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- W1989777746 abstract "Only those Jovian decametric storms whose maximum radio-frequency reaches or exceeds 30 Mc/s exhibit the strong well-known pattern of peak occurrence at Io phases 90° and 230°. The majority of storms, those which fail to reach 30 Mc/s, exhibit a weaker and more complex pattern. The maximum radio-frequency of storms also determines the pattern of occurrence with Jovian longitude, though the structure of this pattern is tens of Mc/s wide. On a fine scale, it is not the radio-frequency, nor primarily the central time, but the commencement time of storms which correlates with Jovian longitude. Most main-source storms are first seen on Earth as Jupiter's Northern Hemisphere magnetic pole (λIII = 200°) crosses the central meridian. The current belief that Jupiter's radio rotation period has lengthened during the last few years is probably erroneous. Яhкo-выpaжehhaя, чopoшo извecтhaя кohфигypaция maкcшmaльhoгo pacпpocтpahehия ha фaзaч Иo 90 и 230°, выявляeтcя лишь тemи дeкameтpoвыmи бypяmи. юпитepa, maкcиmaльhaя paдиoчacтoтa кoтopыч дocтигaeт, либo пpeвышaeт, 30 mгц/ceк. Бoльшиhcтвo бypь, иhaчe гoвopя тe, кoтopыe hecпocoбhы дocтичь 30 mгц/ceк, выявляют бoлee cлaбyю и бoлee кomплeкchyю кohфигypaцию. maкcиmaльhaя paдиoчacтoтa бypь тaкжe oпpeдeляeт кohфигypaцию pacпpocтpahehия copaзmepho c дoлгoтoй юпитepa, чoтя cтpyктypa зтoй кohфигypaции щиpиhoй в дecятки mгц/ceк. hameлкom macштaбe, oпpeдeлehhoe cooтhoшehиe c дoлгoтoй юпитepa cyщecтвyeт he y paдиoчacтoты и he, в пepвyю гoлoвy, y cpeдheгo вpemehи, a y вpemehи paзpaжehия бypь. бoльшиhcтвo бypь глaвhoгo иcтoчhикa впepвыe зameчaютcя ha зemлe в тo вpemя, кaк maгhитhый пoлюc (aIII = 200°) ceвephoгo пoлyшapия юпитepa пepeceкaeт цehтpaльhый mepидиah. pacпpocтpahehhoe mhehиe hacчeт тoгo, чтo пepиoд paдиoвpaщehия Юпитepa yдлиhилcя зa пocлeдhиe hecкoлькo лeт, пo вceй вepoятhocти oшибoчho." @default.
- W1989777746 created "2016-06-24" @default.
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- W1989777746 date "1966-12-01" @default.
- W1989777746 modified "2023-09-26" @default.
- W1989777746 title "Factors controlling Jovian decametric emission" @default.
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- W1989777746 doi "https://doi.org/10.1016/0032-0633(66)90082-1" @default.
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