Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.atnf.csiro.au/computing/software/miriad/userguide/node213.html
Дата изменения: Unknown
Дата индексирования: Mon Apr 11 02:22:05 2016
Кодировка:
Поисковые слова: iss

Tracking accuracy

With the ATCA beam at 3mm being comparatively small ($35''$), it is possible for tracking errors to be significant. This may occur during windy weather (gusts can blow the antennas off the directed tracking position). In additional poor tuning of the antenna drive systems can sometimes cause poor tracking, particiularly soon after a change in source.

Note that tracking errors should be distinguished from pointing errors. Tracking errors are the inability of the antenna drive system to follow the requested path. Pointing errors correspond to the difference between the position that the astronomer requests and the actual position. Tracking errors are caused by flaws in the drive servo system, whereas pointing errors are a sum of tracking errors and errors in the antenna pointing model.

Since October 2003, tracking errors have been saved in the Miriad dataset. The uv variables corresponding to the rms and maximum tracking error in a cycle are axisrms and axismax.

Both the maximum and rms give two tracking error values for each antenna, nominally corresponding to the tracking error in the azimuth and elevation axes. However the ATCA on-line system produces a single composite value, which is replicated for the two axes in the dataset.

When the tracking error is less than $2'$, the ATCA on-line system believes that this error sufficiently small to consider that the antenna is tracking. However this tolerance is not generally good enough for 3-mm observations. The task uvflag can be used to flag based upon rms tracking error. To do this, use the selection pointing subcommand.

UVFLAG
in=vela.uv	Input visibility dataset.
flagval=flag	Flag selected points.
select=pointing(15,1000)	Flag when the rms tracking error
	is between $15''$ and $1000''$.