• 제목/요약/키워드: CMB

검색결과 122건 처리시간 0.026초

천리안 수증기 영상을 이용한 태풍진로의 전향위치 예측 연구 (Study on the Prediction of Turning Point of Typhoon Tracks using COMS Water Vapor Images)

  • 김종석;윤일희
    • 한국지구과학회지
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    • 제35권3호
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    • pp.168-179
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    • 2014
  • 이 연구의 목적은 관측주기가 짧은 천리안 위성의 수증기 영상자료를 활용하여 태풍의 전향위치와 시간까지 예측이 가능하도록 하는데 있다. 즉 수증기의 위성영상의 건조슬롯과 제트류의 남북진동의 관계를 이용하여 태풍진로의 전향위치를 보다 정확히 예측하는 것이다. 제트류는 제트스트리크의 위치와 지균풍 ${\upsilon}$성분의 크기에 따라 움직이는데, 지균풍 ${\upsilon}$ 성분이 남쪽방향으로 강화되면 제트류는 원형 제트로 발달하게 된다. 이때 수증기 영상에서는 건조슬롯이 남쪽으로 확대되고, 굴곡수분밴드(CMB) 거리가 좁혀지기 때문에 태풍이 전향하게 된다. 굴곡수분밴드가 위도 $15^{\circ}$ 이하이면 24시간 내에 태풍이 북 또는 북동으로 전향하게 된다. 결과적으로 태풍진로는 건조슬롯의 위치가 $32^{\circ}N$ 이하이면 $20-23^{\circ}N$이하에서 전향(2007년 1호 태풍 콩레이와 2012년 17호 태풍 즐라왓)하고, 건조슬롯이 $35^{\circ}N$ 이상 일 땐 $27^{\circ}$N에서 전향(2007년 4호 태풍 마니)하는 것으로 분석되었다.

Powdery Mildew Resistance Phenotype Test & Genotype Test in C. moschata

  • Jong-Gyu Park
    • 한국작물학회:학술대회논문집
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    • 한국작물학회 2022년도 추계학술대회
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    • pp.290-290
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    • 2022
  • Powdery mildew is known to be one of the serious diseases in C. moschata cultivation. Plants infected with powdery mildew cause damage to cultivation areas such as occurrence of deformity fruit and decrease in quantity. also, it has been reported that many farms have difficulties in controlling powdery mildew due to the outbreak under various conditions throughout the year. Therefore, this study intends to perform a phenotype test and a genotype test for C. moschata 60 lines grown in Jenong S&T. Podospareaxanthii, known as a pathogen that causes powder mildew disease in pumpkins in Korea, was collected and used as an inoculation source, phenotype test was performed by examining the infection area rate(%) of powdery mildew disease that occurred in leaves 25 days after inoculation. It was determined that 0% of the infection area rate was in the first stage, 1 to 5% in the second stage, 6 to 15% in the third stage, 16 to 30% in the fourth stage, and 31% or more in the fifth stage, The first and second stages were judged as resistance, the third as moderate resistance, and the fourth and fifth stages as sensitivity. As a result of the phenotype test, it was confirmed that the resistance was 21 points, moderate resistance was 14 points, and sensitivity was 25 points. After searching for the genes related to powdery mildew resistance resistance, pm-0, CmbHLH87, and LOC111453072, 21 points of resistance and 9 points of moderate resistance identified through phenotype tests were identified through gel electrophoresis after polymerase chain reaction(PCR) using 5 primers related to 3 genes. As a result of genotype testing of a total 30 points, the CmbHLH87 and LOC111453072 gene were found to be resistant bands in all points, PMR1 was identified as 20 points for resistance, 4 points for moderate resistance, and 6 points for sensitivity, PMR2 was not identified in the entire band, and PMR5 was identified as 18 point for resistance, 3 points for moderate resistance, and 9 points for sensitivity. As a result, when comparing the phenotype test results and genotype test results, CmbHLH87 and LOC111453072 genes was 100% consistent in resistance and moderate resistance, PMR1 was 95.2% in resistance, 44.4% in moderate resistance, and PMR5 was 90% in resistance and 33.3% in moderate resistance, PMR2 was not consistent in resistance and moderate resistance. Therefore, it is expected that more accurate PMR test will be possible by using molecular markers(PMR1, PMR5) and by developing CmbHLH87 and LOC111453072 gene-related molecular markers.

