Lites et al. (1994) (hereafter LMS) have recently published a comparis
on of the response of their magnetograph (the Advanced Stokes Polarime
ter (ASP)) to that they expect from filter-based magnetographs (FM). N
ot surprisingly, they conclude the ASP is better. They claim that only
their instrument is ''quantitative,'' and others are not, and that th
e transverse field strength and azimuth measured by filter magnetograp
hs may be in error by up to 50%. While the calculation is formally cor
rect it ignores the high sensitivity attained by real FM's accumulatin
g thousands of difference frames. Further, FM's have been cross-compar
ed and tested empirically, without any such errors appearing. We point
out that the two instruments have different roles, but the functional
use of the FM is far superior to the ASP for solar research. The ASP
may give accurate results for unresolved unipolar fields; it gives tot
ally erroneous results when the field rapidly changes direction within
its resolution element, as occurs in delta spots.