Currently, solar aspects are showing signs of melt by day and a freeze by night. Only the upper 10-20 cm is re-freezing into a solid crust which typically breaks down by noon. Most solar slopes at lower elevations are becoming
isothermal. You can still find dry, wintery snow on North facing slopes above 2000m and variable wind effect remains. Two crusts exist in the upper snowpack and the bond of the overlying snow is most concerning. The first crust is down 20 to 30 cm and loose wet avalanches have slid on this interface. The deeper one down 60-95 cm has also produced easy shears in test profiles and is potentially just waiting for enough heat to penetrate, creating a cohesive slab that may avalanche, if it does? This will likely become less of a concern over time when temperatures drop to more seasonal norms.