- appear on the skin; "A rash erupted on her arms after she had touched the exotic plant"
- become active and spew forth lava and rocks; "Vesuvius erupts once in a while" (同)belch, extravasate
- start abruptly; "After 1989, peace broke out in the former East Bloc" (同)break_out
- erupt or intensify suddenly; "Unrest erupted in the country"; "Tempers flared at the meeting"; "The crowd irrupted into a burst of patriotism" (同)irrupt, flare_up, flare, break_open, burst_out
- become raw or open; "He broke out in hives"; "My skin breaks out when I eat strawberries"; "Such boils tend to recrudesce" (同)recrudesce, break_out
- break out; "The tooth erupted and had to be extracted" (同)come_out, break_through, push through
- start to burn or burst into flames; "Marsh gases ignited suddenly"; "The oily rags combusted spontaneously" (同)ignite, catch fire, take fire, combust, conflagrate
- (of volcanos) pouring out fumes or lava (or a deposit so formed) (同)eructation, extravasation
- symptom consisting of a breaking out and becoming visible
- the emergence of a tooth as it breaks through the gum
- gush forth in a sudden stream or jet; "water gushed forth" (同)spirt, gush, spout
- 〈火山灰・間欠泉などが〉噴出する,〈火山が〉噴火する / 〈争いなどが〉突然起こる;〈感情が〉爆発する / 〈溶岩・熱湯など〉‘を'噴出させる / 〈怒りなど〉‘を'爆発させる
- (病気・災害などの)『突発』,(戦争などの)勃(ぼっ)発;(怒り・笑いの)爆発《+『of』+『名』》 / (溶岩・熱湯などの)『噴出』;(火山の)『噴出』;(火山の)『噴火』《+『of』+『名』》;(火山・間欠泉などからの)噴出物
- 〈液体などが〉噴出する,ほとばしる《+『out』》 / スパートする,力走(力泳)する / 〈液体など〉‘を'噴出させる,ほとばしらせる / (液体などの)噴出,ほとばしり;(感情・エネルギーなどの)激発 / (レースの途中や最後の)力走,力泳,力闘
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- Precise chronology of differentiation of developing human primary dentition.
- Hu X, Xu S, Lin C, Zhang L, Chen Y, Zhang Y.Author information Fujian Key Laboratory of Developmental and Neuro Biology, College of Life Science, Fujian Normal University, Fuzhou, 350108, Fujian, People's Republic of China.AbstractWhile correlation of developmental stage with embryonic age of the human primary dentition has been well documented, the available information regarding the differentiation timing of the primary teeth was largely based on the observation of initial mineralization and varies significantly. In this study, we aimed to document precise differentiation timing of the developing human primary dentition. We systematically examined the expression of odontogenic differentiation markers along with the formation of mineralized tissue in each developing maxillary and mandibular teeth from human embryos with well-defined embryonic age. We show that, despite that all primary teeth initiate development at the same time, odontogenic differentiation begins in the maxillary incisors at the 15th week and in the mandibular incisors at the 16th week of gestation, followed by the canine, the first primary premolar, and the second primary premolar at a week interval sequentially. Despite that the mandibular primary incisors erupt earlier than the maxillary incisors, this distal to proximal sequential differentiation of the human primary dentition coincides in general with the sequence of tooth eruption. Our results provide an accurate chronology of odontogenic differentiation of the developing human primary dentition, which could be used as reference for future studies of human tooth development.
- Histochemistry and cell biology.Histochem Cell Biol.2014 Feb;141(2):221-7. doi: 10.1007/s00418-013-1149-y. Epub 2013 Oct 6.
- While correlation of developmental stage with embryonic age of the human primary dentition has been well documented, the available information regarding the differentiation timing of the primary teeth was largely based on the observation of initial mineralization and varies significantly. In this st
- PMID 24097047
- Localized sources of water vapour on the dwarf planet (1) Ceres.
