The relation between solar radio burst types II, III and IV due to solar activities

机译：太阳活动引起的太阳无线电突发类型II，III和IV之间的关系

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Solar radio burst becoming an interesting topic among solar physicists in order to study the Space Weather condition. It generally originate at the same level as solar flare, Coronal Mass Ejection (CME) and shock at solar atmosphere which the Sun project the radio energy into the interstellar medium. In this study, the relation between solar radio burst type II, III and IV due to active region AR2157 and AR2158 was investigate. This study was carried out using the data from e-Callisto and was detected that solar radio burst type II, type III and type IV occurred on 10 September 2014 from 17:28 UT until 17:45 UT. The solar burst emission is associated with X1.6 class solar flare which occurred at sunspot AR2157 and AR2158 at 17:21 UT were observed from NOAA. We also compared with other events such as CME and geomagnetic storm that is potentially associated with this three bursts to show their importance role on space weather studies.

机译：为了研究太空天气状况，太阳无线电爆发成为太阳物理学家中一个有趣的话题。它通常与太阳耀斑，日冕质量抛射（CME）和太阳大气中的冲击处于同一水平，太阳将无线电能量投射到星际介质中。在这项研究中，研究了由于有源区AR2157和AR2158而引起的II，III和IV型太阳无线电脉冲串之间的关系。这项研究是使用e-Callisto的数据进行的，发现2014年9月10日UT 17:28至UT 17:45发生了II型，III型和IV型太阳射电爆发。太阳爆发辐射与X1.6级太阳耀斑有关，后者是在美国国家航空航天局（NOAA）观察到的太阳黑子AR2157和AR2158 UT 17:21发生的。我们还与其他事件（例如CME和地磁风暴）进行了比较，这些事件可能与这三个爆发有关，以显示它们在空间天气研究中的重要作用。

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来源
《2015 International Conference on Space Science and Communication : Space Technology for Humanity》|2015年|123-127|共5页
会议地点 Langkawi(MY)
作者
Ramli N.; Hamidi Z.S.; Abidin Z.Z.; Shahar S.N.;
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作者单位

Department of Physics, Faculty of Science, University Malaya, 50603 Kuala Lumpur, Malaysia;

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会议组织
原文格式 PDF
正文语种 eng
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关键词
CME; II; III; IV; Sun; geomagnetic storm; solar burst; solar flare;

机译：CME; II; III; IV;太阳;地磁风暴;太阳爆发;太阳耀斑;

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1. Statistical Survey of Type III Radio Bursts at Long Wavelengths Observed by the Solar TErrestrial RElations Observatory (STEREO)/Waves Instruments:Goniopolarimetric Properties and Radio Source Locations [J] . V. Krupar, M. Maksimovic, O. Santolik, Solar physics . 2014,第12期

机译：太阳地球关系天文台（STEREO）/波仪器观测到的长波长III型无线电爆发的统计调查：极化极特性和无线电源位置
2. Statistical Survey of Type III Radio Bursts at Long Wavelengths Observed by the Solar TErrestrial RElations Observatory (STEREO)/Waves Instruments: Radio Flux Density Variations with Frequency [J] . V. Krupar, M. Maksimovic, O. Santolik, Solar physics . 2014,第8期

机译：太阳地面关系天文台（STEREO）/波仪器观测到的长波长III型无线电爆发的统计调查：无线电通量密度随频率的变化
3. SOLAR CYCLE VARIATIONS OF THE OCCURRENCE OF CORONAL TYPE III RADIO BURSTS AND A NEW SOLAR ACTIVITY INDEX [J] . Vasili Lobzin, Iver H. Cairns, Peter A. Robinson The Astrophysical Journal. Letters . 2011,第1期

机译：冠状Ⅲ型放射性爆裂发生率的太阳周期变化和新的太阳活动指数
4. The relation between solar radio burst types II, III and IV due to solar activities [C] . Ramli N., Hamidi Z.S., Abidin Z.Z., International Conference on Space Science and Communication . 2015

机译：太阳能活动导致的太阳能无线电突发类型II，III和IV之间的关系
5. The Class of Type III-L Solar Radio Bursts and Their Associations with Solar Energetic Proton Events. [D] . Duffin, Robert Thomas. 2011

机译：III-L型太阳射电爆炸的类别及其与太阳能质子事件的关系。
6. Low Altitude Solar Magnetic Reconnection Type III Solar Radio Bursts and X-ray Emissions [O] . I. H. Cairns, V. V. Lobzin, A. Donea, -1

机译：低空太阳磁重连III型太阳射电爆发和X射线发射
7. Statistical Survey of Type III Radio Bursts at Long Wavelengths Observed by the Solar TErrestrial RElations Observatory (STEREO)/Waves Instruments: Goniopolarimetric Properties and Radio Source Locations [O] . Krupar, Vratislav, Maksimovic, Milan, Santolik, Ondrej, 2014

机译：观测到长波长III型射电爆发的统计调查由solar TErrestrial RElations Observatory（sTEREO）/ Waves Instruments提供： Goniopolaritrictric属性和无线电源位置
8. Observations of type iii and type iv solar radio bursts at 26.3 mc/s [R] . Erickson, W. C., Malitson, H. H. 1965

机译：iii型和iv型太阳射电探测器的观测值为26.3 mc / s

The relation between solar radio burst types II, III and IV due to solar activities

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