SOME CHARACTERISTICS OF A CHROMOSPHERIC MODEL

被引:9
作者
ATHAY, RG
THOMAS, RN
机构
关键词
D O I
10.1086/146163
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:309 / 319
页数:11
相关论文
共 30 条
[1]   CORONAL LINE INTENSITIES AT THE KHARTOUM ECLIPSE [J].
ATHAY, RG ;
ROBERTS, WO .
ASTROPHYSICAL JOURNAL, 1955, 121 (01) :231-&
[2]   EMISSION IN HYDROGEN BALMER LINES AND CONTINUUM IN FLASH SPECTRUM OF 1952 TOTAL SOLAR ECLIPSE AT KHARTOUM, SUDAN [J].
ATHAY, RG ;
BILLINGS, DE ;
EVANS, JW ;
ROBERTS, WO .
ASTROPHYSICAL JOURNAL, 1954, 120 (01) :94-&
[3]   TEMPERATURE GRADIENTS IN THE CHROMOSPHERE [J].
ATHAY, RG ;
THOMAS, RN .
ASTROPHYSICAL JOURNAL, 1956, 123 (02) :299-308
[4]   A MODEL OF THE CHROMOSPHERE FROM THE HELIUM AND CONTINUUM EMISSIONS [J].
ATHAY, RG ;
MENZEL, DH .
ASTROPHYSICAL JOURNAL, 1956, 123 (02) :285-298
[5]  
ATHAY RG, 1955, ASTROPHYS J S, V1, P505
[6]  
BIERMANN L, 1948, Z ASTROPHYS, V25, P161
[7]  
CILLIE CG, 1935, 410 HARV OBS CIRC
[8]  
DUNN RB, UNPUBLISHED
[9]  
HEMMINDINGER H, 1939, THESIS PRINCETON U
[10]  
HOUTGAST J, 1953, 1952 CONV VOLT ROM A, P68