{"title":"宇宙射线通量变化对大气环流的影响","authors":"M. B. Bogdanov, S. Morozova","doi":"10.18500/1819-7663-2022-22-2-80-82","DOIUrl":null,"url":null,"abstract":"A comparison of average daily values time series of the axial component of the global wind angular moment and galactic cosmic ray (GCR) flux was made. Using the superposed epoch method it is shown that the Forbush decreases of the GCR flux are accompanied by an increase in the average angular velocity of atmosphericcirculation and, accordingly, by an increase in the zonal transfer.","PeriodicalId":193038,"journal":{"name":"Izvestiya of Saratov University. Earth Sciences","volume":"40 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2022-05-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"The effect of changes in cosmic ray flux on general atmospheric circulation\",\"authors\":\"M. B. Bogdanov, S. Morozova\",\"doi\":\"10.18500/1819-7663-2022-22-2-80-82\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"A comparison of average daily values time series of the axial component of the global wind angular moment and galactic cosmic ray (GCR) flux was made. Using the superposed epoch method it is shown that the Forbush decreases of the GCR flux are accompanied by an increase in the average angular velocity of atmosphericcirculation and, accordingly, by an increase in the zonal transfer.\",\"PeriodicalId\":193038,\"journal\":{\"name\":\"Izvestiya of Saratov University. Earth Sciences\",\"volume\":\"40 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2022-05-23\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Izvestiya of Saratov University. Earth Sciences\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.18500/1819-7663-2022-22-2-80-82\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Izvestiya of Saratov University. Earth Sciences","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.18500/1819-7663-2022-22-2-80-82","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
The effect of changes in cosmic ray flux on general atmospheric circulation
A comparison of average daily values time series of the axial component of the global wind angular moment and galactic cosmic ray (GCR) flux was made. Using the superposed epoch method it is shown that the Forbush decreases of the GCR flux are accompanied by an increase in the average angular velocity of atmosphericcirculation and, accordingly, by an increase in the zonal transfer.
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