• 제목/요약/키워드: $b^{0,+}AT$

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물-결합재 비와 잔골재-결합재 비에 따른 알칼리 활성화 슬래그 모르타르의 기초특성 (The Fundamental Properties of Alkali-Activated Slag Cement (AASC) Mortar with Different Water-Binder Ratios and Fine Aggregate-Binder Ratios)

  • 김태완;함형길;이성행;엄장섭
    • 한국구조물진단유지관리공학회 논문집
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    • 제17권5호
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    • pp.77-86
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    • 2013
  • 본 연구는 물-결합재 비 (W/B)와 잔골재-결합재 비 (F/B)에 따른 알칼리 활성화 슬래그 시멘트 (AASC)의 기초 특성에 관한 연구이다. W/B 비는 0.35, 0.40, 0.45, 그리고 0.50를 선정하였다. 그리고 F/B 비는 1.00에서 3.00까지 0.25 크기로 고려하였다. 알칼리 활성화제는 2M과 4M의 NaOH를 사용하였다. 실험은 플로우, 흡수율, 압축강도, 초음파 속도 그리고 건조수축을 측정하여 비교하였다. 플로우, 압축강도, 흡수율, 초음파 속도 그리고 건조수축 모두 W/B 비가 증가하면 감소하였다. 압축강도는 동일 W/B 비에서 F/B 비가 증가할수록 감소하였다. 또한 특정 F/B 비에서 강도가 증가하는 것을 볼 수 있었다. 그리고 S2 (river sand 2)는 S1 (river sand 1)보다 낮은 물리적 특성을 나타냈는데, 이는 조립률 때문으로 판단된다. 본 실험의 결과 AASC의 공학적 특성은 W/B 비와 F/B 비가 영향을 주는 것으로 판단된다. 최적의 F/B 비는 각 W/B 비에 대해 1.75~2.50 인 것으로 생각된다. 또한 W/(B+F) 비가 0.13과 0.14 사이일 때 AASC 모르타르의 배합설계가 효과적일 것으로 판단된다.

GaAs MESFET를 이용한 ISM 대역 MMIC SPDT 스위치 설계 (Design of MMIC SPDT Switches in the ISM Band Using GaAs MESFETs)

  • 박훈;윤경식;지홍구;김해천
    • 한국통신학회논문지
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    • 제28권3A호
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    • pp.179-184
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    • 2003
  • 본 논문에서는 ISM대역에서 수신경로의 격리도를 크게 송신경로의 삽입손실은 작게 하며 동시에 P1dB를 크게 하는 비대칭구조의 MMIC SPDT 스위치를 제안하였으며, 이를 ETRI에서 지원하는 IDEC MPW의 0.5㎛ GaAs MESFET으로 제작하였다. 이 SPDT 스위치 수신경로의 삽입손실은 3GHz에서 1.518dB, 5.75GHz에서 1.777dB이고, 격리도는 3GHz에서 38.474dB, 5.75GHz에서 29.125dB로 측정되었다. 그리고, 송신경로의 삽입손실은 3GHz에서 0.961dB, 5.75GHz에서 1.162dB이고, 격리도는 3GHz에서 23.259dB, 5.75GHz에서 16.632dB였다. 비대칭구조의 스위치는 대칭구조에 비하여 수신경로의 격리도가 3GHz에서 15.9dB, 5.75GHz에서 11.9dB 정도 개선되었으며, 삽입손실은 약 0.6dB 정도 증가하였다. 또한, SPDT 스위치 송신경로의 P1dB는 21.5dBm로 대칭구조에 비하여3.86dB 증가하였다.

