SOLAR-CYCLE VARIATION OF SUNSPOT INTENSITY

[11] WHY ARE SUNSPOTS DARK AND FACULAE BRIGHT [J]. ASTROPHYSICAL JOURNAL, 1970, 159 (1P1) : 25 - &

[12] EDWARDS AWF, 1957, OBSERVATORY, V77, P69

[13] UMBRAL INTENSITIES OF LARGE SUNSPOTS [J]. SOLAR PHYSICS, 1974, 35 (02) : 317 - 322

[14] RELATION BETWEEN INTENSITIES OF UMBRA AND PENUMBRA OF LARGE SUNSPOTS [J]. SOLAR PHYSICS, 1974, 38 (01) : 73 - 75

[15] Engvold O., 1973, Astronomy and Astrophysics Supplement Series, V10, P11

[16] ERIKSEN G, 1973, 1ST P EUR ASTR M, V1, P87

[17] MOLECULAR LINE HAZE OPACITY IN SUNSPOTS [J]. SOLAR PHYSICS, 1979, 62 (01) : 83 - 87

[18] HALD A, 1952, STATISTICAL THEORY E

[19] Hall D.N.B, 1973, ATLAS INFRARED SPECT

[20] SPREAD FUNCTION FOR STRAY LIGHT [J]. SOLAR PHYSICS, 1973, 32 (02) : 505 - 506

[11] WHY ARE SUNSPOTS DARK AND FACULAE BRIGHT [J]. ASTROPHYSICAL JOURNAL, 1970, 159 (1P1) : 25 - &

[12] EDWARDS AWF, 1957, OBSERVATORY, V77, P69

[13] UMBRAL INTENSITIES OF LARGE SUNSPOTS [J]. SOLAR PHYSICS, 1974, 35 (02) : 317 - 322

[14] RELATION BETWEEN INTENSITIES OF UMBRA AND PENUMBRA OF LARGE SUNSPOTS [J]. SOLAR PHYSICS, 1974, 38 (01) : 73 - 75

[15] Engvold O., 1973, Astronomy and Astrophysics Supplement Series, V10, P11

[16] ERIKSEN G, 1973, 1ST P EUR ASTR M, V1, P87

[17] MOLECULAR LINE HAZE OPACITY IN SUNSPOTS [J]. SOLAR PHYSICS, 1979, 62 (01) : 83 - 87

[18] HALD A, 1952, STATISTICAL THEORY E

[19] Hall D.N.B, 1973, ATLAS INFRARED SPECT

[20] SPREAD FUNCTION FOR STRAY LIGHT [J]. SOLAR PHYSICS, 1973, 32 (02) : 505 - 506