• International Journal of Oral Biology
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• 제41권2호
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• pp.63-68
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• 2016

The aim of this study was to investigate the effect of n-3 polyunsaturated fatty acids (PUFAs) on eruptive movement during tooth development. Sprague-Dawley (SD) rat pups were randomly divided into two groups; control group and experimental group. The experimental group was administered daily with n-3 PUFA by intraperitoneal (IP) injection. After 10 days postpartum, rat pups were sacrificed to evaluate the effect of n-3 PUFA on eruptive tooth movement. Histological analyses were by hematoxylin-eosin (H&E) staining. Tartrate-resistant acid phosphatase (TRAP) assay was performed to compare the osteoclast distribution in the bone matrix above the developing molar teeth. Incisor teeth eruptions were noticeably observed in IP group, as compared to control group. Rat pups in IP group showed faster tooth eruption on day 8 after birth. Through histological analyses, IP group showed thinner bone matrix and more osteoclasts above the $1^{st}$ molar teeth, as compared to control group. TRAP assay showed significantly stronger stained pattern that the osteoclast above the $1^{st}$ molar teeth in IP group, as compared to control group. The results suggested that n-3 PUFA could affect osteoclastic activity involved in bony remodeling during eruptive tooth movement.

• 대한원격탐사학회지
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• 제34권6_4호
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• pp.1545-1553
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• 2018

2018년 4월 말부터 감지되기 시작한 킬라우에아 화산의 최근 마그마 분화 활동은, 5월과 6월에 걸쳐 용암의 분출과 함께 급격한 지표 변형을 발생시켰다. 킬라우에아 정상부에 위치한 Halema'uma'u 분화구에서는 용암호의 수위가 빠르게 하강하여 대규모 지반 침하 및 지반 붕괴가 나타났으며, GPS와 경사계의 기록을 통해 약 2미터 가량의 변화를 감지할 수 있었다. 이 연구에서는 단 기간에 큰 변화를 보인 킬라우에아 분화 활동의 초기과정에 대해 다중 시기 COSMO-SkyMed SAR 영상을 이용한 시계열 지표변위 분석을 수행하고자 하였다. 전체 관측기간에 대해 측정된 최대의 지표 변위는 위성의 관측방향으로 약 -1.5미터이며, 입사각을 고려하여 수직변위로 변환할 때 약 -1.9미터의 침하를 나타낸다. 또한 대부분의 지표 변위는 분화 직후인 5월 초에서 6월말 사이에 발생하며, 7월부터는 안정기에 들어선 것을 확인할 수 있다. 시계열 지표변위를 통해 마그마 소스 모델링을 실시한 결과, 마그마 챔버가 지표로부터 2-3 km 사이에 위치하는 것으로 산출되었으며, 마그마 소스의 중심 위치는 남서부 방향으로 이동하는 것으로 관측되었다. 이러한 마그마 모델의 시계열 변화는 편향된 관측자료를 통한 초기 결과이므로 이후의 연구에서 정밀한 3차원 관측을 이용한 보완이 필요할 것으로 보여진다.

• 자원환경지질
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• 제26권1호
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• pp.55-65
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• 1993

Udo Island, some 3 km off the coast of Sungsan Peninsula at the eastern promontory of Cheju Island, occurs in such a regular pattern on the sequences which reprent an excellent example of an eruptive cycle. The island comprises a horseshoe-shaped tuff cone, a nested cinder cone on the crater floor, and a lava delta which extends over northwest from the moat between two cones. The volcanic sequences suggest volcanic processes that start with emergent Surtseyan eruption, progress through Strombolian eruption and end with lava effusion followed by reworking of smooth tephra on the tuff cone. Eruptive environment and hydrology of vent area in the Udo tuff cone are poorly constrained because the stratigraphic units under the tuff cone are unknown. It is thoughl, however, that the tuff cone could be mainly emergent because the present cone deposits show no evidence of marine reworking, and standing body of sea water could play a great role. The emergent volcano is characterized by distinctive steam-explosivity that results primarily from a bulk interaction between rapidly ascending magma and a highly mobile slurry. The sea water gets into the vent by flooding accross or through the top or breach of tephra cone. Udo tuff cone was constructed from Surtseyan eruption which went into with tephra finger jetting activities in the early stage, late interspersed with continuous uprush activities and proceeded to only continuous uprush activities in the last. When the enclosure of the vent by a long-lived tephra barrier would prevent the flooding and thus allow the vent to dry out, the Surtseyan eruption ceased to transmit into Strombolian activities, which constructed a cinder cone on the crater floor of the tuff cone. The Strombolian eruption ceased when magma in the conduit gradually became depleted in gas. In the case of Udo, the last magmatic activity was Hawaiian-type (and/or fountain) which accumulated basalt lava delta. And then the loose tephra of the tuff cone reworked over the moat lava and the northeastern flank.

