Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.atnf.csiro.au/people/pulsar/tempo/ref_man_sections/tz.txt Дата изменения: Thu Apr 28 12:36:42 2005 Дата индексирования: Tue Dec 25 18:28:38 2007 Кодировка: Поисковые слова: annular solar eclipse

PREDICTION MODE

In prediction mode (indicated by '-z' on the command line, and
sometimes called 'tz' mode), tempo calculates pulsar ephemerides over
short periods of time (typically hours) in the form of a simple
polynomial expansion. Such ephemerides are particularly useful for
on-line folding of pulsar data while observing. Ephemerides are
calculated on a day-by-day basis centered about the transit time of
the pulsar at the observatory. The time spans of the polynomial
series are specified by giving a 'maximum hour angle' for observations
along with a maximum time span over which a single series must be
valid. Multiple series within a day are calculated when necessary.
The user is queried for start and end dates (MJD) for which
ephemerides will be calculated.

The list of pulsars for which ephemerides are to be produced is read
from file 'tz.in'.