HIGH-RESOLATUON OBSERVATIONS OF SOLAR RADIO BURSTS WITH MULTI-ELEMENT COMPOUND INTERFEROMETERS AT 3.75-GHZ AND 9.4-GHZ

被引：28

作者：

ENOME, S

KAKINUMA, T

TANAKA, H

机构：

[1] Research Institute of Atmospherics, Nagoya University, Aichi, Toyokawa

来源：

SOLAR PHYSICS | 1969年 / 6卷 / 03期

关键词：

D O I：

10.1007/BF00146477

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

High-resolution observations of solar radio bursts made simultaneously with multi-element compound interferometers at 3.75 and 9.4 GHz are presented. Preliminary results are: (1) The burst of December 16, 1967 showed a change in polarization distribution in the radio source, which suggests a magnetic field change in the source. (2) The existence of the multi-source burst is also confirmed at 3.75 GHz. (3) The source size of the impulsive burst is estimated to be ≈ 0.'5. (4) Among the GRF bursts there seem to be two kinds; one has a large angular size and the other has a small one. A brief discussion is given of the burst of December 16, 1967. © 1969 D. Reidel Publishing Company.

引用

页码：428 / &

共 10 条

[1] IMPULSIVE PHENOMENA OF THE SOLAR ATMOSPHERE .1. SOME OPTICAL EVENTS ASSOCIATED WITH FLARES SHOWING EXPLOSIVE PHASE [J].