The small pocket os wind slab encountered were 4 finger hard, up to 9 inches thick, and reactive to slope cuts. They appeared to be crossed loaded in some upper entrances to steep chutes leading into the Brighton Back Bowls. Their reactivity appeared to be as a result of a weak layer of light density stellars. In more exposed terrain in the alpine this problem may have been a bit more widespread.
Small sensitive cornices on east facing ridges in the mid canyon area were sensitive and easily triggered, yet they were not creating avalanches upon descent.
Danger today appeared to be an isolated moderate for wind slabs, loose dry, and loose wet. Many steep lines were ridden with only the loose dry issue as a concern.