Jun Tan, Jia-Wei Wang, Cheng-Bing Lyu, Jin-Peng Wang, Hui Wang
{"title":"射电脉冲星J0742-2822 3.1 GHz模式变化研究","authors":"Jun Tan, Jia-Wei Wang, Cheng-Bing Lyu, Jin-Peng Wang, Hui Wang","doi":"10.1002/asna.20250032","DOIUrl":null,"url":null,"abstract":"<div>\n \n <p>The mode switching of PSR J0742-2822 at 3.1 GHz was investigated using single-pulse data from the Parkes 64-m radio telescope in Australia. By analyzing the ratio of the relative intensity of the two components for each sub-integral profile, we classified the integral profile of this source into two modes: normal mode and abnormal mode. We then obtained the average profile of PSR J0742-2822 at 3.1 GHz for each mode. The results indicate that the normal and abnormal modes of integrated pulse profiles occurred 72% and 28% of the time, respectively, over a total of 3.7 h of observation. This study is significant for understanding the theoretical mechanism behind the pulsar mode-switching phenomenon.</p>\n </div>","PeriodicalId":55442,"journal":{"name":"Astronomische Nachrichten","volume":"346 7-8","pages":""},"PeriodicalIF":1.0000,"publicationDate":"2025-03-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"The Study for Mode Changing for Radio Pulsar J0742-2822 at 3.1 GHz\",\"authors\":\"Jun Tan, Jia-Wei Wang, Cheng-Bing Lyu, Jin-Peng Wang, Hui Wang\",\"doi\":\"10.1002/asna.20250032\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div>\\n \\n <p>The mode switching of PSR J0742-2822 at 3.1 GHz was investigated using single-pulse data from the Parkes 64-m radio telescope in Australia. By analyzing the ratio of the relative intensity of the two components for each sub-integral profile, we classified the integral profile of this source into two modes: normal mode and abnormal mode. We then obtained the average profile of PSR J0742-2822 at 3.1 GHz for each mode. The results indicate that the normal and abnormal modes of integrated pulse profiles occurred 72% and 28% of the time, respectively, over a total of 3.7 h of observation. This study is significant for understanding the theoretical mechanism behind the pulsar mode-switching phenomenon.</p>\\n </div>\",\"PeriodicalId\":55442,\"journal\":{\"name\":\"Astronomische Nachrichten\",\"volume\":\"346 7-8\",\"pages\":\"\"},\"PeriodicalIF\":1.0000,\"publicationDate\":\"2025-03-08\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Astronomische Nachrichten\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://onlinelibrary.wiley.com/doi/10.1002/asna.20250032\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomische Nachrichten","FirstCategoryId":"101","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1002/asna.20250032","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
The Study for Mode Changing for Radio Pulsar J0742-2822 at 3.1 GHz
The mode switching of PSR J0742-2822 at 3.1 GHz was investigated using single-pulse data from the Parkes 64-m radio telescope in Australia. By analyzing the ratio of the relative intensity of the two components for each sub-integral profile, we classified the integral profile of this source into two modes: normal mode and abnormal mode. We then obtained the average profile of PSR J0742-2822 at 3.1 GHz for each mode. The results indicate that the normal and abnormal modes of integrated pulse profiles occurred 72% and 28% of the time, respectively, over a total of 3.7 h of observation. This study is significant for understanding the theoretical mechanism behind the pulsar mode-switching phenomenon.
期刊介绍:
Astronomische Nachrichten, founded in 1821 by H. C. Schumacher, is the oldest astronomical journal worldwide still being published. Famous astronomical discoveries and important papers on astronomy and astrophysics published in more than 300 volumes of the journal give an outstanding representation of the progress of astronomical research over the last 180 years. Today, Astronomical Notes/ Astronomische Nachrichten publishes articles in the field of observational and theoretical astrophysics and related topics in solar-system and solar physics. Additional, papers on astronomical instrumentation ground-based and space-based as well as papers about numerical astrophysical techniques and supercomputer modelling are covered. Papers can be completed by short video sequences in the electronic version. Astronomical Notes/ Astronomische Nachrichten also publishes special issues of meeting proceedings.