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) exposure poses substantial risks to human h

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

13 Mercury (Hg) is a global pollutant released from both na

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

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

16 Mercury (Hg) is a highly toxic and widely distributed he

17 Mercury (Hg) is a naturally occurring element that bonds

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

19 Mercury (Hg) is a pervasive environmental pollutant and

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

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

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

23 Mercury (Hg) is an important environmental contaminant,

24 Mercury (Hg) is of particular interest as methylmercury

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

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

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

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

29 Mercury (Hg) methylation is a microbially mediated proce

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

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

32 Mercury (Hg) stable isotope fractionation has been widel

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

34 Mercury (Hg), a global contaminant, is emitted mainly in

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

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

37 Mercury accumulation in fish is a global public health c

38 Mercury and bromine leaching tests were conducted using

39 Mercury and its compounds are highly toxic and can cause

40 Mercury and ozone are rapidly removed from the atmospher

41 Mercury and the Moon both have tenuous atmospheres that

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

43 Mercury atoms, laser-ablated from an amalgam dental fill

44 Mercury BAFs are calculated as the fish Hg concentration

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

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

47 Mercury concentrations are enriched in southern latitude

48 Mercury concentrations in blood were not correlated with

49 Mercury concentrations in burbot in the Lena and Mezen R

50 Mercury concentrations in burbot in the Lena and Mezen R

51 Mercury concentrations in dragonflies differed among fam

52 Mercury concentrations in feathers also were uncorrelate

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

54 Mercury concentrations in leaves were monitored from eme

55 Mercury concentrations in surface precipitation follow a

56 Mercury concentrations in winter feathers were positivel

57 Mercury concentrations ranged between 10.4 and 1411 ng/g

58 Mercury concentrations ranged from 0.057 to 0.203 mug g(

59 Mercury concentrations up to 800 pM were observed in sha

60 Mercury contamination in food can pose serious health ri

61 Mercury content in two certified materials and in ten sa

62 Mercury diffusion in air offers a reasonable explanation

63 Mercury distribution in the oceans is controlled by comp

64 Mercury emissions from major point sources in the hotspo

65 Mercury emissions in North America have declined over th

66 Mercury emitted from dental amalgam may select for incre

67 Mercury exposure has been associated with a wide variety

68 Mercury has a global dayside exosphere, with measured de

69 Mercury has a particularly chaotic orbit and is in dange

70 Mercury has contaminated rivers worldwide, with health c

71 Mercury has the ability to bind to a variety of biomolec

72 Mercury has well-documented endocrine activity; however,

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

74 Mercury in fish was positively and significantly correla

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

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

77 Mercury in urine therefore represents a mixture of demet

78 Mercury increases previously associated with the mid-19t

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

80 Mercury is a contaminant of global concern that is trans

81 Mercury is a diversely bioaccumulating heavy metal pollu

82 Mercury is a global pollutant, and prenatal exposure is

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

84 Mercury is a highly toxic priority pollutant that can be

85 Mercury is a major contaminant in the Arctic marine ecos

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

87 Mercury is a potent neurotoxin for humans, particularly

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

89 Mercury is a toxic, bioaccumulating trace metal whose em

90 Mercury is a widespread contaminant in marine food webs,

91 Mercury is an automated, flexible, and extensible analys

92 Mercury is emanated in the course of various natural eve

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

94 Mercury is one of the primary contaminants of concern in

95 Mercury is surrounded by a tenuous exosphere that is sup

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

97 Mercury is widely distributed in aquatic ecosystems as a

98 Mercury isotope composition and sediment geochemical dat

99 Mercury isotope variations are small and result only fro

100 Mercury isotopic compositions of amphipods and snailfish

101 Mercury levels in biota are mainly controlled by the met

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

103 Mercury levels were measured in colonial waterbird eggs

104 Mercury methylation and/or demethylation have been obser

105 Mercury methylation occurred in solution and was a funct

106 Mercury methylation was inhibited ( approximately 80%) i

107 Mercury obtained from the diet accumulates in mammalian

108 Mercury poisoning and "hot filtration" experiments ruled

109 Mercury pollution is widespread globally, and strategies

110 Mercury pollution poses risks for both human and ecosyst

111 Mercury pulse injection tests on the sorbent material af

112 Mercury resistance mediated by mercuric reductase (MerA)

113 Mercury resistant bacteria have developed a system of tw

114 Mercury speciation showed significant connections to the

115 Mercury species concentrations for levels 2 and 4 of SRM

116 Mercury species extraction was achieved by microwave exp

117 Mercury species were determined using square wave anodic

118 Mercury species were measured on three Baltic Sea campai

119 Mercury stable isotope abundances were used to trace tra

120 Mercury stable isotope tracers were utilized to relate s

121 Mercury stocks in products rose from 700 tonnes in 2001

122 Mercury sulfide minerals are known to nucleate in anoxic

123 Mercury undergoes several transformations that influence

124 Mercury uptake in bacteria represents a key first step i

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

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

127 Mercury was not detected in any of the analyzed samples.

128 Mercury wet deposition also varies by geographic region

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

130 Mercury's images obtained by the 1974 Mariner 10 flybys

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

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

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

134 Mercury-capped platinum ultramicroelectrodes (Hg/Pt UMEs

135 Mercury-containing sulfhydryl modification agents (rho-h

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

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

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

139 Mercury-resistant bacteria express merA to convert highl

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

141 y Interplanetary Magnetic Field, based on 17 Mercury years of MESSENGER Magnetometer data.

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

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

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

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

146 shortly after its insertion into orbit about Mercury.

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

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

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

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

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

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

153 r airless bodies in our solar system such as Mercury and asteroids.

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

155 ing the source processes of the exosphere at Mercury, and the use of plasma spectrometers will be cru

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

