor_parallax");
is(round_4($ref->{attr}->[0]), 36.7449, "swe_pheno_ut(1900, Venus)->attr[0]");
#------------------------------------------------------------------------
# ayanamsha
#------------------------------------------------------------------------
is(round_4(SwissEph::swe_get_ayanamsa(2451544.5)), 24.7403, "swe_get_ayanamsa(2000)");
is(round_4(SwissEph::swe_get_ayanamsa_ut(2451544.5-SwissEph::swe_deltat(2451544.5))), 24.7403, "swe_get_ayanamsa(2000)");
$ref = SwissEph::swe_get_ayanamsa_ex(2451544.5, SwissEph::SEFLG_MOSEPH);
is(round_4($ref->{daya}),24.7364, "swe_get_ayanamsa_ex(2000)");
$ref = SwissEph::swe_get_ayanamsa_ex_ut(2451544.5, SwissEph::SEFLG_MOSEPH);
is(round_4($ref->{daya}),24.7364, "swe_get_ayanamsa_ex(2000)");
is(SwissEph::swe_get_ayanamsa_name(3), "Raman", "swe_get_ayanamsa(Raman)");
is(SwissEph::swe_get_planet_name(SwissEph::SE_VENUS), "Venus", "swe_get_planet_name(Venus)");
#------------------------------------------------------------------------
# refraction, azimuth, and altitude, rise and transit
#------------------------------------------------------------------------
$ref = SwissEph::swe_refrac_extended(0.1,400,1013,15,0.02,1);
is($ref->{retval}, 0, "swe_refrac_extended()->retval");
if (exists($ref->{serr})) {
print STDERR "swe_refrac_extended()->serr = $ref->{serr}\n";
}
is(round_4($ref->{alt_true}), -0.4391, "swe_refrac_extended()->alt_true");
is(round_4($ref->{alt_apparent}), 0.1, "swe_refrac_extended()->alt_apparent");
is(round_4($ref->{refraction}), 0.5392, "swe_refrac_extended()->refraction");
is(round_4($ref->{dip}), -0.5238, "swe_refrac_extended()->dip");
is(round_4($ref->{dret}->[0]), -0.4391, "swe_refrac_extended()->dret[0]");
is(round_4(SwissEph::swe_refrac(0.6,1013,15,1)), 0.1441, "swe_refrac()");
@xx = SwissEph::swe_azalt(2436723.588888888,0,[8.55,47.35,0],1013,15,[252,0,1]);
is(round_4($xx[0]), 38.9512, "swe_azalt()->azimuth");
is(round_4($xx[1]), 10.8971, "swe_azalt()->alt_true");
is(round_4($xx[2]), 10.9771, "swe_azalt()->alt_apparent");
@xx = SwissEph::swe_azalt_rev(2436723.588888888,0,[8.55,47.35,0],\@xx);
is(round_4($xx[0]), 252, "swe_azalt_rev()->ecl_lon");
is(round_4($xx[1]), 0, "swe_azalt_rev()->ecl_lat");
$ref = SwissEph::swe_rise_trans(2415020.5,3,"", 4,0,[8.55,47.23,400],1013,15);
is($ref->{retval}, 0, "swe_rise_trans(1900, Venus)->retval");
if (exists($ref->{serr})) {
print STDERR "swe_rise_trans(1900, Venus)->serr = $ref->{serr}\n";
}
is(round_4($ref->{dret}), 2415020.8696, "swe_rise_trans(1900, Venus)->dret");
#------------------------------------------------------------------------
# eclipses and occultations
#------------------------------------------------------------------------
$ref = SwissEph::swe_lun_eclipse_how(2454517.643069,4,[278,0,0]);
is($ref->{retval}, 4, "swe_lun_eclipse_how(2008)->retval");
if (exists($ref->{serr})) {
print STDERR "swe_lun_eclipse_how(2008)->serr = $ref->{serr}\n";
}
is(round_4($ref->{mag_umbral}), 1.1059, "swe_lun_eclipse_how(2008)->mag_umbral");
is(round_4($ref->{mag_penumbral}), 2.1450, "swe_lun_eclipse_how(2008)->mag_penumbral");
is(round_4($ref->{attr}->[0]), 1.1059, "swe_lun_eclipse_how(2008)->attr[0]");
$ref = SwissEph::swe_sol_eclipse_how(2454503.663212,4,[-150.270493,-67.547072,0]);
is($ref->{retval}, 137, "swe_sol_eclipse_how(2008)->retval");
if (exists($ref->{serr})) {
print STDERR "swe_sol_eclipse_how(2008)->serr = $ref->{serr}\n";
}
is(round_4($ref->{disc_ratio}), 0.9658, "swe_sol_eclipse_how(2008)->disc_ratio");
is(round_4($ref->{fraction_diameter}), 0.9808, "swe_sol_eclipse_how(2008)->fraction_diameter");
is(round_4($ref->{fraction_disc}), 0.9327, "swe_sol_eclipse_how(2008)->fraction_disc");
is(round_4($ref->{core_shadow_km}), 123.5327, "swe_sol_eclipse_how(2008)->core_shadow_km");
is(round_4($ref->{sun_azimuth}), 88.5702, "swe_sol_eclipse_how(2008)->sun_azimuth");
is(round_4($ref->{sun_alt_true}), 16.2305, "swe_sol_eclipse_how(2008)->sun_alt_true");
is(round_4($ref->{separation_angle}), 0.0011, "swe_sol_eclipse_how(2008)->separation_angle");
$ref = SwissEph::swe_sol_eclipse_where(2454503.663212,4);
is($ref->{retval}, 9, "swe_sol_eclipse_where(2008)->retval");
if (exists($ref->{serr})) {
print STDERR "swe_sol_eclipse_where(2008)->serr = $ref->{serr}\n";
}
is(round_4($ref->{geopos}->[0]), -150.3452, "swe_sol_eclipse_where(2008)->geopos[0]");
is(round_4($ref->{geopos}->[1]), -67.5477, "swe_sol_eclipse_where(2008)->geopos[1]");
is(round_4($ref->{disc_ratio}), 0.9658, "swe_sol_eclipse_where(2008)->disc_ratio");
is(round_4($ref->{fraction_diameter}), 0.9809, "swe_sol_eclipse_where(2008)->fraction_diameter");
is(round_4($ref->{fraction_disc}), 0.9327, "swe_sol_eclipse_where(2008)->fraction_disc");
is(round_4($ref->{core_shadow_km}), 123.5327, "swe_sol_eclipse_where(2008)->core_shadow_km");
is(round_4($ref->{sun_azimuth}), 88.6393, "swe_sol_eclipse_where(2008)->sun_azimuth");
is(round_4($ref->{sun_alt_true}), 16.2591, "swe_sol_eclipse_where(2008)->sun_alt_true");
is(round_4($ref->{separation_angle}), 0.0011, "swe_sol_eclipse_where(2008)->separation_angle");
$ref = SwissEph::swe_lun_occult_where(2454531.296945,SwissEph::SE_VENUS,"",4);
is($ref->{retval}, 5, "swe_lun_occult_where(2008)->retval");
if (exists($ref->{serr})) {
print STDERR "swe_lun_occult_where(2008)->serr = $ref->{serr}\n";
}
is(round_4($ref->{geopos}->[0]), -132.4299, "swe_lun_occult_where(2008)->geopos[0]");
is(round_4($ref->{geopos}->[1]), -3.2154, "swe_lun_occult_where(2008)->geopos[1]");
is(round_4($ref->{disc_ratio}), 172.5202, "swe_lun_occult_where(2008)->disc_ratio");
is(rou