The influence of cuttlebone on the target strength of live golden cuttlefish (Sepia esculenta) at 70 and 120 kHz

  • Lee, Daejae
    • Fisheries and Aquatic Sciences
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    • 제19권2호
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    • pp.8.1-8.11
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    • 2016
  • To quantitatively estimate the influence of cuttlebone on the target strength (TS) of golden cuttlefish, the cuttlebone was carefully extracted from 19 live cuttlefish caught using traps in the inshore waters around Geojedo, Korea, in early May 2010 and the TS was measured using split-beam echosounders (Simrad ES60 and EY500). The TS-length relationships for the cuttlefish (before the extraction of cuttlebone, Fish Aquat Sci. 17:361-7, 2014) and the corresponding cuttlebone were compared. The cuttlebone length ($L_b$) ranged from 151 to 195 mm (mean $L_b$ = 168.3 mm) and the mass ($W_b$) ranged from 29.3 to 53.2 g (mean $W_b$ = 38.8 g). The mean TS values at 70 and 120 kHz were -33.60 dB (std = 1.12 dB) and -32.24 dB (std = 1.87 dB), respectively. The mean TS values of cuttlebone were 0.19 dB and 0.04 dB lower than those of cuttlefish at 70 and 120 kHz, respectively. For 70 and 120 kHz combined, the mean TS value of cuttlebone was -32.87 dB, 0.11 dB lower than that of cuttlefish (-32.76 dB). On the other hand, the mean TS value of cuttlebone predicted by the regression ($TS_b$ = 24.86 $log_{10}$ $L_b$ - 4.86 $log_{10}$ ${\lambda}$ - 22.58, $r^2$ = 0.85, N = 38, P < 0.01) was -33.10 dB, 0.04 dB lower than that of cuttlefish predicted by the regression ($TS_c$ = 24.62 $log_{10}$ $L_c$ - 4.62 $log_{10}$ ${\lambda}$ - 22.64, $r^2$ = 0.85, N = 38, P < 0.01). That is, the contribution of cuttlebone to the cuttlefish TS determined by the measured results was slightly greater than that by the predicted results. These results suggest that cuttlebone is responsible for the TS of cuttlefish, and the contribution is estimated to be at least 99 % of the total echo strength.

UBV PHOTOMETRY AT THE OUTSIDE ECLIPSE PHASE OF AZ CASSIOPEIAE

  • Nha, Il-Seong
    • Journal of Astronomy and Space Sciences
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    • 제11권1호
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    • pp.21-30
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    • 1994
  • VV Cep-type long period spectroscopic-eclipsing binary AZ Cas has been observed for five years, 1985 Oct~1990 Feb, UBV at the Ilsan Station of Yonsei University Observatory. A total of 431 observations (U=129, B=142 and V=160) are made for 86 nights. Instrumental differential UBV and B-V light curves made with these observations cover phases nearly a half of one period. There is no appreciable light variation in V but in other two passbands a gradual decrease of the brightness is clearly noticed. The loss of light in B resulted in a reddening in $\Delta(B-V)$ by + 0.06 at phases between 0.4~0.5 as compared with that of at phase ~0.1. This intrinsic reddening arouses a question why at the orbital phase of the transit of a hot star in front of a cool M supergiant the heating of the facing hemisphere of M supergiant by the strong radiation from the B stat is absent. With regard to this unusual situation we propose a hypothesis that a large amount of gas stream of low temperature ejected from the surface of M supergiant component towards the B star dominates the brightness of B star and the reflection effect.

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들깨와 잣이 흰쥐의 혈액 성분에 미치는 영향 (The Effects of Perilla and Pine Nut on Blood Components in Rats)

  • Jho, Hu Jhong
    • 한국환경보건학회지
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    • 제10권1호
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    • pp.99-106
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    • 1984
  • The diets used to this experiment were composed only of stock diet for group A, a mixture of stock diet and 2% cholesterol for group B, and 5%, 10% perilia powder for group C, D and 5%, 10% pine nut for group E, F in addition to group B diet respectively. All groups fed with these experimental diets for 3 weeks were fasted for 15 hours at the end of the experiment, and then they were decapitated to take serum. The serum was used to measure the level of glucose, total cholesterol, triglyceride, HDL-cholesterol and lipoprotein composition. The results were summarized as follows. 1. Perilla and pine nut diets have no influence on body weight and food intake in cholesterolfed male rats 2. The blood glucose level was not changed significantly at groups C-F. 3. Total cholesterol level was significantly decreased by 21.6% ~ 29.7% at group C-F than at group B. 4. HDL-cholesterol level was increased by 51.3% ~ 86.1% at group C-F than at Group B. 5. The $\alpha/\beta$ ratio which is 0.51 at the group A was risen to 0.99 at the group B. However, this ratio was decreased to 0.5 0 - 0.51 at group C, D and to 0.68 - 0.69 at group E.F.

