Joint Astronomy Centre
Show document only
JAC Home
JCMT
UKIRT
Contact info
JAC Divisions
OMP
Outreach
Seminars
Staff-only Wiki
Weather
Web Cameras
____________________

JCMT home
Telescope
Pointing
990122 report

The relationship between inclinometry spikes and temperature gradients


SUMMARY
The expected relationship between thermal gradients within the antenna structure and inclinometry spike height is not well seen.

Justin's theory that the 'spikes' in inclinometry difference spectra (and thence the symmetry of the antenna) are caused by wheel loadings occasionally reaching zero, has a corallary that the effect will be exacerbated by large thermal differences between the upper antenna structure and the lower members. If the lower A-frame beams remain at constant temperature while the upper A-frame members contract under cooling, then the A-frames will 'curl up' and the wheel loadings will diminish.

The inclinometry data are accompanied by temperature readings, in volts (V), from the third channel in each inclinometer. Examination of the data confirms the manufacturer's specification that the temperature = 0.1 * the voltage - with an undetermined (unspecified) zero point. I adopt Tincl = 0.1*V - 6.0 as a determinant of temperature (deg C). The 1998 inclinometry were examined for Tincl from both left and right A-frame inclinometers, and the weather station data were examined for the simultaneously recorded antenna leg temperatures. The means of the inclinometry and the means of the leg data then allow the construction of the temperature difference (Tincl - Tmeanleg), a time history of which is plotted below :

It was hoped that this plot would resemble the asymmetry plot, but such a resemblance is not obvious.


Iain Coulson
22 Jan 1999 - updated 28 Jan 1999
Contact: Iain Coulson. Updated: Sat Nov 6 18:00:30 HST 2004

Return to top ^