Wind on Mars doesn’t follow the large-scale pressure gradient. Newman et al. (arXiv 2604.02095) compared Perseverance rover measurements in Jezero Crater to mesoscale CFD simulations and found that local topography dominates. The 500-meter crater rim creates wind shadows on the lee side, where flow velocity drops to near zero, and acceleration zones at the rim crest, where channeling amplifies speeds by a factor of 2-3 above the regional mean. The large-scale Hadley circulation provides the energy, but the local terrain determines where it goes. Slope winds — driven by differential heating of crater walls — reverse direction on a diurnal cycle, completely overriding the background flow twice per day. At the boundary of Jezero’s rim, the topographic forcing is stronger than the planetary-scale pressure gradient driving it.

Israel’s announced plan on April 3 to destroy civilian infrastructure within a 2-3 km buffer zone along the Lebanese border follows the same structural logic. The large-scale gradient is strategic: Hezbollah’s tunnel networks, weapons caches, and observation posts positioned in southern Lebanon. But the specific pattern of destruction — which villages, which roads, which buildings — is determined by the local topography. Ridgelines provide line-of-sight; wadis channel movement; built structures create cover. The buffer zone is not drawn by strategy alone. It is drawn by what the terrain permits. A 2-3 km zone in flat terrain would have different military meaning than a 2-3 km zone in the hilly terrain of the Galilee-Lebanon border, where elevation changes of 400 meters over short distances create the same wind-shadow effect that Jezero’s rim creates — zones of control and zones of vulnerability determined by the ground, not the map.

The Martian wind and the border zone are both shaped by the same principle: large-scale gradients provide the energy, but local terrain determines the pattern.

At any boundary, the topography decides what the gradient actually does.