/***************************************************************************
                          ksplanet.cpp  -  K Desktop Planetarium
                             -------------------
    begin                : Sun Jul 22 2001
    copyright            : (C) 2001 by Jason Harris
    email                : jharris@30doradus.org
 ***************************************************************************/

/***************************************************************************
 *                                                                         *
 *   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.                                   *
 *                                                                         *
 ***************************************************************************/

#include "ksplanet.h"

#include <math.h>

#include <QFile>
#include <QTextStream>

#include <kdebug.h>
#include <kglobal.h>

#include "ksnumbers.h"
#include "ksutils.h"
#include "ksfilereader.h"

KSPlanet::OrbitDataManager KSPlanet::odm;

KSPlanet::OrbitDataColl::OrbitDataColl() {
}

KSPlanet::OrbitDataManager::OrbitDataManager() {
    //EMPTY
}

bool KSPlanet::OrbitDataManager::readOrbitData(const QString &fname,
        QVector<OrbitData> *vector) {
    QStringList fields;
    QFile f;
    double A, B, C;

    if ( KSUtils::openDataFile( f, fname ) ) {
        KSFileReader fileReader( f ); // close file is included
        while ( fileReader.hasMoreLines() ) {
            fields = fileReader.readLine().split( ' ', QString::SkipEmptyParts );

            if ( fields.size() == 3 ) {
                A = fields[0].toDouble();
                B = fields[1].toDouble();
                C = fields[2].toDouble();
                vector->append( OrbitData(A, B, C) );
            }
        }
    } else {
        return false;
    }
    return true;
}

bool KSPlanet::OrbitDataManager::loadData( KSPlanet::OrbitDataColl &odc, const QString &n ) {
    QString fname, snum, line;
    QFile f;
    int nCount = 0;
    QString nl = n.toLower();

    if ( hash.contains( nl ) ) {
        odc = hash[nl];
        return true;  //orbit data already loaded
    }

    //Create a new OrbitDataColl
    OrbitDataColl ret;

    //Ecliptic Longitude
    for (int i=0; i<6; ++i) {
        snum.setNum( i );
        fname = nl + ".L" + snum + ".vsop";
        if ( readOrbitData( fname, &ret.Lon[i] ) )
            nCount++;
    }

    if ( nCount==0 ) return false;

    //Ecliptic Latitude
    for (int i=0; i<6; ++i) {
        snum.setNum( i );
        fname = nl + ".B" + snum + ".vsop";
        if ( readOrbitData( fname, &ret.Lat[i] ) )
            nCount++;
    }

    if ( nCount==0 ) return false;

    //Heliocentric Distance
    for (int i=0; i<6; ++i) {
        snum.setNum( i );
        fname = nl + ".R" + snum + ".vsop";
        if ( readOrbitData( fname, &ret.Dst[i] ) )
            nCount++;
    }

    if ( nCount==0 ) return false;

    hash[nl] = ret;
    odc = hash[nl];

    return true;
}

KSPlanet::KSPlanet( const QString &s, const QString &imfile, const QColor & c, double pSize ) :
    KSPlanetBase(s, imfile, c, pSize ),
    data_loaded(false)
{ }

KSPlanet::KSPlanet( int n ) 
    : KSPlanetBase()
{
    switch ( n ) {
        case MERCURY:
            KSPlanetBase::init( i18n("Mercury"), "mercury.png", KSPlanetBase::planetColor[KSPlanetBase::MERCURY], 4879.4 );
            break;
        case VENUS:
            KSPlanetBase::init( i18n("Venus"), "venus.png", KSPlanetBase::planetColor[KSPlanetBase::VENUS], 12103.6 );
            break;
        case MARS:
            KSPlanetBase::init( i18n("Mars"), "mars.png", KSPlanetBase::planetColor[KSPlanetBase::MARS], 6792.4 );
            break;
        case JUPITER:
            KSPlanetBase::init( i18n("Jupiter"), "jupiter.png", KSPlanetBase::planetColor[KSPlanetBase::JUPITER], 142984. );
            break;
        case SATURN:
            KSPlanetBase::init( i18n("Saturn"), "saturn.png", KSPlanetBase::planetColor[KSPlanetBase::SATURN], 120536. );
            break;
        case URANUS:
            KSPlanetBase::init( i18n("Uranus"), "uranus.png", KSPlanetBase::planetColor[KSPlanetBase::URANUS], 51118. );
            break;
        case NEPTUNE:
            KSPlanetBase::init( i18n("Neptune"), "neptune.png", KSPlanetBase::planetColor[KSPlanetBase::NEPTUNE], 49572. );
            break;
        default:
            kDebug() << i18n("Error: Illegal identifier in KSPlanet constructor: %1", n) << endl;
            break;
    }
}

