ライフサイエンスコーパス: Mercury

1 Mercury (GM 9.8 nmol/L) was detected in nearly all blood

2 Mercury (Hg) bioaccumulation factors (BAFs) for game fis

3 Mercury (Hg) bioavailability to bacteria in marine syste

4 Mercury (Hg) concentration trends in top predator fish (

5 Mercury (Hg) concentrations have increased in western Ar

6 Mercury (Hg) concentrations were monitored from 1999 to

7 Mercury (Hg) contamination in aquatic systems remains a

8 Mercury (Hg) dynamics in the Arctic is receiving increas

9 Mercury (Hg) emissions from coal combustion contribute a

10 Mercury (Hg) entering aquatic systems and accumulated as

11 Mercury (Hg) in wet deposition in the United States is m

12 Mercury (Hg) is a global pollutant that affects human an

13 Mercury (Hg) is a global threat to wildlife health that

14 Mercury (Hg) is a neurotoxin that can be particularly ha

15 Mercury (Hg) is a toxic metal that is found in aquatic f

16 Mercury (Hg) is a toxic metal that presents public healt

17 Mercury (Hg) is a toxicant of global concern that accumu

18 Mercury (Hg) is an important environmental contaminant,

19 Mercury (Hg) is of particular interest as methylmercury

20 Mercury (Hg) is used in gold mining to extract gold from

21 Mercury (Hg) is widely distributed in the environment, a

22 Mercury (Hg) isotopes can be used as tracers of Hg bioge

23 Mercury (Hg) methylation and methylmercury (MMHg) demeth

24 Mercury (Hg) occurs as a myriad of species in environmen

25 Mercury (Hg) speciation and the activity of Hg(II)-methy

26 Mercury (Hg) wet deposition, transfer from the atmospher

27 Mercury (Hg), a ubiquitous and highly toxic bioaccumulat

28 Mercury (Hg), especially in organic form, is a highly to

29 Mercury accumulation in fish is a global public health c

30 Mercury and bromine leaching tests were conducted using

31 Mercury and its compounds are highly toxic and can cause

32 Mercury and ozone are rapidly removed from the atmospher

33 Mercury and the Moon both have tenuous atmospheres that

34 Mercury associated with sandy soil up to 6 cm below the

35 Mercury BAFs are calculated as the fish Hg concentration

36 Mercury being one of the most toxic heavy metals has lon

37 Mercury complexation by low-molecular-weight (LMW) thiol

38 Mercury concentrations in blood were not correlated with

39 Mercury concentrations in burbot in the Lena and Mezen R

40 Mercury concentrations in burbot in the Lena and Mezen R

41 Mercury concentrations in feathers also were uncorrelate

42 Mercury concentrations in grebe blood, grebe eggs, and s

43 Mercury concentrations in leaves were monitored from eme

44 Mercury concentrations in surface precipitation follow a

45 Mercury concentrations in winter feathers were positivel

46 Mercury concentrations up to 800 pM were observed in sha

47 Mercury contamination in food can pose serious health ri

48 Mercury content in two certified materials and in ten sa

49 Mercury diffusion in air offers a reasonable explanation

50 Mercury distribution in the oceans is controlled by comp

51 Mercury emissions from major point sources in the hotspo

52 Mercury emissions in North America have declined over th

53 Mercury emitted from dental amalgam may select for incre

54 Mercury exposure has been associated with a wide variety

55 Mercury has a particularly chaotic orbit and is in dange

56 Mercury has contaminated rivers worldwide, with health c

57 Mercury has well-documented endocrine activity; however,

58 (Mercury II-Compare the Efficacy and Safety of Lipid Lowe

59 Mercury in fish was positively and significantly correla

60 Mercury in food is present in either inorganic [Hg(II)]

61 Mercury in foods, in inorganic form [Hg(II)] or as methy

62 Mercury in urine therefore represents a mixture of demet

63 Mercury increases previously associated with the mid-19t

64 Mercury injection capillary pressure (MICP) and N2 gas a

65 Mercury is a global pollutant, and prenatal exposure is

66 Mercury is a highly toxic heavy metal, and detection of

67 Mercury is a highly toxic priority pollutant that can be

68 Mercury is a major contaminant in the Arctic marine ecos

69 Mercury is a major threat to the environment and to huma

70 Mercury is a potent neurotoxin for humans, particularly

71 Mercury is a toxic air pollutant, emitted from the combu

72 Mercury is a toxic, bioaccumulating trace metal whose em

73 Mercury is a widespread contaminant in marine food webs,

74 Mercury is an automated, flexible, and extensible analys

75 Mercury is emanated in the course of various natural eve

76 Mercury is one of the most acutely toxic substances at t

77 Mercury is one of the primary contaminants of concern in

78 Mercury is surrounded by a tenuous exosphere that is sup

79 Mercury is toxic for human health and one of the main ro

80 Mercury is widely distributed in aquatic ecosystems as a

81 Mercury isotope composition and sediment geochemical dat

