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      KCI등재 SCOPUS

      Multi-wavelength Observations of Two Explosive Events and Their Effects on the Solar Atmosphere

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      https://www.riss.kr/link?id=A104983062

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      다국어 초록 (Multilingual Abstract)

      We investigated two flares in the solar atmosphere that occurred on June 3, 2012 and July 6, 2012 and caused propagation of Moreton and EIT waves. In the June 3 event, we noticed a filament winking which presumably was caused by the wave propagation from the flare. An interesting feature of this event is that there was a reflection of this wave by a coronal hole located alongside the wave propagation, but not all of this wave was transmitted by the coronal hole. Using the running difference method, we calculated the speed of Moreton and EIT waves and we found values of 926 km/s before the reflection and 276 km/s after the reflection (Moreton wave) and 1,127 km/s before the reflection and 46 km/s after the reflection (EIT wave). In the July 6 event, this phenomenon was accompanied by type II and type III solar radio bursts, and we also performed a running difference analysis to find the speed of the Moreton wave, obtaining a value of 988 km/s. The speed derived from the analysis of the solar radio burst was 1,200 km/s, and we assume that this difference was caused by the different nature of the motions in these phenomena, where the solar radio burst was caused by the propagating particles, not waves.
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      We investigated two flares in the solar atmosphere that occurred on June 3, 2012 and July 6, 2012 and caused propagation of Moreton and EIT waves. In the June 3 event, we noticed a filament winking which presumably was caused by the wave propagation f...

      We investigated two flares in the solar atmosphere that occurred on June 3, 2012 and July 6, 2012 and caused propagation of Moreton and EIT waves. In the June 3 event, we noticed a filament winking which presumably was caused by the wave propagation from the flare. An interesting feature of this event is that there was a reflection of this wave by a coronal hole located alongside the wave propagation, but not all of this wave was transmitted by the coronal hole. Using the running difference method, we calculated the speed of Moreton and EIT waves and we found values of 926 km/s before the reflection and 276 km/s after the reflection (Moreton wave) and 1,127 km/s before the reflection and 46 km/s after the reflection (EIT wave). In the July 6 event, this phenomenon was accompanied by type II and type III solar radio bursts, and we also performed a running difference analysis to find the speed of the Moreton wave, obtaining a value of 988 km/s. The speed derived from the analysis of the solar radio burst was 1,200 km/s, and we assume that this difference was caused by the different nature of the motions in these phenomena, where the solar radio burst was caused by the propagating particles, not waves.

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      참고문헌 (Reference)

      1 J. I. Khan, "X-ray observations of a large-scale solar coronal shock wave" EDP Sciences 383 (383): 1018-1031, 2002

      2 S. T. Wu, "Three-dimensional numerical simulation of MHD waves observed by the Extreme Ultraviolet Imaging Telescope" Wiley-Blackwell 106 (106): 25089-25102, 2001

      3 J. W. Harvey, "The Global Oscillation Network Group (GONG) Project" American Association for the Advancement of Science (AAAS) 272 (272): 1284-1286, 1996

      4 James R. Lemen, "The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO)" Springer Nature 275 (275): 17-40, 2012

      5 Bothmer V, "Space weather - physics and effects" Springer 2007

      6 Daglis IA., "Space storms and space weather hazards" Springer 2001

      7 D. A. Biesecker, "Solar Phenomena Associated with “EIT Waves”" IOP Publishing 569 (569): 1009-1015, 2002

      8 Hugh S. Hudson, "Soft X-ray observation of a large-scale coronal wave and its exciter" Springer Nature 212 (212): 121-149, 2003

      9 N. Narukage, "Simultaneous Observation of a Moreton Wave on 1997 November 3 in Hα and Soft X-Rays" IOP Publishing 572 (572): L109-L112, 2002

      10 Olmedo O, "Secondary waves and/or the "reflection" from and "transmission" through a coronal hole of an extreme ultraviolet wave associated with the 2011 February 15 X2.2 flare observed with SDO/ AIA and STEREO/EUVI" 756 : 143-155, 2012

