定时脉冲星:统计分析和科学过程的练习

J. Walkup, Joseph White, Roger Key
{"title":"定时脉冲星:统计分析和科学过程的练习","authors":"J. Walkup, Joseph White, Roger Key","doi":"10.32374/aej.2021.1.1.006","DOIUrl":null,"url":null,"abstract":"A lab activity for teaching students the fundamentals of statistical analysis by timing pulsar periods is described. The electromagnetic pulses of pulsars have been mapped to sound and uploaded on social media channels, allowing students to “listen” to the beat of the pulsar.  Because these beats are extraordinarily precise, they can serve as cyclic events of known time duration. The three-step process described in this article first requires that students select a timing method of low random error found by comparing standard deviations between two suggested methods. In the second step, students reduce systematic error by calibrating their optimal method using a pulsar of known time duration. Finally, students time an unknown pulsar (the mystery pulsar) using the optimal method chosen in Step 1 and calibrating out the bias found in Step 2. By expressing their results in terms of confidence intervals, they use a professional pulsar database to identify the mystery pulsar. Because students are not informed of the identity of the pulsar until after they turn in their lab reports, they are compelled to perform the measurements as carefully and objectively as possible. This activity provides a perfect vehicle for astronomy labs at the beginning of a semester — including online instruction — because it requires no prior instruction in astronomy and no equipment other than the stopwatch on a cell phone and internet connection. Furthermore, this activity offers an introduction to pulsars and such physics topics as magnetism and the conservation of angular momentum.","PeriodicalId":424141,"journal":{"name":"Astronomy Education Journal","volume":"41 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2021-12-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Timing pulsars: An exercise in statistical analysis and the scientific process\",\"authors\":\"J. Walkup, Joseph White, Roger Key\",\"doi\":\"10.32374/aej.2021.1.1.006\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"A lab activity for teaching students the fundamentals of statistical analysis by timing pulsar periods is described. The electromagnetic pulses of pulsars have been mapped to sound and uploaded on social media channels, allowing students to “listen” to the beat of the pulsar.  Because these beats are extraordinarily precise, they can serve as cyclic events of known time duration. The three-step process described in this article first requires that students select a timing method of low random error found by comparing standard deviations between two suggested methods. In the second step, students reduce systematic error by calibrating their optimal method using a pulsar of known time duration. Finally, students time an unknown pulsar (the mystery pulsar) using the optimal method chosen in Step 1 and calibrating out the bias found in Step 2. By expressing their results in terms of confidence intervals, they use a professional pulsar database to identify the mystery pulsar. Because students are not informed of the identity of the pulsar until after they turn in their lab reports, they are compelled to perform the measurements as carefully and objectively as possible. This activity provides a perfect vehicle for astronomy labs at the beginning of a semester — including online instruction — because it requires no prior instruction in astronomy and no equipment other than the stopwatch on a cell phone and internet connection. Furthermore, this activity offers an introduction to pulsars and such physics topics as magnetism and the conservation of angular momentum.\",\"PeriodicalId\":424141,\"journal\":{\"name\":\"Astronomy Education Journal\",\"volume\":\"41 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2021-12-30\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Astronomy Education Journal\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.32374/aej.2021.1.1.006\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomy Education Journal","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.32374/aej.2021.1.1.006","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

摘要

介绍了一项实验室活动,用于教授学生脉冲星周期计时统计分析的基础知识。脉冲星的电磁脉冲被映射成声音,并上传到社交媒体渠道,让学生们“听”脉冲星的节拍。因为这些跳动非常精确,它们可以作为已知时间持续时间的循环事件。本文中描述的三步过程首先要求学生通过比较两种建议方法的标准差来选择一种随机误差较小的计时方法。在第二步,学生们通过使用已知持续时间的脉冲星校准他们的最佳方法来减少系统误差。最后,学生使用步骤1中选择的最佳方法对未知脉冲星(神秘脉冲星)进行计时,并校准步骤2中发现的偏差。通过用置信区间来表达他们的结果,他们使用专业的脉冲星数据库来识别神秘的脉冲星。因为学生们直到交了实验报告后才被告知脉冲星的身份,他们被迫尽可能仔细客观地进行测量。这项活动为学期初的天文学实验室提供了一个完美的工具——包括在线教学——因为它不需要事先学习天文学,除了手机上的秒表和互联网连接外,不需要其他设备。此外,这项活动还提供了脉冲星的介绍,以及磁学和角动量守恒等物理主题。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Timing pulsars: An exercise in statistical analysis and the scientific process
A lab activity for teaching students the fundamentals of statistical analysis by timing pulsar periods is described. The electromagnetic pulses of pulsars have been mapped to sound and uploaded on social media channels, allowing students to “listen” to the beat of the pulsar.  Because these beats are extraordinarily precise, they can serve as cyclic events of known time duration. The three-step process described in this article first requires that students select a timing method of low random error found by comparing standard deviations between two suggested methods. In the second step, students reduce systematic error by calibrating their optimal method using a pulsar of known time duration. Finally, students time an unknown pulsar (the mystery pulsar) using the optimal method chosen in Step 1 and calibrating out the bias found in Step 2. By expressing their results in terms of confidence intervals, they use a professional pulsar database to identify the mystery pulsar. Because students are not informed of the identity of the pulsar until after they turn in their lab reports, they are compelled to perform the measurements as carefully and objectively as possible. This activity provides a perfect vehicle for astronomy labs at the beginning of a semester — including online instruction — because it requires no prior instruction in astronomy and no equipment other than the stopwatch on a cell phone and internet connection. Furthermore, this activity offers an introduction to pulsars and such physics topics as magnetism and the conservation of angular momentum.
求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
自引率
0.00%
发文量
0
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信