• 대한기계학회논문집B
• /
• 제37권9호
• /
• pp.829-836
• /
• 2013

석탄을 개질한 합성천연가스의 조성에 변화가 있을 경우 화염의 연소특성에 대하여 연구하였다. 본 연구의 목적은 동축 공기 합성천연가스 확산화염을 구현하여 연료조성에 따른 화염안정성과 화염구조, 분광특성, 온도분포를 실험적인 방법으로 연구하는 것이다. 각 화염의 분광특성을 관찰하기 위하여 분광기를 사용하였으며 연소장 내 온도측정을 위하여 K 형 열전대를 사용하였다. 연료 분사기 출구속도는 $u_F$ =5~40 m/s 사이에서 조절하였고 공기 분사기 출구속도는 $u_A$ =0~0.43 m/s 사이에서 조절하였다. 연소 동특성에 대한 실험을 통해 합성천연가스에 수소 성분이 증가하면 화염안정화 영역이 증가하고 부상화염 높이가 낮아져 화염길이가 짧아지는 것을 알 수 있었다.

• Journal of Advanced Marine Engineering and Technology
• /
• 제35권2호
• /
• pp.204-215
• /
• 2011

화염 안정성은 층류부상화염의 중요한 메커니즘 중 하나이며 화염전파속도는 화염안정화를 평가하기 위한 척도가 된다. Bilger는 삼지점을 기준으로 혼합분율과 화염의 형상에 관계된 삼지화염의 화염 전파속도 및 안정화 메키니즘을 제시하였다. 그러나 동축류 작은 노즐을 이용한 실험과 수치해석에서는 화염이 형성되고 소화되는 전 과정을 상세히 관찰 할 수는 없었다. 본 논문에서는 노즐 직경에 따른 화염거동과 화염 형상 및 안정화 메커니즘에 대하여 세분화하였다. 본 논문의 결과로 노즐에 따른 삼지화염의 거동과 삼지화염전파, 화염면 전파 및 평면화염의 존재 등을 구분하였다. 그리고 삼지화염전파 거동에 있어서 열린삼지화염전파 및 닫힌 삼지화염전파 거동에 대해 구분하였다.

• 천문학회지
• /
• 제48권2호
• /
• pp.113-123
• /
• 2015

We present observational results from optical long-slit spectroscopy of parsec-scale jets of DG Tau. From HH 158 and HH 702, the optical emission lines of Hα, [O i] λλ6300, 6363, [N ii] λλ6548, 6584, and [S ii] λλ6716, 6731 are obtained. The kinematics and physical properties (i.e., electron density, electron temperature, ionization fraction, and mass-loss rate) are investigated along the blueshifted jet up to 650′′ distance from the source. For HH 158, the radial velocity ranges from −50 to −250 km s⁻¹. The proper motion of the knots is 0.′′196 − 0.′′272 yr⁻¹. The electron density is ∼10⁴ cm⁻³ close to the star, and decreases to ∼10² cm⁻³ at 14′′ away from the star. Ionization fraction indicates that the gas is almost neutral in the vicinity of the source. It increases up to over 0.4 along the distance. HH 702 is located at 650′′ from the source. It shows ∼ −80 km s⁻¹ in the radial velocity. Its line ratios are similar to those at knot C of HH 158. The mass-loss rate is estimated to be about ∼ 10⁻⁷ M_⊙ yr⁻¹, which is similar to values obtained from previous studies.

