SOLAR NOISE STORMS AND MAGNETIC-SECTOR STRUCTURES

被引:20
作者
STEWART, RT
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D O I
10.1007/BF00149692
中图分类号
P1 [天文学];
学科分类号
0704 ;
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页码:381 / 395
页数:15
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[1]   MAGNETIC FIELDS AND STRUCTURE OF SOLAR CORONA .I. METHODS OF CALCULATING CORONAL FIELDS [J].
ALTSCHULER, MD ;
NEWKIRK, G .
SOLAR PHYSICS, 1969, 9 (01) :131-+
[2]   THE TOPOLOGY OF THE SUNS MAGNETIC FIELD AND THE 22-YEAR CYCLE [J].
BABCOCK, HW .
ASTROPHYSICAL JOURNAL, 1961, 133 (02) :572-&
[3]  
BRATOVA TA, 1983, SOV ASTRON LETT+, V9, P260
[4]   TYPE-I NOISE STORMS AND THE STRUCTURE OF THE EXTREME ULTRAVIOLET CORONA [J].
BRUECKNER, GE .
SOLAR PHYSICS, 1983, 85 (02) :243-265
[5]   MAGNETOIONIC MODE COUPLING AT HIGH FREQUENCIES [J].
COHEN, MH .
ASTROPHYSICAL JOURNAL, 1960, 131 (03) :664-680
[6]  
Dulk G. A., 1973, Proceedings of the Astronomical Society of Australia, V2, P211
[7]  
DULK GA, 1984, ASTRON ASTROPHYS, V130, P39
[8]  
Duncan R. A., 1977, Proceedings of the Astronomical Society of Australia, V3, P154
[9]   TYPE-III SOLAR RADIO BURST STORMS OBSERVED AT LOW FREQUENCIES .1. STORM MORPHOLOGY [J].
FAINBERG, J ;
STONE, RG .
SOLAR PHYSICS, 1970, 15 (01) :222-&
[10]  
FOKKER AD, 1960, THESIS LEIDEN