public SpaceGreen() {
super(WIDTH, HEIGHT, CELL);
Brain2.checkCount();
Background();
fillStars(sTars, MAX_STAR);
Setstars();
GreenfootImage earthp = new GreenfootImage("Images/HalfEarth.png");
getBackground().drawImage(earthp, earth.getX(), earth.getY());
GreenfootImage moonp = new GreenfootImage("Images/Moon.png");
getBackground().drawImage(moonp, moon.getX(), moon.getY());
GreenfootImage saturnp = new GreenfootImage("Images/Saturn.png");
getBackground().drawImage(saturnp, saturn.getX(), saturn.getY());
GreenfootImage marsp = new GreenfootImage("Images/RedPlanet.png");
getBackground().drawImage(marsp, mars.getX(), mars.getY());
ship = new Spaceship();
mothership = new Mothership();
explosion = new Explosion();
addObject(mothership, mothership.getX(mothership.x), mothership.getY(mothership.y));
addObject(ship, ship.getX(), ship.getY(ship.y));
Checkstars();
Checkplanets();
}
@Test
public void callTheSpinAndWarmUpMethods() throws Exception {
Method accessor = checkThatSingletonContainsStaticInstanceAccessorMethod(Earth.class);
Earth earth = (Earth) accessor.invoke(null);
earth.spin();
earth.warmUp();
}
@Test
public void makeEarthWithAnotherClassLoader() throws Exception {
Earth old = Earth.getEarth();
replaceEarth(FastEarth.class.getName());
FastEarth fast = FastEarth.class.cast(Earth.getEarth());
assertNotSame(old, fast);
replaceEarth(SlowEarth.class.getName());
SlowEarth slow = SlowEarth.class.cast(Earth.getEarth());
assertNotSame(old, slow);
assertNotSame(fast, slow);
}
public static void readKeyFromConsoleAndInitPlanet() {
// implement step #5 here - реализуйте задание №5 тут
try (BufferedReader reader = new BufferedReader(new InputStreamReader(System.in))) {
String text = reader.readLine();
switch (text) {
case Planet.EARTH:
thePlanet = Earth.getInstance();
break;
case Planet.MOON:
thePlanet = Moon.getInstance();
break;
case Planet.SUN:
thePlanet = Sun.getInstance();
break;
default:
thePlanet = null;
}
} catch (IOException e) {
}
}
/**
* Calculate a position given an azimuth and distance from another point.
*
* <p>
*
* <p>Algorithm from National Geodetic Survey, FORTRAN program "forward," subroutine "DIRCT1," by
* stephen j. frakes. http://www.ngs.noaa.gov/TOOLS/Inv_Fwd/Inv_Fwd.html
*
* <p>Original documentation:
*
* <pre>
* SOLUTION OF THE GEODETIC DIRECT PROBLEM AFTER T.VINCENTY
* MODIFIED RAINSFORD'S METHOD WITH HELMERT'S ELLIPTICAL TERMS
* EFFECTIVE IN ANY AZIMUTH AND AT ANY DISTANCE SHORT OF ANTIPODAL
* </pre>
*
* @param e Earth object (defines radius and flattening)
* @param lat1 latitude of starting point
* @param lon1 longitude of starting point
* @param az forward azimuth (degrees)
* @param dist distance from the point (km)
* @param result Object to use if non-null
* @return the position as a LatLonPointImpl
*/
public static LatLonPointImpl findPoint(
Earth e, double lat1, double lon1, double az, double dist, LatLonPointImpl result) {
if (result == null) {
result = new LatLonPointImpl();
}
if ((dist == 0)) {
result.setLatitude(lat1);
result.setLongitude(lon1);
return result;
}
A = e.getMajor();
F = e.getFlattening();
R = 1.0 - F;
// Algorithm from National Geodetic Survey, FORTRAN program "forward,"
// subroutine "DIRCT1," by stephen j. frakes.
// http://www.ngs.noaa.gov/TOOLS/Inv_Fwd/Inv_Fwd.html
// Conversion to JAVA from FORTRAN was made with as few changes as
// possible to avoid errors made while recasting form, and
// to facilitate any future comparisons between the original
// code and the altered version in Java.
