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1 s as counterions, forming the so-called "ion atmosphere".
2 perature, and oxygen content in the reaction atmosphere.
3 s when compared to fruits kept in an ambient atmosphere.
4 ks for forests growing in a hotter and drier atmosphere.
5 eoroids tend not to survive entry to Earth's atmosphere.
6 (-1) of Se transferred from land through the atmosphere.
7 -term temporal trends of POPs in the African atmosphere.
8 or volatile carbon compound emissions to the atmosphere.
9 produced by vegetation and released into the atmosphere.
10 o metallic pouches with cover brine or N(2) atmosphere.
11 mages free-floating aerosol particles in the atmosphere.
12 ns through injections of soot into the upper atmosphere.
13 processes which impede equilibrium with the atmosphere.
14 ity to image through fog, rain, dust, or the atmosphere.
15 ise in oxygen concentration in Earth's early atmosphere.
16 ntributor of greenhouse gas emissions to the atmosphere.
17 SSA are an important source of PFAAs to the atmosphere.
18 y reshaped the composition of the oceans and atmosphere.
19 -methane hydrocarbon emitted into the global atmosphere.
20 ll as the rate of carbon accumulation in the atmosphere.
21 mposition and can become a large flux to the atmosphere.
22 of volatile organic compounds (VOCs) to the atmosphere.
23 (oxic) CH(4) production and emission to the atmosphere.
24 o the buildup of greenhouse gases in Earth's atmosphere.
25 qually on constituent parts of the planetary atmosphere.
26 to global change, exposing sediments to the atmosphere.
27 issions of reactive gaseous N forms into the atmosphere.
28 act movement of carbon between soils and the atmosphere.
29 ng the longwave radiative cooling within the atmosphere.
30 ciles anaerobic N(2) fixation with O(2)-rich atmosphere.
31 on of SMSIR upon treatment under a reductive atmosphere.
32 s a real detection of light scattered by the atmosphere.
33 Hg by vegetation, which depletes Hg from the atmosphere.
34 tic solution to curb its accumulation in the atmosphere.
35 affects the chemistry and composition of the atmosphere.
36 lived greenhouse gas that accumulates in the atmosphere.
37 nt biological source of sulfur to the marine atmosphere.
38 nstrained source of methane emissions to the atmosphere.
39 as measurement of vocalizations in a heliox atmosphere.
40 pathway for the fate of benzoic acid in the atmosphere.
41 edstock to repeatedly capture CO(2) from the atmosphere.
42 ng aorta and open the aortic arch vessels to atmosphere.
43 igher than typically measured in the outdoor atmosphere.
44 sing the transfer of biolabile soil C to the atmosphere.
45 sed on anthropogenic changes in land use and atmosphere.
46 s are continuously releasing nitrogen to the atmosphere.
47 e concentration of O(2) in the Archean upper atmosphere.
48 xidation to reach the levels observed in the atmosphere.
49 urces and pathways for AOSC formation in the atmosphere.
50 rt a vital role for methane in Earth's early atmosphere.
51 kg of H(2)O vapour instantaneously into the atmosphere.
52 sms are ubiquitous and highly diverse in the atmosphere.
53 with an increased abundance of oxygen in the atmosphere.
54 b-glacial lakes where they are sealed to the atmosphere.
55 o migrate into groundwater reservoirs or the atmosphere.
56 osely with the water-holding capacity of the atmosphere.
57 s of nanocrystal (NC) size, temperature, and atmosphere.
58 cing the release of accumulated CO(2) to the atmosphere.
59 and pH increases as pCO(2) increases in the atmosphere.
60 ling SOA formation and growth in the ambient atmosphere.
61 of organic compounds from seawater into the atmosphere.
62 r or pass through groundwater systems to the atmosphere.
63 ed by astronauts on missions outside Earth's atmosphere.
64 ring from electrical contractions in an O(2) atmosphere.
65 mation of overall C release from soil to the atmosphere.
66 ion of natural sulfur released to the marine atmosphere.
67 constraints on the dynamics of the sub-cloud atmosphere.
68 for later volcanic outgassing to revive the atmosphere.
69 medium under a 1 atm carbon dioxide (CO(2)) atmosphere.
70 erto unrecognized precursors of AOSCs in the atmosphere.
71 b, whereas cleavage releases sulfur into the atmosphere.
72 and long-term shelf stability under nitrogen atmosphere.
73 non compared to other noble gases in Earth's atmosphere.
74 tigate rising concentrations of CO(2) in the atmosphere.
75 igmatic electrical discharges in the Earth's atmosphere.
76 ertain sources of methane emissions into the atmosphere.
77 portant implications for their corresponding atmospheres.
78 ovide quantitative measurements of their ion atmospheres.
79 a at 10 K when prepared under N(2) versus Ar atmospheres.
80 elevant to both combustion and circumstellar atmospheres.
81 ubsequently formed mantles and the overlying atmospheres.
82 l) winds dominate the bulk flow of planetary atmospheres.
83 ion at pressures between one and hundreds of atmospheres.
