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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Excitation of gravity waves by ocean surface wave packets: Upward propagation and reconstruction of the thermospheric gravity wave field
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Excitation of gravity waves by ocean surface wave packets: Upward propagation and reconstruction of the thermospheric gravity wave field

机译:海洋表面波包对重力波的激励:热层重力波场的向上传播和重建

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In this paper, we derive the atmospheric gravity waves (GWs) and acoustic waves excited by an ocean surface wave packet with frequency ω_F and duration χ in an f plane, isothermal, windless, and inviscid atmosphere. This packet is modeled as a localized vertical body force with Gaussian depth σ_z. The excited GW spectrum has discrete intrinsic frequencies (ω_(Ir)) at ω_F and ω_F±2π∕χ ("sum" and "difference") and has a "continuum" of frequencies for ω_(Ir) < ω_F + 2π∕χ. The momentum flux spectrum peaks at ω_(Ir) ~ ω_F and decreases rapidly as ω_(Ir) decreases. To simulate the effect these GWs have on the thermosphere, we present a new scheme whereby we sprinkleN GW spectra in the ocean wave packet region, ray trace the GWs, and reconstruct the GW field. We model the GWs excited by ocean wave packets with horizontal wavelengths of λ_H = 190 km, periods of τ_F = 2π∕ω_F = 14 ? 20 min and χ = 30 ? 50 min. The excited GWs begin to arrive at z = 250 km at t ~ 75 ? 80 min. Those with the largest temperature perturbations T′ have large ω_(Ir) and arrive at t ~ 90 ? 130 min. If |α| = ω_F + 2π∕χ is a solution of the GW dispersion relation and |α| is less than the buoyancy frequency at z = 250 km, the sum and highest-frequency continuum GWs have much larger phase speeds and arrive 50–60 min earlier with larger T′ than the GWs with frequency ω_F. For a packet with λ_H = 190 km, τ_F = 14 min, χ = 30 min, and height h_0 = 1.3 m, the maximum T′ at z = 250 km is ~9, 22, and 40 K for σ_z = 1, 2, and 4 m, respectively.
机译:在本文中,我们推导出了在f平面,等温,无风和无粘性大气中,频率为ω_F且持续时间为χ的海面波包所激发的大气重力波(GWs)和声波。该数据包被建模为具有高斯深度σ_z的局部垂直体力。激发的GW频谱在ω_F和ω_F±2π∕χ(“和”和“差”)处具有离散的固有频率(ω_(Ir)),并且对于ω_(Ir)<ω_F+2π∕χ具有频率的“连续谱” 。动量通量谱在ω_(Ir)〜ω_F达到峰值,并随着ω_(Ir)的减小而迅速减小。为了模拟这些GW对热圈的影响,我们提出了一种新的方案,在该方案中,将N GW光谱撒在海浪包区域中,用射线追踪GW,并重建GW场。我们对水平波波长为λ_H= 190 km,周期τ_F=2π∕ω_F= 14? 20分钟,χ= 30? 50分钟激发的GW在t〜75时开始到达z = 250 km。 80分钟温度扰动T'最大的那些具有大的ω_(Ir),达到t〜90? 130分钟如果|α| =ω_F+2π∕χ是GW色散关系和|α|的解。小于z = 250 km时的浮力频率,总和和最高频率连续体GW的相速度要大得多,并且比具有频率ω_F的GW的T'提前50-60分钟。对于λ_H= 190 km,τ_F= 14 min,χ= 30 min,高度h_0 = 1.3 m的数据包,对于z_ 250 km,对于σ_z= 1,2的最大T'为〜9、22和40K。和分别为4 m。

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