  The BeSSeL Survey is mapping the spiral structure of the Milky Way by
measuring trigonometric parallaxes of hundreds of maser sources associated with
high-mass star formation. While parallax techniques for water masers at high
frequency (22 GHz) have been well documented, recent observations of methanol
masers at lower frequency (6.7 GHz) have revealed astrometric issues associated
with signal propagation through the ionosphere that could significantly limit
parallax accuracy. These problems displayed as a "parallax gradient" on the sky
when measured against different background quasars. We present an analysis
method in which we generate position data relative to an "artificial quasar" at
the target maser position at each epoch. Fitting parallax to these data can
significantly mitigate the problems and improve parallax accuracy.
