• 제목/요약/키워드: sun: active regions

검색결과 68건 처리시간 0.031초

NON-HYDROSTATIC SUPPORT OF PLASMA IN THE SOLAR CHROMOSPHERE AND CORONA

  • Chae, Jong-Chul
    • 천문학회지
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    • 제43권3호
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    • pp.55-64
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    • 2010
  • We investigate how plasma structures in the solar chromosphere and corona can extend to altitudes much above hydrostatic scale heights from the solar surface even under the force of gravity. Using a simple modified form of equation of motion in the vertical direction, we argue that there are two extreme ways of non-hydrostatic support: dynamical support and magnetic support. If the vertical acceleration is downward and its magnitude is a significant fraction of gravitational acceleration, non-hydrostatic support is dynamical in nature. Otherwise non-hydrostatic support is static, and magnetic support by horizontal magnetic fields is the only other possibility. We describe what kind of observations are needed in the clarification of the nature of non-hydrostatic support. Observations available so far seem to indicate that spicules in the quiet regions and dynamic fibrils in active regions are dynamically supported whereas the general chromosphere as well as prorninences is magnetically supported. Moreover, it appears that magnetic support is required for plasma in some coronal loops as well. We suspect that the identification of a coronal loop with a simple magnetic flux tube might be wrong in this regard.

A NEAR-INFRARED STUDY OF THE HIGHLY-OBSCURED ACTIVE STAR-FORMING REGION W51B

  • Kim, Hyo-Sun;Nakajima, Yasushi;Sung, Hwan-Kyung;Moon, Dae-Sik;Koo, Bon-Chul
    • 천문학회지
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    • 제40권1호
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    • pp.17-28
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    • 2007
  • We present wide-field $JHK_s$-band photometric observations of the three compact H II regions G48.9-0.3, G49.0-0.3, and G49.2-0.3 in the active star-forming region W51B. The star clusters inside the three compact H II regions show the excess number of stars in the $J-K_s$ histograms compared with reference fields. While the mean color excess ratio $(E_{J-H}/E_{H-K_s})$ of the three compact H II regions are similar to ${\sim}2.07$, the visual extinctions toward them are somewhat different: ${\sim}17$ mag for G48.9-0.3 and G49.0-0.3; ${\sim}23$ mag for G49.2-0.3. Based on their sizes and brightnesses, we suggest that the age of each compact H II region is ${\leq}2\;Myr$. The inferred total stellar mass, ${\sim}1.4{\times}10^4M_{\odot}$, of W51B makes it one of the most active star forming regions in the Galaxy with the star formation efficiency of ${\sim}10%$.

태양활동과 우주환경 (SOLAR ACTIVITY AND SPACE ENVIRONMENT)

  • 윤홍식
    • 천문학논총
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    • 제14권2호
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    • pp.83-89
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    • 1999
  • The Earth is exposed to constant outflow of the solar wind from the outer layers of the Sun, and violent transient events taking place from active regions increase the energy flux of both radiation and particles leaving the Sun. Thus the space surrounding the Earth is a highly dynamic environment that responds sensitively to changes in radiation, particles and magnetic field arriving from the Sun. Nowadays, it becomes increasingly important to understand how the physical system of Earth-space works and how the space around the Earth connects to interplanetary space. In the present paper we describe how explosive solar events, such as CME(Coronal Mass Ejection) and flares affect the Earth-space environment and how the space weather reacts to them. Practical consequences are presented to demonstrate why a broader view of Earth's environment is greatly needed to cope with modern day's inhabitation problem in a rapidly developing space age.

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STUDY OF SOLAR ACTIVE REGIONS BASED ON BOAO VECTOR MAGNETOGRAMS

  • MOON YONG-JAE;PARK YOUNG DEUK;YUN HONG SIK;CHO EUN-AH
    • 천문학회지
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    • 제32권2호
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    • pp.127-136
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    • 1999
  • In this study we present the study of solar active regions based on BOAO vector magnetograms and H$\alpha$ filtergrams. With the new calibration method we analyzed BOAO vector magnetograms taken from the SOFT observational system to compare with those of other observing systems. In this study it has been demonstrated that (1) our longitudinal magnetogram matches very well the corresponding Mitaka's magnetogram to the extent that the maximum correlation yields r=0.962 between our re-scaled longitudinal magnetogram and the Mitaka's magnetogram; (2) according to a comparison of our magnetograms of AR 8422 with those taken at Mitaka solar observatory their longitudinal fields are very similar to each other while transverse fields are a little different possibly due to large noise level; (3) main features seen by our longitudinal magnetograms of AR 8422 and AR 8419 and the corresponding Kitt Peak magnetograms are very similar to each other; (4) time series of our vector magnetograms and H-alpha observations of AR 8419 during its flaring (M3.1/1B) activity show that the filament eruption followed the sheared inversion line of the quadrupolar configuration of sunspots, indicating that the flare should be associated with the quadrupolar field configuration and its interaction with new filament eruption. Finally, it may be concluded that the Solar Flare Telescope at BOAO works normally and it is ready to do numerous observational and theoretical works associated with solar activities such as flares.

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Face detection using active contours

  • Chang, Jae-Sik;Lee, Mu-Youl;Moon, Chae-Hyun;Park, Hye-Sun;Lee, Kyung-Mi;Kim, Hang-Joon
    • 대한전자공학회:학술대회논문집
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    • 대한전자공학회 2002년도 ITC-CSCC -3
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    • pp.1515-1518
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    • 2002
  • This paper proposes an active contour model to detect facial regions in a given image. Accordingly we use the color information human faces which is represented by a skin color model. We evolve the active contour using the level set method which allows for cusps, corners, and automatic topological changes. Experimental results show the effectiveness of the proposed method.

