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Convective mixing near the tropical tropopause: Insights from seasonal variations

机译:热带对流层顶附近的对流混合:季节变化的见解

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It has been suggested that convection remains important in the budget of water vapor up to the tropical tropopause or even higher. But observed seasonal variations of CO2 and water vapor in the lower stratosphere, and their timing, call the required convective transport into question. Here, these seasonal variations are modeled using several idealized representations of convection. First, a CO2-like tracer is added to a previously published climate model in which convection explicitly transports air to a variety of heights ranging from 14 to 19 km, in a manner sufficient to dehydrate the stratosphere. It is found that these motions are consistent with the observed lags and amplitudes of seasonal variations near and above the tropopause, including a 2-month phase lag in CO2 at 390 K relative to surface values and a similar lag in H2O relative to tropopause temperatures. This result is explained in terms of the model's mixing physics. Next the ability of other models is considered, where convective outflows are confined below some ceiling at or below the cold-point tropopause, to account for the observed seasonal cycles. Behavior of such models is governed by the placement of the ceiling relative to a known stagnation surface in the radiatively balanced vertical velocity. It is found that convection must reach to within 1 km of the cold point in order for realistic seasonal cycles to exist above the tropopause in these simulations. Importantly, the properties of air entering the stratosphere must be determined by those of the planetary boundary layer rather than the upper troposphere. This work reinforces the view that convective mixing must evanesce gradually in importance through a tropical tropopause layer of substantial thickness, rather than stopping at any particular height. [References: 26]
机译:已经提出,对流在直到热带对流层顶甚至更高的水蒸气的预算中仍然很重要。但是,平流层下部观测到的CO2和水蒸气的季节性变化及其时机,使对流传输产生了疑问。在这里,这些季节性变化是使用对流的几种理想化表示来建模的。首先,在以前发布的气候模型中添加了类似于CO2的示踪剂,在该模型中,对流以足以使平流层脱水的方式将空气显着地输送到14至19 km的各种高度。发现这些运动与在对流层顶附近和上方观测到的时滞和季节变化幅度一致,包括相对于表面值在390 K的CO2中2个月的相位滞后和相对于对流层顶温度的H2O相似的时滞。根据模型的混合物理来解释此结果。接下来考虑其他模型的能力,其中对流流出被限制在冷点对流层顶或以下的某个上限以下,以解释观测到的季节性周期。这种模型的行为受辐射平衡垂直速度中天花板相对于已知停滞表面的放置的影响。发现在这些模拟中,对流必须达到冷点的1公里以内,以使现实的季节周期存在于对流层顶上方。重要的是,进入平流层的空气的属性必须由行星边界层的属性而不是对流层的上部确定。这项工作强化了这样的观点,即对流混合必须通过相当厚的热带对流层顶层逐渐避免重要性,而不是停止在任何特定高度。 [参考:26]

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