Gural Peter S, Otto Paul R, Tedesco Edward F
Leidos Corporation, 14668 Lee Road, Chantilly, VA, USA 20151.
Planetary Science Institute, 1700 East Fort Lowell Road, Suite 106, Tucson, AZ, USA 85719.
Publ Astron Soc Pac. 2018 Jul;130(989). doi: 10.1088/1538-3873/aac1ff. Epub 2018 Jun 12.
There are various algorithms currently in use to detect asteroids from ground-based observatories, but they are generally restricted to linear or mildly curved movement of the target object across the field of view. Space based sensors in high inclination, low Earth orbits can induce significant parallax in a collected sequence of images, especially for objects at the typical distances of asteroids in the inner Solar System. This results in a highly non-linear motion pattern of the asteroid across the sensor, which requires a more sophisticated search pattern for detection processing. Both the classical pattern matching used in ground based asteroid search and the more sensitive matched filtering and synthetic tracking techniques, can be adapted to account for highly complex parallax motion. A new shift vector generation methodology is discussed along with its impacts on commonly used detection algorithms, processing load, and responsiveness to asteroid track reporting. The matched filter, template generator, and pattern matcher source code for the software described herein are available via GitHub.
目前有多种算法用于从地面天文台探测小行星,但它们通常仅限于目标物体在视场中作线性或轻度弯曲运动的情况。处于高倾角、低地球轨道的天基传感器在采集的图像序列中会产生显著的视差,尤其是对于内太阳系中典型距离的小行星。这导致小行星在传感器上呈现高度非线性的运动模式,这就需要更复杂的搜索模式来进行探测处理。地面小行星搜索中使用的经典模式匹配以及更灵敏的匹配滤波和合成跟踪技术,都可以进行调整以适应高度复杂的视差运动。本文讨论了一种新的位移矢量生成方法及其对常用探测算法、处理负载和小行星轨道报告响应能力的影响。本文所述软件的匹配滤波器、模板生成器和模式匹配器的源代码可通过GitHub获取。