// Original documentation:
// SUBROUTINE DIRCT1(GLAT1,GLON1,GLAT2,GLON2,FAZ,BAZ,S)
//
// SOLUTION OF THE GEODETIC DIRECT PROBLEM AFTER T.VINCENTY
// MODIFIED RAINSFORD'S METHOD WITH HELMERT'S ELLIPTICAL TERMS
// EFFECTIVE IN ANY AZIMUTH AND AT ANY DISTANCE SHORT OF ANTIPODAL
//
// A IS THE SEMI-MAJOR AXIS OF THE REFERENCE ELLIPSOID
// F IS THE FLATTENING OF THE REFERENCE ELLIPSOID
// LATITUDES AND LONGITUDES IN RADIANS POSITIVE NORTH AND EAST
// AZIMUTHS IN RADIANS CLOCKWISE FROM NORTH
// GEODESIC DISTANCE S ASSUMED IN UNITS OF SEMI-MAJOR AXIS A
//
// PROGRAMMED FOR CDC-6600 BY LCDR L.PFEIFER NGS ROCKVILLE MD 20FEB75
// MODIFIED FOR SYSTEM 360 BY JOHN G GERGEN NGS ROCKVILLE MD 750608
//
if (az < 0.0) {
az += 360.0; // reset azs from -180 to 180 to 0 to 360
}
double FAZ = az * rad;
double GLAT1 = lat1 * rad;
double GLON1 = lon1 * rad;
double S = dist * 1000.; // convert to meters
double TU = R * Math.sin(GLAT1) / Math.cos(GLAT1);
double SF = Math.sin(FAZ);
double CF = Math.cos(FAZ);
double BAZ = 0.;
if (CF != 0) {
BAZ = Math.atan2(TU, CF) * 2;
}
double CU = 1. / Math.sqrt(TU * TU + 1.);
double SU = TU * CU;
double SA = CU * SF;
double C2A = -SA * SA + 1.;
double X = Math.sqrt((1. / R / R - 1.) * C2A + 1.) + 1.;
X = (X - 2.) / X;
double C = 1. - X;
C = (X * X / 4. + 1) / C;
double D = (0.375 * X * X - 1.) * X;
TU = S / R / A / C;
double Y = TU;
double SY, CY, CZ, E, GLAT2, GLON2;
do {
SY = Math.sin(Y);
CY = Math.cos(Y);
CZ = Math.cos(BAZ + Y);
E = CZ * CZ * 2. - 1.;
C = Y;
X = E * CY;
Y = E + E - 1.;
Y = (((SY * SY * 4. - 3.) * Y * CZ * D / 6. + X) * D / 4. - CZ) * SY * D + TU;
} while (Math.abs(Y - C) > EPS);
BAZ = CU * CY * CF - SU * SY;
C = R * Math.sqrt(SA * SA + BAZ * BAZ);
D = SU * CY + CU * SY * CF;
GLAT2 = Math.atan2(D, C);
C = CU * CY - SU * SY * CF;
X = Math.atan2(SY * SF, C);
C = ((-3. * C2A + 4.) * F + 4.) * C2A * F / 16.;
D = ((E * CY * C + CZ) * SY * C + Y) * SA;
GLON2 = GLON1 + X - (1. - C) * D * F;
BAZ = (Math.atan2(SA, BAZ) + Math.PI) * deg;
result.setLatitude(GLAT2 * deg);
result.setLongitude(GLON2 * deg);
return result;
}
/**
* Computes distance (in km), azimuth (degrees clockwise positive from North, 0 to 360), and back
* azimuth (degrees clockwise positive from North, 0 to 360), from latitude-longituide point pt1
* to latitude-longituide pt2.
*
* <p>Algorithm from U.S. National Geodetic Survey, FORTRAN program "inverse," subroutine
* "INVER1," by L. PFEIFER and JOHN G. GERGEN. See
* http://www.ngs.noaa.gov/TOOLS/Inv_Fwd/Inv_Fwd.html
*
* <p>Original documentation: <br>
* SOLUTION OF THE GEODETIC INVERSE PROBLEM AFTER T.VINCENTY <br>
* MODIFIED RAINSFORD'S METHOD WITH HELMERT'S ELLIPTICAL TERMS <br>
* EFFECTIVE IN ANY AZIMUTH AND AT ANY DISTANCE SHORT OF ANTIPODAL <br>
* STANDPOINT/FOREPOINT MUST NOT BE THE GEOGRAPHIC POLE Reference ellipsoid is the WGS-84
* ellipsoid. <br>
* See http://www.colorado.edu/geography/gcraft/notes/datum/elist.html
*
* <p>Requires close to 1.4 E-5 seconds wall clock time per call on a 550 MHz Pentium with Linux
* 7.2.
*
* @param e Earth object (defines radius and flattening)
* @param lat1 Lat of point 1
* @param lon1 Lon of point 1
* @param lat2 Lat of point 2
* @param lon2 Lon of point 2
* @param result put result here, or null to allocate
* @return a Bearing object with distance (in km), azimuth from pt1 to pt2 (degrees, 0 = north,
* clockwise positive)
*/
public static Bearing calculateBearing(
Earth e, double lat1, double lon1, double lat2, double lon2, Bearing result) {
if (result == null) {
result = new Bearing();
}
if ((lat1 == lat2) && (lon1 == lon2)) {
result.distance = 0;
result.azimuth = 0;
result.backazimuth = 0;
return result;
}
A = e.getMajor();
F = e.getFlattening();
R = 1.0 - F;
// Algorithm from National Geodetic Survey, FORTRAN program "inverse,"
// subroutine "INVER1," by L. PFEIFER and JOHN G. GERGEN.
