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      Development of the Substorm as a Manifestation of Convection Transient

      한글로보기

      https://www.riss.kr/link?id=O111276954

      • 저자
      • 발행기관
      • 학술지명
      • 권호사항
      • 발행연도

        2021년

      • 작성언어

        -

      • Print ISSN

        2169-9380

      • Online ISSN

        2169-9402

      • 등재정보

        SCOPUS;SCIE

      • 자료형태

        학술저널

      • 수록면

        n/a-n/a   [※수록면이 p5 이하이면, Review, Columns, Editor's Note, Abstract 등일 경우가 있습니다.]

      • 구독기관
        • 전북대학교 중앙도서관  
        • 성균관대학교 중앙학술정보관  
        • 부산대학교 중앙도서관  
        • 전남대학교 중앙도서관  
        • 제주대학교 중앙도서관  
        • 중앙대학교 서울캠퍼스 중앙도서관  
        • 인천대학교 학산도서관  
        • 숙명여자대학교 중앙도서관  
        • 서강대학교 로욜라중앙도서관  
        • 계명대학교 동산도서관  
        • 충남대학교 중앙도서관  
        • 한양대학교 백남학술정보관  
        • 이화여자대학교 중앙도서관  
        • 고려대학교 도서관  
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      부가정보

      다국어 초록 (Multilingual Abstract)

      We reproduced the substorm by global simulation and analyzed the development of convection, shear, the dynamo, and the field‐aligned current (FAC) at the final stage of the growth phase. From these investigations, we show that the substorm is a mani...

      We reproduced the substorm by global simulation and analyzed the development of convection, shear, the dynamo, and the field‐aligned current (FAC) at the final stage of the growth phase. From these investigations, we show that the substorm is a manifestation of reconfiguration in global flow dynamics. Ionospheric convection can be understood from two aspects. One understanding is as the potential field generated by the FAC, and the other is as the projection of magnetospheric convection. In order for the two to coincide, the FAC must be transmitted together with the motion. As a consequence, the resulting convection must be continuous from the magnetosphere to the ionosphere. We see this connection from the drawing of shear to recognize that the substorm is the projection process of transient convection. In the growth phase, convective shear that causes the quiet arc and the Harang reversal (HR) occurs on the open/closed boundary along the surface of the plasma sheet with a continuous flow structure from the magnetosphere to the ionosphere. The onset starts from a more local flow that is induced by the near‐earth neutral line (NENL). A narrow shear commences from the NENL in the mid‐tail and extends to the ionosphere to replace growth phase shear. Along a closed magnetic field line connected to the NENL, direct penetration flow, squeezing flow, the near‐earth dynamo, release of the HR, and the onset FAC occur successively and consequently cause the ground onset. Such onset mechanism is quite different from the model adopting the current wedge.



      East‐west shear inducing the upward field‐aligned current at the quiet arc connects from the tail to the ionosphere along the open/close boundary

      The substorm is a manifestation of global reconfiguration of convection system accompanied by the near‐earth neutral line (NENL) formation

      The onset starts from the equatorward‐most quiet arc since causative narrow shear extends from the NENL along a closed magnetic field


      East‐west shear inducing the upward field‐aligned current at the quiet arc connects from the tail to the ionosphere along the open/close boundary
      The substorm is a manifestation of global reconfiguration of convection system accompanied by the near‐earth neutral line (NENL) formation
      The onset starts from the equatorward‐most quiet arc since causative narrow shear extends from the NENL along a closed magnetic field

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