KSPlanet* KSPlanet::clone() const
{
    return new KSPlanet(*this);
}
        
// TODO: Get rid of this dirty hack post KDE 4.2 release
QString KSPlanet::untranslatedName() const {
    if( name() == i18n( "Mercury" ) )
        return "Mercury";
    else if( name() == i18n( "Venus" ) )
        return "Venus";
    else if( name() == i18n( "Mars" ) )
        return "Mars";
    else if( name() == i18n( "Jupiter" ) )
        return "Jupiter";
    else if( name() == i18n( "Saturn" ) )
        return "Saturn";
    else if( name() == i18n( "Uranus" ) )
        return "Uranus";
    else if( name() == i18n( "Neptune" ) )
        return "Neptune";
    else
        return name();
}

//we don't need the reference to the ODC, so just give it a junk variable
bool KSPlanet::loadData() {
    OrbitDataColl odc;
    return odm.loadData( odc, untranslatedName() );
}

void KSPlanet::calcEcliptic(double Tau, EclipticPosition &epret) const {
    double sum[6];
    OrbitDataColl odc;
    double Tpow[6];

    Tpow[0] = 1.0;
    for (int i=1; i<6; ++i) {
        Tpow[i] = Tpow[i-1] * Tau;
    }

    if ( ! odm.loadData( odc, untranslatedName() ) ) {
        epret.longitude = 0.0;
        epret.latitude = 0.0;
        epret.radius = 0.0;
        kError() << "Could not get data for '" << name() << "'" << endl;
        return;
    }

    //Ecliptic Longitude
    for (int i=0; i<6; ++i) {
        sum[i] = 0.0;
        for (int j = 0; j < odc.Lon[i].size(); ++j) {
            sum[i] += odc.Lon[i][j].A * cos( odc.Lon[i][j].B + odc.Lon[i][j].C*Tau );
            /*
            kDebug() << "sum[" << i <<"] =" << sum[i] <<
            	" A = " << odc.Lon[i][j].A << " B = " << odc.Lon[i][j].B <<
            	" C = " << odc.Lon[i][j].C << endl;
            	*/
        }
        sum[i] *= Tpow[i];
        //kDebug() << name() << " : sum[" << i << "] = " << sum[i];
    }

    epret.longitude.setRadians( sum[0] + sum[1] + sum[2] + sum[3] + sum[4] + sum[5] );
    epret.longitude.setD( epret.longitude.reduce().Degrees() );

    //Compute Ecliptic Latitude
    for (uint i=0; i<6; ++i) {
        sum[i] = 0.0;
        for (int j = 0; j < odc.Lat[i].size(); ++j) {
            sum[i] += odc.Lat[i][j].A * cos( odc.Lat[i][j].B + odc.Lat[i][j].C*Tau );
        }
        sum[i] *= Tpow[i];
    }


    epret.latitude.setRadians( sum[0] + sum[1] + sum[2] + sum[3] + sum[4] + sum[5] );

    //Compute Heliocentric Distance
    for (uint i=0; i<6; ++i) {
        sum[i] = 0.0;
        for (int j = 0; j < odc.Dst[i].size(); ++j) {
            sum[i] += odc.Dst[i][j].A * cos( odc.Dst[i][j].B + odc.Dst[i][j].C*Tau );
        }
        sum[i] *= Tpow[i];
    }

    epret.radius = sum[0] + sum[1] + sum[2] + sum[3] + sum[4] + sum[5];

    /*
    kDebug() << name() << " pre: Lat = " << epret.latitude.toDMSString() << " Long = " <<
    	epret.longitude.toDMSString() << " Dist = " << epret.radius << endl;
    */

}

bool KSPlanet::findGeocentricPosition( const KSNumbers *num, const KSPlanetBase *Earth ) {

    if ( Earth != NULL ) {
        double sinL, sinL0, sinB, sinB0;
        double cosL, cosL0, cosB, cosB0;
        double x = 0.0, y = 0.0, z = 0.0;

        double olddst = -1000;
        double dst = 0;

        EclipticPosition trialpos;

        double jm = num->julianMillenia();

