Molecular cores of the high-latitude cloud MBM 40     

Young Chol Minh  Hyun-Goo Kim  Youngung Lee  Hyeran Park  Kwang-Tae Kim  Yong-Sun Park  Sang Joon Kim   《New Astronomy》2003,8(8):795-803

Towards the high-latitude cloud MBM 40, we identify 3 dense molecular cores of M0.2–0.5 M, and sizes of 0.2 pc in diameter embedded in the H I cloud of 8 M which is observed to be extended along the northeast–southwest direction. The molecular cloud is located almost perpendicularly to the H I emission. We confirm the previous result of Magnani et al. that MBM 40 is not a site for new star formations. We found a very poor correlation between the H I and the IRAS 100 μm emissions, but the CO (1–0) and 100 μm emissions show a better correlation of W_CO/I₁₀₀=1±0.2 K km s⁻¹ (MJy sr⁻¹)⁻¹. This ratio is larger by a factor of ≥5 than in dense dark clouds, which may indicate that the CO is less depleted in MBM 40 than in dense dark clouds.  相似文献   

Multiwavelength Study of a Solar Eruption from AR NOAA 11112 I. Flux Emergence, Sunspot Rotation and Triggering of a Solar Flare     

Pankaj Kumar  Sung-Hong Park  K.-S. Cho  S.-C. Bong 《Solar physics》2013,282(2):503-521

We analyze the multiwavelength observations of an M2.9/1N flare that occurred in the active region (AR) NOAA 11112 in the vicinity of a huge filament system on 16 October 2010. SDO/HMI magnetograms reveal the emergence of a bipole (within the existing AR) 50 hours prior to the flare event. During the emergence, both the positive and negative sunspots in the bipole show translational as well as rotational motion. The positive-polarity sunspot shows significant motion/rotation in the south-westward/clockwise direction, and we see continuously pushing/sliding of the surrounding opposite-polarity field region. On the other hand, the negative-polarity sunspot moves/rotates in the westward/anticlockwise direction. The positive-polarity sunspot rotates ≈?70^° within 30 hours, whereas the one with negative polarity rotates ≈?20^° within 10 hours. SDO/AIA 94 Å EUV images show the emergence of a flux tube in the corona, consistent with the emergence of the bipole in HMI. The footpoints of the flux tube were anchored in the emerging bipole. The initial brightening starts at one of the footpoints (western) of the emerging loop system, where the positive-polarity sunspot pushes/slides towards a nearby negative-polarity field region. A high speed plasmoid ejection (speed ≈?1197 km?s^?1) was observed during the impulsive phase of the flare, which suggests magnetic reconnection of the emerging positive-polarity sunspot with the surrounding opposite-polarity field region. The entire AR shows positive-helicity injection before the flare event. Moreover, the newly emerging bipole reveals the signature of a negative (left-handed) helicity. These observations provide unique evidence of the emergence of twisted flux tubes from below the photosphere to coronal heights, triggering a flare mainly due to the interaction between the emerging positive-polarity sunspot and a nearby negative-polarity sunspot by the shearing motion of the emerging positive sunspot towards the negative one. Our observations also strongly support the idea that the rotation can most likely be attributed to the emergence of twisted magnetic fields, as proposed by recent models.  相似文献   

Effects of Green Light on the Stress Response of Olive Flounder Paralichthys olivaceus under Clove Oil Anesthesia     

Choi  Cheol Young  Song  Jin Ah  Park  Young-Su 《Ocean Science Journal》2021,56(1):78-85

Ocean Science Journal - Clove oil (CO) is an effective anesthetic. Many hatcheries and research studies use clove oil to immobilize fish for artificial reproduction and surgery to suppress their...  相似文献   

Late quaternary paleoceanographic changes in the northeastern Ulleung Basin, East Sea, inferred from variations in biogenic components     

Yeon Jee Suh  Sangmin Hyun  Chanhong Park 《Ocean Science Journal》2013,48(3):289-300

