The Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry
(BLASTPol) was a suborbital experiment designed to map magnetic fields in order
to study their role in star formation processes. BLASTPol made detailed
polarization maps of a number of molecular clouds during its successful flights
from Antarctica in 2010 and 2012. We present the next-generation BLASTPol
instrument (BLAST-TNG) that will build off the success of the previous
experiment and continue its role as a unique instrument and a test bed for new
technologies. With a 16-fold increase in mapping speed, BLAST-TNG will make
larger and deeper maps. Major improvements include a 2.5 m carbon fiber mirror
that is 40% wider than the BLASTPol mirror and ~3000 polarization sensitive
detectors. BLAST-TNG will observe in three bands at 250, 350, and 500 microns.
The telescope will serve as a pathfinder project for microwave kinetic
inductance detector (MKID) technology, as applied to feedhorn coupled
submillimeter detector arrays. The liquid helium cooled cryostat will have a
28-day hold time and will utilize a closed-cycle $^3$He refrigerator to cool
the detector arrays to 270 mK. This will enable a detailed mapping of more
targets with higher polarization resolution than any other submillimeter
experiment to date. BLAST-TNG will also be the first balloon-borne telescope to
offer shared risk observing time to the community. This paper outlines the
motivation for the project and the instrumental design