Monthly Notices of the Royal Astronomical Society, Volume 53; Volumes 1892-1893Priestley and Weale, 1893 Includes lists of additions to the Society's library, usually separately paged. |
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Page 22
... moment may be found by making this moment the epoch of the constant part of the total clock correction ; but this may bring in practical diffi- culties in computing , requiring , for example , the 22 LIII . I , Mr. Hedrick , Probable Error.
... moment may be found by making this moment the epoch of the constant part of the total clock correction ; but this may bring in practical diffi- culties in computing , requiring , for example , the 22 LIII . I , Mr. Hedrick , Probable Error.
Page 23
... probable error of AT and p . The probable error of AT will be a function of these probable errors and the interval between the epochs of AT and AT 。, but it will not be a function of these only , if the proper epoch is not chosen for ...
... probable error of AT and p . The probable error of AT will be a function of these probable errors and the interval between the epochs of AT and AT 。, but it will not be a function of these only , if the proper epoch is not chosen for ...
Page 24
... a maximum when the epoch is so chosen as to make the last term zero , or , since [ dd . 3 ] is not infinite , when [ de . 3 ] = 0 . We have the following expressions , in determinant nota- tion 24 LIII . I , Mr. Hedrick , Probable Error.
... a maximum when the epoch is so chosen as to make the last term zero , or , since [ dd . 3 ] is not infinite , when [ de . 3 ] = 0 . We have the following expressions , in determinant nota- tion 24 LIII . I , Mr. Hedrick , Probable Error.
Page 26
... probable error , t ' [ de . 3 ] for the assumed epoch [ ee . 3 ] • ( 5 ) The value found for t ' is the quotient of the same coefficients , after the equations have been freed from all the unknowns except AT 。 and p , of which it would ...
... probable error , t ' [ de . 3 ] for the assumed epoch [ ee . 3 ] • ( 5 ) The value found for t ' is the quotient of the same coefficients , after the equations have been freed from all the unknowns except AT 。 and p , of which it would ...
Page 27
... probable error at this epoch and the product of the square of the probable error of the rate into the square of the interval from this epoch , ( 1 ) . Hence the square of the probable error of the clock correction at this epoch is equal ...
... probable error at this epoch and the product of the square of the probable error of the rate into the square of the interval from this epoch , ( 1 ) . Hence the square of the probable error of the clock correction at this epoch is equal ...
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Academy Andromedæ angle appeared Aquilæ Astronomer Royal Auriga Bisection bright Burnham Camelop Canis Carinæ Cassiopeia Catalogue Centauri centre Cephei cluster coefficient comet comparison stars correction Cygni Dembowski determined diameter distance double stars E. E. Barnard eclipse epoch Equat equatoreal exposure Galactic Long Geminorum Greenwich Greenwich Mean instrument Isaac Roberts June Jupiter Lalande lens Lick Observatory London longitude lunar Lupi Magn magnitude me²e mean measures Meteorological micrometer Monocerotis Monthly Notices Moon motion nebula Nova Auriga observations obtained Ophiuchi orbit Orionis paper parallax Paris period Persei photographs planet plates position probable error Professor proper motion Puppis Refraction right ascension Royal Observatory S. W. Burnham Sagittarii satellite Saturn Schiaparelli Scorpii seen Sept solar spectra spectroscope spectrum stellar Struve Tauri telescope thermometer tion transit transit circle Velorum ΙΟ