82 Mercury isotope variations are small and result only fro

83 Mercury levels in biota are mainly controlled by the met

84 Mercury levels of 6.0 and 5.6 ppm were obtained from the

85 Mercury levels were measured in colonial waterbird eggs

86 Mercury methylation and/or demethylation have been obser

87 Mercury methylation occurred in solution and was a funct

88 Mercury methylation was inhibited ( approximately 80%) i

89 Mercury obtained from the diet accumulates in mammalian

90 Mercury poisoning and "hot filtration" experiments ruled

91 Mercury pollution is widespread globally, and strategies

92 Mercury pollution poses risks for both human and ecosyst

93 Mercury pulse injection tests on the sorbent material af

94 Mercury resistance mediated by mercuric reductase (MerA)

95 Mercury resistant bacteria have developed a system of tw

96 Mercury speciation showed significant connections to the

97 Mercury species concentrations for levels 2 and 4 of SRM

98 Mercury species extraction was achieved by microwave exp

99 Mercury species were measured on three Baltic Sea campai

100 Mercury stable isotope abundances were used to trace tra

101 Mercury stocks in products rose from 700 tonnes in 2001

102 Mercury sulfide minerals are known to nucleate in anoxic

103 Mercury undergoes several transformations that influence

104 Mercury uptake in bacteria represents a key first step i

105 Mercury vapor, generated in the reaction mixture, was ex

106 Mercury was found to bind to the reduced sulfur by the c

107 Mercury wet deposition also varies by geographic region

108 Mercury's global record of large impact basins, which ha

109 Mercury's northern hemisphere crust is thicker at low la

110 Mercury(II), palladium(II), copper(II), iron(II), and ni

111 Mercury, arsenic, manganese, antimony, and crystalline s

112 Mercury-capped platinum ultramicroelectrodes (Hg/Pt UMEs

113 Mercury-containing sulfhydryl modification agents (rho-h

114 Mercury-free compound 5 does not interact with plasmid (

115 Mercury-induced autoimmunity in H-2s mice provides a use

116 Mercury-induced cell death was associated with loss of f

117 Mercury-resistant bacteria express merA to convert highl

118 in Bovine Blood (30 ng x mL(-1)); SRM 1641d Mercury in Water (1.6 microg x mL(-1)); and SRM 1946 Lak

119 ion from ionized calcium concentrated 1 to 2 Mercury radii tailward of the planet.

120 of 10, 20, 40, 80, and 160 ms using SRM 3133 Mercury Spectrometric Solution.

121 ufficient to find a 5-Earth-mass planet in a Mercury-like orbit around a Sun-like star.

122 d by the MESSENGER spacecraft in orbit about Mercury permit the separation of internal and external m

123 shortly after its insertion into orbit about Mercury.

124 It seems plausible that Io, like Earth and Mercury, is a magnetized solid planet.

125 ometry (CIMS) during the Bromine, Ozone, and Mercury Experiment (BROMEX) near Barrow, Alaska, in Marc

126 atering record of the Moon, Mars, Venus, and Mercury and from the size distributions of asteroid popu

127 C/MR(2) = 0.353 +/- 0.017, where M and R are Mercury's mass and radius, and a ratio of the moment of

128 The region around Mercury is filled with ions that originate from interact

129 As part of the Arsenic Mercury Intake Biometric Study involving the Japanese an

130 observed in similar thermal environments at Mercury's poles.

131 by MESSENGER of the fluxes of heavy ions at Mercury, particularly sodium (Na(+)) and oxygen (O(+)),

132 The extreme tail loading observed at Mercury implies that the relative intensity of substorms

133 The total mass of water at Mercury's poles is inferred to be 2 x 10(16) to 10(18) g

134 ran speciation instruments at 13 Atmospheric Mercury Network (AMNet) sites.

135 The Reno Atmospheric Mercury Intercomparison Experiment (RAMIX) was carried o

136 The Reno Atmospheric Mercury Intercomparison Experiment (RAMIX) was in Reno,

137 old in the field during the Reno Atmospheric Mercury Intercomparison eXperiment.

138 inamata Convention on Mercury) and domestic [Mercury and Air Toxics Standards (MATS)] policies, frame

139 from surface sputtering by ions, which enter Mercury's auroral zone.

140 alogs of all the solar system planets except Mercury.

141 During MESSENGER's first Mercury flyby, the Mercury Atmospheric and Surface Compo

142 upplemented by observations during the first Mercury flyby, as well as those by other MESSENGER instr

143 A model for Mercury's radial density distribution consistent with th

144 he flux of epithermal and fast neutrons from Mercury's north polar region that are consistent with th

145 MESSENGER observations from Mercury orbit reveal that a large contiguous expanse of

146 Doubly ionized ions originating from Mercury imply that electrons with energies less than 1 k

147 Oxidized Mercury, the University of Houston Mercury instrument, and a filter-based system under deve

148 uranium (U, 90 +/- 20 parts per billion) in Mercury's northern hemisphere.

