조사후 핵연료 가열(PIA장비)를 이용한 고연소도 UO2 사용후 핵연료의 산화 및 가열후 미세조직의 변화를 관찰하였다. 울진 2호기에서 한국원자력연구소 조사후시험시설로 이송된 국산 경수로용 고연소도 사용후 핵연료는 봉평균 연소도가 57,000 MWd/tU-rod avg.이였다. 본 시험에 사용된 시편은 국부연소도 65,000 MWd/tU UO2 소결체의 고형체 200 mg을 사용하였다. 본 시편을 사용후 핵 연료 가열(PIA) 시험장비를 이용하여 핫셀 내에서 3시간의 산화시험과 연속적으로 까지 가열하였다. 결정립경계까지의 산화를 위하여 에서 헬륨 50 ml, 표준공기 100 ml를 흔합한 산화분위기로 3시간을 유지하였다. 핵분열기체 방출거동을 알기위해 시험 전과정중에 85Kr의 방출량을 베타 측정기와 감마 측정기를 이용하여 실시간으로 측정 하였다. 가열시험이 종료된 후 전자주사현미경을 이용하여 미세구조의 변화를 관찰하였다. 시험결과 가열하는 동안 핵분열생성물은 UO2기지의 결정립경계와 표면으로 이동된 것을 관찰하였다. 이 시편은 환원과정을 통하여 재구조화 되었고, 정도의 결정립크기를 가진 것으로 나타났다.

The fragile X mental retardation (FMR) syndrome is the largest source of inherited mental retardation. The syndrome is usually caused by the transcriptional silencing of fragile X mental retardation gene (FMR-1). An 18 years old male wascompla띠ing of multiple toαh missing and abnormal facial profùe, of which signs were matemally dominant in his family. In the C)π。gene디c analysis the pa디ent and his parents did not show any discontinuity in the long arm end of X chromosome, but in the PCR produαs targeω19 the CGG repeat sequence in the 5' untranslated region of FMR gene both the patient'’ s and his mother' s gDNAs produced a normal and an extra bands, sized about 400 and 800 bps, respectively, while the his father' s gDNA produced only one normal band, sized about 400 bps. 까1US ， we suppose that the pa디.ent has heterozygotic alleles of FMR gene inherited matemally, and that the patient s FMR gene was in a premutated state relevant to the dentofacial abnormalities.

Data acquisition system mounted on the Solar Flare Telescope at Bohyunsan Optical Astronomy Observatory is briefly described. The system is made up with CCD cameras, an image processor, a PCI-type PC and a SUN workstation. The image processor, MVC 150/40 comprises a variable scan acquisition module, an image manager and a binary correlator computational module. A typical polarization image of a sunspot is presented to demonstrate performance of the system.

To derive coronal temperature, electron density and nonthermal velocity, we have analyzed high resolution spectra (e.g., Fe XII 338.3, Fe XII 352.1, Fe XIV 334.2, Fe XIV 353.8, Fe XV 284.2, Fe XV 321.8, Fe XV 327.0, Fe XVI 335.4, and Fe XVI 360.8) taken from AR 6615 by SERTS (Solar Extreme Ultraviolet Rocket Telescope and Spectrograph). Important findings emerging from the present study are as follows: (1) Temperature estimated from Fe XVI 335.4 and Fe XIV, 334.2 is ~2.4 × 106 K and no systematic difference in temperature is found between the active region and its adjacent quiet region; (2) Mean electron density estimated from Fe XV is ~3 × 109 cm -3 and ~10 10 cm-3 from Fe XII and Fe XIV; (3) Mean density of the active region is found to be higher than that of the quiet region by a factor of 2; (4) Nonthermal velocity estimated from Fe XV and Fe XVI is 20 ~ 25 km s-l which decreases with increasing ionization temperatures. This supports the notion that the nonthermal velocity declines outwards above the transition region.