ANALYSIS
OF LUNAR ECLIPSE OBSERVATIONS - BY
BYRON W. SOULSBY, THEODORE LUNAR OBSERVATORY, AUSTRALIA
OBLATENESS
ESTIMATES FOR 19970916
STATISTICAL
RANGE IS 0 % TO 4 %
|
OBSERVER |
TYPE |
O/T |
No |
Ecc |
Re |
Rp |
Fo |
SD |
SK' |
|
|
|
|
|
|
|
|
|
|
|
|
CLARK M. L |
|
|
|
|
|
|
|
|
|
|
|
IM |
O |
58.00 |
0.2015 |
0.7805 |
0.7645 |
48.7712 |
0.1294 |
4.5351 |
|
|
IM |
T |
58.00 |
0.0956 |
0.7459 |
0.7425 |
218.5275 |
0.0593 |
1.0121 |
|
|
EM |
O |
5.00 |
0.2006 |
0.7754 |
0.7596 |
49.1792 |
0.0136 |
4.4975 |
|
|
EM |
T |
5.00 |
0.1205 |
0.7489 |
0.7434 |
137.1283 |
0.0359 |
1.6129 |
VALUE
OF FM (RECIPROCAL) = 221.18
DATE
OF RUN 03-08-2007 AT TIME 15:15:46
For an Excel Chart showing the computed Topocentric umbra (Fi) and slant angle (delta) click here.
For an extended explanation of the Topocentric Umbra theory click here.