首页> 外文期刊>The Astrophysical Journal. Supplement Series >INTERSTELLAR NEUTRAL HELIUM IN THE HELIOSPHERE FROM IBEX OBSERVATIONS. I. UNCERTAINTIES AND BACKGROUNDS IN THE DATA AND PARAMETER DETERMINATION METHOD
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INTERSTELLAR NEUTRAL HELIUM IN THE HELIOSPHERE FROM IBEX OBSERVATIONS. I. UNCERTAINTIES AND BACKGROUNDS IN THE DATA AND PARAMETER DETERMINATION METHOD

机译:来自IBEX观测的岩石圈中的星际中性氦。 I.数据和参数确定方法中的不确定性和背景

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This paper is one of three companion papers presenting the results of our in-depth analysis of the interstellar neutral helium (ISN He) observations carried out using IBEX-Lo during the first six Interstellar Boundary Explorer (IBEX) observation seasons. We derive corrections for losses due to the limited throughput of the interface buffer and determine the IBEX spin-axis pointing. We develop an uncertainty system for the data, taking into account the resulting correlations between the data points. This system includes uncertainties due to Poisson statistics, background, spin-axis determination, systematic deviation of the boresight from the prescribed position, correction for the interface buffer losses, and the expected Warm Breeze (WB) signal. Subsequently, we analyze the data from 2009 to examine the role of various components of the uncertainty system. We show that the ISN He flow parameters are in good agreement with the values obtained by the original analysis. We identify the WB as the principal contributor to the global chi(2) values in previous analyses. Other uncertainties have a much milder role and their contributions are comparable to each other. The application of this uncertainty system reduced the minimum chi(2) value 4-fold. The obtained chi(2) value, still exceeding the expected value, suggests that either the uncertainty system may still be incomplete or the adopted physical model lacks a potentially important element, likely an imperfect determination of the WB parameters. The derived corrections and uncertainty system are used in the accompanying paper by Bzowski et al. in an analysis of the data from six seasons.
机译:本文是三篇伴随论文之一,呈现我们深入分析的星际中性氦(ISN HE)在前六个星际边界探险者(IBEX)观察季节中使用IBEX-LO进行的观察结果。我们由于接口缓冲器的有限吞吐量而导致损失校正,并确定IBEX旋转轴指向。我们开发了数据的不确定性系统,考虑到数据点之间产生的相关性。该系统包括由于泊松统计,背景,旋转轴确定,从规定位置的防旋轴确定,界面缓冲损耗的校正,以及预期的温度微风(WB)信号,因此包括不确定性。随后,我们分析了2009年的数据,以检查不确定性系统各种组成部分的作用。我们表明ISN HE HE流参数与原始分析所获得的值吻合良好。我们将WB识别为先前分析中全球CHI(2)价值的主要贡献者。其他不确定性具有更温和的作用,其贡献彼此相当。这种不确定性系统的应用降低了最小CHI(2)值4倍。所获得的CHI(2)值仍然超过预期值,表明不确定性系统仍然是不完整的,或者采用的物理模型缺乏潜在的重要元素,可能是对WB参数的不完美确定。通过Bzowski等人在随附的纸张中使用衍生的校正和不确定性系统。在分析六个季节的数据。

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