CAN CORONAL LOOP TRANSIENTS BE DRIVEN MAGNETICALLY

被引:107
作者
ANZER, U
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D O I
10.1007/BF00152048
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P1 [天文学];
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0704 ;
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页码:111 / 118
页数:8
相关论文
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  • [1] ANZER U, UNPUBLISHED
  • [2] Batygin V. V., 1964, PROBLEMS ELECTRODYNA
  • [3] SPEEDS OF CORONAL MASS EJECTION EVENTS
    GOSLING, JT
    HILDNER, E
    MACQUEEN, RM
    MUNRO, RH
    POLAND, AI
    ROSS, CL
    [J]. SOLAR PHYSICS, 1976, 48 (02) : 389 - 397
  • [4] FREQUENCY OF CORONAL TRANSIENTS AND SOLAR-ACTIVITY
    HILDNER, E
    GOSLING, JT
    MACQUEEN, RM
    MUNRO, RH
    POLAND, AI
    ROSS, CL
    [J]. SOLAR PHYSICS, 1976, 48 (01) : 127 - 135
  • [5] HILDNER E, 1977, 1977 STIP S DEF MEM
  • [6] KOPP RA, 1976, SOL PHYS, V50, P85, DOI 10.1007/BF00206193
  • [7] OUTER SOLAR CORONA AS OBSERVED FROM SKYLAB - PRELIMINARY RESULTS
    MACQUEEN, RM
    EDDY, JA
    GOSLING, JT
    HILDNER, E
    MUNRO, RH
    NEWKIRK, GA
    POLAND, AI
    ROSS, CL
    [J]. ASTROPHYSICAL JOURNAL, 1974, 187 (02) : L85 - L88
  • [8] MOUSCHOVIAS TC, UNPUBLISHED
  • [9] MUNRO RH, UNPUBLISHED