        Earth->ecLong()->SinCos( sinL0, cosL0 );
        Earth->ecLat()->SinCos( sinB0, cosB0 );

        double eX = Earth->rsun()*cosB0*cosL0;
        double eY = Earth->rsun()*cosB0*sinL0;
        double eZ = Earth->rsun()*sinB0;

        bool once=true;
        while (fabs(dst - olddst) > .001) {
            calcEcliptic(jm, trialpos);

            // We store the heliocentric ecliptic coordinates the first time they are computed.
            if(once){
                helEcPos = trialpos;
                once=false;
            }

            olddst = dst;

            trialpos.longitude.SinCos( sinL, cosL );
            trialpos.latitude.SinCos( sinB, cosB );

            x = trialpos.radius*cosB*cosL - eX;
            y = trialpos.radius*cosB*sinL - eY;
            z = trialpos.radius*sinB - eZ;

            //distance from Earth
            dst = sqrt(x*x + y*y + z*z);

            //The light-travel time delay, in millenia
            //0.0057755183 is the inverse speed of light,
            //in days/AU
            double delay = (.0057755183 * dst) / 365250.0;

            jm = num->julianMillenia() - delay;

        }

        ep.longitude.setRadians( atan2( y, x ) );
        ep.longitude.reduce();
        ep.latitude.setRadians( atan2( z, sqrt( x*x + y*y ) ) );
        setRsun( trialpos.radius );
        setRearth( dst );

        EclipticToEquatorial( num->obliquity() );

        nutate(num);
        aberrate(num);

    } else {

        calcEcliptic(num->julianMillenia(), ep);
        helEcPos = ep;
    }

    //determine the position angle
    findPA( num );

    return true;
}

void KSPlanet::findMagnitude(const KSNumbers* num)
{
    double cosDec, sinDec;
    dec().SinCos(cosDec, sinDec);

    /* Computation of the visual magnitude (V band) of the planet.
    * Algorithm provided by Pere Planesas (Observatorio Astronomico Nacional)
    * It has some simmilarity to J. Meeus algorithm in Astronomical Algorithms, Chapter 40.
    * */

    // Initialized to the faintest magnitude observable with the HST
    float magnitude = 30;

    double param = 5 * log10(rsun() * rearth() );
    double phase = this->phase().Degrees();
    double f1 = phase/100.;

    if( name() == i18n( "Mercury" ) ) {
        if ( phase > 150. ) f1 = 1.5;
        magnitude = -0.36 + param + 3.8*f1 - 2.73*f1*f1 + 2*f1*f1*f1;
    } else if( name() == i18n( "Venus" ) ) {
        magnitude = -4.29 + param + 0.09*f1 + 2.39*f1*f1 - 0.65*f1*f1*f1;
    } else if( name() == i18n( "Mars" ) ) {
        magnitude = -1.52 + param + 0.016*phase;
    } else if( name() == i18n( "Jupiter" ) ) {
        magnitude = -9.25 + param + 0.005*phase;
    } else if( name() == i18n( "Saturn" ) ) {
        double T = num->julianCenturies();
        double a0 = (40.66-4.695*T)* dms::PI / 180.;
        double d0 = (83.52+0.403*T)* dms::PI / 180.;
        double sinx = -cos(d0)*cosDec*cos(a0 - ra().radians());
        sinx = fabs(sinx-sin(d0)*sinDec);
        double rings = -2.6*sinx + 1.25*sinx*sinx;
        magnitude = -8.88 + param + 0.044*phase + rings;
    } else if( name() == i18n( "Uranus" ) ) {
        magnitude = -7.19 + param + 0.0028*phase;
    } else if( name() == i18n( "Neptune" ) ) {
        magnitude = -6.87 + param;
    }
    setMag(magnitude);
}

SkyObject::UID KSPlanet::getUID() const
{
    SkyObject::UID n;
    if( name() == i18n( "Mercury" ) ) {
        n = 1;
    } else if( name() == i18n( "Venus" ) ) {
        n = 2;
    } else if( name() == i18n( "Earth" ) ) {
        n = 3;
    } else if( name() == i18n( "Mars" ) ) {
        n = 4;
    } else if( name() == i18n( "Jupiter" ) ) {
        n = 5;
    } else if( name() == i18n( "Saturn" ) ) {
        n = 6;
    } else if( name() == i18n( "Uranus" ) ) {
        n = 7;
    } else if( name() == i18n( "Neptune" ) ) {
        n = 8;
    } else {
        return SkyObject::invalidUID;
    }
    return solarsysUID(UID_SOL_BIGOBJ) | n;
}
