speed 等于 distance / time。 longitude 和 latitude 可能代表地球表面的位置。如果我们接受一个半径为 6371 公里的球体作为地球的近似值,那么我们可以轻松地将 longitude 和 latitude 转换为 xyz-坐标:
r = 6371000 # meters
df['theta'] = np.deg2rad(df['longitude'])
df['phi'] = np.deg2rad(df['latitude'])
df['x'] = r*np.cos(df['theta'])*np.sin(df['phi'])
df['y'] = r*np.sin(df['theta'])*np.sin(df['phi'])
df['z'] = r*np.cos(df['phi'])
现在计算连续点之间的距离并不难:
df['x2'] = df['x'].shift()
df['y2'] = df['y'].shift()
df['z2'] = df['z'].shift()
df['distance'] = np.sqrt((df['x2']-df['x'])**2 + (df['y2']-df['y'])**2 + (df['z2']-df['z'])**2)
然而,这是一个弦长——球体表面上两点之间的直线距离。如果这些点相距很远,弦就会穿过地球表面。据推测,运动发生在地球表面。所以更准确的距离计算将使用arclength:
df['central angle'] = np.arccos((df['x']*df['x2'] + df['y']*df['y2'] + df['z']*df['z2'])/r**2)
df['arclength'] = df['central angle']*r
圆心角使用dot product formula。
在计算了弧长(距离)之后,我们现在还必须计算连续观察之间的time 间隔(即 DataFrame 的行):
df['time'] = (df.index.to_series().diff() / pd.Timedelta(seconds=1))
所以使用speed = distance / time:
df['speed'] = df['arclength'] / df['time'] # in meters/second
import numpy as np
import pandas as pd
df = pd.DataFrame({'ele': [73.0, 73.0, 73.0, 73.0, 73.0], 'latitude': [-33.816178, -33.81615, -33.816117, -33.816082, -33.816043], 'longitude': [150.871032, 150.871035, 150.87104399999998, 150.87105400000002, 150.871069], 'temp': [7, 7, 7, 7, 7], 'time': ['2017-07-08 22:05:45', '2017-07-08 22:05:46', '2017-07-08 22:05:47', '2017-07-08 22:05:48', '2017-07-08 22:05:49']})
df['time'] = pd.to_datetime(df['time'])
df = df.set_index('time')
columns = df.columns.tolist()
r = 6371000 # radius of the Earth in meters
df['theta'] = np.deg2rad(df['longitude'])
df['phi'] = np.deg2rad(df['latitude'])
df['x'] = r*np.cos(df['theta'])*np.sin(df['phi'])
df['y'] = r*np.sin(df['theta'])*np.sin(df['phi'])
df['z'] = r*np.cos(df['phi'])
df['distance'] = np.sqrt((df['x2']-df['x'])**2 + (df['y2']-df['y'])**2 + (df['z2']-df['z'])**2)
df['x2'] = df['x'].shift()
df['y2'] = df['y'].shift()
df['z2'] = df['z'].shift()
df['central angle'] = np.arccos((df['x']*df['x2'] + df['y']*df['y2'] + df['z']*df['z2'])/r**2)
df['arclength'] = df['central angle']*r
df['time'] = (df.index.to_series().diff() / pd.Timedelta(seconds=1))
df['speed'] = df['arclength'] / df['time'] # in meters/second
df = df[columns + ['speed']]
print(df)
产量
ele latitude longitude temp speed
time
2017-07-08 22:05:45 73.0 -33.816178 150.871032 7 NaN
2017-07-08 22:05:46 73.0 -33.816150 150.871035 7 3.119892
2017-07-08 22:05:47 73.0 -33.816117 150.871044 7 3.712201
2017-07-08 22:05:48 73.0 -33.816082 150.871054 7 3.940673
2017-07-08 22:05:49 73.0 -33.816043 150.871069 7 4.433590
如果你注释掉
df = df[columns + ['speed']]
然后重新运行脚本,您将看到所有中间计算。你会
请注意df['distance'] 非常接近df['arclength']。由于
地球表面上的点相距不是很远,弦长是
弧长的良好近似。所以对于你发布的数据
df['speed'] = df['distance'] / df['time']
本来也可以的。不过arclength的计算有点
更稳健,因为如果点距离较远,它将给出更准确的值
分开。