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Python math.radians函数代码示例

本文整理汇总了Python中math.radians函数的典型用法代码示例。如果您正苦于以下问题:Python radians函数的具体用法?Python radians怎么用?Python radians使用的例子?那么恭喜您, 这里精选的函数代码示例或许可以为您提供帮助。


在下文中一共展示了radians函数的15个代码示例,这些例子默认根据受欢迎程度排序。您可以为喜欢或者感觉有用的代码点赞,您的评价将有助于系统推荐出更棒的Python代码示例。

示例1: gps_to_kmeters

    def gps_to_kmeters(long1, lat1, long2, lat2):
        """Converts gps longitudes and latitudes distance to meters

        Keyword arguments:
        long1 -- longitude for pos 1
        lat1 -- latitute for pos 1
        long2 -- longitude for pos 2
        lat2 -- latitude for pos 2
        """

        #approx radius of earth
        R = 6373.0

        long1 = radians(long1)
        lat1 = radians(lat1)
        long2 = radians(long2)
        lat2 = radians(lat2)

        dist_long = long2 - long1
        dist_lat = lat2 - lat1

        a = sin(dist_lat / 2)**2 + cos(lat1) * cos(lat2) * sin(dist_long)**2
        c = atan2(sqrt(a), sqrt(1 - a))

        dist = R * c

        return dist
开发者ID:chrlofs,项目名称:PU-project,代码行数:27,代码来源:calculator.py

示例2: calc_dist

def calc_dist(plyr_angl,plyr_vel):
    gravity = 9.81                #gravity 9.81 m/s^2
    vel_init_x = plyr_vel * math.cos(math.radians(plyr_angl))    #creates Vix
    vel_init_y = plyr_vel * math.sin(math.radians(plyr_angl))    #creates Viy
    time_in_air = 2 * (vel_init_y / gravity)              #solves for time
    distance_x = vel_init_x * time_in_air                #solves for distance
    return (distance_x, time_in_air)                    #returns horizontal distance, time in air
开发者ID:frapp,项目名称:gravity,代码行数:7,代码来源:gravity2.py

示例3: __create_board

    def __create_board(self):
        """
        Creates a Canvas widget where Hexagon fields are marked on it
        """
        m = self.size[0]
        n = self.size[1]
        edge_length = 24
        # calculates the size of the Hexagon
        y_top, x_right = self.__Hex_size(edge_length)
        canvas_width = x_right * n + x_right * m / 2 + 50
        canvas_height = y_top * m + 100

        self.w = Canvas(self.master, width=canvas_width, height=canvas_height)
        self.w.configure(background=self.bg)
        self.w.pack()
        # creates Hexagon Grid
        for j in range(m):
            for i in range(n):
                x = 40 + x_right * i + x_right / 2 * j
                y = 50 + y_top * j
                k = 0
                for angle in range(0, 360, 60):
                    y += math.cos(math.radians(angle)) * edge_length
                    x += math.sin(math.radians(angle)) * edge_length
                    self.point_coordinates[j][i][k] = x
                    self.point_coordinates[j][i][k + 1] = y
                    k += 2
                # draws Hexagon to the canvas widget
                self.w.create_polygon(list(
                    self.point_coordinates[j][i]),
                    outline=self.tile_outline, fill=self.tile, width=3)
开发者ID:N00b00dY,项目名称:Hex_git,代码行数:31,代码来源:Hex.py

示例4: sumVectors

    def sumVectors(self, vectors):
        """ sum all vectors (including targetvector)"""
        endObstacleVector = (0,0)

        ##generate endvector of obstacles
        #sum obstaclevectors
        for vector in vectors:
            vectorX = math.sin(math.radians(vector[1])) * vector[0] # x-position
            vectorY = math.cos(math.radians(vector[1])) * vector[0] # y-position
            endObstacleVector = (endObstacleVector[0]+vectorX,endObstacleVector[1]+vectorY)
        #mean obstaclevectors
        if len(vectors) > 0:
            endObstacleVector = (endObstacleVector[0]/len(vectors), endObstacleVector[1]/len(vectors))