- Küppers M1, O'Rourke L1, Bockelée-Morvan D2, Zakharov V2, Lee S3, von Allmen P3, Carry B4, Teyssier D1, Marston A1, Müller T5, Crovisier J2, Barucci MA2, Moreno R2.Author information 1European Space Agency, European Space Astronomy Centre, PO Box 78, Villanueva de la Cañada 28691, Spain.2Laboratoire d'études spatiales et d'instrumentation en astrophysique, Observatoire de Paris, CNRS, Université Pierre et Marie Curie (UPMC), Université Paris-Diderot, 5 Place Jules Janssen, 92195 Meudon, France.3Jet Propulsion Laboratory, Pasadena, 4800 Oak Grove Drive, La Cañada Flintridge, California 91011, USA.41] European Space Agency, European Space Astronomy Centre, PO Box 78, Villanueva de la Cañada 28691, Spain  Institut de Mécanique Céleste et de Calcul des Éphémérides, Observatoire de Paris, Unité Mixte de Recherche (UMR) 8028, CNRS, 77 Avenue Denfert Rochereau, 75014 Paris, France.5Max-Planck-Institut für extraterrestrische Physik (MPE), Giessenbachstrasse 1, 85748 Garching, Germany.AbstractThe 'snowline' conventionally divides Solar System objects into dry bodies, ranging out to the main asteroid belt, and icy bodies beyond the belt. Models suggest that some of the icy bodies may have migrated into the asteroid belt. Recent observations indicate the presence of water ice on the surface of some asteroids, with sublimation a potential reason for the dust activity observed on others. Hydrated minerals have been found on the surface of the largest object in the asteroid belt, the dwarf planet (1) Ceres, which is thought to be differentiated into a silicate core with an icy mantle. The presence of water vapour around Ceres was suggested by a marginal detection of the photodissociation product of water, hydroxyl (ref. 12), but could not be confirmed by later, more sensitive observations. Here we report the detection of water vapour around Ceres, with at least 10(26) molecules being produced per second, originating from localized sources that seem to be linked to mid-latitude regions on the surface. The water evaporation could be due to comet-like sublimation or to cryo-volcanism, in which volcanoes erupt volatiles such as water instead of molten rocks.
- Nature.Nature.2014 Jan 23;505(7484):525-7. doi: 10.1038/nature12918.
- The 'snowline' conventionally divides Solar System objects into dry bodies, ranging out to the main asteroid belt, and icy bodies beyond the belt. Models suggest that some of the icy bodies may have migrated into the asteroid belt. Recent observations indicate the presence of water ice on the surfac
- PMID 24451541
- Primitive layered gabbros from fast-spreading lower oceanic crust.
- Gillis KM1, Snow JE2, Klaus A3, Abe N4, Adrião AB5, Akizawa N6, Ceuleneer G7, Cheadle MJ8, Faak K9, Falloon TJ10, Friedman SA11, Godard M12, Guerin G13, Harigane Y14, Horst AJ15, Hoshide T16, Ildefonse B12, Jean MM17, John BE8, Koepke J18, Machi S6, Maeda J19, Marks NE20, McCaig AM21, Meyer R22, Morris A23, Nozaka T24, Python M19, Saha A25, Wintsch RP26.Author information 1School of Earth and Ocean Sciences, University of Victoria, PO Box 1700 Station CSC, Victoria, British Columbia V8W 2Y2, Canada.2Earth and Atmospheric Sciences, University of Houston, 312 Science and Research Building 1, Houston, Texas 77204-5007, USA.3United States Implementing Organization, Integrated Ocean Drilling Program, Texas A&M University, 1000 Discovery Drive, College Station, Texas 77845, USA.4Institute for Research on Earth Evolution, Japan Agency for Marine-Earth Science and Technology, 2-15 Natsushima-cho, Yokosuka 237-0061, Japan.5Institute of Geoscience, Rio Grande do Sul Federal University, Avenida Bento Gonçalves, 9500 Bloco I Prédio, 43113 Sala 207, Porto Alegre/RS 91501-970, Brazil.6Department of Earth Sciences, Kanazawa University, Kakuma-machi, Kanazawa Ishikawa 920-1192, Japan.7Observatoire Midi-Pyrénées (UMS 831), CNRS, Université Paul Sabatier, 14 Avenue Edouard Belin, Toulouse Cedex 31400, France.8Department of Geology and Geophysics, University of Wyoming, 1000 University Avenue, Department 3006, Laramie, Wyoming 82071, USA.91] School of Earth and Ocean Sciences, University of Victoria, PO Box 1700 Station CSC, Victoria, British Columbia V8W 2Y2, Canada  Institut für Geologie, Mineralogie, and Geophysik, Ruhr-Universität Bochum, Universitätsstrasse 150, 44780 Bochum, Germany.10Institute for Marine and Antarctic Studies and School of Earth Sciences, University of Tasmania, Hobart, Tasmania 7001, Australia.11Department of Geology, Southern Illinois University at Carbondale, Carbondale, Illinois 62901, USA.12Géosciences Montpellier, Université Montpellier 2, CNRS UMR5243, CC 60, 34095 Montpellier Cedex 5, France.13Borehole Research Group, Lamont-Doherty Earth Observatory of Columbia University, PO Box 1000, 61 Route 9W, Palisades, New York 10964, USA.14Institute of Geology and Geoinformation, Geological Survey