نوع مقاله : مقالة‌ تحقیقی‌ (پژوهشی‌)

نویسندگان

1 دانشجوی دکتری، دانشکده مهندسی هوافضا، دانشگاه صنعتی خواجه نصیرالدین طوسی، تهران، ایران

2 دانشیار، دانشکده مهندسی هوافضا، دانشگاه صنعتی خواجه نصیرالدین طوسی، تهران، ایران

3 استاد، دانشکده مهندسی هوافضا، صنعتی خواجه نصیرالدین طوسی، تهران، ایران

چکیده

در این مقاله الگوریتم جدیدی جهت تعیین چگالی داده‌های پراکنده بر روی سطح کره ارائه و سپس از الگوریتم پیشنهادی به همراه روش خوشه‌بندی Geodesic Weighted K-Means و مثلث‌بندی دلونی جهت تولید کاتالوگ ستارگان یکنواخت استفاده شده است. مقایسه نتایج با نتایج حاصل از سایر مقالات مرتبط نشان داد که الگوریتم پیشنهادی منجر به کاهش قابل توجه در احتمال مشاهده تعداد زیاد ستاره‌ها در تمام میدان دیدهای شبیه‌سازی شده حس‌گر ستاره شده است. این بهبود، نتیجه افزایش یکنواختی کاتالوگ ستاره علی‌الخصوص در قطبین کره سماوی ناشی از الگوریتم تعیین چگالی پیشنهادی است. از سوی دیگر، استفاده از الگوریتم تعیین چگالی داده مناسب، منجر به افزایش احتمال مشاهده چند ستاره (مانند 3 یا 5) در همه میدان‌های دید مورد استفاده در شبیه‌سازی مونت‌کارلو شده است.

کلیدواژه‌ها

موضوعات

عنوان مقاله [English]

Determination of the density of scattered spherical data for use in star catalog uniformity

نویسندگان [English]

  • Farshad Somayehee 1
  • Amir Ali Nikkhah 2
  • Jafar Roshanian 3

1 PhD Student, Department of Aerospace Engineering, K.N Toosi University of Technology, Tehran, Iran

2 Associate Professor, Faculty of Aerospace Engineering, K. N. Toosi University of Technology, Tehran, Iran

3 Professor, Faculty of Aerospace Engineering, K. N. Toosi University of Technology, Tehran, Iran

چکیده [English]

In this paper, a new algorithm for determining the density of scattered data at the surface of the sphere is presented and then the proposed algorithm along with Geodesic Weighted K-Means clustering and Deluany triangulation are used to make uniform star catalogs. Comparison of the results with the results of other related articles shows that the proposed algorithm resulted in a significant decrease in the probability of observing a large number of stars in all simulated star sensor fields of view. This improvement is due to the uniformity of the star catalog, especially in the celestial sphere poles due to the proposed density determination algorithm. On the other hand, the use of a proper data density algorithm has increased the likelihood of observing a few stars (such as 3 or 5) in all fields of view used in the Monte Carlo simulation.

کلیدواژه‌ها [English]

  • Star sensor
  • uniform star catalog
  • density of scattered data
  • clustering
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