Radio fine structures in dm-cm wavelength range associated with magnetic reconnection processes

Y. Yan; J. Huang; Bin Chen; Y. Liu; C. Tan

doi:10.1016/j.asr.2010.03.016

Radio fine structures in dm-cm wavelength range associated with magnetic reconnection processes

Y. Yan, J. Huang, Bin Chen, Y. Liu, C. Tan

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

9 Scopus citations

Abstract

Radio bursts with fine structures in decimetric-centimetric wave range are generally believed to manifest the primary energy release process during flare/CME events. By spectropolarimeters in 1-2 GHz, 2.6-3.8 GHz, and 5.2-7.6 GHz at NAOC/Huairou with very high temporal (1.25-8 ms) and spectral (4-20 MHz) resolutions, the zebra patterns, spikes, and new types of radio fine structures with mixed frequency drift features are observed during several significant flare/CME events. In this paper we will discuss the occurrence of radio fine structures during the impulsive phase of flares and/or CME initiations, which may be connected to the magnetic reconnection processes.

Original language	English (US)
Pages (from-to)	413-418
Number of pages	6
Journal	Advances in Space Research
Volume	46
Issue number	4
DOIs	https://doi.org/10.1016/j.asr.2010.03.016
State	Published - Aug 16 2010

All Science Journal Classification (ASJC) codes

Aerospace Engineering
Astronomy and Astrophysics
Geophysics
Atmospheric Science
Space and Planetary Science
General Earth and Planetary Sciences

Keywords

CME
Fine structures
Solar activities
Solar flares
Solar radio bursts

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10.1016/j.asr.2010.03.016

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title = "Radio fine structures in dm-cm wavelength range associated with magnetic reconnection processes",

abstract = "Radio bursts with fine structures in decimetric-centimetric wave range are generally believed to manifest the primary energy release process during flare/CME events. By spectropolarimeters in 1-2 GHz, 2.6-3.8 GHz, and 5.2-7.6 GHz at NAOC/Huairou with very high temporal (1.25-8 ms) and spectral (4-20 MHz) resolutions, the zebra patterns, spikes, and new types of radio fine structures with mixed frequency drift features are observed during several significant flare/CME events. In this paper we will discuss the occurrence of radio fine structures during the impulsive phase of flares and/or CME initiations, which may be connected to the magnetic reconnection processes.",

keywords = "CME, Fine structures, Solar activities, Solar flares, Solar radio bursts",

author = "Y. Yan and J. Huang and Bin Chen and Y. Liu and C. Tan",

note = "Funding Information: The authors thank the anonymous referees for helpful comments in improving the paper. The work is supported by NSFC (Grant No. 10921303 ), MOST (Grant No. 2006CB806301 ) and CAS-NSFC Key Project (Grant No. 10778605 ).",

year = "2010",

month = aug,

day = "16",

doi = "10.1016/j.asr.2010.03.016",

language = "English (US)",

volume = "46",

pages = "413--418",

journal = "Advances in Space Research",

issn = "0273-1177",

publisher = "Elsevier Limited",

number = "4",

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TY - JOUR

T1 - Radio fine structures in dm-cm wavelength range associated with magnetic reconnection processes

AU - Yan, Y.

AU - Huang, J.

AU - Chen, Bin

AU - Liu, Y.

AU - Tan, C.

N1 - Funding Information: The authors thank the anonymous referees for helpful comments in improving the paper. The work is supported by NSFC (Grant No. 10921303 ), MOST (Grant No. 2006CB806301 ) and CAS-NSFC Key Project (Grant No. 10778605 ).

PY - 2010/8/16

Y1 - 2010/8/16

N2 - Radio bursts with fine structures in decimetric-centimetric wave range are generally believed to manifest the primary energy release process during flare/CME events. By spectropolarimeters in 1-2 GHz, 2.6-3.8 GHz, and 5.2-7.6 GHz at NAOC/Huairou with very high temporal (1.25-8 ms) and spectral (4-20 MHz) resolutions, the zebra patterns, spikes, and new types of radio fine structures with mixed frequency drift features are observed during several significant flare/CME events. In this paper we will discuss the occurrence of radio fine structures during the impulsive phase of flares and/or CME initiations, which may be connected to the magnetic reconnection processes.

AB - Radio bursts with fine structures in decimetric-centimetric wave range are generally believed to manifest the primary energy release process during flare/CME events. By spectropolarimeters in 1-2 GHz, 2.6-3.8 GHz, and 5.2-7.6 GHz at NAOC/Huairou with very high temporal (1.25-8 ms) and spectral (4-20 MHz) resolutions, the zebra patterns, spikes, and new types of radio fine structures with mixed frequency drift features are observed during several significant flare/CME events. In this paper we will discuss the occurrence of radio fine structures during the impulsive phase of flares and/or CME initiations, which may be connected to the magnetic reconnection processes.

KW - CME

KW - Fine structures

KW - Solar activities

KW - Solar flares

KW - Solar radio bursts

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U2 - 10.1016/j.asr.2010.03.016

DO - 10.1016/j.asr.2010.03.016

M3 - Article

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SN - 0273-1177

VL - 46

SP - 413

EP - 418

JO - Advances in Space Research

JF - Advances in Space Research

IS - 4

ER -

Radio fine structures in dm-cm wavelength range associated with magnetic reconnection processes

Abstract

All Science Journal Classification (ASJC) codes

Keywords

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