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

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

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

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

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

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

163 re compared with those obtained using Direct Mercury Analyser (DMA).

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

165 etic flux rope, has been observed downstream Mercury, together with low energy solar wind.

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

167 alogs of all the solar system planets except Mercury.

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

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

170 conditions spanning over those expected for Mercury's core, and ex situ chemical analysis of recover

171 However, the estimated daily intake for Mercury and Arsenic exceeded the oral reference dose set

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

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

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

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

176 high temperature or extreme radiation (e.g. Mercury, Jupiter's moon Europa, near-Sun comets), as wel

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

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

179 of observational evidence of ring current in Mercury's magnetosphere, which has a significantly weake

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

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

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

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

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

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

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

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

188 ions of SERENA ion sensors nearby and inside Mercury's magnetosphere.

189 195 +/- 10 nanotesla-R(M)(3), where R(M) is Mercury's mean radius.

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

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

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

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

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

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

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

197 g protons are potentially present for all of Mercury's heliocentric distances, despite the relatively

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

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

200 uct of the global cooling and contraction of Mercury.

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

202 re, we present the observational evidence of Mercury's ring current by analysing particle measurement

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

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

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

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

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

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

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

210 ographic model of the northern hemisphere of Mercury.

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

212 le of volcanism in the geological history of Mercury.

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

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

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

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

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

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

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

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

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

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

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

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

225 and the high core-to-silicate mass ratio of Mercury.

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

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

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

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

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

231 radius fraction of 86 5%, similar to that of Mercury's interior.

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

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

234 The Minamata Convention on Mercury (ref. 1) is a global treaty to protect human and

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

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

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

238 nic Hg emissions (the Minamata Convention on Mercury) entered into force in 2017.

239 ess evaluation of the Minamata Convention on Mercury.

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

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

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

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

244 phases suggests their potential existence on Mercury and their magnetism may contribute to its presen

245 ent larger than any previously identified on Mercury.

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

247 on attributed to preferential resurfacing on Mercury.

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

249 er the emplacement of the oldest terrains on Mercury.

250 eilites formed in bodies as large as Mars or Mercury.

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

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

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

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

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

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

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

258 and the University of Nevada, Reno-Reactive Mercury Active System (UNR-RMAS) at a rural/suburban fie

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

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

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

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

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

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

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

266 e report a planet significantly smaller than Mercury.

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

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

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

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

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

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

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

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

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

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

277 Observations by the Mercury Atmospheric and Surface Composition Spectrometer

278 00-kilometers-long profile of Mercury by the Mercury Laser Altimeter on the MESSENGER spacecraft span

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

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

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

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

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

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

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

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

287 Detection of these waves throughout Mercury's highly eccentric orbit suggests the conditions

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

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

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

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

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

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

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

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

296 that the wave occurrence rate increases with Mercury's heliocentric distance.

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

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

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

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