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B16세포주의 방사선 및 항암제감수성에 관한 실험적 연구 (AN EXPERIMENTAL STUDY ON THE RADIOSENSITIVITY AND CHEMOSENSITIVITY OF B16 CELL LINE)

  • 나승목;고광준
    • 치과방사선
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    • 제25권2호
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    • pp.331-341
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    • 1995
  • The purpose of this study was to aid in the prediction of tumor cell tolerance to radiotherapy and/or chemotherapy. For this study, cell surviving curves were obtained for murine melanoma Bl6 cell line using semiautomated M1T assay. 2,4,6,8, 10Gy were irradiated at a dose rate of 210cGy/min using /sup 60/Co Irradiator ALOORADO 8. After irradiatior, B16 cell lines(2.5×10⁴ cells/ml) were exposed to bleomycin and cisplatin at concentration of 0.2㎍/㎖, 2㎍/㎖ and 20㎍/㎖ for I hour respectively. The viable cells were determined for each radiation dose and/or each concentration of drug. And they were compared to control values. The obtained results were as follows : 1. There was significant difference of surviving fraction at 4, 6, 8, 10Gy on B16 cell line(P<0.05). 2. There was significant difference of cytotoxicity between bleomycin and cisplatin at concentration of 0.2㎍/㎖ and 2㎍/㎖(P<0.05) on B16 cell line, but there was no significant difference of cytotoxicity at concentration of 20㎍/㎖ on B16 cell line. 3. There was significant difference of cytotoxicity of bleomycin after irradiation of 2Gy and 10Gy on B16 cell line(P<0.01). 4. There was significant difference of cytotoxicity of cisplatin at concentration of 20㎍/㎖ after irradiation on B16 cell line.

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부궤환을 이용한 광대역 전력증폭기 설계 (The Design of Ultra-broadband Power Amplifier using a Negative Feedback)

  • 이한영;김대중
    • 전기학회논문지
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    • 제58권8호
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    • pp.1572-1579
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    • 2009
  • In this dissertation ultra-broadband power amplifier(UPA) was designed and fabricated using negative feedback technique. UPA was made of pre-amplifier, drive amplifier and power amplifier. Negative feedback technique was used to achieve ultra-broadband performance. Designed power amplifier has 30dB gain and 2W output power. The load-pull data of power amplifier for optimal power matching was extracted from the measured S-parameter. Fabricated PCB material, permittivity is 4.6 and thickness is 0.8mm, is FR4 and UPA was fabricated 3 modules for comparison of the simulated and measured results. Size of the fabricated pre-amplifier and drive amplifier module is 40mm'50mm'16mm. And from the experimental results, gain of the pre-amplifier module is 9.87dB at 2GHz and flatness is 0.63dB. Experimental result of the drive amplifier module is 10.97dB at 2GHz and flatness of that is 0.26dB. Test result of the power amplifier module is 10.71dB at 2GHz and flatness is 0.72dB. Total size of the power amplifier is 45mm'134mm'16mm. According to the test results, gain of the UPA is 28.98dB at 2GHz and flatness is 1.68dB. Output power was 32.098dBm at 2GHz, 32.154dBm at 1GHz and 31.273dBm at 100MHz.

