Radio and soft X-ray investigation of the solar flares of February 4, 1986

Shuchen Ji; Youji Ding; Guoqiang Chen; Wenda Cao

doi:10.1007/BF00658992

Radio and soft X-ray investigation of the solar flares of February 4, 1986

Shuchen Ji, Youji Ding, Guoqiang Chen, Wenda Cao

Research output: Contribution to journal › Article › peer-review

Abstract

In this paper, the 3B flare of February 4, 1986 is studied comprehensively. The escape electrons accelerated to 10-100 keV at the top of coronal loop are confirmed by III type bursts. The energetic electron beams moved downward trigger the eruptions in the low layer of solar atmosphere. The radio and soft X-ray bursts are interpreted, respectively, by the maser mechanism and evaporation effect. Finally, the important role of energetic electron beams in solar flares is pointed out.

Original language	English (US)
Pages (from-to)	241-246
Number of pages	6
Journal	Astrophysics and Space Science
Volume	203
Issue number	2
DOIs	https://doi.org/10.1007/BF00658992
State	Published - May 1993
Externally published	Yes

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1007/BF00658992

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title = "Radio and soft X-ray investigation of the solar flares of February 4, 1986",

abstract = "In this paper, the 3B flare of February 4, 1986 is studied comprehensively. The escape electrons accelerated to 10-100 keV at the top of coronal loop are confirmed by III type bursts. The energetic electron beams moved downward trigger the eruptions in the low layer of solar atmosphere. The radio and soft X-ray bursts are interpreted, respectively, by the maser mechanism and evaporation effect. Finally, the important role of energetic electron beams in solar flares is pointed out.",

author = "Shuchen Ji and Youji Ding and Guoqiang Chen and Wenda Cao",

year = "1993",

month = may,

doi = "10.1007/BF00658992",

language = "English (US)",

volume = "203",

pages = "241--246",

journal = "Astrophysics and Space Science",

issn = "0004-640X",

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AU - Ji, Shuchen

AU - Ding, Youji

AU - Chen, Guoqiang

AU - Cao, Wenda

PY - 1993/5

Y1 - 1993/5

N2 - In this paper, the 3B flare of February 4, 1986 is studied comprehensively. The escape electrons accelerated to 10-100 keV at the top of coronal loop are confirmed by III type bursts. The energetic electron beams moved downward trigger the eruptions in the low layer of solar atmosphere. The radio and soft X-ray bursts are interpreted, respectively, by the maser mechanism and evaporation effect. Finally, the important role of energetic electron beams in solar flares is pointed out.

AB - In this paper, the 3B flare of February 4, 1986 is studied comprehensively. The escape electrons accelerated to 10-100 keV at the top of coronal loop are confirmed by III type bursts. The energetic electron beams moved downward trigger the eruptions in the low layer of solar atmosphere. The radio and soft X-ray bursts are interpreted, respectively, by the maser mechanism and evaporation effect. Finally, the important role of energetic electron beams in solar flares is pointed out.

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Radio and soft X-ray investigation of the solar flares of February 4, 1986

Abstract

All Science Journal Classification (ASJC) codes

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