论文标题

干涉法中闭合阶段的几何视图

A Geometric View of Closure Phases in Interferometry

论文作者

Thyagarajan, Nithyanandan, Carilli, Christopher L.

论文摘要

闭合阶段是$ \ ge 3 $元素干涉仪阵列中相关性的闭环乘积的阶段。它对基于元素的相位腐败的不变性使其对于否则需要高准确阶段校准的干涉应用程序来说是无价的。但是,它的理解主要是数学上的,并且仅限于光圈平面(图像平面的傅立叶双重双重)。在这里,我们为几何见解奠定了基础。我们表明,封闭阶段及其对基于元素的损坏和翻译的不变性与主三角形的保守特性(形状,方向,大小或SOS)无关,由由封闭的三大阵列元素形成的三个条纹包含的主三角形,这是“ SOS保护原理”。当不需要基于元素的振幅校准,而在光学干涉仪中典型的校准也是如此,除了可能的偏移外,由相位未校准的相关形成的3元素干扰图像是源对象形态的真实且无腐败的表示。基于该SOS保护原则,我们提出了两种几何方法,可以直接从3元素干扰图像(不需要孔径平面视图)直接测量闭合相位:图像平面分别。我们使用来自非常大的阵列和事件范围望远镜的数据来验证各种干涉条件的几何理解。这种几何见解可能对其他干涉应用(例如光学干涉仪)有价值。这些几何关系是针对$ n $ element干涉仪的概括的。

Closure phase is the phase of a closed-loop product of correlations in a $\ge 3$-element interferometer array. Its invariance to element-based phase corruption makes it invaluable for interferometric applications that otherwise require high-accuracy phase calibration. However, its understanding has remained mainly mathematical and limited to the aperture plane (Fourier dual of image plane). Here, we lay the foundations for a geometrical insight. we show that closure phase and its invariance to element-based corruption and to translation are intricately related to the conserved properties (shape, orientation, and size, or SOS) of the principal triangle enclosed by the three fringes formed by a closed triad of array elements, which is referred herein as the "SOS conservation principle". When element-based amplitude calibration is not needed, as is typical in optical interferometry, the 3-element interference image formed from phase-uncalibrated correlations is a true and uncorrupted representation of the source object's morphology, except for a possible shift. Based on this SOS conservation principle, we present two geometric methods to measure the closure phase directly from a 3-element interference image (without requiring an aperture-plane view): (i) the closure phase is directly measurable from any one of the triangle's heights, and (ii) the squared closure phase is proportional to the product of the areas enclosed by the triad of array elements and the principal triangle in the aperture and image planes, respectively. We validate this geometric understanding across a wide range range of interferometric conditions using data from the Very Large Array and the Event Horizon Telescope. This geometric insight can be potentially valuable to other interferometric applications such as optical interferometry. These geometric relationships are generalised for an $N$-element interferometer.

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