      1 J. I. Khan, "X-ray observations of a large-scale solar coronal shock wave" EDP Sciences 383 (383): 1018-1031, 2002

      2 S. T. Wu, "Three-dimensional numerical simulation of MHD waves observed by the Extreme Ultraviolet Imaging Telescope" Wiley-Blackwell 106 (106): 25089-25102, 2001

      3 J. W. Harvey, "The Global Oscillation Network Group (GONG) Project" American Association for the Advancement of Science (AAAS) 272 (272): 1284-1286, 1996

      4 James R. Lemen, "The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO)" Springer Nature 275 (275): 17-40, 2012

      5 Bothmer V, "Space weather - physics and effects" Springer 2007

      6 Daglis IA., "Space storms and space weather hazards" Springer 2001

      7 D. A. Biesecker, "Solar Phenomena Associated with “EIT Waves”" IOP Publishing 569 (569): 1009-1015, 2002

      8 Hugh S. Hudson, "Soft X-ray observation of a large-scale coronal wave and its exciter" Springer Nature 212 (212): 121-149, 2003

      9 N. Narukage, "Simultaneous Observation of a Moreton Wave on 1997 November 3 in Hα and Soft X-Rays" IOP Publishing 572 (572): L109-L112, 2002

      10 Olmedo O, "Secondary waves and/or the "reflection" from and "transmission" through a coronal hole of an extreme ultraviolet wave associated with the 2011 February 15 X2.2 flare observed with SDO/ AIA and STEREO/EUVI" 756 : 143-155, 2012

      11 A. N. Zhukov, "STEREO/SECCHI Observations on 8 December 2007: Evidence Against the Wave Hypothesis of the EIT Wave Origin" Springer Nature 259 (259): 73-85, 2009

      12 Eto S, "Relation between a Moreton wave and an EIT wave observed on 1997 November 4" 54 : 481-491, 2002

      13 Yutaka Uchida, "Propagation of hydromagnetic disturbances in the solar corona and Moreton's wave phenomenon" Springer Nature 4 (4): 30-44, 1968

      14 Balasubramaniam KS, "On the origin of the solar Moreton wave of 2006 December 6" 723 : 587-601, 2010

      15 Edward W. Cliver, "On the origin of solar metric type II bursts" Springer Nature 187 (187): 89-114, 1999

      16 A. N. Zhukov, "On the nature of EIT waves, EUV dimmings and their link to CMEs" EDP Sciences 427 (427): 705-716, 2004

      17 E. W. Cliver, "On the Origins of Solar EIT Waves" IOP Publishing 631 (631): 604-611, 2005

      18 I. Ballai, "On the Nature of Coronal EIT Waves" IOP Publishing 633 (633): L145-L148, 2005

      19 B.J. Thompson, "Observations of the 24 September 1997 coronal flare waves" Springer Nature 193 (193): 161-180, 2000

      20 M.J. Wills-Davey, "Observations of a propagating disturbance in TRACE" Springer Nature 190 (190): 467-483, 1999

      21 B. Vršnak, "Multi-wavelength study of coronal waves associated with the CME-flare event of 3 November 2003" EDP Sciences 448 (448): 739-752, 2006

      22 Admiranto AG, "Moreton waves and EIT waves related to the flare events of June 3, 2012 and July 6, 2012" 2014

      23 AGUSTINUS GUNAWAN ADMIRANTO, "MORETON WAVES RELATED TO THE SOLAR ERUPTION OCCURRED ON 3 JUNE 2012 AND 6 JULY 2012" The Korean Astronomical Society 30 (30): 57-58, 2015

      24 Astrid M. Veronig, "Interaction of a Moreton/EIT Wave and a Coronal Hole" IOP Publishing 647 (647): 1466-1471, 2006

      25 R. Grant Athay, "Impulsive Phenomena of the Solar Atmosphere. I. Some Optical Events Associated with Flares Showing Explosive Phase." IOP Publishing 133 : 935-945, 1961

