Ideal Data to Determine Accurate Fajr Time

Adi Damanhuri, Akhmad Mukarram
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Abstract

Early fajr time research was carried out by various parties with various techniques, one of which was using a sky quality meter (SQM) photometric tool. Observational data from various regions that have varying night levels result in a varying early fajr time as well. By paying attention to the effect of sky quality represented by the night level at the observation location, this research wants to answer whether the 20 mpsas night level limit is ideal data by looking at the correlation coefficient between night level and the turning point solution. From 1068 data with varying night levels, the correlation coefficient ( ) between the night level and the turning point solution is 0,42 which means there is an effect, while for data with a minimum night level of 20mpsas the correlation coefficient is 0,07 which means there is no influence. Based on the results of the analysis, the night level of 20mpsas can be the minimum limit for conducting an ideal early fajr time research. From 241 ideal observation data from 6 LAPAN observation stations, early fajr time presents when the Sun's elevation angle is -16,51°. Early fajr time is also the beginning of subuh prayer time, with its standard used in Indonesia, which is -20° or 3,49° different from the analysis results, if it is converted there is a difference of 13 minutes 57 seconds.
确定准确Fajr时间的理想数据
早期的fajr时间研究是由各方使用各种技术进行的,其中之一是使用天空质量计(SQM)光度测量工具。来自不同地区的观测数据显示,不同的夜间水平也导致不同的黎明时间。本研究通过关注观测点夜平所代表的天空质量的影响,通过观察夜平与拐点解的相关系数来回答20 mpsas夜平限值是否为理想数据。在1068个不同夜间水平的数据中,夜间水平与拐点解的相关系数()为0.42,表示有影响,而对于最低夜间水平为20mpsas的数据,相关系数为0.07,表示没有影响。根据分析结果,20mpsa的夜间水平可以作为进行理想的早期fajr时间研究的最小限制。从6个LAPAN观测站的241个理想观测资料中可以看出,太阳仰角为- 16.51°时,fajr时间较早。早fajr时间也是subuh祈祷时间的开始,其在印度尼西亚使用的标准与分析结果相差-20°或3.49°,如果换算有13分57秒的差异。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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