The estimation of contact times for any one point begins with an interpolation for the time of maximum eclipse at that location. The time of maximum eclipse is proportional to a point's distance between two adjacent lines of maximum eclipse, measured along a line parallel to the center line. This relationship is valid along most of the path with the exception of the extreme ends, where the shadow experiences its largest acceleration. The center line duration of totality D and the path width W are similarly interpolated from the values of the adjacent lines of maximum eclipse as listed in Table 3. Since the location of interest probably does not lie on the center line, it is useful to have an expression for calculating the duration of totality d as a function of its perpendicular distance a from the center line:
where:
d | = | duration of totality at desired location (seconds) |
D | = | duration of totality on the center line (seconds) |
a | = | perpendicular distance from the center line (kilometers), and |
W | = | width of the path (kilometers) |
If t_{m} is the interpolated time of maximum eclipse for the location, then the approximate times of second and third contacts (t_{2} and t_{3}, respectively) are:
Second Contact: | t_{2} | = | t_{m} - d/2 | [4] |
Third Contact: | t_{3} | = | t_{m} + d/2 | [5] |
The position angles of second and third contact (either P or
Second Contact: | x_{2} | = | X_{2} - arcsin (2a/W) | [6] |
Third Contact: | x_{3} | = | X_{3} + arcsin (2a/W) | [7] |
where:
x_{n} | = | interpolated position angle (either P or V) of contact n at location |
X_{n} | = | interpolated position angle (either P or V) of contact n on center line |
a | = | perpendicular distance from the center
line (kilometers) (use negative values for locations south of the center line), and |
W | = | width of the path (kilometers) |