15793453064

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Add support for touch clicks and moves

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/src/core/StelUtils.hpp

/*
 * Stellarium
 * Copyright (C) 2002 Fabien Chereau
 *
 * 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 2
 * of the License, 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., 51 Franklin Street, Suite 500, Boston, MA  02110-1335, USA.
 */

#ifndef STELUTILS_HPP
#define STELUTILS_HPP

#include <cmath>
#include "VecMath.hpp"

#include <QVariantMap>
#include <QDateTime>
#include <QString>

// astronomical unit (km)
#define AU 149597870.691
#define AUf 149597870.691f
#define AU_KM (1.0/149597870.691)
#define AU_KMf (1.0f/149597870.691f)
// Parsec (km)
#define PARSEC 30.857e12
// Parsec (LY)
#define PARSEC_LY 3.261563777
// speed of light (km/sec)
#define SPEED_OF_LIGHT 299792.458
// Ecliptic obliquity of J2000.0, degrees
#define EPS_0 23.4392803055555555555556
// Equatorial radius of the Earth in km (WGS-84)
#define EARTH_RADIUS 6378.1366
// Equatorial radius of the Sun in km
#define SUN_RADIUS 696000.
// Equatorial radius of the Moon in km
#define MOON_RADIUS 1738.
// 1 mas to 1 radian, is M_PI / (3600000. * 180.)
#define MAS2RAD 4.8481368110953594e-9
// julian year in seconds that is 365.25 * 86400.
#define JYEAR_SECONDS 31557600.0

// Add a few frequently used extra math-type literals
#ifndef M_PI_180
        #define M_PI_180    (M_PI/180.)
#endif
#ifndef M_180_PI
        #define M_180_PI    (180./M_PI)
#endif
// Add some math literals in float version to avoid many static_casts
#ifndef M_PIf
        #define M_PIf       3.14159265358979323846f   // pi
#endif
#ifndef M_PI_2f
        #define M_PI_2f     1.57079632679489661923f   // pi/2
#endif
#ifndef M_PI_4f
        #define M_PI_4f     0.785398163397448309616f  // pi/4
#endif
#ifndef M_1_PIf
        #define M_1_PIf     0.318309886183790671538f  // 1/pi
#endif
#ifndef M_2_PIf
        #define M_2_PIf     0.636619772367581343076f  // 2/pi
#endif
#ifndef M_PI_180f
        #define M_PI_180f   (M_PIf/180.f)
#endif
#ifndef M_180_PIf
        #define M_180_PIf   (180.f/M_PIf)
#endif

#define stelpow10f(x) std::exp((x) * 2.3025850930f)

#define L1S(x) QLatin1String(x)

// Allow parallel evaluation of std::transform_reduce(std::execution::par, ...) or
// std::sort(std::execution::par, ...) where known. Not all compilers know it.
// Use std::transform_reduce(STD_EXECUTION_PAR_COMMA ...) for the general case.
#if STD_EXECUTION_KNOWN
# define STD_EXECUTION_PAR_COMMA std::execution::par,
#else
# define STD_EXECUTION_PAR_COMMA
#endif

constexpr double DEFAULT_FONT_SIZE = 13;

//! @namespace StelUtils contains general purpose utility functions.
namespace StelUtils
{
        static inline constexpr double J2000 = 2451545.0;

        //! Return the full name of stellarium, i.e. "Stellarium 23.1"
        QString getApplicationName();

        //! Return the version of stellarium, i.e. "23.1.0"
        QString getApplicationVersion();

        //! Return the public version of stellarium, i.e. "23.1"
        QString getApplicationPublicVersion();

        //! Return the series of stellarium, i.e. "23.0"
        QString getApplicationSeries();

        //! Return the name and the version of operating system, i.e. "macOS 12.5"
        QString getOperatingSystemInfo();

        //! Return the user agent name, i.e. "Stellarium/0.15.0 (Linux)"
        QString getUserAgentString();

        //! Return the addressing mode string, i.e. "64-bit"
        QString getAddressingMode();

        /*! \brief Get a long integer from a JSON value
         *
         *  QJsonValue stores JSON numbers as double-precision floating-point values. This means
         *  that numbers greater than 2^53-1 will be rounded, which is unacceptable for e.g. ids
         *  like those of the Gaia catalog.
         *  This function supports, in addition to normal JSON numbers, also representations of
         *  numbers by JSON strings. If the value passed is a JSON string, it will be parsed to a
         *  number. If it's a JSON number less than 2^53, it will be returned as is. Otherwise it
         *  will return 0, as QJsonValue's getters would in case of a type mismatch.
         */
        qint64 getLongLong(const class QJsonValue& v);

        inline const QString getEndLineChar() {
                #ifdef Q_OS_WIN
                const QString stelEndl="\r\n";
                #else
                const QString stelEndl="\n";
                #endif
                return stelEndl;
        }

        //! Convert hours, minutes, seconds to decimal hours
        inline double hmsToHours(const unsigned int h, const unsigned int m, const double s){
                return static_cast<double>(h)+static_cast<double>(m)/60.+s/3600.;
        }

        //! Convert an angle in hms format to radian.
        //! @param h hour component
        //! @param m minute component
        //! @param s second component
        //! @return angle in radian
        inline double hmsToRad(const unsigned int h, const unsigned int m, const double s){
                return hmsToHours(h, m, s)*M_PI/12.;
        }

        //! Convert an angle in +-dms format to radian.
        //! @param d degree component
        //! @param m arcmin component
        //! @param s arcsec component
        //! @return angle in radian
        inline double dmsToRad(const int d, const unsigned int m, const double s){
                double rad = M_PI_180*qAbs(d)+M_PI/10800.*m+s*M_PI/648000.;
                return (d<0 ? -rad : rad);
        }

        //! Convert an angle in radian to hms format.
        //! @param rad input angle in radian
        //! @param h hour component
        //! @param m minute component
        //! @param s second component
        void radToHms(double rad, unsigned int& h, unsigned int& m, double& s);

