SOLAR-WIND FLOW PAST A COMETARY IONOSPHERE

[1] BABENKO KI, 1965, 2 T VS JAZN SEZD THE

[2] ION COMPOSITION AND DYNAMICS AT COMET HALLEY [J]. NATURE, 1986, 321 (6067) : 330 - 334

[3] BARANOV VB, 1970, DOKL AKAD NAUK SSSR+, V194, P41

[4] BARANOV VB, 1986, ASTRON ZH+, V63, P170

[5] BARANOV VB, 1982, FLUID DYN, P754

[6] BARANOV VB, 1981, ASTRONOM ZH, V12

[7] BARANOV VB, 1981, ASTRONOM ZH, V7, P378

[8] Biermann L., 1967, SOL PHYS, V1, P254, DOI DOI 10.1007/BF00150860

[9] Brosowski B, 1973, METHOD VERFAHREN MAT, V8, P125

[10] Gringauz K. I., 1985, Advances in Space Research, V5, P165, DOI 10.1016/0273-1177(85)90082-1

[1] BABENKO KI, 1965, 2 T VS JAZN SEZD THE

[2] ION COMPOSITION AND DYNAMICS AT COMET HALLEY [J]. NATURE, 1986, 321 (6067) : 330 - 334

[3] BARANOV VB, 1970, DOKL AKAD NAUK SSSR+, V194, P41

[4] BARANOV VB, 1986, ASTRON ZH+, V63, P170

[5] BARANOV VB, 1982, FLUID DYN, P754

[6] BARANOV VB, 1981, ASTRONOM ZH, V12

[7] BARANOV VB, 1981, ASTRONOM ZH, V7, P378

[8] Biermann L., 1967, SOL PHYS, V1, P254, DOI DOI 10.1007/BF00150860

[9] Brosowski B, 1973, METHOD VERFAHREN MAT, V8, P125

[10] Gringauz K. I., 1985, Advances in Space Research, V5, P165, DOI 10.1016/0273-1177(85)90082-1