Two piston cores (DD09-ST21, DD09-ST39B) from the northeastern Ulleung Basin in the East Sea were obtained to investigate variations in the biogenic components (calcium carbonate, organic carbon) and biogeochemical processes (δ¹³C and δ¹⁵N). The two cores had distinctive characteristics in terms of surface production, preservation and dissolution capacity of carbonate, and redox conditions of bottom-water. Core DD09-ST21 was characterized by an oxygen-depleted condition from 15 ka (MIS 2) to 60 ka (MIS 3). Core DD09-ST39B, on the other hand, showed oxic bottom-water conditions, possibly due to shallow water depth. These two cores with different redox condition showed opposite trends in terms of CaCO₃, TOC, and C₃₇ alkenone concentrations. CaCO₃ and C₃₇ concentrations were higher during the LGM in DD09-ST21 while lower contents were observed in DD09-ST39B in the same period. Moreover, consistently low TOC in DD09-ST39B and higher fluctuation of organic matters in DD09-ST21 may suggest difference in primary productivity, preservation capacity, or a potential dissolution effect. During the Holocene, the surface productivity of both cores increased, probably due to renewed ventilation and vertical mixing in the East Sea. Therefore, this study suggests spatial variation in production and preservation of biogenic components in the two cores since last 50 ka for DD09-ST39B and 80 ka for DD09-ST21 due to difference in environmental conditions such as water depth, bottom-water conditions, surface productivity and preservation.  相似文献   

Site-specific success of three transplanting methods and the effect of planting time on the establishment of Zostera marina transplants     

Park JI  Lee KS 《Marine pollution bulletin》2007,54(8):1238-1248

Eelgrass, Zostera marina, is the most abundant seagrass species on the coast of Korea, but most large eelgrass meadows have disappeared since the 1970s due to human-induced disturbance. To restore disturbed seagrass habitats in die-off areas, seagrass transplanting has been attempted using various methods. Here, we assessed the feasibility and efficiency of seagrass transplanting methods depending on the sediment type at the planting site. Additionally, the effect of planting time on the establishment of transplant was examined to determine the optimal season for planting. We conducted an eelgrass transplanting experiment from fall 2003 to summer 2004 at three sites with different sediment types using three planting techniques. The staple method resulted in the highest transplant survival rate (77.1-93.8%) at all three sites, but was labor intensive. Transplanting Eelgrass Remotely with Frame Systems (TERFS) method also resulted in relatively a high survival rate (58.7-69.0%) at all sites. The shell method is a newer eelgrass transplanting method in which oyster shells are used as an anchoring device, and does not require SCUBA diving for subtidal transplanting. The shell method resulted in high survival rates in muddy (81.3%) and silty sediments (76.5%), but remarkably low survival rate in sandy sediments (5.0%). The TERFS, and shell methods reduced underwater labor; thus, these methods is suitable for large-scale seagrass restoration. Eelgrass transplants planted in summer had exhibited significant mortality due to high summer water temperatures. Although transplants planted in fall to spring had relatively high survival rates, transplanting and collection of vegetative shoots are difficult in winter and spring. Therefore, fall was suggested as the most effective transplanting season off the coast of Korea.  相似文献   

Astrophysically relevant radiation hydrodynamics experiment at the National Ignition Facility     

C. C. Kuranz  H.-S. Park  B. A. Remington  R. P. Drake  A. R. Miles  H. F. Robey  J. D. Kilkenny  C. J. Keane  D. H. Kalantar  C. M. Huntington  C. M. Krauland  E. C. Harding  M. J. Grosskopf  D. C. Marion  F. W. Doss  E. Myra  B. Maddox  B. Young  J. L. Kline  G. Kyrala  T. Plewa  J. C. Wheeler  W. D. Arnett  R. J. Wallace  E. Giraldez  A. Nikroo 《Astrophysics and Space Science》2011,336(1):207-211

The National Ignition Facility (NIF) is capable of creating new and novel high-energy-density (HED) systems relevant to astrophysics. Specifically, a system could be created that studies the effects of a radiative shock on a hydrodynamically unstable interface. These dynamics would be relevant to the early evolution after a core-collapse supernova of a red supergiant star. Prior to NIF, no HED facility had enough energy to perform this kind of experiment. The experimental target will include a 340 ??m predominantly plastic ablator followed by a low-density SiO₂ foam. The interface will have a specific, machined pattern that will seed hydrodynamic instabilities. The growth of the instabilities in a radiation-dominated environment will be observed. This experiment requires a ??300?eV hohlraum drive and will be diagnosed using point projection pinhole radiography, which have both been recently demonstrated on NIF.  相似文献   

Establishing boundary classes for the classification of UK marine waters using phytoplankton communities   总被引：2，自引：0，他引：2  

Devlin M  Best M  Coates D  Bresnan E  O'Boyle S  Park R  Silke J  Cusack C  Skeats J 《Marine pollution bulletin》2007,55(1-6):91-103