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Accumulation characteristics and correlation analysis of five ginsenosides with different cultivation ages from different regions

  • Xiao, Dan;Yue, Hao;Xiu, Yang;Sun, Xiuli;Wang, YiBo;Liu, ShuYing
    • Journal of Ginseng Research
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    • 제39권4호
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    • pp.338-344
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    • 2015
  • Background: Ginseng (the roots of Panax ginseng Meyer) is a well-known traditional Oriental medicine and is now widely used as a health food. It contains several types of ginsenosides, which are considered the major active medicinal components of ginseng. It has recently been reported that the qualitative and quantitative properties of ginsenosides found in ginseng may differ, depending on cultivation regions, ages, species, and so on. Therefore, it is necessary to study these variations with respect to cultivation ages and regions. Methods: In this study, 3-6-yr-old roots of P. ginseng were collected from three different cultivation regions. The contents of five ginsenosides (Rb1, Rd, Rc, Re, and Rgl) were measured by rapid resolution liquid chromatography coupled with quadruple-time-of-flight mass spectrometry. The Kruskal-Wallis Rank sum test and multiple t test were used for comparative analysis of the data to evaluate the dynamic changes in the accumulation of these ginsenosides affected by cultivation regions and ages. Results: The content and composition of ginsenosides varied significantly among specimens collected from different cultivation regions and having different cultivation ages. For all samples, the content of Rg1 and Re ginsenosides increases with age and this rate of increase is different for each sample. The contents of Rb1, Rc, and Rd varied with cultivation ages in samples from different cultivation regions; especially, Rb1 from a 6-yr-old root showed approximately twofold variation among the samples from three cultivation regions. Furthermore, the content of Rb1 highly correlated with that of Rd (r = 0.89 across all locations and ages). Conclusion: In our study, only the contents of ginsenosides Rg1 and Re were affected by the root age. Ginsenosides Rb1, Rc, and Rd varied widely with ages in samples from different cultivation regions.

Postnatal Development of Subcallosal Zone Following Suppression of Programmed Cell Death in Bax-deficient Mice

  • Kim, Woon Ryoung;Sun, Woong
    • 한국발생생물학회지:발생과생식
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    • 제17권3호
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    • pp.179-186
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    • 2013
  • Neural stem cells are found in adult mammalian brain regions including the subgranular zone (SGZ) of the dentate gyrus (DG) and the subventricular zone (SVZ). In addition to these two regions, other neurogenic regions are often reported in many species. Recently, the subcallosal zone (SCZ) has been identified as a novel neurogenic region where new neuroblasts are spontaneously generated and then, by Bax-dependent apoptosis, eliminated. However, the development of SCZ in the postnatal brain is not yet fully explored. The present study investigated the precise location and amount of neuroblasts in the developing brain. To estimate the importance of programmed cell death (PCD) for SCZ histogenesis, SCZ development in the Bax-knockout (KO) mouse was examined. Interestingly, an accumulation of extra neurons with synaptic fibers in the SCZ of Bax-KO mice was observed. Indeed, Bax-KO mice exhibited enhanced startle response to loud acoustic stimuli and reduced anxiety level. Considering the prevention of PCD in the SCZ leads to sensory-motor gating dysfunction in the Bax-KO mice, active elimination of SCZ neuroblasts may promote optimal brain function.

지역주민 특성이 친수공간의 유지관리 활동에 미치는 영향 - 일본 치바현 카즈사지구의 사례 - (Effect of Personal Character of Rural Residents on Management Activities for Amenity Oriented Waterside Area - A Case of Kazusa District, Chiba Pref, Japan -)

  • 양용석;김선주;센가유타로
    • 농촌계획
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    • 제11권4호
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    • pp.1-8
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    • 2005
  • For the purpose of finding correlation between the characteristics of the rural residents and the maintenance activities of naturally favorable waterside spaces, this paper has conducted a research with the focus on the three model case regions in Japan. The methods of the research included surveys, interviews, and documents. The research confirmed that the three regions in focus have characteristics distinct from one another. The rate of participation in group activities was high in a region, with members that belong to groups most active in the maintenance activities. Reasons for their participation included: to manage the local area themselves; and to promote cooperation and friendships among the residents. This proves that participation in the maintenance activities has also attributed to the formation of close communities in the regions. According to the analytic conclusion of the factors related to participation, the residents' experience to have been involved in a professional education program which induces communal participation, acted more as the major factor than the individual ones.

위전도(胃電圖)의 최근(最近) 연구(硏究) 동향(動向) - 중국논문(中國論文)을 중심(中心)으로 (A Review on Recent Study of Electrogastrography - in Traditional Chinese Medicine)

  • 김선혁;박영재;박영배
    • 대한한의진단학회지
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    • 제12권1호
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    • pp.13-21
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    • 2008
  • Objectives: To review the history, method, parameters, system of electrogastrography(EGG) and to study its oriental medical application in Traditional Chinese Medicine. Methods: We investigate the research results through internet search engine, CNKI (China National Knowledge Infrastructure). Results: In China, EGG was studied on various regions, including multifarious regions of Traditional Chinese Medical. And also regions of Traditional Chinese Medical could divide classification of diseases, herbal medicine, acupuncture and the like. Conclusions: EGG is a noninvasive, easy and painless method that is kept recordings of the electrical activity of the stomach, therefore it has used for studies and clinics widely. EGG in Traditional Chinese Medicine has used an objective parameter that verified efficacies of oriental medicine. I would therefore like to conclude that there should be continued study and active application of EGG in the wide variety of oriental medicine.

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

  • 조경석;박성홍;;;;;;임은경
    • 천문학회보
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    • 제37권2호
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    • pp.137.1-137.1
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    • 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.

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