Unfortunately, our sparse network of morning upper-air observations fails to resolve the full scope of most MCVs. The result? Both human and numerical analyses have little sense of the true thermodynamic and kinematic environment in its vicinity; if not for satellite and sometimes radar observations, we would be rendered nearly blind to one’s existence. Thus, remnant MCV tornadoes often come as a “surprise” to a local area, with the attendant SPC 1300z outlooks examined carrying a less than satisfactory detection rate. Using operational knowledge of the conventional supercell parameter space for deep-layer shear and instability have proven unsuccessful for these, but upon closer examination, a near-surface environment rich in both shear and instability does exist. This study will explore what we can observe about MCVs, including satellite presentations, and the positions relative to them that tornadoes tend to occur. It will also explore the climatological patterns and mesoscale precursors leading up to these events that may be the early warning we need.
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