149 es in the fluid outer core operated early in Mercury's history.

150 electron volt are substantially energized in Mercury's magnetosphere.

151 the flyby, the average abundance of iron in Mercury's surface material is less than 6% by weight.

152 , we have detected remanent magnetization in Mercury's crust.

153 and potassium have already been observed in Mercury's atmosphere, with abundances that require a vol

154 aveling compression regions were observed in Mercury's magnetotail, all products of reconnection.

155 olcanism was a globally extensive process in Mercury's post-heavy bombardment era.

156 l the distribution of even single species in Mercury's exosphere.

157 195 +/- 10 nanotesla-R(M)(3), where R(M) is Mercury's mean radius.

158 ent of 230 to 290 nanotesla RM3 (where RM is Mercury's mean radius) tilted between 5 degrees and 12 d

159 s formed on other planets (i.e., Moon, Mars, Mercury), where the mantle oxidation state [oxygen fugac

160 nd Surface Composition Spectrometer measured Mercury's exospheric emissions, including those from the

161 airless planetary bodies, such as the Moon, Mercury, and asteroids.

162 flectance of permanently shadowed areas near Mercury's north pole reveal regions of anomalously dark

163 discovery of calcium in the atmosphere near Mercury's poles.

164 In some regions near Mercury, especially the nightside equatorial region, the

165 neities in the color and thus composition of Mercury's crust.

166 bservations and with the low iron content of Mercury's crust inferred from MESSENGER elemental compos

167 uct of the global cooling and contraction of Mercury.

168 perature conditions relevant to the cores of Mercury-sized to Earth-sized planets, using a dynamicall

169 During MESSENGER's second flyby of Mercury, a steady southward IMF was observed and the mag

170 During MESSENGER's third flyby of Mercury, the magnetic field in the planet's magnetic tai

171 During MESSENGER's third flyby of Mercury, the Mercury Atmospheric and Surface Composition

172 During MESSENGER's first flyby of Mercury, the Mercury Atmospheric and Surface Composition

173 During its first flyby of Mercury, the MESSENGER spacecraft measured the planet's

174 During its first two flybys of Mercury, the MESSENGER spacecraft acquired images confir

175 nt with physical models for the formation of Mercury requiring extreme heating of the planet or its p

176 ographic model of the northern hemisphere of Mercury.

177 The composition and evolutionary history of Mercury's crust are not well determined.

178 le of volcanism in the geological history of Mercury.

179 Multispectral images of Mercury obtained by the MESSENGER spacecraft reveal that

180 High-resolution images of Mercury's surface from orbit reveal that many bright dep

181 ius, and a ratio of the moment of inertia of Mercury's solid outer shell to that of the planet of C(m

182 oefficient C22, indicates that the mantle of Mercury is decoupled from a core that is at least partia

183 ns in composition and regolith maturation of Mercury's surface.

184 rbital vector magnetic field measurements of Mercury taken by the MErcury Surface, Space ENvironment,

185 fish using the National Descriptive Model of Mercury in Fish (NDMMF) based on bird spatial assignment

186 MESSENGER spacecraft has provided a model of Mercury's gravity field.

187 uous expanse of smooth plains covers much of Mercury's high northern latitudes and occupies more than

188 er, MESSENGER and Mariner 10 observations of Mercury now provide a near-global look at the planet, re

189 The MESSENGER spacecraft's observations of Mercury's ionized exosphere during its first flyby yield

190 A 3200-kilometers-long profile of Mercury by the Mercury Laser Altimeter on the MESSENGER

191 Thermal models for the north polar region of Mercury, calculated from topographic measurements made b

192 on the Moon, at least in part the result of Mercury's higher gravity.

193 dar speckle patterns tied to the rotation of Mercury establish that the planet occupies a Cassini sta

194 that polar regions are important sources of Mercury's ionized exosphere, presumably through solar-wi

195 Here we report global crater statistics of Mercury's most heavily cratered terrains on the entire s

196 On Mercury, solar heating of the surface implies that therm

197 in, the youngest known large impact basin on Mercury, is revealed in MESSENGER images to be modified

198 of the United Nations Minamata Convention on Mercury for emissions from Asian coal-fired power genera

199 missions through the "Minamata Convention on Mercury", our study provides valuable information on the

200 States of global (UN Minamata Convention on Mercury) and domestic [Mercury and Air Toxics Standards

201 o 10 kilometers, secondary impact craters on Mercury are more abundant than primaries; this transitio

202 Sampled craters on Mercury are shallower than their counterparts on the Moo

203 frequency distributions of impact craters on Mercury imaged during MESSENGER's first flyby elucidate

204 nt with the presence of volcanic deposits on Mercury's surface.

