We have made a comprehensive statistical study on the coronal mass ejections(CMEs) associated with helmet streamers. A total number of 3810 CMEs observed by SOHO/LASCO coronagraph from 1996 to 2000 have been visually inspected. By comparing their LASCO images and running difference images, we picked out streamer-associated CMEs, which are classified into two sub-groups: Class-A events whose morphological shape seen in the LASCO running difference image is quite similar to that of the pre-existing streamer, and Class-B events whose ejections occurred in a part of the streamer. The former type of CME may be caused by the destabilization of the helmet streamer and the latter type of CME may be related to the eruption of a filament underlying the helmet streamer or narrow CMEs such as streamer puffs. We have examined the distributions of CME speed and acceleration for both classes as well as the correlation between their speed and acceleration. The major results from these investigations are as follows. First, about a quarter of all CMEs are streamer-associated CMEs. Second, their mean speed is 413 km s-1 for Class-A events and 371 km s-1 for Class-B events. And the fraction of the streamer-associated CMEs decreases with speed. Third, the speed-acceleration diagrams show that there are no correlations between two quantities for both classes and the accelerations are nearly symmetric with respect to zero acceleration line. Fourth, their mean angular width are about 60°, which is similar to that of normal CMEs. Fifth, the fraction of streamer-associated CMEs during the solar minimum is a little larger than that during the solar maximum. Our results show that the kinematic characteristics of streamer-associated CMEs, especially Class-A events, are quite similar to those of quiescent filament-associated CMEs.

In the present study, we investigated the effects of genotypes on in vitro maturation and fertilization in porcine fresh/frozen-thawed oocytes. The porcine cumulus-oocyte complexes (COCs) were divided into four groups according to whether they were: (1) in vitro matured; (2) cryopreserved and in vitro matured; (3) in vitro fertilized and (4) cryopreserved, and in vitro fertilized. Maturation of porcine COCs was accomplished by incubation in NCSU23 medium. Immature oocytes were cryopreserved by Open Pulled Straws (OPS) method according to Vajta et al., (1998). Oocytes stained by Acetic-Orcein method were observed under the microscope. DNA extracted from the ovaries was analyzed by RAPD (random amplified polymorphic DNA) and SSCP (single strand conformational polymorphisrrt) method. The rates of oocytes maturation and fertilization were significantly high in AA genotype. The results indicated that in vitro maturation and fertilization in porcine fresh/frozen-thawed oocytes may be affected by genotypes in pigs.

본 연구는 한우 난포란이 체외성숙된 환경의 변화를 단백질 측면으로부터 검토하기 위하여 체외성숙 배지와 세포질내 단백질 변화와 종류를 검토하였다. 그 결과 배지 내의 단백질 발현량은 배양 4.5시간째까지 감소하였고, 배양 13.5시간째까지는 변화가 없었다. 그러나 배양 13.5~18시간 사이에 증가한 후 배양 18시간 이후에 다시 감소하는 경향이었다. 세포질내의 단백질 발현량은 배양 4.5시간째까지 증가하였고 배양 9시간째까지 급격히 감소하였다. 배양 9시간째부터 18시간째 까지는 단백질 발현량이 유사한 경향이었으나 배양 18시간째부터 24시간째까지 다시 증가하였다. 한편 체외성숙한 배지와 세포질을 2차원 전기영동하여 각각 298개 및 35개의 단백질 spot을 확인하였고, 그 중 배지에서는 28개, 세포질에서는 5개의 spot이 유의적인 변화를 확인하였다. 이들 spot 대한MALDI-TOP분석으로 배지와 세포질에서 각각 8개 및 1개의 단백질을 동정하였다. 그 종류는 aldose reductase, alpha enolase, apolipoprotein A-1 precursor, 43M1a collectin precursor, heat shock 27kDa protein, plasminogen activator inhibitor-1 precursor, thrombospondin 1 transitional endoplasmic reticulum ATPase 및 β-tubulin이었다.

본 연구에서는 배양 체계(혈청 첨가 TCM199, TALP, CRlaa 및 혈청 미첨가; IVMD101, IVF100, IVMD101)가 체외수정 또는 미세주입된 수정란의 체외 발달에 미치는 효과를 검토하였다. 또한 미세주입에 사용하는 GFP유전자의 양 및 미세주입 수정란에서 형광발현 양상을 검토하였다. 체외수정된 수정란의 ≥2세포기, 8세포기 및 배반포 도달율이 미세주입 수정란에 비하여 유의하게 높았다. 혈청 미첨가 배지에서의 8세포기 발달율이 수정란의 종류에 관계없이 유의하게 높았으나(p<0.05; 3.3% vs. 15.5% 및 21.4% vs. 39.4%, respectively), 배반포 도달율은 유사한 경향이었다(2.7% vs. 2.3% 및 23.0% vs. 23.6%, respectively). 한편, 2ng/uL 유전자를 미세주입한 수정란의 ≥2세포기, 8세포기 및 배반포 도달율이 4 및 8ng/uL의 것에 비하여 높은 경향이었다. 미세주입 수정란의 형광발현율은 1세포기가2및 8세포기에 비하여 유의하게 높았으나(p<0.05), 4세포기 및 배반포 단계와는 차이가 없었다.

X-ray plasma ejections often occurred around the impulsive phases of solar flares and have been well observed by the SXT aboard Yohkoh. Though the X-ray plasma ejections show various morphological shapes, there has been no attempt at classifying the morphological groups for a large sample of the X-ray plasma ejections. In this study, we have classified 137 X-ray plasma ejections according to their shape for the first time. Our classification criteria are as follows: (1) a loop type shows ejecting plasma with the shape of loops, (2) a spray type has a continuous stream of plasma without showing any typical shape, (3) a jet type shows collimated motions of plasma, (4) a confined ejection shows limited motions of plasma near a flaring site. As a result, we classified the flare-associated X-ray plasma ejections into five groups as follows: loop-type (60 events), spray-type (40 events), jet-type (11 events), confined ejection (18 events), and others (8 events). As an illustration, we presented time sequence images of several typical events to discuss their morphological characteristics, speed, CME association, and magnetic field configuration. We found that the jet-type events tend to have higher speeds and better association with CMEs than those of the loop-type events. It is also found that the CME association (11/11) of the jet-type events is much higher than that (5/18) of the confined ejections. These facts imply that the physical characteristics of the X-ray plasma ejections are closely associated with magnetic field configurations near the reconnection regions.