• 제목/요약/키워드: Bach2

검색결과 88건 처리시간 0.031초

Relaxor Behaviors in xBaTiO3-(1-x)CoFe2O4 Materials

  • Dung, Cao Thi My;Thi, Nhu Hoa Tran;Ta, Kieu Hanh Thi;Tran, Vinh Cao;Nguyen, Bao Thu Le;Le, Van Hieu;Do, Phuong Anh;Dang, Anh Tuan;Ju, Heongkyu;Phan, Bach Thang
    • Journal of Magnetics
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    • 제20권4호
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    • pp.353-359
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    • 2015
  • Dielectric properties of $xBaTiO_3-(1-x)CoFe_2O_4$ composite materials have been investigated. Dielectric properties of $BaTiO_3$, $CoFe_2O_4$ and $0.5BaTiO_3-0.5CoFe_2O_4$ samples show frequency dependence, which is classified as relaxor behavior with different relaxing degree. The relaxor behaviors were described using the modified Curier-Weiss and Vogel-Fulcher laws. Among three above samples, the $BaTiO_3$ sample has highest relaxing degree. Photoluminescence spectral indicated defects, which might in turn control relaxing degree.

The polarimetric study of (331471) 1984QY1: an asteroid in comet-like orbit

  • Kim, Jooyeon;Ishiguro, Masateru;Bach, Yoonsoo P.;Kuroda, Daisuke;Naito, Hiroyuki;Kim, Yoonyoung;Kwon, Yuna G.;Imai, Masataka;Kuramoto, Kiyoshi;Watanabe, Makoto
    • 천문학회보
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    • 제42권2호
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    • pp.50.2-50.2
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    • 2017
  • Spatial distribution of atmosphereless bodies in the solar system provides an important clue as to their origins, namely asteroids from Mainbelt or comets from outer solar system. It is, however, difficult to distinguish asteroids and dormant comets due to their similar appearances. In this study, we conducted a unique observation to differentiate asteroids and dormant comets in terms of 'polarimetry'. We observed (331471) 1984 QY1 (hereafter QY1) at large phase angles using the Multi-Spectral Imager (MSI) on the 1.6-m Pirka Telescope from UT 2016 May 25 to June 24. QY1 is a dormant comet candidate in terms of the dynamical properties (i.e. the Tisserand parameter with respect to Jupiter, TJ = 2.68). We analyzed the polarization degree of QY1 as a function of phase angle and found its maximum polarization degree, $Pmax=8.68{\pm}0.28%$ and $8.72{\pm}0.38%$, in RC-and V-band, respectively, around the phase angle of ${\alpha}=100^{\circ}$. In addition, we obtained the geometric albedo, $pV=0.16{\pm}0.02$ by means of an empirical slope-albedo law. The polarimetric properties and the albedo value we acquired are similar to those of S-type asteroids rather than cometary nuclei. In this presentation, we introduce our observation and findings. In addition, we further discuss a dynamical transportation process from Mainbelt to the current orbit.

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The Geometric Albedo of (4179) Toutatis

  • Bach, Yoonsoo P.;Ishiguro, Masateru;Jin, Sunho;Yang, Hongu;Moon, Hong-Kyu;Choi, Young-Jun;JeongAhn, Youngmin;Kim, Myung-Jin;Kwak, Sungwon
    • 천문학회보
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    • 제43권2호
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    • pp.44.4-45
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    • 2018
  • (4179) Toutatis (Toutatis hereafter) is one of the Near-Earth Asteroids which has been studied most rigorously not only via ground-based photometric, spectroscopic, polarimetric, and radar observations, but also via the in-situ observation by the Chinese Chang'e-2 spacecraft. However, one of the most fundamental physical properties, the geometric albedo, is less determined. In order to derive the reliable geometric albedo and further study the physical condition on the surface, we made photometric observations of Toutatis near the opposition (i.e., the opposite direction from the Sun). We thus observed it for four days on 2018 April 7-13 using three 1.6-m telescopes, which consist of the Korean Microlensing Telescope Network (KMTNet). Since the asteroid has a long rotational period (5.38 and 7.40 days from Chang'e-2, Zhao et al., 2015), the continuous observations with KMTNet matches the purpose of our photometric study of the asteroid. The observed data cover the phase angle (Sun-asteroid-observer's angle) of 0.65-2.79 degree. As a result, we found that the observed data exhibited the magnitude changes with an amplitude of ~0.8 mag. We calculated the time-variable geometrical cross-section using the radar shape model (Hudson & Ostro 1995), and corrected the effect from the observed data to derive the geometric albedo. In this presentation, we will present our photometric results. In addition, we will discuss about the regolith particles size together with the polarimetric properties based on the laboratory measurements of albedo-polarization maximum.

