• Title/Summary/Keyword: ICME

Search Result 37, Processing Time 0.027 seconds

Asymmetric cosmic ray modulation of Forbush decreases related to the propagation direction of ICMEs

  • Oh, Suyeon;Park, Wooyeon;Yi, Yu
    • The Bulletin of The Korean Astronomical Society
    • /
    • v.38 no.2
    • /
    • pp.96.1-96.1
    • /
    • 2013
  • A Forbush decrease(FD) is a depression of cosmic ray intensity observed by ground-based neutron monitors(NMs). The cosmic ray intensity is thought to be modulated by the heliospheric magnetic structures including the interplanetary coronal mass ejection(ICME) surrounding the Earth. The different magnitude of the decreasing in intensity at each NM was explained only by the geomagnetic cutoff rigidity of NM station. However, sometimes NMs of the almost same rigidity in northern and southern hemispheres observe the asymmetric intensity depression magnitudes of FD events. Thus, in this study we intend to see the effects on cosmic ray intensity depression rate of FD event recorded at different NMs due to different ICME propagation direction as an additional parameter in the model explaining the cosmic ray modulation. Fortunately, since 2006 the coronagraphs of twin spacecraft of the STEREO mission allow us to infer the propagation direction of ICME associated with the FD event in 3-dimension with respect to the Earth. We confirm that the asymmetric cosmic ray decreasing modulations of FD events are determined by the propagation directions of the associated ICMEs.

  • PDF

Comparison between observation and theory for the stand-off distance ratios of CMEs and their associated ICMEs

  • Lee, Jae-Ok;Moon, Yong-Jae;Lee, Jin-Yi;Jang, Soojeong;Lee, Harim
    • The Bulletin of The Korean Astronomical Society
    • /
    • v.41 no.1
    • /
    • pp.81.3-81.3
    • /
    • 2016
  • We examine whether the observational stand-off distance ratios of CMEs and their associated ICMEs could be explained by theoretical model or not. For this, we select 16 CME-ICME pairs from September 2009 to October 2012 with the following conditions: (1) limb CMEs by SOHO and their associated ICMEs by twin STEREO spacecraft and vice versa when both spacecraft were roughly in quadrature; (2) the faint structure ahead of a limb CME is well identified; and (3) its associated ICME clearly has a sheath structure. We determine the observational stand-off distance ratios of the CMEs by using brightness profiles from LASCO-C2 (or SECCHI-COR2) observations and those of the ICMEs by solar wind data from STEREO-IMPACT/PLASTIC (or OMNI database) observations. We also determine the theoretical stand-off distance ratios of the CME-ICME pairs using semi-empirical relationship based on the bow shock theory. We find the following results. (1) Observational CME stand-off distance ratio decreases with increasing Mach number at the Mach numbers between 2 and 6. This tendency is consistent with the results from the semi-empirical relationship. (2) The observational stand-off distance ratios of several ICMEs can be explained by the relationship.

  • PDF

COMPARISON OF HELICITY SIGNS IN INTERPLANETARY CMES AND THEIR SOLAR SOURCE REGIONS

  • Cho, Kyungsuk;Park, Sunghong;Marubashi, Katsuhide;Gopalswamy, Nat;Akiyama, Sachiko;Yashiro, Seiji;Kim, Roksoon;Lim, Eunkyung
    • The Bulletin of The Korean Astronomical Society
    • /
    • v.37 no.2
    • /
    • pp.137.1-137.1
    • /
    • 2012
  • If all Coronal mass ejections (CMEs) have flux ropes, then the CMEs should keep their helicity signs from the Sun to the Earth according to the helicity conservation principle. We select 34 CME-ICME pairs whose source active regions (ARs) have continuous SOHO/MDI magnetogram data covering more than 24 hr without data gap during the passage of the ARs near the solar disk centre. The helicity signs in the ARs are determined by estimation of accumulating amounts of helicity injections through the photospheric surfaces in the entire source ARs. The helicity signs in the ICMEs are estimated by applying the cylinder model developed by Marubashi (2000) to 16 second resolution magnetic field data from the MAG instrument onboard the ACE spacecraft. It is found that 30 out of 34 events (88%) are helicity sign-consistent events, while 4 events (12%) are sign-inconsistent. Through a detailed investigation of the AR solar origins of the 4 exceptional events, we find that those exceptional events can be explained by the local AR helicity sign opposite to that of the entire AR helicity (2000 July 28 ICME), incorrectly reported solar source in CDAW (2005 May 20 ICME), or the helicity sign of the pre-existing coronal magnetic field (2000 October 13 and 2003 November 20 ICMEs). We conclude that the helicity signs of the ICMEs are quite consistent with those of the injected helicities in the AR regions where CMEs were erupted.

