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用于确定北方的天空偏振维京导航第二步中太阳定位的准确性:一项天象仪实验。

Accuracy of sun localization in the second step of sky-polarimetric Viking navigation for north determination: a planetarium experiment.

作者信息

Farkas Alexandra, Száz Dénes, Egri Ádám, Blahó Miklós, Barta András, Nehéz Dóra, Bernáth Balázs, Horváth Gábor

出版信息

J Opt Soc Am A Opt Image Sci Vis. 2014 Jul 1;31(7):1645-56. doi: 10.1364/JOSAA.31.001645.

Abstract

It is a widely discussed hypothesis that Viking seafarers might have been able to locate the position of the occluded sun by means of dichroic or birefringent crystals, the mysterious sunstones, with which they could analyze skylight polarization. Although the atmospheric optical prerequisites and certain aspects of the efficiency of this sky-polarimetric Viking navigation have been investigated, the accuracy of the main steps of this method has not been quantitatively examined. To fill in this gap, we present here the results of a planetarium experiment in which we measured the azimuth and elevation errors of localization of the invisible sun. In the planetarium sun localization was performed in two selected celestial points on the basis of the alignments of two small sections of two celestial great circles passing through the sun. In the second step of sky-polarimetric Viking navigation the navigator needed to determine the intersection of two such celestial circles. We found that the position of the sun (solar elevation θ(S), solar azimuth φ(S)) was estimated with an average error of +0.6°≤Δθ≤+8.8° and -3.9°≤Δφ≤+2.0°. We also calculated the compass direction error when the estimated sun position is used for orienting with a Viking sun-compass. The northern direction (ω(North)) was determined with an error of -3.34°≤Δω(North)≤+6.29°. The inaccuracy of the second step of this navigation method was high (Δω(North)=-16.3°) when the solar elevation was 5°≤θ(S)≤25°, and the two selected celestial points were far from the sun (at angular distances 95°≤γ(1), γ(2)≤115°) and each other (125°≤δ≤145°). Considering only this second step, the sky-polarimetric navigation could be more accurate in the mid-summer period (June and July), when in the daytime the sun is high above the horizon for long periods. In the spring (and autumn) equinoctial period, alternative methods (using a twilight board, for example) might be more appropriate. Since Viking navigators surely also committed further errors in the first and third steps, the orientation errors presented here underestimate the net error of the whole sky-polarimetric navigation.

摘要

有一种广泛讨论的假说认为,维京海员可能能够借助二向色性或双折射晶体(即神秘的太阳石)来确定被遮挡太阳的位置,通过这些晶体他们可以分析天空光的偏振。尽管大气光学前提条件以及这种基于天空偏振的维京导航效率的某些方面已经得到研究,但该方法主要步骤的准确性尚未进行定量检验。为了填补这一空白,我们在此展示一项天文馆实验的结果,在该实验中我们测量了不可见太阳定位的方位角和仰角误差。在天文馆中,基于两条穿过太阳的天球大圆的两个小部分的对齐情况,在两个选定的天球点进行太阳定位。在基于天空偏振的维京导航的第二步中,导航员需要确定两个这样的天球大圆的交点。我们发现,太阳位置(太阳仰角θ(S),太阳方位角φ(S))的估计平均误差为 +0.6°≤Δθ≤ +8.8° 以及 -3.9°≤Δφ≤ +2.0°。我们还计算了将估计的太阳位置用于用维京太阳罗盘定向时的罗盘方向误差。确定北方方向(ω(北))时的误差为 -3.34°≤Δω(北)≤ +6.29°。当太阳仰角为 5°≤θ(S)≤25°,且两个选定的天球点远离太阳(角距离 95°≤γ(1), γ(2)≤115°)且彼此远离(125°≤δ≤145°)时,这种导航方法第二步的不准确性很高(Δω(北)= -16.3°)。仅考虑这第二步,基于天空偏振的导航在仲夏时期(6 月和 7 月)可能更准确,此时白天太阳长时间高悬于地平线之上。在春秋分时期,其他方法(例如使用晨昏仪)可能更合适。由于维京导航员在第一步和第三步肯定也会出现进一步的误差,所以这里呈现的定向误差低估了整个基于天空偏振导航的净误差。

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