利用新方法绘制彗星核表面元素分布的光度法。

Ruaa F. Hanash, Salman Z. Khalaf, Khaleel I. Abood
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摘要

这项研究在这个领域是独一无二的。它代表了三个技术分支的混合:光度学、光谱学和图像处理。该作品通过根据图像中的每个像素的颜色来处理图像,其中颜色表示RGB线上的特定波长;因此,任何图像都会有来自其所有像素的许多波长。这项研究的结果是具体的,并确定了彗星核表面的元素,不仅是细节,还有它们在核上的映射。这项工作考虑了两颗彗星(Temple 1和67P/Churyumoy-Gerasimenko)中的12种元素。这些元素在可见光范围内有很强的发射线,我们的MATLAB程序在处理图像时识别了这些发射线。测定了元素与铁的比值,其中在Temple 1彗星中,钾与铁的比值最高为K / Fe ~ 28.2%,最低为Ca / Fe ~ 1.3%。67P/Churyumov-Gerasimenko彗星中,相对于铁元素的元素比例最大的也是钾,K / Fe ~ 89.5%,最低的是Ni / Fe ~ 0.26。总的来说,比较这两颗彗星,铁元素的最大比例是K / f。铁是这两颗彗星结构中的基本元素,其次是钾。
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Photometry technique to map elements’ distribution on comets’ nuclei surfaces by using the new method.
This study is unique in this field. It represents a mix of three branches of technology: photometry, spectroscopy, and image processing. The work treats the image by treating each pixel in the image based on its color, where the color means a specific wavelength on the RGB line; therefore, any image will have many wavelengths from all its pixels. The results of the study are specific and identify the elements on the nucleus’s surface of a comet, not only the details but also their mapping on the nucleus. The work considered 12 elements in two comets (Temple 1 and 67P/Churyumoy-Gerasimenko). The elements have strong emission lines in the visible range, which were recognized by our MATLAB program in the treatment of the image. The percentage of the elements was determined relative to iron, where in comet Temple 1, the most significant percentage of the element ratio potassium to iron is K / Fe ~ 28.2%, while the lowest value is Ca / Fe ~  1.3%. For the comet, 67P/Churyumov-Gerasimenko, the most significant percentage of the elements relative to iron is also for potassium, K / Fe ~ 89.5%, while the lowest value is Ni / Fe ~ 0.26.  In general, comparing both comets, the greatest percentage of the elements relative to iron is K / F. Iron is the base element in the structure of both comets, followed by potassium.
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