        //! Convert an angle in radian to +-dms format.
        //! @param rad input angle in radian
        //! @param sign true if positive, false otherwise
        //! @param d degree component
        //! @param m minute component
        //! @param s second component
        void radToDms(double rad, bool& sign, unsigned int& d, unsigned int& m, double& s);

        //! Convert an angle in radian to decimal degree.
        //! @param rad input angle in radian
        //! @param sign true if positive, false otherwise
        //! @param deg decimal degree
        Q_DECL_DEPRECATED_X("just use rad*M_180_PI instead")
        void radToDecDeg(double rad, bool& sign, double& deg);

        //! Convert an angle in radian to a decimal degree string.
        //! @param angle input angle in radian
        //! @param precision
        //! @param useD Define if letter "d" must be used instead of deg sign
        //! @param positive Define if function should use 0-360 degrees
        QString radToDecDegStr(const double angle, const int precision = 4, const bool useD=false, const bool positive=false);

        //! Convert an angle in radian to a hms formatted string.
        //! If the second, minute part is == 0, it is not output
        //! @param angle input angle in radian
        QString radToHmsStrAdapt(const double angle);

        //! Convert an angle in radian to a hms formatted string.
        //! @param angle input angle in radian
        //! @param decimal output decimal second value
        QString radToHmsStr(const double angle, const bool decimal=false);

        //! Convert an angle in radian to a dms formatted string.
        //! If the second, minute part is == 0, it is not output
        //! @param angle input angle in radian
        //! @param useD Define if letter "d" must be used instead of deg sign
        QString radToDmsStrAdapt(const double angle, const bool useD=false);

        //! Convert an angle in radian to a dms formatted string.
        //! @param angle input angle in radian        
        //! @param decimal output second value with decimal fraction
        //! @param useD Define if letter "d" must be used instead of deg sign
        QString radToDmsStr(const double angle, const bool decimal=false, const bool useD=false);

        //! Convert an angle in radian to a dms formatted string.
        //! @param angle input angle in radian
        //! @param precision
        //! @param useD Define if letter "d" must be used instead of deg sign
        QString radToDmsPStr(const double angle, const int precision = 0, const bool useD=false);

        //! Convert an angle in decimal degree to +-dms format.
        //! @param angle input angle in decimal degree
        //! @param sign true if positive, false otherwise
        //! @param d degree component
        //! @param m minute component
        //! @param s second component
        void decDegToDms(double angle, bool& sign, unsigned int& d, unsigned int& m, double& s);

        //! Convert an angle in decimal degrees to a dms formatted string.
        //! @param angle input angle in decimal degrees
        QString decDegToDmsStr(const double angle);

        //! Convert latitude in decimal degrees to a dms formatted string or use decimal values.
        //! @param latitude in decimal degrees
        //! @param dms set true to use DMS formatted string
        QString decDegToLatitudeStr(const double latitude, bool dms = true);

        //! Convert longitude in decimal degrees to a dms formatted string.
        //! @param longitude in decimal degrees
        //! @param eastPositive set true to counting East direction positive
        //! @param semiSphere set true to use -180..180 degrees range (0..360 degrees otherwise)
        //! @param dms set true to use DMS formatted string
        QString decDegToLongitudeStr(const double longitude, bool eastPositive = true, bool semiSphere = true, bool dms = true);

        //! Convert a dms formatted string to an angle in radian
        //! @param s The input string
        double dmsStrToRad(const QString& s);

        //! Convert from spherical coordinates to Rectangular direction.
        //! @param lng longitude in radian
        //! @param lat latitude in radian
        //! @param v the resulting 3D unit vector
        inline void spheToRect(const double lng, const double lat, Vec3d& v){
                const double cosLat = cos(lat);
                v.set(cos(lng) * cosLat, sin(lng) * cosLat, sin(lat));
        }

        //! Convert from spherical coordinates to Rectangular direction.
        //! @param lng longitude in radian
        //! @param lat latitude in radian
        //! @param v the resulting 3D unit vector
        inline void spheToRect(const float lng, const float lat, Vec3f& v){
                const double dlng = static_cast<double>(lng), dlat = static_cast<double>(lat), cosLat = cos(dlat);
                v.set(static_cast<float>(cos(dlng) * cosLat), static_cast<float>(sin(dlng) * cosLat), sinf(lat));
        }

        //! Convert from spherical coordinates to Rectangular direction.
        //! @param lng longitude in radian
        //! @param lat latitude in radian
        //! @param v the resulting 3D unit vector
        inline void spheToRect(const double lng, const double lat, Vec3f& v){
                const float cosLat = cos(static_cast<float>(lat));
                v.set(cos(static_cast<float>(lng)) * cosLat, sin(static_cast<float>(lng)) * cosLat, sin(static_cast<float>(lat)));
        }

        //! Convert from spherical coordinates to Rectangular direction.
        //! @param lng longitude in radian
        //! @param lat latitude in radian
        //! @param v the resulting 3D unit vector
        inline void spheToRect(const float lng, const float lat, Vec3d& v){
                const double dlng = static_cast<double>(lng), dlat = static_cast<double>(lat), cosLat = cos(dlat);
                v.set(cos(dlng) * cosLat, sin(dlng) * cosLat, sin(dlat));
        }

        //! Convert from Rectangular direction to spherical coordinate components.
        //! @param lng double* to store longitude in radian [-pi, pi]
        //! @param lat double* to store latitude in radian
        //! @param v the input 3D vector
        inline void rectToSphe(double *lng, double *lat, const Vec3d& v){
                *lat = atan2(v[2], sqrt(v[0]*v[0] + v[1]*v[1]));
                *lng = atan2(v[1],v[0]);
        }

        //! Convert from Rectangular direction to spherical coordinate components.
        //! @param lng float* to store longitude in radian [-pi, pi]
        //! @param lat float* to store latitude in radian
        //! @param v the input 3D vector
        inline void rectToSphe(float *lng, float *lat, const Vec3d& v){
                *lng = static_cast<float>(atan2(v[1],v[0]));
                *lat = atan2(v[2], sqrt(v[0]*v[0] + v[1]*v[1]));
        }


