LARGE-SCALE INHOMOGENEITIES IN SOLAR-WIND OF SOLAR ORIGIN

[31] COMPARISON OF SOLAR-FLARE ENERGY ESTIMATES MADE BY ANALYTICAL AND NUMERICAL TECHNIQUES [J]. JOURNAL OF GEOPHYSICAL RESEARCH, 1972, 77 (25): : 4851 - &

[32] DRYER M, 1974, SPACE SCI REV, V15, P403, DOI 10.1007/BF00178215

[33] Dryer M., 1972, Cosmic Electrodynamics, V3, P184

[34] DRYER M, IN PRESS

[35] DRYER M, 1972, SOLAR ACTIVITY OBSER, P197

[36] DRYER M, 1972, SP308 NASA SPEC PUBL, P453

[37] MOVING TYPE-IV RADIO BURST AND ITS RELATION TO CORONAL MAGNETIC-FIELD [J]. SOLAR PHYSICS, 1971, 20 (02) : 438 - +

[38] STRUCTURE OF MIDDLE CORONA FROM OBSERVATIONS AT 80 AND 160 MHZ [J]. SOLAR PHYSICS, 1974, 36 (01) : 191 - 202

[39] DULK GA, 1971, AUST J PHYS, V24, P239

[40] DULK GA, 1971, ASTROPHYS LETT COMM, V8, P235

[31] COMPARISON OF SOLAR-FLARE ENERGY ESTIMATES MADE BY ANALYTICAL AND NUMERICAL TECHNIQUES [J]. JOURNAL OF GEOPHYSICAL RESEARCH, 1972, 77 (25): : 4851 - &

[32] DRYER M, 1974, SPACE SCI REV, V15, P403, DOI 10.1007/BF00178215

[33] Dryer M., 1972, Cosmic Electrodynamics, V3, P184

[34] DRYER M, IN PRESS

[35] DRYER M, 1972, SOLAR ACTIVITY OBSER, P197

[36] DRYER M, 1972, SP308 NASA SPEC PUBL, P453

[37] MOVING TYPE-IV RADIO BURST AND ITS RELATION TO CORONAL MAGNETIC-FIELD [J]. SOLAR PHYSICS, 1971, 20 (02) : 438 - +

[38] STRUCTURE OF MIDDLE CORONA FROM OBSERVATIONS AT 80 AND 160 MHZ [J]. SOLAR PHYSICS, 1974, 36 (01) : 191 - 202

[39] DULK GA, 1971, AUST J PHYS, V24, P239

[40] DULK GA, 1971, ASTROPHYS LETT COMM, V8, P235