        #add targetvector
        targetVector = self.target
        if targetVector != 0 and targetVector != None:
            vectorX = math.sin(math.radians(targetVector[1])) * targetVector[0] # x-position
            vectorY = math.cos(math.radians(targetVector[1])) * targetVector[0] # y-position
            endVector = (endObstacleVector[0]+vectorX,endObstacleVector[1]+vectorY)
            #endVector = (endVector[0]/2, endVector[1]/2)
        else:
            endVector = endObstacleVector


        return endVector
开发者ID:diederikvkrieken,项目名称:Asjemenao,代码行数:26,代码来源:vectorfield.py

示例5: update

    def update(self):
        if self.turning_right:
            self.rot -= 5
        if self.turning_left:
            self.rot += 5

        a = [0.0,0.0]
        if self.boost_endtime > rabbyt.get_time():
            f = 3*(self.boost_endtime - rabbyt.get_time())/self.boost_length
            a[0] += cos(radians(self.boost_rot))*f
            a[1] += sin(radians(self.boost_rot))*f
            self.create_boost_particle()

        if self.accelerating:
            a[0] += cos(radians(self.rot))*.9
            a[1] += sin(radians(self.rot))*.9
            self.create_dust_particle(self.dust_r)
            self.create_dust_particle(self.dust_l)

        ff = .9 # Friction Factor

        self.velocity[0] *= ff
        self.velocity[1] *= ff

        self.velocity[0] += a[0]
        self.velocity[1] += a[1]

        self.x += self.velocity[0]
        self.y += self.velocity[1]
开发者ID:0918901,项目名称:PY-Projects,代码行数:29,代码来源:driving.py

示例6: set_3d

    def set_3d(self):
        """ Configure OpenGL to draw in 3d.

        """
        width, height = self.get_size()

        gl.glEnable(gl.GL_DEPTH_TEST)

        gl.glViewport(0, 0, width, height)
        gl.glMatrixMode(gl.GL_PROJECTION)
        gl.glLoadIdentity()
        gl.gluPerspective(65.0, width / float(height), 0.1, DIST)
        gl.glMatrixMode(gl.GL_MODELVIEW)
        gl.glLoadIdentity()

        x, y = self.rotation
        gl.glRotatef(x, 0, 1, 0)
        gl.glRotatef(-y, math.cos(math.radians(x)), 0, math.sin(math.radians(x)))
        x, y, z = self.position
        gl.glTranslatef(-x, -y, -z)

        gl.glEnable(gl.GL_LIGHTING)
        gl.glLightModelfv(gl.GL_LIGHT_MODEL_AMBIENT, GLfloat4(0.05,0.05,0.05,1.0))
        gl.glEnable(gl.GL_COLOR_MATERIAL)
        gl.glColorMaterial(gl.GL_FRONT, gl.GL_AMBIENT_AND_DIFFUSE)
        #gl.glLightfv(gl.GL_LIGHT1,gl.GL_SPOT_DIRECTION, GLfloat3(0,0,-1))
        gl.glLightfv(gl.GL_LIGHT1, gl.GL_AMBIENT, GLfloat4(0.5,0.5,0.5,1.0))
        gl.glLightfv(gl.GL_LIGHT1, gl.GL_DIFFUSE, GLfloat4(1.0,1.0,1.0,1.0))
        gl.glLightfv(gl.GL_LIGHT1, gl.GL_POSITION, GLfloat4(0.35,1.0,0.65,0.0))
        #gl.glLightfv(gl.GL_LIGHT0,gl.GL_SPECULAR, GLfloat4(1,1,1,1))
        gl.glDisable(gl.GL_LIGHT0)
        gl.glEnable(gl.GL_LIGHT1)
开发者ID:spillz,项目名称:minepy,代码行数:32,代码来源:main.py

示例7: calculate_initial_compass_bearing

    def calculate_initial_compass_bearing(self, pointA, pointB):
        """
        Calculates direction between two points.
        Code based on compassbearing.py module
        https://gist.github.com/jeromer/2005586

        pointA: latitude/longitude for first point (decimal degrees)
        pointB: latitude/longitude for second point (decimal degrees)
    
        Return: direction heading in degrees (0-360 degrees, with 90 = North)
        """

        if (type(pointA) != tuple) or (type(pointB) != tuple):
            raise TypeError("Only tuples are supported as arguments")
    
        lat1 = math.radians(pointA[0])
        lat2 = math.radians(pointB[0])
    
        diffLong = math.radians(pointB[1] - pointA[1])
    