        //! Convert from Rectangular direction to spherical coordinate components.
        //! @param lng float* to store longitude in radian [-pi, pi]
        //! @param lat float* to store latitude in radian
        //! @param v the input 3D vector
        inline void rectToSphe(float *lng, float *lat, const Vec3f& v){
                *lat = atan2(v[2], sqrt(v[0]*v[0] + v[1]*v[1]));
                *lng = atan2f(v[1],v[0]);
        }

        //! Convert from Rectangular direction to spherical coordinate components.
        //! @param lng double* to store longitude in radian [-pi, pi]
        //! @param lat double* to store latitude in radian
        //! @param v the input 3D vector
        inline void rectToSphe(double *lng, double *lat, const Vec3f &v){
                *lat = atan2(static_cast<double>(v[2]), sqrt(static_cast<double>(v[0]*v[0] + v[1]*v[1])));
                *lng = atan2(static_cast<double>(v[1]),static_cast<double>(v[0]));
        }

        //! Convert from spherical coordinates (including distance) to Rectangular direction.
        //! @param lng longitude in radian
        //! @param lat latitude in radian
        //! @param r length of radius vector (distance)
        //! @param v the resulting 3D unit vector
        inline void spheToRect(const double lng, const double lat, const double r, Vec3d& v){
                const double cosLat = cos(lat);
                v.set(cos(lng) * cosLat * r, sin(lng) * cosLat * r, sin(lat) * r);
        }

        //! Convert from Rectangular direction to spherical coordinate components (including distance).
        //! @param lng double* to store longitude in radian [-pi, pi]
        //! @param lat double* to store latitude in radian
        //! @param r double*   length of radius vector (distance)
        //! @param v the input 3D vector
        inline void rectToSphe(double *lng, double *lat, double *r, const Vec3d& v){
                *r = v.norm();
                *lat = atan2(v[2], sqrt(v[0]*v[0] + v[1]*v[1]));
                *lng = atan2(v[1],v[0]);
        }

        //! Coordinate Transformation from equatorial to ecliptical
        inline void equToEcl(const double raRad, const double decRad, const double eclRad, double *lambdaRad, double *betaRad){
                *lambdaRad=std::atan2(std::sin(raRad)*std::cos(eclRad)+std::tan(decRad)*std::sin(eclRad), std::cos(raRad));
                *betaRad=std::asin(std::sin(decRad)*std::cos(eclRad)-std::cos(decRad)*std::sin(eclRad)*std::sin(raRad));
        }

        //! Coordinate Transformation from ecliptical to equatorial
        inline void eclToEqu(const double lambdaRad, const double betaRad, const double eclRad, double *raRad, double *decRad){
                *raRad = std::atan2(std::sin(lambdaRad)*std::cos(eclRad)-std::tan(betaRad)*std::sin(eclRad), std::cos(lambdaRad));
                *decRad = std::asin(std::sin(betaRad)*std::cos(eclRad)+std::cos(betaRad)*std::sin(eclRad)*std::sin(lambdaRad));
        }

        //! Convert a string longitude, latitude, RA or declination angle
        //! to radians.
        //! @param str the angle in a format according to:
        //!   angle ::= [sign¹] ( real [degs | mins | secs]
        //!                     | [integer degs] ( [integer mins] real secs
        //!                                       | real mins )
        //!                     ) [cardinal¹]            
        //!   sign ::= + | -
        //!   digit := 0 | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9
        //!   integer ::= digit [digits]
        //!   real ::= integer [. integer]
        //!   degs ::= d | h² | U+00B0 | U+00BA³
        //!   mins ::= m | '
        //!   secs ::= s | "
        //!   cardinal ::= N² | S² | E | W
        //!   ¹) A cardinal point overrides any sign. N and E result in a positive,
        //!      W and S in a negative angle.
        //!   ²) The use of the cardinal points N and S together with the hour sign
        //!      'H' or 'h' is forbidden.
        //!   ³) The MASCULINE ORDINAL INDICATOR U+00BA is accepted, considering
        //!      Spanish QWERTY keyboards.
        //! The string is parsed without regarding to case, except that, after a
        //! single real, a solitary 's' indicates seconds whereas an 'S' indicates South.
        //! It is highly recommended to use lower case for hdms and upper case for NSEW.
        //! Latitude: North is positive, South is negative.
        //! Longitude: East is positive, West is negative.
        //! @return the angle in radians.
        double getDecAngle(const QString& str);

        //! Check if a number is a power of 2.
        inline bool isPowerOfTwo(const int value){
                return (value & -value) == value;
        }

        //! Return the smallest power of two greater than or equal to the given value.
        int getBiggerPowerOfTwo(int value);

        //! Return the largest power of two smaller than or equal to the given value
        int getSmallerPowerOfTwo(const int value);

        //! Return the inverse sinus hyperbolic of z.
        inline double asinh(const double z){
                return (z>0 ? std::log(z + std::sqrt(z*z+1)) :
                             -std::log(-z + std::sqrt(z*z+1)));
        }

        //! Integer modulo where the result is always nonnegative. [0..b-1]
        inline int imod(const int a, const int b){
                int ret = a % b;
                if(ret < 0)
                        ret+=b;
                return ret;
        }
        //! Integer modulo where the result is always positive. [1..b]
        inline int amod(const int a, const int b){
                int ret = a % b;
                if(ret <= 0)
                        ret+=b;
                return ret;
        }
        //! Integer interval modulo. [a..b)
        inline int amod(const int x, const int a, const int b){
                if (a==b)
                        return x;
                int ret = imod(x-a, b-a);
                return ret+a;
        }
        //! Double modulo where the result is always nonnegative. [0..(b
        inline double fmodpos(const double a, const double b){
                double ret = fmod(a, b);
                if(ret < 0)
                        ret+=b;
                return ret;
        }
        //! Float modulo where the result is always nonnegative. [0..(b
        inline float fmodpos(const float a, const float b){
                float ret = fmodf(a, b);
                if(ret < 0)
                        ret+=b;
                return ret;
        }

