본 연구는 반밀폐형 토마토 재배 온실에서 광합성율 극대화를 위한 적정 탄산가스 시비 농도를 구명하고자 광합성 모델을 이용하여 잎의 최대 카복실화율(Vcmax), 최대 전자전달속도(Jmax), 열파괴, 잎 호흡 등을 계산하고 실제 측정값과 비교하였다. 다양한 광도(PAR 200μmol·m -2 ·s -1 to 1500μmol·m -2 ·s -1 )와 온도(20°C to 35°C) 조건에서 CO2 농도에 대한 A-Ci curve는 광합성 측정 기기를 사용하여 측정하였고, 모델링 방정식으로 아레니우스 함수값 (Arrhenius function), 순광합성율(net CO2 assimilation, An), 열파괴(thermal breakdown), Rd(주간의 잎호흡)를 계산 하였다. 엽온이 30°C 이상으로 상승하였을 때 Jmax, An 및 thermal breakdown 예측치가 모두 감소하였고, 예측 Jmax의 가장 최고점은 엽온 30°C였으며 그 이상의 온도에서는 감소하였다. 생장점 아래 5번째 잎의 광합성율은 PAR 200－ 400μmol·m -2 ·s -1 수준에서는 CO2 600ppm, PAR 600－800μmol·m -2 ·s -1 수준에서는 CO2 800ppm, PAR 1000μmol·m -2 ·s -1 수 준에서는 CO2 1000ppm, PAR 1200－1500μmol·m -2 ·s -1 수준에서는 CO2 1500ppm을 공급했을 때 포화점에 도달하였다. 앞으로 광합성 모델식을 활용하여 과채류 온실 재배 시 광합성을 높일 수 있는 탄산시비 농도를 추정할 수 있을 것으로 판단된다.

The thermoelectric power and dc conductivity of La2/3+xTiO3-δ (x = 0, 0.13) were investigated. The thermoelectric power was negative between 80K and 300K. The measured thermoelectric power of x = 0.13 increased linearly with increased temperatures and was represented by S0+BT. The x = 0 sample exhibited insulating behavior, while the x = 0.13 sample showed metallic behavior. The electric resistivity of x = 0.13 had a linear temperature dependence at high temperatures and a T3/2 dependence below about 100K. On the other hand, the electric resistivity of x = 0 has a linear relation between lnρ/T and 1/T in the range of 200 to 300K, and the activation energy for small polaron hopping was 0.23 eV. The temperature dependence of thermoelectric power and the resistivity of x = 0 suggests that the charge carriers responsible for conduction are strongly localized. This temperature dependence indicates that the charge carrier (x = 0) is an adiabatic small polaron. These experimental results are interpreted in terms of spin (x = 0.13) and small polaron (x = 0) hopping of almost localized Ti 3d electrons.

Various assumptions used in interpreting the observations of hydrogen recombination lines are critically assessed to confirm the gradient of electron temperature with distance from the galactic center. The total temperature increase from 5 to 13 kpc is about 2,500 K. Among many suggestions, we have singled out the decrease of trace dement abundances with the galactoccntric distance as the most viable cause for the temperature gradient. This will impose an important constraint on evolutionary models of the Galaxy.