        # Direction angle (-180 to +180 degrees):
        # θ = atan2(sin(Δlong).cos(lat2),cos(lat1).sin(lat2) − sin(lat1).cos(lat2).cos(Δlong))

        x = math.sin(diffLong) * math.cos(lat2)
        y = math.cos(lat1) * math.sin(lat2) - (math.sin(lat1) * math.cos(lat2) * math.cos(diffLong))
    
        initial_bearing = math.atan2(x, y)
    
        # Direction calculation requires to normalize direction angle (0 - 360)
        initial_bearing = math.degrees(initial_bearing)
        compass_bearing = (initial_bearing + 360) % 360
    
        return compass_bearing
开发者ID:hemanthk92,项目名称:gpstransmode,代码行数:33,代码来源:gps_data_engineering.py

示例8: distance_to_coords_formula

def distance_to_coords_formula(latitude, longitude, bearing1, bearing2):
    """ math formula for calculating the lat, lng based on
        distance and bearing """

    # one degree of latitude is approximately 10^7 / 90 = 111,111 meters.
    # http://stackoverflow.com/questions/2187657/calculate-second-point-
    # knowing-the-starting-point-and-distance
    # one degree of latitude is approximately 10^7 / 90 = 111,111 meters
    # http://stackoverflow.com/questions/13836416/geohash-and-max-distance
    distance = 118  # meters

    east_displacement_a = distance * sin(radians(bearing1)) / 111111
    north_displacement_a = distance * cos(radians(bearing1)) / 111111

    east_displacement_b = distance * sin(radians(bearing2)) / 111111
    north_displacement_b = distance * cos(radians(bearing2)) / 111111

    # calculate the total displacement for N, S respectively
    waypoint_latitude_a = latitude + north_displacement_a
    waypoint_longitude_a = longitude + east_displacement_a

    waypoint_latitude_b = latitude + north_displacement_b
    waypoint_longitude_b = longitude + east_displacement_b

    return [(waypoint_latitude_a, waypoint_longitude_a),
            (waypoint_latitude_b, waypoint_longitude_b)]
开发者ID:Munnu,项目名称:Stroll-Safely,代码行数:26,代码来源:middle.py

示例9: distance

 def distance(a, b):
     """Calculates distance between two latitude-longitude coordinates."""
     R = 3963  # radius of Earth (miles)
     lat1, lon1 = math.radians(a[0]), math.radians(a[1])
     lat2, lon2 = math.radians(b[0]), math.radians(b[1])
     return math.acos( math.sin(lat1)*math.sin(lat2) +
         math.cos(lat1)*math.cos(lat2)*math.cos(lon1-lon2) ) * R
开发者ID:Ecotrust,项目名称:aquatic-priorities,代码行数:7,代码来源:anneal.py

示例10: create_circle

def create_circle(cx, cy, r, a1, a2):
    points = []
    for a in range(a1, a2 + 1):
        x = cx + r * cos(radians(a))
        y = cy + r * sin(radians(a))
        points.append((x, y))
    return points
开发者ID:fogleman,项目名称:Carolina,代码行数:7,代码来源:sophia.py

示例11: dayLength

def dayLength(date, latitude):
    # Formulas from: http://www.gandraxa.com/length_of_day.xml
    # I don't really understand them, and the numbers don't quite match
    # what I get from calendar sites. Perhaps this is measuring the exact
    # moment the center of the sun goes down, as opposed to civil twilight?
    # But I think it's close enough to get the idea across.

    # Tilt of earth's axis relative to its orbital plane ("obliquity of ecliptic")
    axis = math.radians(23.439)

    # Date of winter solstice in this year. Not quite right, but good
    # enough for our purposes.
    solstice = date.replace(month=12, day=21)

    # If a year is a full circle, this is the angle between the solstice
    # and this date, in radians. May be negative if we haven't reached the
    # solstice yet.
    dateAngle = (date - solstice).days * 2 * math.pi / 365.25

    latitude = math.radians(latitude)
    m = 1 - math.tan(latitude) * math.tan(axis * math.cos(dateAngle))

    # If m is less than zero, the sun never rises; if greater than two, it never sets.
    m = min(2, max(0, m))
    return math.acos(1 - m) / math.pi
开发者ID:jimblandy,项目名称:spiral-calendar,代码行数:25,代码来源:gen_calendar.py

示例12: set_3d

    def set_3d(self):
        """ Configure OpenGL to draw in 3d.