        //! Floor integer division provides truncating to the next lower integer, also for negative numerators.
        //! https://stackoverflow.com/questions/2622441/c-integer-floor-function
        //! @returns floor(num/den)
        inline int intFloorDiv (int num, int den)
        {
          if (0 < (num^den)) // lgtm [cpp/bitwise-sign-check]
            return num/den;
          else
            {
              ldiv_t res = ldiv(num,den);
              return (res.rem)? res.quot-1
                              : res.quot;
            }
        }

        //! version of intFloorDiv() for large integers.
        inline int intFloorDivLL(qint64 num, qint64 den)
        {
          if (0 < (num^den)) // lgtm [cpp/bitwise-sign-check]
            return int(num/den);
          else
            {
              lldiv_t res = lldiv(num,den);
              qint64 ret= (res.rem)? res.quot-1
                              : res.quot;
              return int(ret);
            }
        }

        ///////////////////////////////////////////////////
        // New Qt based General Calendar Functions.
        //! Extract from julianDay a year, month, day for the Julian Date julianDay represents.
        //! @attention Under rare circumstances with a rounded result where julianDay=*.49999999xyz this will still round off whereas the time is less than a fraction from midnight of the next day.
        //! Depending on circumstances this may matter or not. If you need a full decoding of a Julian day number, prefer to use getDateTimeFromJulianDay()
        void getDateFromJulianDay(const double julianDay, int *year, int *month, int *day);

        //! Extract from julianDay an hour, minute, second.
        //! @attention Under rare circumstances with a rounded result where julianDay=*.49999999xyz this will lead to a factual result for *.5000000abc, i.e. not 24 but 0 hours, and wrapDay will be true.
        //! Depending on circumstances this may matter or not. If you need a full decoding of a Julian day number, prefer to use getDateTimeFromJulianDay()
        void getTimeFromJulianDay(const double julianDay, int *hour, int *minute, int *second, int *millis=Q_NULLPTR, bool *wrapDay=Q_NULLPTR);

        //! Extract from julianDay a year, month, day, hour, minute, second and (optional) millisecond for the Julian Day julianDay represents.
        //! This is the preferred method of complete decoding of a Julian day number.
        void getDateTimeFromJulianDay(const double julianDay, int *year, int *month, int *day, int *hour, int *minute, int *second, int *millis=Q_NULLPTR);

        //! Make hours (decimal format) from julianDay
        double getHoursFromJulianDay(const double julianDay);

        //! Parse an ISO8601 date string.
        //! Also handles negative and distant years.
        bool getDateTimeFromISO8601String(const QString& iso8601Date, int* y, int* m, int* d, int* h, int* min, float* s);
        
        //! Format the given Julian Day in (UTC) ISO8601 date string.
        //! Also handles negative and distant years.
        QString julianDayToISO8601String(const double jd, bool addMS = false);

        //! Return the Julian Date matching the ISO8601 date string.
        //! Also handles negative and distant years.
        double getJulianDayFromISO8601String(const QString& iso8601Date, bool* ok);
        
        //! Format the date and day-of-week per the format in fmt
        //! (see QDateTime::toString()). Uses the @b system locale, not
        //! the one set in Stellarium.
        //! @return QString representing the formatted date
        QString localeDateString(const int year, const int month, const int day, const int dayOfWeek, const QString &fmt);

        //! Format the date and day-of-week per the @b system locale's
        //! QLocale::ShortFormat.
        //! @return QString representing the formatted date
        QString localeDateString(const int year, const int month, const int day, const int dayOfWeek);

        //! Return a day number of week for date
        //! @return number of day: 0 - sunday, 1 - monday,..
        int getDayOfWeek(int year, int month, int day);
        inline int getDayOfWeek(double JD)
        {
                double d= fmodpos(JD+1.5, 7);
                return std::lround(floor(d));
        }

        //! Format the discovery date
        //! @return QString representing the formatted date
        QString localeDiscoveryDateString(const QString& discovery);

        //! Get the current Julian Date from system time.
        //! @return the current Julian Date
        double getJDFromSystem();

        //! Get the Julian Day Number (JD) from Besselian epoch.
        //! @param epoch Besselian epoch, expressed as year with decimal fraction
        //! @return Julian Day number (JD) for B<Year>
        double getJDFromBesselianEpoch(const double epoch);

        //! Get the Julian Day Number (JD) from Julian epoch.
        //! @param epoch Julian epoch, expressed as year with decimal fraction
        //! @return Julian Day number (JD) for J<Year>
        double getJDFromJulianEpoch(const double epoch);

        //! Convert a time of day to the fraction of a Julian Day.
        //! Note that a Julian Day starts at 12:00, not 0:00, and
        //! so 12:00 == 0.0 and 0:00 == 0.5
        double qTimeToJDFraction(const QTime& time);

        //! Convert a fraction of a Julian Day to a QTime
        QTime jdFractionToQTime(const double jd);

        //! Convert a QT QDateTime class to julian day.
        //! @param dateTime the UTC QDateTime to convert
        //! @result the matching decimal Julian Day
        inline double qDateTimeToJd(const QDateTime& dateTime){
                Q_ASSERT(dateTime.timeSpec()==Qt::UTC);
                return dateTime.date().toJulianDay()+static_cast<double>(1./(24*60*60*1000))*QTime(0, 0, 0, 0).msecsTo(dateTime.time())-0.5;
        }

        //! Convert a Julian Day number to a QDateTime.
        //! @param jd Julian Day number (with fractions) to convert
        //! @param timeSpec a @c Qt::TimeSpec constant. Meaningful in this context seem only Qt::UTC (preferred) and Qt::LocalTime (useful in some GUI contexts).
        //! @note From 2008 to 2022-05 this converted to local time zone, not to UTC as specified and intended.
        //!        The old behaviour is kept with @p timeSpec set to Qt::LocalTime.
        //! If you use Qt::LocalTime, you should add StelCore::getUTCOffset(jd)/24 to the current JD before calling this to have @p jd as a "local time zone corrected JD" before conversion.
        //! @result the matching QDateTime
        //! @note QDate has no year zero. This and other idiosyncrasies of QDateTime may limit the applicability of program parts which use this method to positive years or may cause other issues.
        QDateTime jdToQDateTime(const double& jd, const Qt::TimeSpec timeSpec);

