doPause ! Logical GLOBALwhich can be set to
.true.
or .false.
with
let doPause yesrespectively
let doPause noIt is used to halt the execution of
MIRA\SOLVE
until the
user types continue
.
writeXML ! Logical GLOBALis used to write (
let writeXML yes
) XML files with pointing, focus, and
calibration solutions applied to the data (respectively to suppress this via
let writeXML no
). The files are named
iram30-pointing-20071022s99.xml
for pointings, and
iram30m-focus-...
and iram30m-calibration-...
for focus
solutions and calibration parameters, respectively.
The following variables are used by the automatic online data processing (see
section 2), and specify, for the 30m file system, the paths to the imbFits raw
data location (ncsData) and to the MIRA data products (visData), respectively:
ncsData ! Character* 256 GLOBAL visData ! Character* 256 GLOBAL
calByChannel ! Logical GLOBALBy default, one separate calibration temperature is applied for each spectral baseband. If you want to use a different calibration temperature for each spectral channel, use
let calByChannel yes
) before reading a calibration
scan. This feature is to be used e.g. if the image gain is not neglectable (e.g.
DSB tuning) and varies significantly across the spectral bandpass.
calCheck ! Logical GLOBALThe SIC logical variable
calCheck
(default: .true.
) allows to
check the consistency of an observation and its calibration measurement. If
only part of the backend units are calibrated, then MIRA tries to identify
backend units that can be calibrated. Use let calCheck = no
when you
connect two or more parts of the same backend to the same receiver, with
identical spectral setup (otherwise the assignment of the calibration
parameters will not be unique anymore).
ignoreTraceflag ! Logical GLOBALThe
TRACEFLAG
parameter in the raw data indicates whether the antenna was
in a defined state (e.g. tracking or scanning) or not. The latter may happen in
the data if synthesizer data are taken while the antenna is in stow position (thus
simulating astronomical observations). The default is let ignoreTraceflag no
.
For data taken while the antenna is in stow position please set it to yes
.
badLevel ! Real GLOBALThe
badLevel
parameter allows to automatically flag bad spectral
channels. Default: if in the calibration the total power of a spectral
channel is more than a factor 20 above or below the median total power
across the baseband under consideration, this raw data point will be
flagged (and the calibrated spectral channel too).
flagBSwSpikes ! Logical GLOBALA recent analysis has shown that some dumps in beam switched pointings have abnormally short integration times (5 msec and more below the nomincal value). However, the actual integration times are longer. The wrong normalization (from counts to count rates) thus results in spikes. With
let flagBSwSpikes .true.
this data are automatically flagged (default:
no flagging).
timingCheck ! Logical GLOBALBy default (
timingCheck = yes
) MIRA checks that each backend data
point is framed in time by data point from the other data streams (subreflector,
antenna, fast and slow traces). If this is not the case although the data point
is between the nominal subscan start and end time, the latter are modified
accordingly in order to avoid hazardous extrapolations. This automatic correction
can be switched off by setting let timingCheck no
(after a change of the
timingCheck
flag, the scan needs to be read again in order to validate the
new settings.
traceExtrapolation ! Logical GLOBALOnly for
timingCheck = no
. Allows for extrapolation of antenna trace data
(fast and slow) for backend data at scan start without a trace data point before,
or for backend data at scan end without a trace data point after.