MODEL FOR CHROMOSPHERE-CORONA TRANSITION REGION BASED ON RADIO OBSERVATIONS AND ON HYDRODYNAMICAL CONSERVATION EQUATIONS

被引:21
作者
LANTOS, P
机构
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D O I
10.1007/BF00148704
中图分类号
P1 [天文学];
学科分类号
0704 ;
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页码:387 / &
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共 46 条
[31]  
ORRALL FQ, 1961, SOLAR PHYS, V134, P72
[32]  
OSTERBROCK DE, 1961, SOLAR PHYS, V134, P347
[33]  
PARKER EN, 1963, INTERPLANETARY DYNAM, pCH7
[34]  
PECKER JC, 1969, ASTRON ASTROPHYS, V2, P81
[35]  
PIDDINGTON JH, 1954, SOLAR PHYS, V119, P531
[36]  
POTTASCH SR, 1965, B ASTRON I NETH, V18, P7
[37]  
POTTASCH SR, 1964, SPACE SCI REV, V3, P816
[38]   COARSE STRUCTURE OF SOLAR ATMOSPHERE [J].
SIMON, M ;
ZIRIN, H .
SOLAR PHYSICS, 1969, 9 (02) :317-+
[39]   RADIO-FREQUENCY RADIATION FROM THE QUIET SUN [J].
SMERD, SF .
AUSTRALIAN JOURNAL OF SCIENTIFIC RESEARCH SERIES A-PHYSICAL SCIENCES, 1950, 3 (01) :34-59
[40]  
SPITZER L, 1962, PHYSICS FULLY IONIZE