        //! Compute Julian day number from calendar date.
        //! Uses QDate functionality if possible, but also works for negative JD.
        //! Dates before 1582-10-15 are in the Julian Calendar.
        //! @param newjd pointer to JD
        //! @param y Calendar year.
        //! @param m month, 1=January ... 12=December
        //! @param d day
        //! @param h hour
        //! @param min minute
        //! @param s second
        //! @result true in all conceivable cases.
        bool getJDFromDate(double* newjd, const int y, const int m, const int d, const int h, const int min, const float s);

        int numberOfDaysInMonthInYear(const int month, const int year);
        //! @result true if year is a leap year. Observes 1582 switch from Julian to Gregorian Calendar.
        bool isLeapYear(const int year);
        //! Find day number for date in year.
        //! Meeus, Astronomical Algorithms 2nd ed., 1998, ch.7, p.65
        int dayInYear(const int year, const int month, const int day);
        //! Find date from day number within year and the year.
        //! Meeus, AA 2nd, 1998, ch.7 p.66
        //! @returns Vec3i(year, month, day)
        Vec3i dateFromDayYear(const int day, const int year);
        //! Return a fractional year like YYYY.ddddd. For negative years, the year number is decreased. E.g. -500.5 occurs in -501.
        double yearFraction(const int year, const int month, const double day);

        bool changeDateTimeForRollover(int oy, int om, int od, int oh, int omin, int os,
                                       int* ry, int* rm, int* rd, int* rh, int* rmin, int* rs);

        //! Output a QVariantMap to qDebug().  Formats like a tree where there are nested objects.
        void debugQVariantMap(const QVariant& m, const QString& indent="", const QString& key="");


        /// Compute acos(x)
        //! The taylor serie is not accurate around x=1 and x=-1
        inline float fastAcos(const float x)
        {
                return static_cast<float>(M_PI_2) - (x + x*x*x * (1.f/6.f + x*x * (3.f/40.f + 5.f/112.f * x*x)) );
        }

        //! Compute exp(x) for small exponents x
        inline float fastExp(const float x)
        {
                return (x>=0)?
                        (1.f + x*(1.f+ x/2.f*(1.f+ x/3.f*(1.f+x/4.f*(1.f+x/5.f))))):
                                1.f / (1.f -x*(1.f -x/2.f*(1.f- x/3.f*(1.f-x/4.f*(1.f-x/5.f)))));
        }

        // Calculate and return sidereal period in days from semi-major axis (in AU)
        //double calculateSiderealPeriod(const double SemiMajorAxis);  MOVED TO Orbit.h

        //! Convert decimal hours to hours, minutes, seconds
        //! Format for:
        //! @p colonFormat        |      false     |   true
        //! ----------------------|----------------|----------
        //! @p minutesOnly=false  |  "HhMMmSS.Ss"  | "HHhMMm"
        //! @p minutesOnly=true   |  "H:MM:SS.S"   | "HH:MM"
        QString hoursToHmsStr(const double hours, const bool minutesOnly = false, const bool colonFormat=false);
        QString hoursToHmsStr(const float hours, const bool minutesOnly = false, const bool colonFormat=false);

        //! Convert JD to hours and minutes
        QString getHoursMinutesFromJulianDay(const double julianDay);

        //! Convert a hms formatted string to decimal hours
        double hmsStrToHours(const QString& s);

        //! Convert days (float) to a time string
        QString daysFloatToDHMS(float days);

        //! The method to splitting the text by substrings by some limit of string length
        QString wrapText(const QString& s, const int limit = 52);