205 ent larger than any previously identified on Mercury.

206 The origin of plains on Mercury, whether by volcanic flooding or impact ejecta p

207 on attributed to preferential resurfacing on Mercury.

208 The most heavily cratered terrains on Mercury have been estimated to be about 4 billion years

209 er the emplacement of the oldest terrains on Mercury.

210 cal data from other planets (Venus, Mars, or Mercury) and asteroids.

211 btained by the MESSENGER spacecraft orbiting Mercury indicate that the planet's surface differs in co

212 aircraft during the 2013 Nitrogen, Oxidants, Mercury, and Aerosol Distributions, Sources, and Sinks (

213 iversity of Washington-Detector for Oxidized Mercury, the University of Houston Mercury instrument, a

214 ome of the heavy metals including Lead (Pb), Mercury (Hg), Arsenic (As), Chromium (Cr) and Cadmium (C

215 o Ogygia as relating to the motion of planet Mercury.

216 ecame the first probe to fly past the planet Mercury in 33 years.

217 d by the University of Nevada, Reno-Reactive Mercury Active System (UNRRMAS, 1 Lpm) CEM and a Tekran

218 We show here that addition of a reduced Mercury-like body (or, alternatively, an enstatite-chond

219 anets orbiting them--ranging from metal-rich Mercury-sized planets to more hospitable volatile-rich E

220 MESSENGER's second Mercury flyby revealed a ~715-kilometer-diameter impact

221 ition Spectrometer during MESSENGER's second Mercury flyby revealed the presence of neutral magnesium

222 production has declined substantially since Mercury's formation, consistent with widespread volcanis

223 he innermost planet was Jupiter (rather than Mercury) sized, and its chaotic evolution was terminated

224 e report a planet significantly smaller than Mercury.

225 that do not orbit closer to their star than Mercury is to the Sun travel on highly elliptical paths.

226 his set of characteristics demonstrates that Mercury's weak magnetic field does not support Van Allen

227 These observations indicate that Mercury's magnetosphere is much more responsive to IMF d

228 The neutron data indicate that Mercury's radar-bright polar deposits contain, on averag

229 These features support the inference that Mercury's interior contains higher abundances of volatil

230 The encounter revealed that Mercury is a dynamic system; its liquid iron-rich outer

231 Observations by MESSENGER show that Mercury's magnetosphere is immersed in a comet-like clou

232 These observations suggest that Mercury has undergone complex differentiation like the o

233 surface Fe abundance, supports the view that Mercury formed from highly reduced precursor materials,

234 of nearly 24 million kilometers between the Mercury Laser Altimeter (MLA) aboard the MESSENGER (MErc

235 Observations by the Mercury Atmospheric and Surface Composition Spectrometer

236 00-kilometers-long profile of Mercury by the Mercury Laser Altimeter on the MESSENGER spacecraft span

237 ress these challenges, we have developed the Mercury analysis pipeline and deployed it in local hardw

238 During MESSENGER's first Mercury flyby, the Mercury Atmospheric and Surface Composition Spectrometer

239 Measurements from the Mercury Deposition Network (MDN) containing single rainf

240 ring MESSENGER's third flyby of Mercury, the Mercury Atmospheric and Surface Composition Spectrometer

241 ring MESSENGER's first flyby of Mercury, the Mercury Atmospheric and Surface Composition Spectrometer

242 ions are largest near the planet, but these Mercury-derived ions fill the magnetosphere.

243 MESSENGER's third Mercury flyby revealed a 290-kilometer-diameter peak-rin

244 , which describes plasma circulation through Mercury's magnetosphere, suggests that such circulation

245 atures imply that long-wavelength changes to Mercury's topography occurred after the earliest phases

246 gy and an updated dynamical extrapolation to Mercury, we find that the oldest surfaces were emplaced

247 physics of secular chaos and applying it to Mercury and to hot Jupiters.

248 d strengths that range from those similar to Mercury's present dipole field to Earth-like values are

249 e of orbit period to spin period, similar to Mercury's present state.

250 ocky with no atmosphere or water, similar to Mercury.

251 f these elements contribute substantially to Mercury's low and variable surface reflectance.

252 taking advantage of cloud computing and with Mercury implemented on the DNAnexus platform, we have de

253 ate from interactions of the solar wind with Mercury's space environment and through ionization of it

254 ethanol, N2O, and NH3 from a 2006 model year Mercury Grand Marquis flexible fuel vehicle (FFV) operat

255 A Zeeman Mercury analyzer Model RA-915(+) (Lumex, St.

256 A Zeeman Mercury analyzer Model RA-915(+) (Lumex, St. Petersburg,