// http://www.ngs.noaa.gov/TOOLS/Inv_Fwd/Inv_Fwd.html
// Conversion to JAVA from FORTRAN was made with as few changes as possible
// to avoid errors made while recasting form, and to facilitate any future
// comparisons between the original code and the altered version in Java.
// Original documentation:
// SOLUTION OF THE GEODETIC INVERSE PROBLEM AFTER T.VINCENTY
// MODIFIED RAINSFORD'S METHOD WITH HELMERT'S ELLIPTICAL TERMS
// EFFECTIVE IN ANY AZIMUTH AND AT ANY DISTANCE SHORT OF ANTIPODAL
// STANDPOINT/FOREPOINT MUST NOT BE THE GEOGRAPHIC POLE
// A IS THE SEMI-MAJOR AXIS OF THE REFERENCE ELLIPSOID
// F IS THE FLATTENING (NOT RECIPROCAL) OF THE REFERNECE ELLIPSOID
// LATITUDES GLAT1 AND GLAT2
// AND LONGITUDES GLON1 AND GLON2 ARE IN RADIANS POSITIVE NORTH AND EAST
// FORWARD AZIMUTHS AT BOTH POINTS RETURNED IN RADIANS FROM NORTH
//
// Reference ellipsoid is the WGS-84 ellipsoid.
// See http://www.colorado.edu/geography/gcraft/notes/datum/elist.html
// FAZ is forward azimuth in radians from pt1 to pt2;
// BAZ is backward azimuth from point 2 to 1;
// S is distance in meters.
//
// Conversion to JAVA from FORTRAN was made with as few changes as possible
// to avoid errors made while recasting form, and to facilitate any future
// comparisons between the original code and the altered version in Java.
//
// IMPLICIT REAL*8 (A-H,O-Z)
// COMMON/CONST/PI,RAD
// COMMON/ELIPSOID/A,F
double GLAT1 = rad * lat1;
double GLAT2 = rad * lat2;
double TU1 = R * Math.sin(GLAT1) / Math.cos(GLAT1);
double TU2 = R * Math.sin(GLAT2) / Math.cos(GLAT2);
double CU1 = 1. / Math.sqrt(TU1 * TU1 + 1.);
double SU1 = CU1 * TU1;
double CU2 = 1. / Math.sqrt(TU2 * TU2 + 1.);
double S = CU1 * CU2;
double BAZ = S * TU2;
double FAZ = BAZ * TU1;
double GLON1 = rad * lon1;
double GLON2 = rad * lon2;
double X = GLON2 - GLON1;
double D, SX, CX, SY, CY, Y, SA, C2A, CZ, E, C;
int loopCnt = 0;
do {
loopCnt++;
// Check for an infinite loop
if (loopCnt > 1000) {
throw new IllegalArgumentException(
"Too many iterations calculating bearing:"
+ lat1
+ " "
+ lon1
+ " "
+ lat2
+ " "
+ lon2);
}
SX = Math.sin(X);
CX = Math.cos(X);
TU1 = CU2 * SX;
TU2 = BAZ - SU1 * CU2 * CX;
SY = Math.sqrt(TU1 * TU1 + TU2 * TU2);
CY = S * CX + FAZ;
Y = Math.atan2(SY, CY);
SA = S * SX / SY;
C2A = -SA * SA + 1.;
CZ = FAZ + FAZ;
if (C2A > 0.) {
CZ = -CZ / C2A + CY;
}
E = CZ * CZ * 2. - 1.;
C = ((-3. * C2A + 4.) * F + 4.) * C2A * F / 16.;
D = X;
X = ((E * CY * C + CZ) * SY * C + Y) * SA;
X = (1. - C) * X * F + GLON2 - GLON1;
// IF(DABS(D-X).GT.EPS) GO TO 100
} while (Math.abs(D - X) > EPS);
if (loopCnt > maxLoopCnt) {
maxLoopCnt = loopCnt;
// System.err.println("loopCnt:" + loopCnt);
}
FAZ = Math.atan2(TU1, TU2);
BAZ = Math.atan2(CU1 * SX, BAZ * CX - SU1 * CU2) + Math.PI;
X = Math.sqrt((1. / R / R - 1.) * C2A + 1.) + 1.;
X = (X - 2.) / X;
C = 1. - X;
C = (X * X / 4. + 1.) / C;
D = (0.375 * X * X - 1.) * X;
X = E * CY;
S = 1. - E - E;
S = ((((SY * SY * 4. - 3.) * S * CZ * D / 6. - X) * D / 4. + CZ) * SY * D + Y) * C * A * R;
result.distance = S / 1000.0; // meters to km
result.azimuth = FAZ * deg; // radians to degrees
if (result.azimuth < 0.0) {
result.azimuth += 360.0; // reset azs from -180 to 180 to 0 to 360
}
result.backazimuth = BAZ * deg; // radians to degrees; already in 0 to 360 range
return result;
}