예제 #1
0
파일: polar.py 프로젝트: nadvornik/astro
	def camera_position(self, ci, noise = 2):
		if len(self.campos[ci]) < 2:
			return None
		avg = Quaternion.average(self.campos[ci])
		
		d = np.array([avg.distance_metric(q) for q in self.campos[ci]])
		
		d2 = d**2
		var = np.mean(d2)
		#print var * noise**2
		#print d2
		#print np.where(d2 < var * noise**2)[0]
		self.campos[ci] = [self.campos[ci][i] for i in np.where(d2 < var * noise**2)[0]]
		
		avg = Quaternion.average(self.campos[ci])
		self.campos_avg[ci] = avg
		return avg
예제 #2
0
파일: polar.py 프로젝트: nadvornik/astro
	def solve(self, noise=2):
		if self.mode == 'adjust':
			return self.ra, self.dec
		if len(self.pos[0]) < 3:
			return None, None

		weights = np.matrix(np.zeros((2, 2)))
		wsum = np.zeros((2,1))

		for ci in range(0, len(self.pos)):
			if len(self.pos[ci]) < 3:
				continue
			try:
				qlist = [ p for (p, t) in self.pos[ci]]
				
				avg = Quaternion.average(qlist).inv()
				alist = []
				for q in qlist:
					q0 = q * avg
					if abs(q0.a[0]) < 0.7:
						ax, roll = q0.to_axis_roll()
						q0 = Quaternion.from_axis_roll(ax, roll - 180)

					a = q0.a[1:4] / q0.a[0]
					alist.append(a)
				aa = np.array(alist)


				d2 = np.sum(aa[:, 0:2] ** 2, axis = 1)
				var = np.mean(d2)

				aa = aa[np.where(d2 < var * 4)]


				line = cv2.fitLine(aa / aa[0,2] * 100, cv2.DIST_L2, 0.001, 0.000001, 0.000001)[0:3].reshape(3)

				line2d = line[0:2] / line[2]
				aa2d = aa[:, 0:2] - np.outer(aa[:, 2],  line2d)
				cov =np.cov(aa2d.T)
				#print cov
				w = np.matrix(cov).I
				#print ci, "w", w
				weights += w
				wsum += w * line2d.reshape((2,1))
	
				#print ci, "weights", weights
				#print ci, "wsum", wsum
			except:
				continue
	
		try:
			line2d = weights.I * wsum
			#print "res", line2d
			line = np.array([line2d[0,0], line2d[1,0], 1])

			ra, dec = xyz_to_ra_dec(line)
		
			if dec < 0:
				dec = -dec
				ra -= 180
			if ra < 0.0 :
				ra += 360
		
			self.ra = ra
			self.dec = dec
			self.solved = True
		except:
			return None, None
		#print "rotation center", ra, dec
		#print "prec", self.prec_ra, self.prec_dec
		return ra, dec
예제 #3
0
파일: polar.py 프로젝트: nadvornik/astro
		poslist = []
		for i in range(0, len(self.pos)):
			if self.campos_adjust[i] is None:
				continue
			prev_pos, prev_t = self.campos_adjust[i]
			if abs(t - prev_t) > 10:
				continue
			if i > 0  and self.campos_avg[i] is None:
				self.camera_position(i)
			if i > 0  and self.campos_avg[i] is not None:
				prev_pos =  prev_pos * self.campos_avg[i]
			poslist.append(prev_pos)
		
		print [p.to_euler() for p in poslist]
		
		pos = Quaternion.average(poslist)

		if self.p2_from is None:
			self.mode_adjust_set_ref_pos()
			self.p2_from = pos
			self.save()
			
		t = pos / self.p2_from
		print t.to_euler()
		self.ra, self.dec = t.transform_ra_dec([self.ref_ra, self.ref_dec])
	

	def plot2(self, size = 960, area = 0.1):
		ha = celestial_rot() + self.status['gps'][1]
		qha = Quaternion([90-ha, 0, 0])