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Polarimetry of (162173) Ryugu at the Bohyunsan Optical Astronomy Observatory using the 1.8-m Telescope with TRIPOL

  • Jin, Sunho;Ishiguro, Masateru;Kuroda, Daisuke;Geem, Jooyeon;Bach, Yoonsoo P.;Seo, Jinguk;Sasago, Hiroshi;Sato, Shuji
    • 천문학회보
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    • 제46권1호
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    • pp.45.2-46
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    • 2021
  • The Hayabusa 2 mission target asteroid (162173) Ryugu is a near-Earth, carbonaceous (C-type) asteroid. Before the arrival, this asteroid is expected to be covered with mm- to cm- sized grains through the thermal infrared observations [1]. These grains are widely understood to be formed by past impacts with other celestial bodies and fractures induced by thermal fatigue [2]. However, the close-up images by the MASCOT lander showed lumpy boulders but no abundant fine grains [3]. Morota et al. suggested that there would be submillimeter particles on the top of these boulders but not resolved by Hayabusa 2's onboard instruments [4]. Hence, we conducted polarimetry of Ryugu to investigate microscopic grain sizes on its surface. Polarimetry is a powerful tool to estimate physical properties such as albedo and grain size. Especially, it is known that the maximum polarization degree (Pmax) and the geometric albedo (pV) show an empirical relationship depending on surface grain sizes [5]. We observed Ryugu from UT 2020 November 30 to December 10 at large phase angles (ranging from 78.5 to 89.7 degrees) to derive Pmax. We modified TRIPOL (Triple Range Imager and POLarimeter, [6]) to attach to the 1.8-m telescope at the Bohyunsan Optical Astronomy Observatory (BOAO). With this instrument, we observed the asteroid and determined linear polarization degrees at the Rc-band filter. We obtained sufficient data sets from 7 nights at this observatory to determine the Pmax value, and collaborated with other observatories in Japan (i.e., Hokkaido University, Higashi-Hiroshima, and Nishi-Harima) to acquire linear polarization degrees of the asteroid from total 24 nights observations with large phase angle coverage (From 28 to 104 degrees). The observational results have been published in Kuroda et al. (2021) [7]. We thus found the dominance of submillimeter particles on the surface of Ryugu from the comparison with other meteorite samples from the campaign observation. In this presentation, we report our activity to modify the TRIPOL for the 1.8-m telescope and the polarimetric performance. We also examine the rotational variability of the polarization degree using the TRIPOL data.

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Near-Infrared Photopolarimetry of Large Main Belt Asteroid - (4) Vesta

  • Bach, Yoonsoo P.;Ishiguro, Masateru;Takahashi, Jun;Naito, Hiroyuki;Kwon, Jungmi;Kuroda, Daisuke
    • 천문학회보
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    • 제46권1호
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    • pp.45.1-45.1
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    • 2021
  • The polarization degree as a function of phase angle (the Sun-target-observer's angle), so-called the polarimetric phase curves (PPC), have provided priceless information on asteroids' albedos since B. Lyot (1929). Succeeding experimental works in 1970s have confirmed the Umow law: There is a universal and strong correlation between the albedo and the PPC slope (slope of the tangential line at the zero of the PPC at phase angle ~ 20 degrees). Experiments in 1990s (ref [1]), on the other hand, have demonstrated that the negative branch of PPC is dependent on the size parameter (X ~ π * particle-size / wavelength), especially when X <~5. The change in particle size changed the minimum polarization degree, location of the minimum, and the width of the negative branch (called the inversion angle). From polarimetry[2] and spectroscopy[3], large asteroids are expected to be covered with fine (<~ 10 ㎛ size) particles due to the gravity. The size parameters are X ~ 30 at the optical wavelength (λ ~ 0.5 ㎛) and X ~ 10 in near-infrared (J, H, Ks bands; λ ~ 1.2-2.2 ㎛), if the representative particle size of 5 ㎛ is considered. Accordingly, the near-infrared polarimetry has a great potential to validate the idea in ref[1]. We conducted near-infrared photopolarimetry of the large asteroid (4) Vesta using the Nishiharima Infrared Camera (NIC) at Nishi-Harima Astronomical Observatory (NHAO). NIC allows simultaneous polarimetric measurements in J, H, and Ks bands, and thus the change of PPC is obtained for three different size parameters. As a result, we found a signature of the change in the negative branch in the PPC of asteroid (4) Vesta. We will introduce our observation and the results and give an interpretation of the regolith on Vesta.