        //! Get Delta-T estimation for a given date.
        //! This is just an "empty" correction function, returning 0.
        double getDeltaTwithoutCorrection(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Note that this method is recommended for the year range:
        //! -1999 to +3000. It gives details for -500...+2150.
        //! Implementation of algorithm by Espenak & Meeus (2006) for DeltaT computation
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByEspenakMeeus(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Note that this method is recommended for the year range:
        //! -1999 to +3000. It gives details for -500...+2150.
        //! Implementation of algorithm by Espenak & Meeus (2006) with modified formulae for DeltaT computation
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByEspenakMeeusModified(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Schoch (1931) for DeltaT computation,
        //! outdated but may be useful for science-historical purposes.
        //! Source: Schoch, C. (1931). Die sekulare Accelaration des Mondes und der Sonne.
        //! Astronomische Abhandlungen, Ergnzungshefte zu den Astronomischen Nachrichten,
        //! Band 8, B2. Kiel.
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTBySchoch(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Clemence (1948) for DeltaT computation,
        //! outdated but may be useful for science-historical purposes.
        //! Source: On the system of astronomical constants.
        //! Clemence, G. M.
        //! Astronomical Journal, Vol. 53, p. 169
        //! 1948AJ.....53..169C [http://adsabs.harvard.edu/abs/1948AJ.....53..169C]
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByClemence(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by IAU (1952) for DeltaT computation,
        //! outdated but may be useful for science-historical purposes.
        //! Source: Spencer Jones, H., "The Rotation of the Earth, and the Secular Accelerations of the Sun, Moon and Planets",
        //! Monthly Notices of the Royal Astronomical Society, 99 (1939), 541-558
        //! http://adsabs.harvard.edu/abs/1939MNRAS..99..541S
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByIAU(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Astronomical Ephemeris (1960) for DeltaT computation.
        //! Sources: Spencer Jones, H., "The Rotation of the Earth, and the Secular Accelerations of the Sun, Moon and Planets",
        //! Monthly Notices of the Royal Astronomical Society, 99 (1939), 541-558
        //! http://adsabs.harvard.edu/abs/1939MNRAS..99..541S
        //! or Explanatory Supplement to the Astr. Ephemeris, 1961, p.87.
        //! Also used by Mucke&Meeus, Canon of Solar Eclipses, Vienna 1983.
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByAstronomicalEphemeris(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Tuckerman (1962, 1964) & Goldstine (1973) for DeltaT computation
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByTuckermanGoldstine(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Muller & Stephenson (1975) for DeltaT computation.
        //! Source: The accelerations of the earth and moon from early astronomical observations
        //! Muller, P. M.; Stephenson, F. R.
        //! Growth rhythms and the history of the earth's rotation; Proceedings of the Interdisciplinary
        //! Winter Conference on Biological Clocks and Changes in the Earth's Rotation: Geophysical and
        //! Astronomical Consequences, Newcastle-upon-Tyne, England, January 8-10, 1974. (A76-18126 06-46)
        //! London, Wiley-Interscience, 1975, p. 459-533; Discussion, p. 534.
        //! 1975grhe.conf..459M [http://adsabs.harvard.edu/abs/1975grhe.conf..459M]
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByMullerStephenson(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Stephenson (1978) for DeltaT computation.
        //! Source: Pre-Telescopic Astronomical Observations
        //! Stephenson, F. R.
        //! Tidal Friction and the Earth's Rotation, Proceedings of a Workshop, held in Bielefeld,
        //! September 26-30, 1977, Edited by P. Brosche, and J. Sundermann. Berlin: Springer-Verlag, 1978, p.5
        //! 1978tfer.conf....5S [http://adsabs.harvard.edu/abs/1978tfer.conf....5S]
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByStephenson1978(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Stephenson (1997) for DeltaT computation.
        //! Source: Book "Historical Eclipses and Earth's Rotation" by F. R. Stephenson (1997)
        //! http://ebooks.cambridge.org/ebook.jsf?bid=CBO9780511525186
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByStephenson1997(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Schmadel & Zech (1979) for DeltaT computation.
        //! Outdated, but may be useful for science-historical purposes.
        //! Source: Polynomial approximations for the correction delta T E.T.-U.T. in the period 1800-1975
        //! Schmadel, L. D.; Zech, G.
        //! Acta Astronomica, vol. 29, no. 1, 1979, p. 101-104.
        //! 1979AcA....29..101S [http://adsabs.harvard.edu/abs/1979AcA....29..101S]
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        //! @note The polynome is strictly applicable 1800...1975 only! Delivers values for the nearer edge (1800/1989) if jDay is outside.
        double getDeltaTBySchmadelZech1979(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Morrison & Stephenson (1982) for DeltaT computation
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByMorrisonStephenson1982(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Stephenson & Morrison (1984) for DeltaT computation
        //! Source: Long-term changes in the rotation of the earth - 700 B.C. to A.D. 1980.
        //! Stephenson, F. R.; Morrison, L. V.
        //! Philosophical Transactions, Series A (ISSN 0080-4614), vol. 313, no. 1524, Nov. 27, 1984, p. 47-70.
        //! 1984RSPTA.313...47S [http://adsabs.harvard.edu/abs/1984RSPTA.313...47S]
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds or Zero if date outside years -391..1600
        double getDeltaTByStephensonMorrison1984(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Stephenson & Morrison (1995) for DeltaT computation
        //! Source: Long-Term Fluctuations in the Earth's Rotation: 700 BC to AD 1990.
        //! Stephenson, F. R.; Morrison, L. V.
        //! Philosophical Transactions: Physical Sciences and Engineering, Volume 351, Issue 1695, pp. 165-202
        //! 1995RSPTA.351..165S [http://adsabs.harvard.edu/abs/1995RSPTA.351..165S]
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByStephensonMorrison1995(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Stephenson & Houlden (1986) for DeltaT computation
        //! Source: STEPHENSON F.R and HOULDEN M.A. - Atlas of Historical Eclipse Maps - Cambridge Univ.Press. (1986)
        //! [https://assets.cambridge.org/97805212/67236/frontmatter/9780521267236_frontmatter.pdf]
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds or 0 if year > 1600
        double getDeltaTByStephensonHoulden(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Espenak (1987, 1989) for DeltaT computation.
        //! This relation should not be used before around 1950 or after around 2100 (Espenak, pers. comm.).
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByEspenak(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Borkowski (1988) for DeltaT computation.
        //! Source: ELP 2000-85 and the dynamic time-universal time relation
        //! Borkowski, K. M.
        //! Astronomy and Astrophysics (ISSN 0004-6361), vol. 205, no. 1-2, Oct. 1988, p. L8-L10.
        //! 1988A&A...205L...8B [http://adsabs.harvard.edu/abs/1988A&A...205L...8B]
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByBorkowski(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Schmadel & Zech (1988) for DeltaT computation.
        //! Source: Empirical Transformations from U.T. to E.T. for the Period 1800-1988
        //! Schmadel, L. D.; Zech, G.
        //! Astronomische Nachrichten 309, 219-221
        //! 1988AN....309..219S [http://adsabs.harvard.edu/abs/1988AN....309..219S]
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        //! @note The polynome is strictly applicable 1800...1988 only! Delivers values for the nearer edge (1800/1989) if jDay is outside.
        double getDeltaTBySchmadelZech1988(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Chapront-Touzé & Chapront (1991) for DeltaT computation
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds or 0 if year not in -391..1600
        double getDeltaTByChaprontTouze(const double jDay);        

