基于GPS载噪比下降的太阳射电暴检测方法

doi:10.3969/j.issn.1001-506X.2020.08.23

Abstract

Abstract:

Taking advantage of the influence of solar radio bursts on the performance of global positioning system (GPS), a detection method of solar radio bursts based on the decrease of GPS carrier-to-noise ratio is proposed. Firstly, the solar incidence angle of the observation ground is calculated, then the "falling points" and "rising points" are selected to determine the time interval of the trough of a single satellite from the single observation ground, and finally the detection results of the solar radio bursts are determined by integrating multiple satellites and multiple observation grounds. The experimental results show that the detection rate of solar radio bursts increases with the increase of the solar incidence angle, the detection rate of solar radio bursts above 600 SFU on the L2 frequency band reaches more than 80%, and the detection effect on the L2 frequency band is better than that on L1. This detection method has a high recognition rate, low cost, does not depend on the radio telescope, and can carry out all-weather real-time monitoring.

Key words: global positioning system (GPS), solar radio burst, carrier-to-noise ratio, detection rate

CLC Number:

P353.7

Xuefen ZHU, Fan YANG, Xiyuan CHEN, Mengying LIN, Xin CHEN. Detection method of solar radio bursts based on decrease of GPS carrier-to-noise ratio[J]. Systems Engineering and Electronics, 2020, 42(8): 1820-1825.

Figures/Tables 8

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References 21

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台站	纬度/(°)	经度/(°)	国家
ISPA	110W	27S	智利
AREQ	72W	16S	秘鲁
BOGT	75W	4N	哥伦比亚
MDO1	105W	30N	美国
CHPI	45W	22S	巴西
CRO1	65W	17N	美国
KOUR	53W	5N	圭亚那
NNOR	116E	31S	澳大利亚
PERT	115E	31S	澳大利亚
SUNM	153E	27S	澳大利亚
TIDB	148E	35S	澳大利亚
PIMO	121E	14N	菲律宾
CCJM	142E	27N	日本
KUNM	102E	25N	中国
GUAM	144E	13N	关岛
USUD	138E	36N	日本
TSKB	140E	36N	日本
DARW	131E	12S	澳大利亚
TOW2	147E	19S	澳大利亚
RABT	7W	33N	摩洛哥
MAS1	16W	27N	西班牙
SFER	7W	36N	西班牙
VILL	4W	40N	西班牙
YEBE	4W	40N	西班牙
KOKB	160W	22N	美国

日期	时间段	峰值时刻	台站及太阳入射角/(°)
06.12.06	12:11~20:24	19:30	ISPA:83.5 AREQ:58.3 BOGT:50.6 MDO1:37.6 CHPI:34.8 CRO1:34.5 KOUR:32.3
06.12.13	00:00~10:00	03:30	NNOR:77.1 PERT:76.3 SUNM:66.6 TIDB:68.5 PIMO:52.4 CCJM:38 KUNM:36
11.02.15	00:00~10:45	03:00	PIMO:75.8 GUAM:80 USUD:72.6 TSKB:72.2 DARW:59 KUNM:58.8 TOW2:50.4
11.09.24	11:00~22:00	13:00	RABT:56.2 MAS1:63 CHPI:53.4 SFER:53.2 KOUR:51.7 VILL:48.8 YEBE:48.8

射电流量/SFU	样本容量	N_station
射电流量/SFU	样本容量	5	4	3	2
900~1 000	5	20%	40%	60%	100%
800~900	21	29%	38%	48%	95%
700~800	21	0%	19%	38%	81%
600~700	25	12%	24%	60%	84%
500~600	37	14%	27%	73%	86%
400~500	28	11%	18%	29%	68%
300~400	58	2%	7%	28%	60%
200~300	126	2%	2%	23%	47%
100~200	1 242	0%	0%	1%	2%

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Detection method of solar radio bursts based on decrease of GPS carrier-to-noise ratio

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