• 천문학회보
• /
• 제36권2호
• /
• pp.115.1-115.1
• /
• 2011

We analyzed the line profiles of the planetary nebula (PN) NGC 7009 secured with the Keck I HIES and BOES's spectral data. The 5 positions were taken over the nebular image, 4 points on the bright rim plus 1 point at the central position. The covered spectral wavelength range was $3250{\AA}-8725{\AA}$ in these observations. We decomposed the lines of HI, HeI, HeII, CII, NIII, [ClIII], [NII], [OII], [OIII], [SII], [SIII], [ClIII], and [ArIII] using the IRAF and StarLink/Dipso. After correcting the Earth's movement and the PN's radial velocities, -48.6 & -48.9 km/s, respectively, for the Keck & BOES, we produced the line profiles in a velocity scale. The zero velocity at each line profile clearly indicates which part of the components is approaching or receding, giving a general information of the kinematical structure. Almost all of the low-to-medium excitation lines, such as [NII], [SII], [O III], and [ArIII], secured at the central position and four positions along the major & minor axes, showed 3 components, double peak + a wide wing component, suggesting the fast outflow structures are present. The overall geometry is a prolate shell which also has a fainter outer shell in the halo zone, but there appears to be some peculiar sub-structures inside the main shell. The high excitation He I, HeII, NIII lines which might be formed close to the inner boundary of the shell show unusual features, completely different from the other lines. The HeII and these high excitation lines may be indicative of a relative recent fast outflow from the central star and the permitted lines such as NIII might be affected by the innermost structure. We discuss a possible presence of a jet-like fast outflow structure in an out-flow axis different from the main axis of the spheroid shell.

• 한국항해항만학회:학술대회논문집
• /
• 한국항해항만학회 2006년도 추계학술대회 논문집(제1권)
• /
• pp.45-49
• /
• 2006

물분사장치가 부착된 NACA-0021 익 주변의 흐름을 입자영상유속계를 이용하여 고찰하였다. $R_w=6.0261{\times}10^4$에서 영각(a)을 $0^{\circ}{\sim}35^{\circ}$로 변화시켜가며, 물분사 속도를 0[m/s], 9.2[m/s]의 2가지로 조절한 결과 익 후류영역에서는 박리 후 비정상적인(unsteady) 재순환 ${\cdot}$ 재부착 영역이 형성되었으며, 박리영역의 폭이 콴다 효과(Coanda effect)를 갖는 물분사로 인하여 최대 1/3만큼 감소하는 경향을 확인하였다. ?Nㄴ사가 없는 조건에서의 박리는 영각(a) $17^{\circ}{\sim}18^{\circ}$ 부근에서 시작되는 것이 관측되었으나, 물분사를 시켰을 경우 $20^{\circ}{\sim}21^{\circ}$에서 박리가 시작되는 것을 유동관측을 통해 알 수 있었다. 유동계측을 통해 익의 후연부(trailing edge)에서 생성되었던 와(vortex, eddy)가 물제트분사로 인해 소멸되는 것을 알 수 있었고, 영각이 작고 물분사 유속이 빠를수록 박리영역의 감소가 더욱 가속화됨을 알 수 있었다.

• 대한의용생체공학회:의공학회지
• /
• 제24권1호
• /
• pp.37-44
• /
• 2003

본 실험연구에서는 정상유동상태에서 새롭게 설계된 자가팽창성 그래프트 스텐트의 수력학적 성능을 평가하고자 하였다. 코팅 재질이 다른 두 개의 그래프트 스텐트와 한 개의 타이티놀 금속스텐트가 실험에 사용되었으며, 유량이 가자 5, 10, 15 1/min에서 스텐트 전후에서의 압력변화 및 속도분포를 측정하였다. 스텐트 삽입에 의한 압력손실은 유량이 증가함에 지수적으로 증가하였다. 특히 15 1/min의 유량에서 다공성 PTFE 그래프트 스텐트와 TiNi 금속스텐트의 압력손실은 거의 동일하나 PU 그래프트 스텐트는 약 6배 이상의 현저한 증가를 보이고 있다. 스텐트 후류에서의 속도분포는 다공성 PTFE 그래프트 스텐트와 TiNi 금속스텐트는 유량에 관계없이 유사한 형태를 보여주고 있다. 그러나, PU 그래프트 스텐트에서는 특히 유량이 10 1/min 이상에서 속도분포가 비대칭적이고 관 중심에서의 상대적인 낮은 유속을 보여주고 있으며, 결과적으로 벽면전단응력 및 수직응력의 증가론 초래하고 있다. 이와같이 PU 그래프트 스텐트의 상대적으로 낮은 수력학적 성능은 스텐트가 보다 작은 관에 삽입되었을때 코팅재질의 낮은 유연성으로 인하여 스텐트의 표면에 주름이 발생하여 유동단면이 비대칭적으로 되고 벽면의 조도가 증가하며, 관벽과 스텐트와 틈새가 존재하여 제트류가 형성되기 때문으로 해석된다.

