  The longitudinal distribution of solar active regions shows non-homogeneous
spatial behaviour, which is often referred to as Active Longitude (AL).
Evidence for a significant statistical relationships between the AL and the
longitudinal distribution of flare and coronal mass ejections (CME) occurrences
is found in Gyenge et al, 2017 (ApJ, 838, 18). The present work forecasts the
spatial position of AL, hence the most flare/CME capable active regions are
also predictable. Our forecast method applies Autoregressive Integrated Moving
Average model for the next 2 years time period. We estimated the dates when the
solar flare/CME capable longitudinal belts face towards Earth.
