Abstract. As a result of the large difference in heat capacity
between land and ocean, global climate and atmospheric circulation patterns
over the supercontinent of Pangaea were significantly different from those of
today. Modelling experiments indicate a seasonal alternation in
cross-equatorial flow induced by the seasonal reversal in the direction of
the monsoonal circulation; however, there are large discrepancies between
model-generated surface wind patterns and the reported palaeowind
directions from aeolian dune records. Here, we present the spatial
distribution of dune slip-face azimuths recorded in the Lower Jurassic
aeolian sandstones over a wide area of the western United States
(palaeolatitude: ∼19–27∘ N). The
azimuth data for dune slip faces reveal a bidirectional and oblique angular
pattern that resembles the internal structures of modern longitudinal dunes.
Based on the spatial pattern of slip-face directions and outcrop evidence,
we suggest that most Lower Jurassic aeolian sandstones were NNE–SSW- to
NNW–SSE-oriented longitudinal dunes, which likely formed as the result of
a combination of westerly, northwesterly, and northeasterly palaeowinds.
The reconstructed palaeowind pattern at ∼19–27∘ N appears to be consistent with the model-generated surface
wind pattern and its seasonal alternation. The reconstructed palaeowind
patterns also suggest an influence of orbitally induced changes in
atmospheric pressure patterns over Pangaea.