{"title":"银河系磁旋结构在恒星旋臂上的叠加——用两个星系旋臂片段匹配独特的星系磁场反转区","authors":"Jacques P Vallée","doi":"10.4236/ijaa.2022.124017","DOIUrl":null,"url":null,"abstract":". To pinpoint the peak location of the synchrotron total intensity emission in a spiral arm, we use a map of the spiralarm locations (from the observed arm tangent). Thus In a typical spiral arm in Galactic Quadrant I, we find the peak of the synchrotron radiation to be located about 220 ±40 pc away from the inner arm edge (hot dust lane) inside the spiral arm.While most of the galactic disk has a clockwise largescale magnetic field, we make a statistical analysis to delimitate more precisely the smaller reverse annulus wiith a counterclockwise galactic magnetic field. We find an annulus width of 2.1 ±0.3 kpc (measured along the Galactic radius), located from 5.5 to 7.6 kpc from the Galactic Center). The annulus does not overlay with a single spiral arm - it encompasses segments of two different spiral arms. Using a recent delineation of the position of spiral arms, the field-reversed annulus is seen to encompass the Crux-Centaurus arm (in Galactic Quadrant IV) and the Sagittarius arm (in Galactic Quadrant I). Thus the full Sagittarius-Carina arm is composed of : (1) a Sagittarius arm (in Galactic quadrant I) with a counterclockwise magnetic field, and (2) a Carina arm (in Galactic Quadrant IV). with a clockwise magnetic field. Also the full Scutum-Crux-Centaurus arm is composed of: (1) a Scutum arm (in Galactic Quadrant I) with a clockwise magnetic field, and (2) a Crux-Centaurus arm (in Galactic Quadrant IV) with a counterclockwise magnetic field.","PeriodicalId":434427,"journal":{"name":"International Journal of Astronomy and Astrophysics","volume":"26 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2022-10-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"Superposing the Magnetic Spiral Structure of the Milky Way, on the Stellar Spiral Arms—Matching the Unique Galactic Magnetic Field Reversal Zone with Two Galactic Spiral Arm Segments\",\"authors\":\"Jacques P Vallée\",\"doi\":\"10.4236/ijaa.2022.124017\",\"DOIUrl\":null,\"url\":null,\"abstract\":\". To pinpoint the peak location of the synchrotron total intensity emission in a spiral arm, we use a map of the spiralarm locations (from the observed arm tangent). Thus In a typical spiral arm in Galactic Quadrant I, we find the peak of the synchrotron radiation to be located about 220 ±40 pc away from the inner arm edge (hot dust lane) inside the spiral arm.While most of the galactic disk has a clockwise largescale magnetic field, we make a statistical analysis to delimitate more precisely the smaller reverse annulus wiith a counterclockwise galactic magnetic field. We find an annulus width of 2.1 ±0.3 kpc (measured along the Galactic radius), located from 5.5 to 7.6 kpc from the Galactic Center). The annulus does not overlay with a single spiral arm - it encompasses segments of two different spiral arms. Using a recent delineation of the position of spiral arms, the field-reversed annulus is seen to encompass the Crux-Centaurus arm (in Galactic Quadrant IV) and the Sagittarius arm (in Galactic Quadrant I). Thus the full Sagittarius-Carina arm is composed of : (1) a Sagittarius arm (in Galactic quadrant I) with a counterclockwise magnetic field, and (2) a Carina arm (in Galactic Quadrant IV). with a clockwise magnetic field. Also the full Scutum-Crux-Centaurus arm is composed of: (1) a Scutum arm (in Galactic Quadrant I) with a clockwise magnetic field, and (2) a Crux-Centaurus arm (in Galactic Quadrant IV) with a counterclockwise magnetic field.\",\"PeriodicalId\":434427,\"journal\":{\"name\":\"International Journal of Astronomy and Astrophysics\",\"volume\":\"26 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2022-10-27\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"International Journal of Astronomy and Astrophysics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.4236/ijaa.2022.124017\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"International Journal of Astronomy and Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.4236/ijaa.2022.124017","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Superposing the Magnetic Spiral Structure of the Milky Way, on the Stellar Spiral Arms—Matching the Unique Galactic Magnetic Field Reversal Zone with Two Galactic Spiral Arm Segments
. To pinpoint the peak location of the synchrotron total intensity emission in a spiral arm, we use a map of the spiralarm locations (from the observed arm tangent). Thus In a typical spiral arm in Galactic Quadrant I, we find the peak of the synchrotron radiation to be located about 220 ±40 pc away from the inner arm edge (hot dust lane) inside the spiral arm.While most of the galactic disk has a clockwise largescale magnetic field, we make a statistical analysis to delimitate more precisely the smaller reverse annulus wiith a counterclockwise galactic magnetic field. We find an annulus width of 2.1 ±0.3 kpc (measured along the Galactic radius), located from 5.5 to 7.6 kpc from the Galactic Center). The annulus does not overlay with a single spiral arm - it encompasses segments of two different spiral arms. Using a recent delineation of the position of spiral arms, the field-reversed annulus is seen to encompass the Crux-Centaurus arm (in Galactic Quadrant IV) and the Sagittarius arm (in Galactic Quadrant I). Thus the full Sagittarius-Carina arm is composed of : (1) a Sagittarius arm (in Galactic quadrant I) with a counterclockwise magnetic field, and (2) a Carina arm (in Galactic Quadrant IV). with a clockwise magnetic field. Also the full Scutum-Crux-Centaurus arm is composed of: (1) a Scutum arm (in Galactic Quadrant I) with a clockwise magnetic field, and (2) a Crux-Centaurus arm (in Galactic Quadrant IV) with a counterclockwise magnetic field.