      26 G. E. Moreton, "Hα Observations of Flare-Initiated Disturbances with Velocities ~1000 km/sec." IOP Publishing 65 : 494-, 1960

      27 Chen PF, "Global coronal waves, in low-frequency waves in space plasmas" John Wiley & Sons 379-394, 2016

      28 B. Vršnak, "Flare waves observed in Helium I 10 830 Å" EDP Sciences 394 (394): 299-310, 2002

      29 Asai A, "First simultaneous observation of an Hα Moreton wave, EUV wave, and filament/prominence oscillations" 745 : L18-, 2012

      30 A. Warmuth, "Evolution of Two EIT/Hα Moreton Waves" IOP Publishing 560 (560): L105-L109, 2001

      31 P. F. Chen, "Evidence of EIT and Moreton Waves in Numerical Simulations" IOP Publishing 572 (572): L99-L102, 2002

      32 Gopalswamy N, "EUV wave reflection from a coronal hole" 691 : L123-L127, 2009

      33 M. J. Wills-Davey, "EIT Waves: A Changing Understanding over a Solar Cycle" Springer Nature 149 (149): 325-353, 2009

      34 Y.-M. Wang, "EIT Waves and Fast-Mode Propagation in the Solar Corona" IOP Publishing 543 (543): L89-L93, 2000

      35 G.D.R. Attrill, "Coronal “wave”: A signature of the mechanism making CMEs largescale in the low corona?" Wiley-Blackwell 328 (328): 760-763, 2007

      36 A. Klassen, "Catalogue of the 1997 SOHO–EIT coronal transient waves and associated type II radio burst spectra" EDP Sciences 141 (141): 357-369, 2000

      37 C. Delannée, "CME associated with transequatorial loops and a bald patch flare" Springer Nature 190 (190): 107-129, 1999

      38 K. S. Balasubramaniam, "Are Moreton Waves Coronal Phenomena?" IOP Publishing 658 (658): 1372-1379, 2007

      39 C. Delannee, "Another View of the EIT Wave Phenomenon" IOP Publishing 545 (545): 512-523, 2000

      40 Muhr N, "Analysis of a global Moreton wave observed on 2003 October 28" 708 : 1639-1649, 2010

      41 A. Warmuth, "A multiwavelength study of solar flare waves" EDP Sciences 418 (418): 1117-1129, 2004

      42 Holly R. Gilbert, "A comparison of CME-associated atmospheric waves observed in coronal (FeXII 195 Å) and chromospheric (HeI 10830 Å) lines" IOP Publishing 607 (607): 540-553, 2004

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      학술지 이력

      학술지 이력
      연월일 이력구분 이력상세 등재구분
      2023 평가예정 해외DB학술지평가 신청대상 (해외등재 학술지 평가)
      2020-01-01 평가 등재학술지 유지 (해외등재 학술지 평가) KCI등재
      2011-05-12 학술지명변경 외국어명 : 미등록 -> Journal of Astronomy and Space Sciences KCI등재
      2010-06-10 학술지명변경 한글명 : 한국우주과학회지 -> Journal of Astronomy and Space Sciences KCI등재
      2010-01-01 평가 등재학술지 유지 (등재유지) KCI등재
      2008-01-01 평가 등재학술지 유지 (등재유지) KCI등재
      2006-01-01 평가 등재학술지 유지 (등재유지) KCI등재
      2004-01-01 평가 등재학술지 유지 (등재유지) KCI등재
      2001-07-01 평가 등재학술지 선정 (등재후보2차) KCI등재
      1999-01-01 평가 등재후보학술지 선정 (신규평가) KCI등재후보
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      학술지 인용정보

      학술지 인용정보
      기준연도 WOS-KCI 통합IF(2년) KCIF(2년) KCIF(3년)
      2016 0.18 0.18 0.18
      KCIF(4년) KCIF(5년) 중심성지수(3년) 즉시성지수
      0.15 0.15 0.28 0.07
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