BRIGHTNESS OF HELIUM D3 LINE IN UNDISTURBED CHROMOSPHERE FROM ECLIPSE OBSERVATIONS

被引：8

作者：

GULYAEV, RA ^{[1
]}

机构：

[1] ACAD SCI USSR,TERR MAGNETISM IONOSPHERE & RADIOWAVE PROPAGATION INST,SOLAR ACTIV LAB,AKADEMOGORODOK,USSR

来源：

关键词：

D O I：

10.1007/BF00156844

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：25 / 40

页数：16

共 37 条

[1] Allen C. W., 1955, ASTROPHYSICAL QUANTI
[2] AMBARTSUMYAN VA, 1958, THEORETICAL ASTROPHY
[3] A MODEL OF THE CHROMOSPHERE FROM THE HELIUM AND CONTINUUM EMISSIONS
ATHAY, RG
MENZEL, DH
[J]. ASTROPHYSICAL JOURNAL, 1956, 123 (02) : 285 - 298
[4] ATHAY RG, 1965, P S U UTRECHT, P151
[5] ATHAY RG, 1957, SMITHSONIAN CONTR AS, V2, P35
[6] Belkina I. L., 1972, Soviet Astronomy, V16, P476
[7] BRUGGENCATE TP, 1950, Z ASTROPHYS, V27, P223
[8] CILLIE GG, 1935, 410 HARV OBS CIRC, P1
[9] THE PROFILES OF CHROMOSPHERIC H-ALPHA AND D3 FROM INTERFEROMETRIC OBSERVATIONS
CLUBE, SVM
[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1958, 118 (01) : 18 - 30
[10] DEJAGER C, 1966, B ASTRON I NETH, V18, P128