먼지응애류인 벼먼지응애(신칭, Steneotarsonemus spinki Smiely 1967)는 쌀생산국인 태국, 필리핀, 중국, 대만 등에서 쌀의 중요한 해충이다. S. spinki가 국내에서 처음으로 환경조절온실에서 재배중인 쌀에서 발견되었다. 응애 피해를 입은 쌀은 이삭에서 기형을 나타내었으며 잎집내부 표면의 갈변증상, 쌀알의 표면 갈변증상 등을 나타내었다. S. spinki암컷의 체장은 263.0(246.5~12.2), 체폭은(79.5~7.6)였으며 전체적인 모양은 난형으로 중앙부위가 가장 폭이 넓었다. 채색은 연한 황색이었다. 다리는 잘 발달되어 있었으며 암컷 제4각 끝은 채찍모양의 강모로 이루어진 전형적인 먼지응애류의 특징을 가지고 있었다. 수컷 체장은 196.5(176.5~222.815.8), 체폭은 109.3 98.6~6.4)였으며 전체적인 모양은 길쭉하고 전동체부 중앙부가 가장 체폭이 넓었다. 내돌기 III은 내돌기 IV보다 전방으로 신장되어 있었다. 제4각퇴절은 커다란 안쪽귀가 발달되어 있었으며 안쪽 및 바깥쪽 강모는 같은 길이로 짧게 잘 발달되어 있었다. 부절 발톱은 강하고 복부쪽으로 굽어 있었다
In this study we present a new improved nonlinear calibration method for vector magnetograms made by the Solar Flare Telescope of BOAO. To identify Fe I 6302.5 line, we have scanned monochromatic images of the line integrated over filter passband, changing the location of the central transmission wavelength of a Lyot filter. Then we obtained a filter-convolved line profile, which is in good agreement with spectral atlas data provided by the Sacramento Peak Solar Observatory. The line profile has been used to derive calibration coefficients of longitudinal and transverse fields, employing the conventional line slope method under the weak field approximation. Our improved nonlinear calibration method has also been used to calculate theoretical Stokes polarization signals with various angles of inclination of magnetic fields. For its numerical test, we have compared input magnetic fields with the calibrated ones, which have been derived from the new improved non-linear method and the conventional method respectively. The numerical test shows that the calibrated fields obtained from the improved method are consistent with the input fields, but not with those from the conventional method. Finally, we applied our new improved method to a dipole model which characterizes a typical field configuration of a single, round sunspot. It is noted that the conventional method remarkably underestimates the transverse field component near the inner penumbra.
This paper is aimed to study the computer simulation of sintering process for ceramics by Monte Carlo and molecular dynamics methods. Plural mechanisms of mass transfer were designed in the MC simulation of sintering process for micron size particles; the transfer of pore lattices for shrinkage and the transfer of solid lattices for grain growth ran in the calculation arrays. The MD simulation was performed in the case of nano size particles of ionic ceramics and showed the characteristic features in sintering process at atomic levels. The MC and MD simulations for sintering process are useful for microstructural design for ceramics.