Table_2.html
ANALYSIS OF LUNAR ECLIPSE OBSERVATIONS
- BY BYRON W. SOULSBY, CALWELL LUNAR OBSERVATORY, AUSTRALIA
OBLATENESS ESTIMATES FOR 2001 JANUARY 9
STATISTICAL RANGE of umbral enlargement %E IS 0 % TO 4 %
|
OBSERVER |
TYPE |
No |
Ecc |
Re |
Rp |
Fo |
SD |
SK' |
|
|
|
|
|
|
|
|
|
|
|
CLARK MAURICE AND NORMA |
||||||||
|
IM |
O |
117.00 |
0.0807 |
0.7535 |
0.7511 |
306.9315 |
0.0332 |
0.7148 |
|
IM |
T |
117.00 |
0.0899 |
0.7392 |
0.7362 |
246.7270 |
0.0364 |
0.8892 |
|
KEREKE KATARINA |
|
|||||||
|
IM |
O |
27.00 |
0.0700 |
0.7537 |
0.7518 |
407.2154 |
0.0051 |
0.5387 |
|
IM |
T |
27.00 |
0.0838 |
0.7387 |
0.7361 |
284.4384 |
0.0375 |
0.7713 |
|
EM |
O |
32.00 |
0.0347 |
0.7520 |
0.7516 |
500.0000 |
0.0054 |
0.1318 |
|
EM |
T |
32.00 |
0.0867 |
0.7392 |
0.7364 |
265.4762 |
0.0336 |
0.8264 |
|
RAPAVA DANIELA |
||||||||
|
IM |
O |
20.00 |
0.0482 |
0.7526 |
0.7518 |
500.0000 |
0.0057 |
0.0003 |
|
IM |
T |
20.00 |
0.0729 |
0.7378 |
0.7358 |
375.5105 |
0.0363 |
0.0007 |
|
EM |
O |
21.00 |
0.1421 |
0.7576 |
0.7499 |
98.4851 |
0.0062 |
0.0026 |
|
EM |
T |
21.00 |
0.0912 |
0.7396 |
0.7365 |
239.7466 |
0.0367 |
0.0011 |
|
COOPER TIM BREDELL OBSERVATORY |
||||||||
|
IM |
O |
48.00 |
0.1548 |
0.7648 |
0.7556 |
82.9915 |
0.0796 |
2.6434 |
VALUE OF FM (RECIPROCAL) = 219.38
DATE OF RUN 02-17-2001 AT TIME 21:29:06
Nomenclature
OBSERVER, the
person conducting the crater timings
TYPE, O is
observed, T is theoretical, IM are immersions, EM are emersions
No, the number of
timings used that are within the statistical limits of umbral enlargement (see
also Table_1.html)
Ecc, the
eccentricity of the umbra
Re, the
equatorial radius of the umbra
Rp, the polar radius of the umbra
Fo, the observed oblateness, expressed as a reciprocal (if it is 500 then no
observed value has been obtained)
SD, the standard
deviation of the observation
SK', the value of
observed oblateness as a ratio
to that expected
