EXPANDING ARCH STRUCTURE OF A SOLAR RADIO OUTBURST

[1] THE SOLAR CORONA IN ACTIVE REGIONS AND THE THERMAL ORIGIN OF THE SLOWLY VARYING COMPONENT OF SOLAR RADIO RADIATION [J]. ASTROPHYSICAL JOURNAL, 1961, 133 (03) : 983 - 1013

[2] STRUCTURE OF SOLAR CORONA [J]. ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1967, 5 : 213 - &

[3] Saito K., 1968, Solar Physics, V5, P61, DOI 10.1007/BF00147121

[4] OBSERVATION OF MAGNETIC STRUCTURE OF A TYPE-4 SOLAR RADIO OUTBURST [J]. SOLAR PHYSICS, 1969, 9 (02) : 260 - &

[5] 80 MHZ PHOTOGRAPHY OF ERUPTION OF A SOLAR PROMINENCE [J]. NATURE, 1968, 218 (5141) : 536 - &

[6] 1968, SOLAR GEOPHYSICAL DA

[1] THE SOLAR CORONA IN ACTIVE REGIONS AND THE THERMAL ORIGIN OF THE SLOWLY VARYING COMPONENT OF SOLAR RADIO RADIATION [J]. ASTROPHYSICAL JOURNAL, 1961, 133 (03) : 983 - 1013

[2] STRUCTURE OF SOLAR CORONA [J]. ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1967, 5 : 213 - &

[3] Saito K., 1968, Solar Physics, V5, P61, DOI 10.1007/BF00147121

[4] OBSERVATION OF MAGNETIC STRUCTURE OF A TYPE-4 SOLAR RADIO OUTBURST [J]. SOLAR PHYSICS, 1969, 9 (02) : 260 - &

[5] 80 MHZ PHOTOGRAPHY OF ERUPTION OF A SOLAR PROMINENCE [J]. NATURE, 1968, 218 (5141) : 536 - &

[6] 1968, SOLAR GEOPHYSICAL DA