		"""
        width, height = self.get_size()
        glEnable(GL_DEPTH_TEST)
        glViewport(0, 0, width, height)
        glMatrixMode(GL_PROJECTION)
        glLoadIdentity()
        # gluPerspective(45.0f,(GLfloat)width/(GLfloat)height,near distance,far distance);
        # gluPerspective(65.0, width / float(height), 0.1, 60.0)
        gluPerspective(65.0, width / float(height), 0.1, 6000.0)
        glMatrixMode(GL_MODELVIEW)
        glLoadIdentity()

        # glDepthMask(GL_FALSE)
        # drawSkybox()
        # glDepthMask(GL_TRUE)

        x, y = self.rotation
        # http://wiki.delphigl.com/index.php/glRotate
        # procedure glRotatef(angle: TGLfloat; x: TGLfloat; y: TGLfloat; z: TGLfloat);
        glRotatef(x, 0, 1, 0)
        glRotatef(-y, math.cos(math.radians(x)), 0, math.sin(math.radians(x)))
        x, y, z = self.position
        glTranslatef(-x, -y, -z)
开发者ID:leonslg,项目名称:DICraft,代码行数:26,代码来源:DICraft.py

示例13: precisionToDim

    def precisionToDim(self):
        """Convert precision from Wikibase to GeoData's dim and return the latter.

        dim is calculated if the Coordinate doesn't have a dimension, and precision is set.
        When neither dim nor precision are set, ValueError is thrown.

        Carrying on from the earlier derivation of precision, since
        precision = math.degrees(dim/(radius*math.cos(math.radians(self.lat)))), we get
            dim = math.radians(precision)*radius*math.cos(math.radians(self.lat))
        But this is not valid, since it returns a float value for dim which is an integer.
        We must round it off to the nearest integer.

        Therefore::
            dim = int(round(math.radians(precision)*radius*math.cos(math.radians(self.lat))))

        @rtype: int or None
        """
        if self._dim is None and self._precision is None:
            raise ValueError('No values set for dim or precision')
        if self._dim is None and self._precision is not None:
            radius = 6378137
            self._dim = int(
                round(
                    math.radians(self._precision) * radius * math.cos(math.radians(self.lat))
                )
            )
        return self._dim
开发者ID:Darkdadaah,项目名称:pywikibot-core,代码行数:27,代码来源:__init__.py

示例14: bird_blave

def bird_blave(timestamp, place, tilt=0, azimuth=180, cloudCover=0.0):
    #SUN Position
    o = ephem.Observer()
    o.date = timestamp #'2000/12/21 %s:00:00' % (hour - self.tz)
    latitude, longitude = place
    o.lat = radians(latitude)
    o.lon = radians(longitude)
    az = ephem.Sun(o).az
    alt = ephem.Sun(o).alt

    #Irradiance
    day = dayOfYear(timestamp)
    record = {}
    record['utc_datetime'] = timestamp
    Z = pi/2-alt
    aaz = radians(azimuth+180)
    slope = radians(tilt)

    #incidence angle
    theta = arccos(cos(Z)*cos(slope) + \
            sin(slope)*sin(Z)*cos(az - pi - aaz))
    ETR = apparentExtraterrestrialFlux(day)
    #pressure?
    t, Bh, Gh = bird(theta, 1010.0)
    Dh = diffuseHorizontal(alt, Bh, day)

    record['DNI (W/m^2)'] = Bh #8 Direct normal irradiance
    record['GHI (W/m^2)'] = Gh #5 Global horizontal irradiance
    record['DHI (W/m^2)'] = Dh #11 Diffuse horizontal irradiance
    record['ETR (W/m^2)'] = ETR
    return record
开发者ID:yanglijn,项目名称:solpy,代码行数:31,代码来源:irradiation.py

示例15: getDec

	def getDec(self,j):
		j=float(j)
		m = 357.0+(0.9856*j) 
		c = (1.914*sin(radians(m))) + (0.02*sin(radians(2.0*m)))
		l = 280.0 + c + (0.9856*j)
		sinDec= 0.3978*sin(radians(l))
		return degrees(asin(sinDec))
开发者ID:CaptainStouf,项目名称:api-domogeek,代码行数:7,代码来源:ClassDawnDusk.py


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