火箭紫外线的绝对通量测量。

R. Bohlin, D. Frimout, C. Lillie
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引用次数: 13

摘要

在波长1200- 3400a的区域校准了双通道光谱仪,并搭载Aerobee火箭对天琴座α星、UMa星和蛇夫星进行观测。标准钨丝灯提供了低至2250 A的绝对校准,而由国家标准局校准的光电二极管是短波长的参考。用CO、NO、N2气体进行相对定标的分子分支比技术是对绝对定标的检验。eta UMa的通量与氢线覆盖模式大气在1700 - 3400 a之间的10%范围内和在该波长大部分区域的4%范围内的预测一致。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Absolute Flux Measurements in the Rocket Ultraviolet.
A two-channel spectrometer was calibrated in the wavelength region 1200-3400 A and flown on an Aerobee rocket to observe the stars alpha Lyr, eta UMa, and zeta Oph. Standard tungsten lamps provided the absolute calibration down to 2250 A, and a photodiode calibrated by the National Bureau of Standards was the reference at shorter wavelengths. The molecular branching-ratio technique of relative calibration using the gases CO, NO, and N2 was a check on the absolute calibration. The flux from eta UMa agrees with the prediction of a hydrogen line blanketed model atmosphere within 10% between 1700 and 3400 A and within 4% over most of this wavelength region.
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