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Second, the flight track design in the form of a wind-aligned 46kmwide racetrack allowed some three dimensional aspects of the wave field to be determined, such as the lee wave alignment and lateral amplitude heterogeneity. The length of the racetrack (~180km) allows massif scale flow structures to be distinguished from shorter lee waves associated with atmospheric resonances. Also, the combined use of Bernoulli's and Crocco's theorems allowed the potential vorticity to be determined.
The third important aspect of the GV campaign in T-Rex was the accurate repeatability of the tracks during each mission and from flight to flight. Our primary focus will be on the eight missions (87 racetracks) that used the so-called Track B, with a cross-Sierra WSW-ENE orientation. This standardization allowed the dynamic differences between legs to be attributed to real atmospheric differences, rather than to an altered location relative to the complex Sierra Nevada terrain. By using racetrack data from three altitudes (~9, 11 and 13km), variation in wave properties between the troposphere and stratosphere can be seen. The properties of each wave encounter are summarized in a table, including indices describing the degree of non-hydrostatic and non-linear wave dynamics. Some statistical relationships regarding wave propagation properties are discussed.
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