  We propose a combination of a modified Wide-Fast-Deep survey, a mini-survey
of the South Celestial Pole, and a Deep Drilling-style survey to produce a 3-D
map of the Magellanic System and to provide a detailed census of the transient
and variable populations in the Clouds. We support modifying the Wide-Fast-Deep
survey to cover the declination range $-72.25\deg<{\rm Dec}<12.4\deg$ and the
Galactic latitude range $|b|>15\deg$, as proposed in a separate white paper. We
additionally propose a mini-survey covering the 950$\deg^2$ with ${\rm Dec} <
-72.25$ in $ugriz$ to the standard LSST single-exposure depth and with 40
visits per filter per field. Finally, we propose a mini-survey covering
$\sim100 \deg^2$ of the main bodies of the Clouds with twelve total pointings,
2000 total visits per field, and shorter exposure time.