  相似文献   

Optimization of operational parameters for ethanol production from Korean food waste leachate   总被引：2，自引：2，他引：0  

H. Le Man M. Sc.  S. K. Behera  H. S. Park Ph.D. P.E. 《International Journal of Environmental Science and Technology》2010,7(1):157-164

Recently, research on the production of ethanol from waste has been accelerating for both ecological and economical reasons, primarily for its use as an alternative to petroleum based fuels. In this study, response surface methodology based 2³ -full factorial central composite design was employed to optimize the parameters of ethanol production from Korean food waste leachate. The reducing sugar concentration of the food waste leachate determined by the dinitrosalicylic acid method was 75 g/L. A second order polynomial model was developed to evaluate the quantitative effects of temperature, pH and reducing sugar concentration in order to find an optimum condition for the ethanol production from food waste leachate. From the experimental result, maximum ethanol concentration of 24.17 g/L was obtained at the optimum condition of temperature (38 °C), pH (5.45) and reducing sugar concentration (75 g/L). The experimental value (24.17 g/L) agreed very well with the predicted one (23.66 g/L), indicating the suitability of the model employed and the success of response surface methodology in optimizing the conditions of ethanol production from food waste leachate. Canonical analysis indicated that the stationary point was a saddle point for the ethanol yield. Despite being a waste, an ethanol yield of 0.32 g ethanol/g reducing sugar demonstrated the potential of food waste leachate as a promising biomass resource for the production of ethanol.  相似文献   

Clockwise rotations recorded in Early Cretaceous rocks of South Korea: implications for tectonic affinity between the Korean Peninsula and North China   总被引：12，自引：0，他引：12  

Xixi Zhao  Robert S. Coe  Ki-Hong Chang  Soon-Ok Park  Sheraz K. Omarzai  Rixiang Zhu  Yaoxiu Zhou  Stuart Gilder  & Zhong Zheng 《Geophysical Journal International》1999,139(2):447-463

Recent interest has focused on whether South Korea may have undergone variable tectonic rotations since the Cretaceous. In an effort to contribute to the answer to this question, we have completed a palaeomagnetic reconnaissance study of Early Cretaceous sedimentary and igneous rocks from the Kyongsang basin in southeast Korea. Stepwise thermal demagnetization isolated well-defined characteristic magnetization in all samples. The palaeomagnetic directions reveal patterns of increasing amounts of clockwise (CW) rotation with increasing age for Aptian rock units. Palaeomagnetic declinations indicate clockwise vertical-axis rotations of R = 34.3° ± 6.9° for the early Aptian rock unit, R = 24.9° ± 10.6° for the middle Aptian, and R = −0.9° ± 11.8° for the late Aptian relative to eastern Asia. The new Cretaceous palaeomagnetic data from this study are consistent with the hypothesis that Korea and other major parts of eastern Asia occupied the same relative positions in terms of palaeolatitudes in the Cretaceous. An analysis of and comparison with previously reported palaeomagnetic data corroborates this hypothesis and suggests that much of Korea may have been connected to the North China Block since the early Palaeozoic. A plausible cause of the rotation is the westward subduction of the Kula plate underneath the Asian continent, which is inferred to have occurred during the Cretaceous according to several geological and tectonic analyses.  相似文献   

Distribution of caustic-crossing intervals for Galactic binary-lens microlensing events     

Cheongho Han  Seong-Hong Park  Yong-Sam Lee 《Monthly notices of the Royal Astronomical Society》2000,314(1):59-64

Detection of caustic crossings of binary-lens gravitational microlensing events is important because by detecting them one can obtain useful information about both the lens and the source star. In this paper, we compute the distribution of the intervals between two successive caustic crossings, f ( t _cc), for Galactic bulge binary-lens events to investigate the observational strategy for the optimal detection and resolution of caustic crossings. From this computation, we find that the distribution is highly skewed towards short t _cc and peaks at t _cc∼1.5 d. For the maximal detection of caustic crossings, therefore, prompt initiation of follow-up observations for intensive monitoring of events will be important. We estimate that, under the strategy of the current follow-up observations with a second caustic-crossing preparation time of ∼2 d, the fraction of events with resolvable caustic crossing is ∼80 per cent. We find that if the follow-up observations can be initiated within 1 d after the first caustic crossing by adopting more aggressive observational strategies, the detection rate can be improved to ∼90 per cent.  相似文献