ISS016-E-6986 Click the photo number to access all resolutions available and the database record.
Sand grains that make up the dunes are small enough to be moved along by the wind (a process known as saltation), although much of the dune field is now anchored by vegetation. Winds blow predominately to the east, so that sand in the San Luis Valley (part of which appears at image lower left) is driven towards and piled against the Sangre de Cristo Mountains. The sand of the dunes is mostly derived from ancient exposed lakebed sediments—now the floor of the San Luis Valley—that formed by erosion of rocks in the Sangre de Cristo and San Juan Mountains (located to the west). The action of streams and occasional storms today returns some of the impounded sand back to the valley, where the prevailing winds begin the sand’s migration to the dune field anew.
The dune field has settled in a low spot along the Sangre de Cristo Mountains; the location of snow cover shows the relative altitudes of the mountains. Areas to the north of the dune field (Cleveland Peak and northward), and to the south around Blanca Peak, are higher than the ridgeline next to the dune field, where almost no snow is visible. Since winds are preferentially channeled over the lower parts of any range (hundreds of meters lower here than ridgelines to north and south), sand grains are carried up to, but not over, the low point of the range.