• 암석학회지
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• 제1권2호
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• pp.91-103
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• 1992

Eruptive mechanisms and processes at Udo tuff cone can be inferred from indicative characters of products, bedforms and lithofacies, and ring faults. In terms of bedforms and lithofa-cies in particular, massive lapilli tuff beds and chaotic lapilli tuff beds are derived from subaerial falls of aggregated tephra of wet tephra finger jets, occurring dominantly at the lower sequences of proximal part at the tuff cone. Crudely stratified lapilli tuff are derived from subaerial falls of slightly aggregated tephra of less wet tephra finger jets, whereas reversely graded lapilli tuff beds are from slightly disaggregated subaerial falls of continuous uprush. Both beds frequently occur in the middle sequences at proximal and near medial part of the tuff cone. Block and lapilli tephra lenses, ash-coated lapilli tephra beds(lenses) and thin-bedded tuff beds are derived from extremely disaggregated subaerial falls of dry tephra in the continuous uprush, frequently occurring at the upper sequences of medial part at the tuff cone. Udo tuff cone is a basaltic volcano emergent through the sea water surface while water could flood across or into the vent area. Emergence of the tuff cone was from the type-Surtseyan eruption characterized by earlier tephra finger jets and later continuous uprush columns of tephra with copious volumes of steam. Explosions began when boiling of wter produced a bubble column reducing the hydrostatic pres-sure, allowing exsolution of gases from the magma. This expansion of magma into a vesiculating froth fragmented the magma and permitted mixing of magma and water so that a more vigorous generation of steam could proceed. Tephra finger jetting explosions continued to build the crater rims, then remove water from the vent that their deposits flowed like slsurries until the continuous uprush explosion ensued. Continuous uprush explosions were associated with most rapid accumula-tion of tephra. The increasing volume rate led to partial removal of water from the vent area by the newly tephra ring so that more vigorous activity could be attended by a reducing water supply. This might restrain surplus of cold water entering the vent and thus enhance the vigour of the eruption by allowing optimal heat exchange. Eventually the crater became so deep and unsuported that piecemeal sliding, or massive subsidence on indipping ring faults, filled and closed the vent, and the cycle of explosions and collapse began anew.

• 암석학회지
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• 제7권1호
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• pp.1-14
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• 1998

당산봉 화산은 제주도 서쪽 끝 해안에 위치하며, 응회구, 분석구, 용암대지 및 애추층 등으로 구성된다. 이들의 암상과 층서는 써제이언분출, 스트롬볼리언분출, 하와이언분출 순으로 전개되는 화산 과정과 외력쇄설 지표과정을 나타낸다. 당산봉 응회구는 마그마와 해수가 상호작용하여 스팀폭발함으로서 형성되는 써쩨이언분출에 의한 구조물이다. 이 분출은 초기에 습윤한 테프라수지상분사 활동상이었고, 중기에 보다 덜 습윤한 테프라의 연속분승 활동상과 테프라수지상분사 활동상이 교대로 진행되었으며, 후기에 보다 건조한 초써쩨이언분사 활동상으로 전환되었다. 분석구는 응회구의 축조로 외부 물의 완전한 제한으로 인해 써제이언분출이 종식되고 스트롬볼리안분출로 전환됨으로써 형성되었다. 이 분출은 초기에 분석 위주로 포출하였으며 후기에 스패터 위주로 포출하는 활동상으로 변화되었다. 용암대지는 화도내 마그마 개스의 고갈로 폭발력이 소진되어 하와이언분출로 전환되므로써 형성되었다. 이 분출은 초기에 용암분천 활동상 위주로 진행되었으나 후기에 용암분류 활동상으로 변화되었다.