        //! Get Delta-T estimation for a given date.
        //! Implementation of the "historical" part of the algorithm by JPL Horizons for DeltaT computation.
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds or 0 if year not in -2999..1620 (!)
        double getDeltaTByJPLHorizons(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Morrison & Stephenson (2004, 2005) for DeltaT computation.
        //! Sources: Historical values of the Earth's clock error ΔT and the calculation of eclipses
        //! Morrison, L. V.; Stephenson, F. R.
        //! Journal for the History of Astronomy (ISSN 0021-8286), Vol. 35, Part 3, No. 120, p. 327 - 336 (2004)
        //! 2004JHA....35..327M [http://adsabs.harvard.edu/abs/2004JHA....35..327M]
        //! Addendum: Historical values of the Earth's clock error
        //! Morrison, L. V.; Stephenson, F. R.
        //! Journal for the History of Astronomy (ISSN 0021-8286), Vol. 36, Part 3, No. 124, p. 339 (2005)
        //! 2005JHA....36..339M [http://adsabs.harvard.edu/abs/2005JHA....36..339M]
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByMorrisonStephenson2004(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Reijs (2006) for DeltaT computation
        //! Details: http://www.iol.ie/~geniet/eng/DeltaTeval.htm
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByReijs(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Chapront, Chapront-Touze & Francou (1997) & Meeus (1998) for DeltaT computation
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByChaprontMeeus(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Meeus & Simons (2000) for DeltaT computation.
        //! Source: Polynomial approximations to Delta T, 1620-2000 AD
        //! Meeus, J.; Simons, L.
        //! Journal of the British Astronomical Association, vol.110, no.6, 323
        //! 2000JBAA..110..323M [http://adsabs.harvard.edu/abs/2000JBAA..110..323M]
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds or 0 if year not in 1620..2000
        double getDeltaTByMeeusSimons(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Montenbruck & Pfleger (2000) for DeltaT computation,
        //! a data fit through the table of values found in Meeus, Astronomical algorithms (1991).
        //! Book "Astronomy on the Personal Computer" by O. Montenbruck & T. Pfleger (4th ed., 2000), p.181-182
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds or 0 if not 1825<=year<2005
        double getDeltaTByMontenbruckPfleger(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Reingold & Dershowitz (1997, 2001, 2002, 2007, 2018) for DeltaT computation.
        //! This is again mostly a data fit based on the table in Meeus, Astronomical Algorithms (1991).
        //! This is the version given in the 4th edition ("the ultimate edition"; 2018) which added the fit
        //! for -500..1699 and 2006..2150 omitted from previous editions.
        //! Calendrical Calculations: The Ultimate Edition / Edward M. Reingold, Nachum Dershowitz - 4th Edition,
        //! Cambridge University Press, 2018. - 660p. ISBN: 9781107057623, DOI: 10.1017/9781107415058
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByReingoldDershowitz(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Banjevic (2006) for DeltaT computation.
        //! Source: Ancient eclipses and dating the fall of Babylon
        //! Banjevic, B.
        //! Publications of the Astronomical Observatory of Belgrade, Vol. 80, p. 251-257 (2006)
        //! 2006POBeo..80..251B [http://adsabs.harvard.edu/abs/2006POBeo..80..251B]
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByBanjevic(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of algorithm by Islam, Sadiq & Qureshi (2008 + revisited 2013) for DeltaT computation.
        //! Source: Error Minimization of Polynomial Approximation of DeltaT
        //! Islam, S. & Sadiq, M. & Qureshi, M. S.
        //! Journal of Astrophysics & Astronomy, Vol. 29, p. 363-366 (2008)
        //! http://www.ias.ac.in/jaa/dec2008/JAA610.pdf
        //! Note: These polynomials are based on the uncorrected deltaT table from the Astronomical Almanac, thus
        //! ndot = -26.0 arcsec/cy^2. Meeus & Simons (2000) corrected the deltaT table for years before 1955.5 using
        //! ndot = -25.7376 arcsec/cy^2. Therefore the accuracies stated by Meeus & Simons are correct and cannot be
        //! compared with accuracies from Islam & Sadiq & Qureshi.
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByIslamSadiqQureshi(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of polynomial approximation of time period 1620-2013 for DeltaT by M. Khalid, Mariam Sultana and Faheem Zaidi (2014).
        //! Source: Delta T: Polynomial Approximation of Time Period 1620-2013
        //! Journal of Astrophysics, Vol. 2014, Article ID 480964
        //! https://doi.org/10.1155/2014/480964
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds
        double getDeltaTByKhalidSultanaZaidi(const double jDay);

        //! Get Delta-T estimation for a given date.
        //! Implementation of a spline approximation for time period -720-2019.0 for DeltaT by Stephenson, Morrison and Hohenkerk (2016).
        //! Source: Measurement of the Earth's rotation: 720 BC to AD 2015, published in 2016 in the Royal Society's
        //! Proceedings A 472, and made freely available via Open Access, by Stephenson, F.R., Morrison, L.V. and
        //! Hohenkerk, C.Y..
        //! https://doi.org/10.1098/rspa.2016.0404
        //! Addendum 2020 to "Measurement of the Earth's Rotation: 720 BC to AD 2015", published in 2021 February
        //! in the Royal Society's Proceedings A 478, by Morrison, L. V., Stephenson, F.R., Hohenkerk, C.Y. and
        //! M. Zawilski, M..
        //! https://doi.org/10.1098/rspa.2020.0776
        //! @param jDay the date and time expressed as a Julian day
        //! @return Delta-T in seconds. For times outside the limits, return result from the fitting parabola.
        double getDeltaTByStephensonMorrisonHohenkerk2016(const double jDay);

        //! Get Secular Acceleration estimation for a given year.
        //! Method described is here: http://eclipse.gsfc.nasa.gov/SEcat5/secular.html
        //! For adapting from -26 to -25.858, use -0.91072 * (-25.858 + 26.0) = -0.12932224
        //! For adapting from -26 to -23.895, use -0.91072 * (-23.895 + 26.0) = -1.9170656
        //! @param jDay the JD
        //! @param ndot value of n-dot (secular acceleration of the Moon) which should be used in the lunar ephemeris instead of the default values.
        //! @param useDE4xx true if function should adapt calculation of the secular acceleration of the Moon to the DE43x/DE44x ephemerides
        //! @return SecularAcceleration in seconds
        //! @note n-dot for secular acceleration of the Moon in ELP2000-82B is -23.8946 "/cy/cy and for DE43x/DE44x is -25.8 "/cy/cy
        double getMoonSecularAcceleration(const double jDay, const double ndot, const bool useDE4xx);

        //! Get the standard error (sigma) for the value of DeltaT
        //! @param jDay the JD
        //! @return sigma in seconds
        double getDeltaTStandardError(const double jDay);