  • PDF

Asymmetric Cosmic Ray Modulation of Forbush Decreases Associated with the Propagation Direction of Interplanetary Coronal Mass Ejection

  • Jongil Jung;Suyeon Oh;Yu Yi;Jongdae Sohn
    • Journal of The Korean Astronomical Society
    • /
    • v.56 no.1
    • /
    • pp.117-124
    • /
    • 2023
  • A Forbush decrease (FD) is a depression of cosmic ray (CR) intensity observed by ground-based neutron monitors (NMs). The CR intensity is thought to be modulated by the heliospheric magnetic structures including the interplanetary coronal mass ejection (ICME) surrounding the Earth. The different magnitude of the decreasing in intensity at each NM was explained only by the geomagnetic cutoff rigidity of the NM station. However, sometimes NMs of almost the same cutoff rigidity in northern and southern hemispheres observe the asymmetric intensity depression magnitudes of FD events. Thus, in this study we intend to see the effects on CR intensity modulation of FD event recorded at different NMs due to different ICME propagation directions as an additional parameter in the model explaining the CR modulation. Fortunately, since 2006 the coronagraphs of twin spacecraft of the STEREO mission allow us to infer the propagation direction of ICME associated with the FD event in 3-dimension with respect to the Earth. We suggest the hypothesis that the asymmetric CR modulations of FD events are determined by the propagation directions of the associated ICMEs.

ICME에의 참가

  • Park, Han-Sik
    • Communications of Mathematical Education
    • /
    • v.18 no.2 s.19
    • /
    • pp.1-8
    • /
    • 2004
  • PDF

수학 영재교육의 최근 동향에 대한 분석 - APCR 8, ERIC, ICME 10, ICCME&EGS'03을 중심으로 -

  • Lee, Gang-Seop;Hwang, Dong-Ju
    • Communications of Mathematical Education
    • /
    • v.18 no.3 s.20
    • /
    • pp.199-208
    • /
    • 2004
  • 본 연구는 2004년은 한국에서 개최된 APCG 8(The 8th Asia-Pacific Conference on Giftedness, 2004)을 통하여 일반 영재교육의 최근 동향을 탐색하였다. 1980에서 2002년까지의 ERIC(Education Research Information Center)에 나타난 수학영재관련 문헌을 검색하여 644개를 선정 분석하여 그 연구 동향을 파악하고, 2003년에서 2004년까지는 ICME 10(the 10th International Congress on Mathematical Education, 2004)과 ICCME&EGS'03 (The Third International Conference Creativity in Mathematics Education and the Education of Gifted Students, 2003)을 통하여 수학영재교육의 최근 연구 동향을 분석하여 수학영재교육 발전과 활성화에 도움을 주는데 목적을 두고 있다.

  • PDF

Felix Christian Klein (펠릭스 클라인의 수학과 교육 개혁)

  • Kim Sung Sook;Kim Ju Young
    • Journal for History of Mathematics
    • /
    • v.17 no.4
    • /
    • pp.77-86
    • /
    • 2004
  • Felix Klein profoundly influenced mathematical developments throughout the world by showing a new direction for modem geometry. He also influenced the lives of excellent scientists like Einstein by reforming mathematical education. The first Felix Klein medal of the Internal Commission on Mathematical Instruction was awarded at ICME-10 in July of 2004. In this article, we discuss Klein's Erlangen Program and investigate his influence on modem mathematics and mathematical education with this medal as momentum.

  • PDF

Toward Students' Full Understanding of Trigonometric Ratios

  • Yi, Jung-A;Yoo, Jae-Geun;Lee, Kyeong Hwa
    • Research in Mathematical Education
    • /
    • v.17 no.1
    • /
    • pp.63-78
    • /
    • 2013
  • Trigonometric ratios are difficult concepts to teach and learn in middle school. One of the reasons is that the mathematical terms (sine, cosine, tangent) don't convey the idea literally. This paper deals with the understanding of a concept from the learner's standpoint, and searches the orientation of teaching that make students to have full understanding of trigonometric ratios. Such full understanding contains at least five constructs as follows: skill-algorithm, property-proof, use-application, representation-metaphor, history-culture understanding [Usiskin, Z. (2012). What does it mean to understand some mathematics? In: Proceedings of ICME12, COEX, Seoul Korea; July 8-15,2012 (pp. 502-521). Seoul, Korea: ICME-12]. Despite multi-aspects of understanding, especially, the history-culture aspect is not yet a part of the mathematics class on the trigonometric ratios. In this respect this study investigated the effect of history approach on students' understanding when the history approach focused on the mathematical terms is used to teach the concept of trigonometric ratios in Grade 9 mathematics class. As results, the experimental group obtained help in more full understanding on the trigonometric ratios through such teaching than the control group. This implies that the historical derivation of mathematical terms as well as the context of mathematical concepts should be dealt in the math class for the more full understanding of some mathematical concepts.

Freudenthal and ICMI (프로이덴탈과 ICM)

  • Kim, Sung-Sook;Khang, Mee-Kyung
    • Journal for History of Mathematics
    • /
    • v.24 no.4
    • /
    • pp.87-96
    • /
    • 2011
  • Hans Freudenthal made important contributions to algebraic topology and geometry. He also made significant contributions in history of mathematics and mathematics education. In the 1970s, his intervention prevented the Netherlands from the movement of "new math". He had a very important role as a founder of realistic mathematics education and became famous internationally by that. Because he raised the profile of ICMI strongly, Bass used the expression 'Freudenthal Era' for the period that Freudenthal was the president of ICMI. Now many mathematics educator agree to use the Freudenthal Era when they mention about the history of ICMI. In this paper, we present on the life of Freudenthal and his contributions for mathematics education, especially ICMI.