The Big Bear videomagnetograph is calibrated using three methods. Longitudinal magnetograms are calibrated by using the differences in radial velocity of the Sun caused by solar rotation, or by measuring the line profile in the Zeeman-sensitive 6103 Å line used by the magnetograph system. Transverse magnetograms can be calibrated by obtaining spectra in the more magnetically sensitive 5250 Å line which measure the total magnetic field and then subtracting the longitudinal component. The calibration of the transverse magnetograms is in agreement with that obtained by line profile measurements. Observations of an active region on 1993 March 8 with both the magnetograph system and with the BBSO spectrograph showed that good agreement was found between all three methods, provided the effect of seeing on the magnetograms is allowed for. Magnetograph saturation does not occur for magnetic fields below about 2100 G.
|Original language||English (US)|
|Number of pages||22|
|State||Published - Nov 1 1995|
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science