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Chemical Modification of Intracellular Cytosine Deaminase from Chromobacterium violaceum YK 391

  • Kim, Jung;Kim, Tae-Hyun;Yu, Tae-Shick
    • Biotechnology and Bioprocess Engineering:BBE
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    • 제10권3호
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    • pp.180-185
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    • 2005
  • Cytosine deaminase (cytosine aminohydrolase, EC 3.5.4.1) stoichiometrically catalyzes the hydrolytic deamination of cytosine and 5-fluorocytosine to uracil and 5-fluorouracil, respectively. Amino acid residues located in or near the active sites of the intracellular cytosine deaminase from chromobacterium violaceum YK 391 were identified by chemical modification studies. The enzymic activity was completely inhibited by chemical modifiers, such as 1mM NBS, chloramine-T, $\rho-CMB,\;\rho-HMB$ and iodine, and was strongly inhibited by 1mM PMSF and pyridoxal 5'-phosphate. This chemical deactivation of the enzymic activity was reversed by a high concentration of cytosine. Furthermore, the deactivation of the enzymic activity by $\rho-CMB$ was also reversed by 1mM cysteine-HCI, DTT and 2-mercaptoethanol. These results suggested that cysteine, tryptophan and methionine residues might be located in or near the active sites of the enzyme, while serine and lysine were indirectly involved in the enzymic activity. The intracellular cytosine deaminase from C violaceum YK 391 was assumed to be a thiol enzyme.

CONSTRAINTS ON PRE-INFLATION COSMOLOGY AND DARK FLOW

  • MATHEWS, GRANT J.;LAN, N.Q.;KAJINO, T.
    • 천문학논총
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    • 제30권2호
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    • pp.309-313
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    • 2015
  • If the present universe is slightly open then pre-inflation curvature would appear as a cosmic dark-flow component of the CMB dipole moment. We summarize current cosmological constraints on this cosmic dark flow and analyze the possible constraints on parameters characterizing the pre-inflating universe in an inflation model with a present-day very slightly open ${\Lambda}CDM$ cosmology. We employ an analytic model to show that for a broad class of inflation-generating effective potentials, the simple requirement that the observed dipole moment represents the pre-inflation curvature as it enters the horizon allows one to set upper and lower limits on the magnitude and wavelength scale of pre-inflation fluctuations in the inflaton field and the curvature parameter of the pre-inflation universe, as a function of the fraction of the total initial energy density in the inflaton field. We estimate that if the current CMB dipole is a universal dark flow (or if it is near the upper limit set by the Planck Collaboration) then the present constraints on ${\Lambda}CDM$ cosmological parameters imply rather small curvature ${\Omega}_k{\sim}0.1$ for the pre-inflating universe for a broad range of the fraction of the total energy in the inflaton field at the onset of inflation. Such small pre-inflation curvature might be indicative of open-inflation models in which there are two epochs of inflation.

저잡음 증폭기를 위한 새로운 자동 보상 회로 (A New Automatic Compensation Circuit for Low Noise Amplifiers)

  • 류지열;길버트;노석호
    • 한국정보통신학회:학술대회논문집
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    • 한국해양정보통신학회 2005년도 춘계종합학술대회
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    • pp.995-998
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    • 2005
  • 본 논문에서는 시스템 온 칩 (SoC, System-on-Chip) 트랜시버에 적용이 가능하며. 저잡음 증폭기(LNA, Low Noise Amplifier)를 위한 자동 보상 회로 (ACC, automatic compensation circuit)를 제안한다. 개발된 회로는 고주파 내부 자체 검사 (BIST, Built-In Self-Test) 회로, 커패시터 미러 뱅크 (CMB, Capacitor Mirror Banks)와 디지털 처리장치로 구성되어 있다. 자동 보상 회로는 LNA가 정상 동작을 하지 않을 때 SoC 트랜시버의 구성요소인 디지털 프로세서를 이용하여 LNA가 정상 동작을 하도록 자동적으로 조정하는 역할을 한다.