• 대한원격탐사학회지
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• 제30권3호
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• pp.341-350
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• 2014

Landsat images can monitor the snow-covered Earth surface variations with the ground resolution of 30m and the multi-spectral bands in the visible, NIR, SWIR and TIR spectral regions for the last 30 years. The Southern Volcanic Zone (SVZ) of Chile consists of many volcanoes, and all of the volcanoes are covered with snow at the top of mountain. Snow cover area in southern province of the SVZ of Chile (37 to $46^{\circ}S$) have been influenced by significant frontal retreats as well as eruptive activities. In this study, we have investigated the changes of the snow-cover area and snow-line elevation at Mt. Villarrica and Mt. Llaima, Chile from three Landsat images acquired on Feb. 1990, 2005 and 2011. The snow-cover areas are 13.42, 26.75 and $21.60km^2$ at Mt. Villarrica in 1990, 2005 and 2011, respectively, and 3.82, 25.12 and $8.89km^2$ at Mt. Llaima in 1990, 2005 and 2011, respectively. The snow-line elevations are 1871, 1738 and 1826m at Mt. Villarrica in 1990, 2005 and 2011, respectively, and 2007, 1822 and 1818m at Mt. Llaima in 1990, 2005 and 2011, respectively. The results indicate that both of the snow-cover and snow-line changes are strongly related with the volcanic activity change. The results demonstrate that the snow-cover area and snow-line elevation changes can be used as an indicator of the volcanic activity at Mt. Villarrica and Mt. Llaima, Chile.

• Ocean and Polar Research
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• 제23권2호
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• pp.97-107
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• 2001

The Sejong Formation of Late Paleocene to Eocene is a lower volcaniclastic sequence unconformably overlain by upper volcanic sequence, and distributed along the southern and southeastern cliffs of the Barton Peninsula. The Sejong Formation is divided into five sedimentary facies; disorganized matrix-supported conglomerate (Facies A), disorganized clast-supported conglomerate (Facies B), stratified clast-supported conglomerate (Facies C), thin-bedded sandstone (Facies D), and lapilli tuff (Facies E), based on sedimentary textures, primary sedimentary structures and bed geometries. Individual sedimentary facies is characterized by distinct sedimentary process such as gravel-bearing mudflows or muddy debris flows (Facies A), cohesionless debris flows (Facies B),unconfined or poorly confined hyperconcentrated flood flows and sheet floods (Facies C), subordinate streamflows (Facies D), and pyroclastic flows (Facies E). Deposition of the Sejong Formation was closely related to volcanic activity which occurred around the sedimentary basin. Four different phases of sediment filling were identified from constituting sedimentary facies. Thick conglomerate and sandstone were deposited during inter-eruptive phases (stages 1, 3 and 4), whereas lapilli tuff was formed by pyroclastic flows during active volcanism (stage 2). These records indicate that active volcanism occurred around the Barton Peninsula during Late Paleocene to Eocene.