소리의 종류와 크기에 따른 일과성 청력 역치 상승과 회복의 차이 (Differences in Temporary Threshold Shift and Recovery Patterns Depending on Sound Type and Pressure)

  • 이채관
    • 한국산업보건학회지
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    • 제30권4호
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    • pp.387-393
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    • 2020
  • Objective: This study aimed to investigate the differences in temporary threshold shift (TTS) and recovery patterns according to different types of sound and volume. Methods: TTS and recovery patterns were assessed for eight students after 30-minute exposure to both 70.0 dB and 90.0 dB of factory noise (noise) as well as music. TTS was measured before exposure and two minutes post exposure, and recovery patterns were evaluated every 10 minutes for one hour. The subjects performed activities of daily life and sleeping times as usual but taking drugs or drinking alcohol were prohibited. The experiment was repeated three times with an interval of at least 16 hours. ANOVA and T-test were carried out using SPSS 19.0 for Windows. Results: The hearing threshold of all subjects before exposure was less than 30 dB at all frequencies. Mean TTSs of 70 dB noise and 90 dB noise exposure were 0.14 and 4.48 dB (p<0.001). Meanwhile, the difference in music was insignificant (-0.63 dB and 0.55 dB, p=0.063). A significance in the difference was also found between the mean TTS of music and noise exposure, more obviously at 90.0 dB (p<0.001) than at 70 dB (p=0.232). The TTS differences were found frequency-wise in terms of sound type. Mean TTS by frequency was higher at 4,000 and 6,000 Hz than at other frequencies, and higher in noise than music at the same sound pressure. The TTS difference in each frequency between both sound types was significant at 90 dB (p<0.001). Subjects mostly recovered from TTS in one hour after exposure, but not with 90 dB-noise exposure. Conclusion: TTS and recovery patterns were different depending on the sound type. When exposed to factory noise, TTS was greater and recovery time was longer compared to music at the same sound pressure. These results suggested that the difference in cognitive processes and psychological factors according to the type of sound causes a change in TTS and recovery.

The Radiation Spot Size due to Wiggler Errors in a Free-Electron Laser Oscillator

  • Nam, Soon-Kwon;Park, Y.S.
    • Journal of the Korean Physical Society
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    • 제73권10호
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    • pp.1495-1501
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    • 2018
  • We have developed an extended three-dimensional free-electron laser (3D FEL) code with source-dependent expansion to calculate the intensity of the radiation field and the spot size in a free-electron laser oscillator. The effect of the wiggler field errors was evaluated for the case of a planar wiggler generated by a magnet stack with parabolic shaped pole faces by using the extended three-dimensional equations in a free-electron laser oscillator based on the proposed FEL facility which is to be operated in the far-infrared and the infrared regions. The radiation spot size due to the wiggler field errors also have been analyzed for wiggler errors of ${\Delta}B/B=0.0$, 0.03, 0.06 and 0.09% at z = 1 m and z = 2 m. The effect of the diffraction of radiation field due to the wiggler field errors of ${\Delta}B/B=0.0$ and ${\Delta}B/B=0.09%$ at 200 passes was evaluated by using the extended 3D code that we developed. The variation of the curvature of the phase front and the effect of the radiation field intensity due to the wiggler field errors were also evaluated for B = 0.5 T and B = 0.7 T with the wiggler error of ${\Delta}B/B=0.09%$ at 200 passes and the results were compared to those of without errors. The intensity of the radiation, behavior of the radiation spot size and the variation of the curvature of the phase were highly sensitive to the wiggler error of ${\Delta}B/B$ > 0.09%, but were less sensitive to the wiggler errors for ${\Delta}B/B$ < 0.09% in a free-electron laser (FEL) oscillator based on the proposed FEL facility.

멀티미디어용 고주파 Active Filter개발에 관한 연구 (Development of High Frequency Active Filter for Multimedia)

  • 윤종남
    • 마이크로전자및패키징학회지
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    • 제9권1호
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    • pp.1-7
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    • 2002
  • 본 연구에서는 이동통신 시스템의 키부품으로 필수적인 멀티미디어용 고주파 Active Filter 및 초소형 설계기술(SMD타입)을 개발하였으며, 멀티미디어 고주파 능동필터의 카오프 주파수는 2.5 mHz, 이득은100 kHz에서 0.5d B, 통과대역 리플은 100 kHz에서 2 MHz까지 최고1.2dB, GDT는 100 kHz에서 2.0 MHz까지 최고 60 nsec이며, 감쇄는 3.7 MHz에서 최소 40dB임.

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