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Accuracy and resolution of atmospheric profiles obtained from radio occultation measurements.

机译:从无线电掩星测量获得的大气廓线的准确性和分辨率。

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A new formulation for interpreting radio occultation phase data is achieved by treating the radio occultation method as a straight-ray tomography experiment in which only one parallel projection of the object is available. This approach yields the inherent two-dimensional, geometrical optics (GO), resolution kernel directly. The kernel has a strong positive peak in the vertical direction at its lowest point and a decaying negative branch significant over a few kilometers above the positive peak; along the ray the kernel is constant. The three-dimensional resolution kernel incorporating the full-wave nature of radio waves resembles the two-dimensional result in the vertical direction smoothed on the order of a Fresnel zone. In the across-propagation horizontal direction it has the shape of the Fresnel zone; along the ray its shape is unchanged from GO. The curving of rays due to the spherically symmetric background is included in the kernel by using a set of transformations which convert the problem into an equivalent problem where curved rays are represented as straight rays. The curved-ray kernel exhibits the shortcoming of the radio occultation method in the event of critical refraction. For perfect data for a spherical atmosphere the inverse problem is solved exactly with the kernel formulation.; Large-scale departures from sphericity are modeled as locally spherical structures with center of symmetry offset from the center of mass. A first-order perturbation analysis yields analytic expressions for the errors in radius, refractivity, pressure, and temperature for general conditions. The resulting errors depend on the orientation and magnitude of the horizontal gradient at ray periapsis, and on the trajectory. For the atmosphere of Mars fractional errors in refractivity, temperature, and pressure can be as large as a few percent for altitudes above 30 km. For Earth's troposphere the errors are highly sensitive to horizontal gradients because of the large bending; typically, the error magnitude remains less than two percent because the horizontal gradients are mild. Comparison of results from the analysis with those from simulated occultations by the atmospheres of Mars and Earth and subsequent Abel inversion shows good agreement.
机译:通过将无线电掩藏方法作为仅在对象上有一个平行投影的直线射线层析成像实验进行处理,即可获得一种解释无线电掩藏相位数据的新公式。这种方法直接产生固有的二维几何光学(GO)分辨率内核。籽粒的最低点在垂直方向上有一个强的正峰,而在正峰上方几公里处有一个衰减的负分支。沿着射线,内核是恒定的。结合了无线电波的全波特性的三维分辨率内核类似于在垂直方向上按菲涅耳区域平滑的二维结果。在横向传播方向上,它具有菲涅耳带的形状;沿着射线,其形状与GO保持不变。通过使用一组转换将归因于球对称背景的射线弯曲包括在内核中,这些转换将问题转换为等效问题,其中弯曲射线表示为直射线。弯曲射线核在临界折射的情况下表现出无线电掩藏方法的缺点。对于球形大气的完美数据,反问题可以通过核公式精确解决。球形的大规模偏离被建模为局部球形结构,其对称中心偏离质心。一阶扰动分析可得出一般条件下半径,折射率,压力和温度误差的解析表达式。所产生的误差取决于射线根尖处水平梯度的方向和大小以及轨迹。对于火星大气层,在海拔30公里以上的地方,折射率,温度和压力的分数误差可能高达百分之几。对于地球的对流层,由于弯曲较大,因此误差对水平梯度高度敏感;通常,由于水平梯度较小,因此误差幅度保持在百分之二以下。将分析的结果与火星和地球大气的掩星和随后的Abel反演得到的结果进行比较,显示出很好的一致性。

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