of Japan, National Institute of Advanced Industrial Science and Technology, AIST Tsukuba Central 7, 1-1-1 Higashi, Tsukuba Ibaraki 305-8567, Japan.15Department of Geology, Oberlin College, Oberlin, Ohio 44074, USA.16Graduate School of Science, Tohoku University, Aoba-ku, Sendai 980-8578, Japan.17Department of Geology and Environmental, Geosciences, Northern Illinois University, Davis Hall 312, Normal Road, DeKalb, Illinois 60115, USA.18Institut für Mineralogie, University of Hannover, Callinstrasse 3, Hannover 30167, Germany.19Department of Natural History Sciences, Hokkaido University, North 10, West 8, Kita-ku, Sapporo, Hokkaido 060-0810, Japan.20Chemistry and Material Sciences Department, Lawrence Livermore National Laboratory, PO Box 808, L-231, Livermore, California 94551, USA.21School of Earth and Environment, University of Leeds, Leeds LS2 9JT, UK.22Centre for Geobiology and Department of Earth Science, University of Bergen, Allegaten 41, Bergen 5007, Norway.23School of Geography, Earth and Environmental Sciences, Plymouth University, Drake Circus, Plymouth PL4 8AA, UK.24Department of Earth Sciences, Okayama University, 3-1-1 Tsushima-naka, Okayama 700-8530, Japan.25Department of Geology, University of Calcutta, 35 Ballygunge Circular Road, Kolkata 700 019, India.26Department of Geological Sciences, Indiana University, 1001 East 10th Street, Bloomington, Indiana 47405, USA.AbstractThree-quarters of the oceanic crust formed at fast-spreading ridges is composed of plutonic rocks whose mineral assemblages, textures and compositions record the history of melt transport and crystallization between the mantle and the sea floor. Despite the importance of these rocks, sampling them in situ is extremely challenging owing to the overlying dykes and lavas. This means that models for understanding the formation of the lower crust are based largely on geophysical studies and ancient analogues (ophiolites) that did not form at typical mid-ocean ridges. Here we describe cored intervals of primitive, modally layered gabbroic rocks from the lower plutonic crust formed at a fast-spreading ridge, sampled by the Integrated Ocean Drilling Program at the Hess Deep rift. Centimetre-scale, modally layered rocks, some of which have a strong layering-parallel foliation, confirm a long-held belief that such rocks are a key constituent of the lower oceanic crust formed at fast-spreading ridges. Geochemical analysis of these primitive lower plutonic rocks--in combination with previous geochemical data for shallow-level plutonic rocks, sheeted dykes and lavas--provides the most completely constrained estimate of the bulk composition of fast-spreading oceanic crust so far. Simple crystallization models using this bulk crustal composition as the parental melt accurately predict the bulk composition of both the lavas and the plutonic rocks. However, the recovered plutonic rocks show early crystallization of orthopyroxene, which is not predicted by current models of melt extraction from the mantle and mid-ocean-ridge basalt differentiation. The simplest explanation of this observation is that compositionally diverse melts are extracted from the mantle and partly crystallize before mixing to produce the more homogeneous magmas that erupt.
- Nature.Nature.2014 Jan 9;505(7482):204-7. doi: 10.1038/nature12778. Epub 2013 Dec 1.
- Three-quarters of the oceanic crust formed at fast-spreading ridges is composed of plutonic rocks whose mineral assemblages, textures and compositions record the history of melt transport and crystallization between the mantle and the sea floor. Despite the importance of these rocks, sampling them i
- PMID 24291793
- Recurrent vesicular eruption on the right hand.
- Ishak RS, Abbas O.Author information Department of Dermatology, American University of Beirut Medical Center, Lebanon. Email: email@example.com.AbstractThe 8-year-old boy was otherwise healthy. So what was causing these painful lesions to erupt on his hand?
- The Journal of family practice.J Fam Pract.2014 Jan;63(1):33-5.
- The 8-year-old boy was otherwise healthy. So what was causing these painful lesions to erupt on his hand
- PMID 24475465
- A3-10 浅間山の一連の噴火活動(2004年〜2015年)とVLP活動との比較(モニタリング,口頭発表)
- いまを読み解く 大噴火・大地震は自然界からの警告である : 川内原発再稼働を止めよう!
- eruptとは。意味や和訳。[動](自)[I（[副]）]1 〈溶岩・火山灰などが〉（…から）噴出する((from ...))；〈火山が〉噴火する；〈間欠泉が〉噴き上がる.2 〈うっ積していた感情が〉ほとばしり出る；〈言葉などが〉（せきを切った ...
- verb (used without object) 1. to burst forth: Molten lava erupted from the top of the volcano. Synonyms: vent. 2. (of a volcano, geyser, etc.) to eject matter. ... 1650s, of diseases, etc., from L. erupt-, pp. stem of erumpere (see eruption).
- ERUPT. 1,107 likes · 1 talking about this. Musician/Band ... Recent Posts by Others on ERUPT See All Christopher Eades Photoshoot/behind the scenes video with Alexander Vlad for ERUPT September 9, 2012 at 4:10pm
- unerupted teeth