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대체의학(代替醫學)과 한의학(韓醫學)의 비교연구(比較硏究) (A Comparative Study of Alternative Medicine with Oriental Medicine)

  • 류영수
    • 동의신경정신과학회지
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    • 제8권2호
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    • pp.1-12
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    • 1997
  • As there has recently been growing interest in Alternative Medicine, Oriental Medicals have been trying to incorporate Alternative Medicine into Oriental Medicine evolutionarily. The purpose of this study is to make a comparative study of the historical background and present condition, the view of life, the principle of therapeutics, and the various therapeutics in Alterative Medicine and Oriental Medicine from the viewpoint of Oriental Medicine. The conclusion of this study is; 1. Although Alternative Medicine has become influential mainly in the effort of finding a solution the limit of western medicine, the clinical effect of Alternative Medicine should be verified continuously. 2. Alternative Medicine includes all of the therapeutics such as Traditional Medicine, Naturopathy, Complementary Medicine and Selective Medicine whose characters are different from Western Medicine and Oriental Medicine can be regarded as a sort of Alternative Medicine. 3. The holistic, systematic view of life of Alternative Medicine, from which viewpoint human considered as a harmonious vital existence, is a sort of recurrence to the view of Hipporcrates. 4. From the viewpoint of Alternative Medicine, a disease is not partial but holistic disorder and is treated by utilizing natural products as a medicine based on the principle that pursues harmonious and balanced psychosomatic function. This principle of therapeutic is the same as Oriental Medicine is based on. 5. Alternative Medicine may be classified largely five category, (1) Eastern Therapy, (2) Manipulative Therapy, (3) Natural Therapy, (4) Active Therapy, (5) Therapy Involving External Powers. 6. Besides Alternative Medicine which is used in clinical treatment, Massage, Homeopathy, Bach Flower remedies, Meditation, and other Music Therapy and Color Therapy is relatively accordant with therapeutics in Oriental Medicine and should be more actively accepted in clinics and improved.

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Enhancing the Intrinsic Bioremediation of PAH-Contaminated Anoxic Estuarine Sediments with Biostimulating Agents

  • Bach Quang-Dung;Kim Sang-Jin;Choi Sung-Chan;Oh Young-Sook
    • Journal of Microbiology
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    • 제43권4호
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    • pp.319-324
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    • 2005
  • Estuarine sediments are frequently polluted with hydrocarbons from fuel spills and industrial wastes. Polycyclic aromatic hydrocarbons (PAHs) are components of these contaminants that tend to accumulate in the sediment due to their low aqueous solubility, low volatility, and high affinity for particulate matter. The toxic, recalcitrant, mutagenic, and carcinogenic nature of these compounds may require aggressive treatment to remediate polluted sites effectively. In petroleum-contaminated sediments near a petrochemical industry in Gwangyang Bay, Korea, in situ PAH concentrations ranged from 10 to 2,900 ${\mu}g/kg$ dry sediment. To enhance the biodegradation rate of PAHs under anaerobic conditions, sediment samples were amended with biostimulating agents alone or in combination: nitrogen and phosphorus in the form of slow-release fertilizer (SRF), lactate, yeast extract (YE), and Tween 80. When added to the sediment individually, all tested agents enhanced the degradation of PAHs, including naphthalene, acenaphthene, anthracene, fluorene, phenanthrene, fluoranthene, pyrene, chrysene, and benzo [a] pyrene. Moreover, the combination of SRF, Tween 80, and lactate increased the PAH degradation rate 1.2-8.2 times above that of untreated sediment (0.01-10 ${\mu}g$ PAH/ kg dry sediment/day). Our results indicated that in situ contaminant PAHs in anoxic sediment, including high molecular weight PAHs, were degraded biologically and that the addition of stimulators increased the biodegradation potential of the intrinsic microbial populations. Our results will contribute to the development of new strategies for in situ treatment of PAH-contaminated anoxic sediments.

살균제의 벼 육묘상 처리에 의한 도열병 방제 효과 (The Effect of Fungicides against Rice Blast by the Nursery Treatment at Rice Seedling)

  • 강범관;민지영;김윤식;;정해연;조인준;김흥태
    • 식물병연구
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    • 제10권1호
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    • pp.69-72
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    • 2004
  • Carbosulfan과 합제로 개발한 isoprothiolane과 tricyclazole, 그리고 probenazole을 벼 육묘상자에 처리하고, 처리 당일에 본답에 이앙한 후, 잎도열병과 목도열병에 대한 방제 효과를 조사하였다. 세 가지의 살균제는 모두 이앙하고 3개월 후까지도 잎도열병을 방제할 수 있었다. 특히 tricyclazole 합제의 경우에는 시간이 경과하면서 그 효과가 더 상승하였으며, 9월 6일 조사 때에 85.5%의 잎도열병 방제 효과를 보였다. 목도열병에 대한 효과는 probenazole이 가장 우수하였는데, 10월 14일에 조사한 probenazole 처리구의 목도열병 이병수율은 6.9%로 78.7%의 무처리구에 비하여 91.2%의 방제 효과를 보였다. Isoprothiolane과 tricyclazole 합제는 잎도열병보다 목도열병에 대한 방제 효과가 저조하였으며, 두 처리구는 각각 47.5%와 61.1%의 효과를 보였다. 이상의 결과처럼 침투이행효과가 우수한 살균제가 벼의 육모상 처리제로 개발이 가능해진다면 포장에서의 도열병 방제가 효과적이고 간편하게 수행될 수 있을 것이다.