• 한국연소학회:학술대회논문집
• /
• 한국연소학회 제26회 KOSCO SYMPOSIUM 논문집
• /
• pp.159-165
• /
• 2003

Self-excited noise generation from laminar flames in thin annular jets of methane/air premixture has been investigated experimentally. Various flames were observed in this flow configuration, including conical shape flames, ring shape flames, steady crown shape flames, and oscillating crown shape flames. Self-excited noise with the total sound pressure level of about 70dB was generated from the oscillating crown shape flames for the equivalence ratio larger than 0.95. Sound pressure and $CH^{\ast}$ chemiluminescence were measured by using a microphone and a photomultiplier tube. The frequency of generated noise was measured as functions of equivalence ratio and premixture velocity. A frequency doubling phenomena have also been observed. The measured $CH^{\ast}$ chemiluminescence data were analyzed from which the corresponding sound pressure has been calculated. By comparing the data with those of measured ones, the noise source can be attributed to the flame front fluctuation near the edge of the oscillating crown-shape flames. The flame stability regime was influenced sensitively to the supplying air through the inner tube.

• 한국연소학회:학술대회논문집
• /
• 한국연소학회 제26회 KOSCO SYMPOSIUM 논문집
• /
• pp.93-101
• /
• 2003

The extinction of unsteady diffusion flame was experimentally studied in an opposing jet counterflow burner using diluted methane. The stabilized flame was perturbed by linearly varying velocity change that was generated by pistons installed on both sides of the air and fuel stream. As the results, the extinction of unsteady flame is dependent not only on the history of unsteadiness, but also on the initial condition. We found that there are several unsteady effects on the flame extinction. First, the extinction strain rates of unsteady cases are extended well beyond steady state extinction limits. Second, as the slope of the strain rate change increases, the unsteady extinction strain rate becomes larger. Third, the extension of unsteady extinction strain rate becomes smaller as the initial strain rate increases. We also found that the extension of the extinction limit mainly results from the unsteady response of the reaction zone because there is no retardation effect of a mixing layer for our experimental condition.

• 한국가시화정보학회지
• /
• 제9권4호
• /
• pp.47-53
• /
• 2011

A water driven ejector loop was designed and constructed for air absorption. The used ejector was horizontally installed in the loop and annular water jet at the throat entrained air through the circular pipe placed at the center of the ejector. Wide range of water flow rate was provided using two kinds of pumps in the loop. The tested range of water flow rate was 100${\ell}$ /min to 1,000 ${\ell}$/min. Two-phase flow inside the ejector loop was simulated by CFD analysis. Homogeneous particle model was used for void fraction prediction. Water and air flow rates and pressure drop through the ejector were automatically recorded by using the LabView based data acquisition system. Flow characteristics and air bubble velocity field downstream of the ejector were investigated by two-phase flow visualization and PIV measurement based on bubble shadow images. Overall performance of the two-phase ejector predicted by the CFD simulation agrees well with that of the experiment.

• 대한기계학회논문집B
• /
• 제21권7호
• /
• pp.841-848
• /
• 1997

Combustion of gaseous fuel combustor in a high temperature vitiated air stream was studied with computer simulation. It is for application to afterburner of gas turbine engine which the exact mechanism is not yet clarified. As the jet velocity from fuel nozzle is very high and the geometry of combustor is three dimensional complex structure, many time and money are required to have good results. To consider this demerit, it is simplified to 2-dimensional and modified with the nozzle hole area to same area of annual status. As the thickness of annual is too thin, it is to divide with the many grids for reasonable results. Accordingly, new method which injected fuel mass, momentum and energy are added to source terms of each governing conservation equation as a source terms is introduced like as two phase analysis. Reaction rate is determined by taking into account the Arrhenius reaction based on a single step reaction mechanism. It is focused to temperature and product concentration distribution at each equivalence ratio of inlet hot product.