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<br />I <br /> <br />13 <br /> <br />I <br /> <br />A. Storm Structure and Sequence <br /> <br />1. Typical storm <br /> <br />Fig. 3.1 is a schematic of the typical height-time cross-section for a <br /> <br />storm as it moves across Holf Creek Pass. The schematic was derived by con- <br /> <br />I <br /> <br />I <br /> <br />structing a height-time cross-section for each storm studied over the San <br /> <br />I <br /> <br />Juans with instrumented aircraft during the 1973, 1974 and 1974-75 winter <br /> <br />seasons. In all there were 12 separate storms studied. All but one of the <br /> <br />I <br /> <br />storms contained most of the significant characteristics displayed in Fig. <br /> <br />I <br /> <br />3.1. The special storm ~vill be discussed separately. <br /> <br />Contained in Fig. 3.1 is the time sequence of cloud tops as determined <br /> <br />from the Durango rawinsonde. Cloud tops are assumed to be at saturation with <br /> <br />I <br /> <br />respect to ice. The clouds tops during the front half of the storm were <br /> <br />often not precisely determinable because the temperature and dewpoint would <br /> <br />I <br /> <br />slowly separate with height. \{hen the cloud tops began to lower they did so <br /> <br />because of subsidence from aloft, thus well defined cloud tops associated ~vith <br /> <br />I <br /> <br />I <br /> <br />subsidence inversions developed later in the storm. <br /> <br />The time sequence of cloud bases was easier to determine. Throughout <br /> <br />I <br /> <br />the storm the saturation level was generally well defined on the Durango <br /> <br />rawinsonde. The typical sequence of cloud bases was as shown in Fig. 3.1. <br /> <br />The cloud bases lowered rapidly at the front end of the storm because the <br /> <br />mid-level moist air was rapidly approaching from the southwest. ~~en pre- <br /> <br />I <br /> <br />I <br /> <br />cipitation began to fall over and upwind of the San Juans, the air mass was <br /> <br />I <br /> <br />soon saturated to the ground. Hith the formation of convection the convec- <br /> <br />tive cloud bases became distinct and typically occurred at 2.5 to 3.0 km. <br /> <br />The region of convective instability was determined by examining th~ <br /> <br />I <br /> <br />I <br /> <br />vertical profile of B (the equivalent potential temperature) as a function <br />e <br />of time and by examining the individual wind profiles and soundings plotted <br /> <br />I <br />I <br />