고저 접합 에미터 구조를 갖는 $N^+NPP^+$ Si 태양전지의 효율 개선 (Efficiency Improvement of $N^+NPP^+$ Si Solar Cell with High Low Junction Emitter Structure)

  • 장지근;김봉렬
    • 대한전자공학회논문지
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    • 제21권1호
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    • pp.62-70
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    • 1984
  • 비저항이 10Ω-cm, 두께가 13∼15mi1인 <111> oriented, p형 Si기판을 이용하여 N+PP+ BSF 전지와 에미터 영역이 N+N 고저 접합으로 이루어진 N+NPP+ HELEBSF(high low emitter bach surface field) 전지를 설계 제작하였다. 접합형 태양전지의 에미터 영역에서 고저 접합구조가 효율 개선에 미치는 영향을 검토하기 위해 HLEBSF 전지의 N영역을 제외하고는 같은 마스크와 동시 공정을 통해 N+PP-전지와 N+NPP+ 전지의 가영역에서 물리적 파라미터들(불순물 농도, 두께)을 동일하게 만들었다. 100mW/㎠의 인공조명에서 측정한 결과 N+PP+ 전지들의 전면적 (유효 수광면적) 평균 변환효율이 10.94%(12.16%)이었고, N+NPP+ 전지들의 평균 변환효율은 12.07% (13.41%)로 나타났다. N+NPP+ 전지의 효율개선은 N+N-고저 접합 에미터 구조가 N+ 에미터 영역에서 나타나는 heavy doping effects를 제거함으로써 에미터 재결합 전류의 증가를 억제하고 나아가 개방전압(Voc)과 단락전류(Ish)의 값을 증가시켜 준 결과로 볼 수 있다.

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Sensitivity of Escherichia coli to Seaweed (Ascophyllum nodosum) Phlorotannins and Terrestrial Tannins

  • Wang, Yuxi;Xu, Z.;Bach, S.J.;McAllister, T.A.
    • Asian-Australasian Journal of Animal Sciences
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    • 제22권2호
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    • pp.238-245
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    • 2009
  • Pure culture experiments were conducted to assess the bacteriostatic and bactericidal effects of phlorotannins (PT) isolated from Ascophyllum nodosum (brown seaweed) on Escherichia coli O157:H7. In Exp. 1, one non-O157:H7 strain (25922) and three strains of E. coli O157:H7 (3081, EDL933 and E318N) were cultured in M9 medium with PT included at 0 (control), 25, 50 or $100{\mu}g/ml$ (n = 3). Bacterial growth was monitored by $OD_{600}$ at 0, 4, 6, 12 and 24 h, and by dilution plating at 0, 4, 6 and 24 h. All strains were inhibited (p<0.001) by PT to varying degrees. At 50 or $100{\mu}g/ml$, PT prevented growth of all four strains. At $25{\mu}g\;PT/ml$, growth of 25922, 3081, E318N and EDL933 was inhibited for 6, 12 and 24 h, respectively, but 25922 and 3081 resumed growth by 12 and 24 h. Direct plating confirmed bactericidal effects of PT on all four strains at $100{\mu}g/ml$, and on EDL933 and E318N at $50{\mu}g/ml$. In Exp. 2, strains 25922 and 3081 were incubated with no tannins or with $50{\mu}g/ml$ of PT, purified condensed tannins (CT) from Quebracho (Schinopsis balansaei), or purified tannic acid from Rhus semialata (Anacardiaceae) as hydrolysable tannins (HT). Strain 3081 was unaffected by HT or CT, but was completely inhibited (p<0.001) by PT at 4, 6 and 24 h. Strain 25922 was unaffected by HT, slightly inhibited by CT, and almost eradicated by PT at 4 and 6 h. Transmission electron microscopy revealed tannin-mediated alterations to bacterial cell walls. Phlorotannins from A. nodosum exhibit growth-inhibiting and bactericidal effects in vitro against the strains of E. coli O157:H7 investigated. Anti-E. coli efficacy of A. nodosum PT is superior to that of terrestrial tannins purified from Quebracho and from Rhus semialata.