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Testing Gravity with Cosmic Shear Data from the Deep Lens Survey

  • Sabiu, Cristiano G.;Yoon, Mijin;Jee, Myungkook James
    • 천문학회보
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    • 제43권2호
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    • pp.40.4-41
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    • 2018
  • The current 'standard model' of cosmology provides a minimal theoretical framework that can explain the gaussian, nearly scale-invariant density perturbations observed in the CMB to the late time clustering of galaxies. However accepting this framework, requires that we include within our cosmic inventory a vacuum energy that is ~122 orders of magnitude lower than Quantum Mechanical predictions, or alternatively a new scalar field (dark energy) that has negative pressure. An alternative approach to adding extra components to the Universe would be to modify the equations of Gravity. Although GR is supported by many current observations there are still alternative models that can be considered. Recently there have been many works attempting to test for modified gravity using the large scale clustering of galaxies, ISW, cluster abundance, RSD, 21cm observations, and weak lensing. In this work, we compare various modified gravity models using cosmic shear data from the Deep Lens Survey as well as data from CMB, SNe Ia, and BAO. We use the Bayesian Evidence to quantify the comparison robustly, which naturally penalizes complex models with weak data support. In this talk we present our methodology and preliminary results that show f(R) gravity is mildly disfavoured by the data.

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화학적수식에 의한 Bacillus subtilis ED 213 Cytidine Deaminase의 활성부위에 관한 연구 (A study on the Active Site of Cytidine Deaminase from Bacillus subtilis ED 213 by Chemical Modification)

  • 박정문;박상원;서태수;김정;유대식
    • 미생물학회지
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    • 제35권2호
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    • pp.133-138
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    • 1999
  • Bacillus subtilis ED 213의 cytidine deaminase 의 활성부위에 존재하는 필수 아미노산잔기를 화학수식 방법으로 측정하였다. 본 효소는 1mM o-phenanthroline 에 의하여 효소활성이 43% 저해되어 효소활성 발현에 Fe\sup 2+\가 요구된다고 추정되며, 1mM ethylenediaminetetraacetic acid 에 의해서는 효소활성이 오히려 28% 정도 촉진되었다. 본 효소는 1mM N-bromosuccinimide, 1mM chloramine-T 와 1mM $\rho$-chloromercuribenzoic acid에 의하여 100% 저해되었으며, 그의 저해 양상은 경쟁적 저해 양상을 나타내었다. 본 효소의 효소활성은 1mM pyridoxal-5-phosphate 에 의항 36% 저해되었으며, 1mM 1ethyl-3-carbodiamide 와 1mM glycine methylester에 의해 저해된 효소활성이 5mM cysteine에 의해 완전히 회복되었다. 이상의 결과로부터 Bacillus subtilis ED 213 cytidine deaminase의 활성부위에는 tyrosine, methionine, cysteine 과 serine 잔기가 관여할 뿐만 아니라 lysine 과 glycine 도 효소활성에 관여하는 것으로 추정된다.

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전자선 가속기에 의해 방사선 처리한 양이온교환막을 이용한 전해-전기투석에 의한 HIx용액으로부터 HI의 농축 (Electro-electrodialysis Using the Radiation-treated Cation Exchange Membrane by Accelerated Electron Radiation to Concentrate HI from HIx Solution)

  • 황갑진;김정근;이상호;최호상
    • 멤브레인
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    • 제17권4호
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    • pp.338-344
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    • 2007
  • HI몰랄리티가 9.5 $mol/kg-H_2O$인 HI의 전해-전기투석을 시판의 양이온교환막(CMB)을 이용하여 요오드의 존재하에 실험을 진행하였다. 수소이온 투과의 선택성을 증가시키기 위해, 막은 전자선 가속기를 이용하여 방사선 처리하였다. 방사선 처리한 막의 막특성(막 저항, 이온교환용량, 함수율)을 측정하였다. 각각의 방사선량에서 처리한 막의 2 $mol/dm^3$의 KCl 용액에서 막저항, 이온교환용량과 함수율은 처리하지 않은 막과 거의 동등의 값을 가졌다. HI몰랄리티가 9.5 $mol/kg-H_2O$인 HI의 전해-전투기투석을 $75^{\circ}C$, 9.6 $A/dm^2$에서 진행하였다. 전자선 가속기에 의해 방사선 처리한 양이온교환막은 처리하지 않은 막과 비교하여 고분자의 가교구조와 함께 수소이온투과의 높은 선택성을 가졌다.

HAMILTONIAN OF A SECOND ORDER TWO-LAYER EARTH MODEL

  • Selim, H.H.
    • 천문학회지
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    • 제40권2호
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    • pp.49-60
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    • 2007
  • This paper deals with the theory for rotational motion of a two-layer Earth model (an inelastic mantle and liquid core) including the dissipation in the mantle-core boundary(CMB) along with tidal effects produced by Moon and Sun. An analytical solution being derived using Hori's perturbation technique at a second order Hamiltonian. Numerical nutation series will be deduced from the theory.