LINE-BLANKETING PROBLEM IN NON-LTE APPROACH

[1] Avrett E. H., 1965, MON NOT R ASTRON SOC, V130, P295

[2] BOHM KH, 1954, Z ASTROPHYS, V34, P182

[3] CAYREL R, 1963, CR HEBD ACAD SCI, V257, P3309

[4] CHANDRASEKHAR, 1935, M N, V96, P21

[5] DUMONT S, 1966, CR ACAD SCI B PHYS, V262, P740

[6] LABS D, 1951, Z ASTROPHYS, V29, P199

[7] Pecker J.-C., 1951, ANN ASTROPHYS, V14, P152

[8] PIRON H, 1963, THESIS U PARIS

[9] COMMENT ON DIFFERENCE BETWEEN A NON-LTE AND A PURE-ABSORPTION MODEL FOR LINE-BLANKETING EFFECT [J]. ASTROPHYSICAL JOURNAL, 1965, 141 (01) : 333 - &

[10] THOMAS RN, 1961, PHYSICS SOLAR CHROMO

[1] Avrett E. H., 1965, MON NOT R ASTRON SOC, V130, P295

[2] BOHM KH, 1954, Z ASTROPHYS, V34, P182

[3] CAYREL R, 1963, CR HEBD ACAD SCI, V257, P3309

[4] CHANDRASEKHAR, 1935, M N, V96, P21

[5] DUMONT S, 1966, CR ACAD SCI B PHYS, V262, P740

[6] LABS D, 1951, Z ASTROPHYS, V29, P199

[7] Pecker J.-C., 1951, ANN ASTROPHYS, V14, P152

[8] PIRON H, 1963, THESIS U PARIS

[9] COMMENT ON DIFFERENCE BETWEEN A NON-LTE AND A PURE-ABSORPTION MODEL FOR LINE-BLANKETING EFFECT [J]. ASTROPHYSICAL JOURNAL, 1965, 141 (01) : 333 - &

[10] THOMAS RN, 1961, PHYSICS SOLAR CHROMO