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Homologous flare-CME events and their metric type Ⅱ radio burst association

机译:同源耀斑-CME事件及其度量Ⅱ型无线电爆发关联

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摘要

Active region NOAA 11158 produced many flares during its disk passage. At least two of these flares can be considered as homologous: the C6.6 flare at 06:51 UT and C9.4 flare at 12:41 UT on February 14, 2011. Both flares occurred at the same location (eastern edge of the active region) and have a similar decay of the GOES soft X-ray light curve. The associated coronal mass ejections (CMEs) were slow (334 and 337 km/s) and of similar apparent widths (43° and 44°), but they had different radio signatures. The second event was associated with a metric type Ⅱ burst while the first one was not. The COR1 coronagraphs on board the STEREO spacecraft clearly show that the second CME propagated into the preceding CME that occurred 50 min before. These observations suggest that CME-CME interaction might be a key process in exciting the type Ⅱ radio emission by slow CMEs.
机译:主动区NOAA 11158在其磁盘通过过程中产生了许多耀斑。这些耀斑中至少有两个可以被认为是同源的:2011年2月14日在UT 06:51处发生的C6.6耀斑,而在UT 12:41处发生C9.4的耀斑。这两个耀斑都发生在相同的位置(有效区域),并具有类似的GOES软X射线光曲线衰减。相关的冠状物质抛射(CME)较慢(334和337 km / s),并且具有相似的表观宽度(43°和44°),但是它们具有不同的无线电信号。第二个事件与Ⅱ类度量标准爆发有关,而第一个事件与Ⅱ类事件无关。 STEREO航天器上的COR1日冕照片清楚地表明,第二个CME传播到50分钟前发生的前一个CME中。这些观察结果表明,CME-CME相互作用可能是激发慢速CME激发Ⅱ型无线电发射的关键过程。

著录项

  • 来源
    《Advances in space research》 |2014年第9期|1941-1948|共8页
  • 作者单位

    The Catholic University of America, Washington, DC 20064, USA,NASA Goddard Space Flight Center, Greenbelt, 20771, USA;

    NASA Goddard Space Flight Center, Greenbelt, 20771, USA;

    The Catholic University of America, Washington, DC 20064, USA,NASA Goddard Space Flight Center, Greenbelt, 20771, USA;

    The Catholic University of America, Washington, DC 20064, USA,NASA Goddard Space Flight Center, Greenbelt, 20771, USA;

    ARIES Nainital, Manora Peak, Nainital 263 129, India;

    Department of Physics, Indian Institute of Technology (BHU), Varanasi 221 005, India;

    School of Space Research, Kyung Hee University, Yongin, Gyeonggi-Do 446-701, South Korea;

    Department of Physics, DSB Campus, Kumaun University, Nainital 263 002, India;

    TIFR/NCRA Radio Astronomy Center, P. O. Box 8, Ootacamund 643 001, India;

    TIFR/NCRA Radio Astronomy Center, P. O. Box 8, Ootacamund 643 001, India;

    TIFR/NCRA Radio Astronomy Center, P. O. Box 8, Ootacamund 643 001, India;

    Kadi Sarva Vishwavidyalaya, Gandhinagar 382 015, Gujarat, India;

    ARIES Nainital, Manora Peak, Nainital 263 129, India,Physical Research Laboratory, Navrangapura, Ahmedabad 380 009, India;

    Lockheed Martin Solar and Astrophysical Laboratory, Palo Alto, CA 94304, USA;

    Lockheed Martin Solar and Astrophysical Laboratory, Palo Alto, CA 94304, USA;

    Department of Physics and Astronomy, California State University Northridge, Northridge, CA 91330, USA;

  • 收录信息
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Flares; CMEs; Shocks; Radio emission;

    机译:耀斑;CME;冲击;无线电发射;
  • 入库时间 2022-08-17 13:21:39

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