• 암석학회지
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• 제23권2호
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• pp.119-138
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• 2014

활화산을 감시하는 방법은 육안으로 직접 관찰하는 방법, 과거의 분화 기록 문건을 참조하는 방법, 직접적으로 관측 장비를 동원하여 화산체를 감시하는 방법 등이 있다. 이 중 관측 장비를 이용하여 화산체를 감시하는 방법 중 가장 기본적인 것은 지진활동도의 감시이며, 이외에도 지진계에 기록된 지진활동 중 인위적인 노이즈를 걸러내는 데 효과적인 공진 관측, 그리고 정밀수준기, 전자거리측정기, 경사계, GPS, InSAR 관측법을 통한 지표변형의 감시, 화산가스 감시, 수문학적/기상학적 감시, 기타 지구물리학적 감시 등의 방법이 있다. 이러한 감시 기법을 통해 화산의 활동을 효과적으로 감시하고 이를 통해 지하 마그마방에서의 마그마 거동을 파악함으로써 미래의 화산 분화를 보다 정확하게 예측하고 조기 경보하여 그에 따른 재해의 피해를 경감하고 최소화 할 수 있다.

• 자원환경지질
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• 제53권5호
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• pp.553-564
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• 2020

울릉도에서 폭발성 및 분류성 분출 간의 전환은 돔형성 분출을 나타내는 나리분석층과 알봉조면안산암(용암돔)에서 관찰되며, 유동성 마그마, 상승률 및 탈기작용과 같은 요인과 연관된다. 그러나 이들에 대한 해석은 요인들 간의 상호작용이 복잡할 뿐만 아니라 분출과정에서의 거동을 예측하기 어렵기 때문에 지금까지 해결되지 않았다. 이 논문은 나리 칼데라에서 알봉 용암돔 형성과정에서 인지되는 폭발성 및 분류성 분출에 초점을 두었다. 시료는 분석층과 용암돔에서 시간에 따라 채취하였으며, 분출 단계 및 활동 양식과 연계되어 있다. 이 시료들에서 석기 장석미정의 조직은 면적 개수밀도, 평균 미정크기, 결정 종횡비, 석기 결정률 등을 포함하며 정량적으로 분석되었다. 이러한 미정의 조직은 천부에서 분출전 및 분출동시 마그마 과정이 분출 동안 거동변화를 제어하면서 진행되었다는 것을 보여준다. 폭발성 및 분류성 분출 간의 전환은 주로 화도 내 마그마 상승의 역학관계에 의해 일어났으며, 탈기작용과 결정작용이 피드백 메카니즘을 통해 일어남으로서 분류성 및 폭발성 분출의 한 윤회를 초래했다.

• 천문학회지
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• 제37권1호
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• pp.41-53
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• 2004

It has been a big mystery what drives filament eruptions and flares. We have studied in detail an X1.8 flare and its associated filament eruption that occurred in NOAA Active Region 9236 on November 24,2000. For this work we have analyzed high temporal (about 1 minute) and spatial (about 1 arcsec) resolution images taken by Michelson Doppler Imager (MDI) onboard the Solar and Heliospheric Observatory, Hoc centerline and blue wing ($-0.6{\AA}$) images from Big Bear Solar Observatory, and 1600 ${\AA}$ UV images by the Transition Region and Corona Explorer (TRACE). We have found that there were several transient brightenings seen in H$\alpha$ and, more noticeably in TRACE 1600 ${\AA}$ images around the preflare phase. A closer look at the UV brightenings in 1600 ${\AA}$ images reveals that they took place near one end of the erupting filament, and are a kind of jets supplying mass into the transient loops seen in 1600 ${\AA}$. These brightenings were also associated with canceling magnetic features (CMFs) as seen in the MDI magnetograms. The flux variations of these CMFs suggest that the flux cancellation may have been driven by the emergence of the new flux. For this event, we have estimated the ejection speeds of the filament ranging from 10 to 160 km $s^{-1}$ for the first twenty minutes. It is noted that the initiation of the filament eruption (as defined by the rise speed less than 20 km $s^{-1}$) coincided with the preflare activity characterized by UV brightenings and CMFs. The speed of the associated LASCO CME can be well extrapolated from the observed filament speed and its direction is consistent with those of the disturbed UV loops associated with the preflare activity. Supposing the H$\alpha$/UV transient brightenings and the canceling magnetic features are due to magnetic reconnect ion in the low atmosphere, our results may be strong observational evidence supporting that the initiation of the filament eruption and the preflare phase of the associated flare may be physically related to low-atmosphere magnetic reconnection.