        //! Get value of the Moon fluctuation
        //! Source: The Rotation of the Earth, and the Secular Accelerations of the Sun, Moon and Planets
        //! Spencer Jones, H.
        //! Monthly Notices of the Royal Astronomical Society, 99 (1939), 541-558
        //! 1939MNRAS..99..541S [http://adsabs.harvard.edu/abs/1939MNRAS..99..541S]
        //! @param jDay the JD
        //! @return fluctuation in seconds
        double getMoonFluctuation(const double jDay);

        //! Sign function from http://stackoverflow.com/questions/1903954/is-there-a-standard-sign-function-signum-sgn-in-c-c
        template <typename T> int sign(T val)
        {
                return (T(0) < val) - (val < T(0));
        }
        
        //! Compute cosines and sines around a circle which is split in "slices" parts.
        //! Values are stored in the global static array cos_sin_theta.
        //! Used for the sin/cos values along a latitude circle, equator, etc. for a spherical mesh.
        //! @param slices number of partitions (elsewhere called "segments") for the circle
        float *ComputeCosSinTheta(const unsigned int slices);
        
        //! Compute cosines and sines around a half-circle which is split in "segments" parts.
        //! Values are stored in the global static array cos_sin_rho.
        //! Used for the sin/cos values along a meridian for a spherical mesh.
        //! @param segments number of partitions (elsewhere called "stacks") for the half-circle
        float *ComputeCosSinRho(const unsigned int segments);
        
        //! Compute cosines and sines around part of a circle (from top to bottom) which is split in "segments" parts.
        //! Values are stored in the global static array cos_sin_rho.
        //! Used for the sin/cos values along a meridian.
        //! This allows leaving away pole caps. The array now contains values for the region minAngle+segments*phi
        //! @param dRho a difference angle between the stops
        //! @param segments number of segments
        //! @param minAngle start angle inside the half-circle. maxAngle=minAngle+segments*phi
        float* ComputeCosSinRhoZone(const float dRho, const unsigned int segments, const float minAngle);

        //! Calculate fixed days (R.D.) from Gregorian date (proleptic Gregorian calendar)
        //! @param year
        //! @param month
        //! @param day
        //! @return days from Rata Die
        int getFixedFromGregorian(const int year, const int month, const int day);

        //! Comparison two string versions and return a result in range -1,0,1
        //! @param v1 string for version 1
        //! @param v2 string for version 2
        //! @return result (-1: v1<v2; 0: v1==v2; 1: v1>v2)
        int compareVersions(const QString v1, const QString v2);

        //! Uncompress gzip or zlib compressed data.
        QByteArray uncompress(const QByteArray& data);

        //! Uncompress (gzip/zlib) data from this QIODevice, which must be open and readable.
        //! @param device The device to read from, must already be opened with an OpenMode supporting reading
        //! @param maxBytes The max. amount of bytes to read from the device, or -1 to read until EOF.  Note that it
        //! always stops when inflate() returns Z_STREAM_END. Positive values can be used for interleaving compressed data
        //! with other data.
        QByteArray uncompress(QIODevice &device, qint64 maxBytes=-1);

        //! Greatest Common Divisor (Euclid's algorithm)
        //! @param a first number
        //! @param b second number
        //! @return Greatest Common Divisor
        int gcd(int a, int b);

        //! Least Common Multiple
        //! @param a first number
        //! @param b second number
        //! @return Least Common Multiple
        int lcm(int a, int b);

        //! Given regularly spaced steps x1, x2, x3 and curve values y1, y2, y3,
        //! calculate an intermediate value of the 3 arguments for the given interpolation point n.
        //! @param n Interpolation factor: steps from x2
        //! @param y1 Argument 1
        //! @param y2 Argument 2
        //! @param y3 Argument 3
        //! @return interpolation value
        template<class T> T interpolate3(T n, T y1, T y2, T y3)
        {
                // See "Astronomical Algorithms" by J. Meeus

                // Equation 3.2
                T a = y2-y1;
                T b = y3-y2;
                T c = b-a;

                // Equation 3.3
                return y2 + n * 0.5f * (a + b + n * c);
        }

        //! Given regularly spaced steps x1, x2, x3, x4, x5 and curve values y1, y2, y3, y4, y5,
        //! calculate an intermediate value of the 5 arguments for the given interpolation point n.
        //! @param n Interpolation factor: steps from x3
        //! @param y1 Argument 1
        //! @param y2 Argument 2
        //! @param y3 Argument 3
        //! @param y4 Argument 4
        //! @param y5 Argument 5
        //! @return interpolation value
        template<class T> T interpolate5(T n, T y1, T y2, T y3, T y4, T y5)
        {
                // See "Astronomical Algorithms" by J. Meeus
                // Eq. 3.8
                T A=y2-y1; T B=y3-y2; T C=y4-y3; T D=y5-y4;
                T E=B-A; T F=C-B; T G=D-C;
                T H=F-E; T J=G-F;
                T K=J-H;

                return (((K*(1.0/24.0)*n + (H+J)/12.0)*n  + (F*0.5-K/24.0))*n + ((B+C)*0.5 - (H+J)/12.0))*n +y3;
        }

        //! Interval test. This checks whether @p value is within [@p low, @p high]
        template <typename T> bool isWithin(const T& value, const T& low, const T& high)
        {
                return !(value < low) && !(high < value);
        }

        template <class Arg1, class Arg2, class Result>
        struct binary_function
        {
                typedef Arg1 first_argument_type;
                typedef Arg2 second_argument_type;
                typedef Result result_type;
        };


#ifdef _MSC_BUILD
        inline double trunc(double x)
        {
                return (x < 0 ? std::ceil(x) : std::floor(x));
        }
        inline float trunc(float x)
        {
                return (x < 0 ? std::ceil(x) : std::floor(x));
        }
#else
        inline double trunc(double x) { return ::trunc(x); }
        inline float trunc(float x) { return ::trunc(x); }
#endif
}

#endif // STELUTILS_HPP

Stellarium / stellarium / 15793453064

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