SCATTERED LIGHT - COMPARISON BETWEEN THEORY AND EXPERIMENTS DURING 1973 TRANSIT OF MERCURY

被引:11
作者
WITTMANN, A [1 ]
WOHL, H [1 ]
机构
[1] UNIV GOTTINGEN,GOTTINGEN,FED REP GER
关键词
D O I
10.1007/BF00156858
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:231 / 237
页数:7
相关论文
共 12 条
[1]   CORRECTION OF SOLAR OBSERVATIONS FOR STRAY LIGHT BY NUMERICAL-INTEGRATION, WITH APPLICATION TO MERCURYS DROP [J].
BRAHDE, R .
SOLAR PHYSICS, 1972, 26 (02) :318-334
[2]  
David K.H., 1962, ZAP, V54, P12
[3]   HARVARD-SMITHSONIAN REFERENCE ATMOSPHERE [J].
GINGERICH, O ;
NOYES, RW ;
KALKOFEN, W ;
CUNY, Y .
SOLAR PHYSICS, 1971, 18 (03) :347-+
[4]   SPREAD FUNCTION FOR STRAY LIGHT [J].
HANSEN, T .
SOLAR PHYSICS, 1973, 32 (02) :505-506
[5]  
Kneer F., 1968, Solar Physics, V5, P42, DOI 10.1007/BF00147118
[7]   SUNSPOT INTENSITY OBSERVATIONS DURING 9 MAY 1970 MERCURY TRANSIT [J].
MALTBY, P ;
STAVELAND, L .
SOLAR PHYSICS, 1971, 18 (03) :443-+
[9]  
STAVELAND L, 1972, 36 I THEOR ASTR OSL
[10]   ELIMINATION OF SEEING EFFECTS FROM SOLAR INTENSITY MEASUREMENTS [J].
WITTMANN, A .
SOLAR PHYSICS, 1971, 21 (01) :237-&