86 pyridine solutions of 4a under H(2) and D(2) atmospheres (150 psi), which leads to the exclusive form
88 vidence for rocky material floating in their atmospheres(5), in warm debris disks(6-9) or orbiting ve
89 ed increase in global methane (CH(4)) in the atmosphere, accompanied by a decrease in its (13)C/(12)C
90 on from cobalt alkyls occurred under an N(2) atmosphere, alkylation of (R,R)-((iPr) DuPhos)Co(CO)(2)
91 minal NRP opening the aortic arch vessels to atmosphere allows collateral flow to be diverted away fr
92 , our results show that gas leakage into the atmosphere also occurred directly from the tunnel portal
93 errestrial vegetation removes CO(2) from the atmosphere; an important climate regulation service that
94 ctions of diphenyl ether under H(2) and D(2) atmosphere and a positive dependence of the rate on H(2)
95 dine-bearing molecules are ubiquitous in the atmosphere and a source of new atmospheric aerosol parti
97 fuel combustion into the air, they warm the atmosphere and contribute to millions of premature death
98 naerobic methanotrophy) may feed back to the atmosphere and destabilize the climate, triggering a tra
100 n activities and by nitration of PAHs in the atmosphere and may be equally or more toxic, but their s
107 s, and conduits for gas exchange between the atmosphere and soil, and effectively link these terrestr
108 ion of NHCs-based SAMs either requires inert atmosphere and strong base for deprotonation of imidazol
110 of CO(2) budget, CO(2) exchanged between the atmosphere and terrestrial biosphere, are necessary to b
111 (3) ) emissions from fertilized soils to the atmosphere and the subsequent deposition to land surface
112 nsport of energy and momentum throughout the atmosphere and their parameterization or simulation in n
113 including the composition of oceans and the atmosphere and thus the climate, the microbial world is
115 for land management to remove CO(2) from the atmosphere and understanding the processes responsible f
116 al Gas and Ion Mass Spectrometer on the Mars Atmosphere and Volatile Evolution spacecraft, we demonst
117 the metal surface protects it from corrosive atmospheres and carbon (carburization), thus allowing Fe
119 s as much carbon as currently resides in the atmosphere, and it is critical to understand how soil gr
120 h site density (up to 5 wt %) under reducing atmosphere, and its unique catalytic performance for hyd
121 and dry deposition remove aerosols from the atmosphere, and these processes control aerosol lifetime
122 duce substantial carbon (C) emissions to the atmosphere, and thus trigger a positive feedback to clim
124 n, we report the characterization of the ion atmosphere around DNA using NMR spectroscopy and directl
126 he measured disparity in ion composition and atmospheres around each homopolymer, revealing a complex
129 l concern that is transported throughout the atmosphere as elemental mercury Hg(0) and its oxidized f
130 es in the vertical distribution of Hg in the atmosphere as Mount Bachelor received free tropospheric
131 riginating near the 5-bar level of Jupiter's atmosphere (assuming photon scattering from points benea
132 follow the trajectory of many spores in the atmosphere at different times of day, seasons, and locat
133 and can withstand water pressure of about 20 atmospheres (atm) for the species Sepia officinalis Curr
134 model of plant hydraulics into the Community Atmosphere Biosphere Land Exchange (CABLE) land surface
137 The introduction of oxygen into the Earth's atmosphere brought challenges for the microbes that had
138 rogen is the main constituent of the Earth's atmosphere, but its provenance in the Earth's mantle rem
139 nts while increasing their water loss to the atmosphere, but the effects on C gain might diminish ove
140 cs are considered as their precursors in the atmosphere, but the mechanism for the formation of these
141 issions, there will be more CO(2) in Earth's atmosphere by 2025 than at any time in at least the last
142 nisms of P2-Na(x)TmO(2) in different ambient atmospheres by using various microscopic/spectroscopic c
143 Pa, 0 degrees C, and a CO(2)-enriched anoxic atmosphere (called low-PTA conditions) was tested on fiv
145 olcanic activity occurring in tropical moist atmospheres can promote deep convection and trigger volc
146 amined Holocene sea ice, moisture, and ocean-atmosphere circulation in Arctic Alaska, limiting our un
147 of SCA at MLO was elusive according to land-atmosphere CO(2) flux estimated by DGVMs and atmospheric
148 Time-resolved estimates of global ocean-atmosphere CO(2) flux provide an important constraint on
150 Here we calculate a time history of ocean-atmosphere CO(2) fluxes from 1992 to 2018, corrected for
151 releasing large quantities of GHGs into the atmosphere (CO(2) and CH(4) ) when subjected to anthropo
156 cost of water transport along the soil-plant-atmosphere continuum increases as water available in the
159 highlights the importance of including land-atmosphere coupling, which can alter deforestation-induc
161 of a respiratory quotient dynamic controlled atmosphere (DCA - RQ), which induces ethanol production
165 n the elemental and oxidized Hg forms in the atmosphere determines the scale and geographical pattern
166 ar hydrogen produced from water in the lower atmosphere diffuses into the upper atmosphere where it i
167 erature and, key to this study, CO(2) in the atmosphere) do not drive carbon isotope discrimination.
169 Controlled exposure of the device to ambient atmosphere during a long-term (1000 h) test does not deg
170 the forest was a net source of CO(2) to the atmosphere during every year of measurement with annual
172 ns of tons of mineral dust released into the atmosphere each year provide an important surface for re
174 eleased from bottom sediments that reach the atmosphere (ebullition); spring release of CH(4) trapped
176 very profitable for the analysis of gaseous atmospheres, especially when used as detector for FIA in
178 etween 29 and 36 Gg of Se are emitted to the atmosphere every year, doubling previous estimates of em
179 ar-weight atmosphere using a simple model of atmosphere evolution (including atmosphere loss to space
182 nd transport of radioactive materials in the atmosphere following a nuclear incident (explosion or re
183 e consequences of early loss of a thick H(2) atmosphere for subsequent occurrence of a high-molecular
187 tudy has quantified net GHG removal from the atmosphere from a seagrass restoration project, which wo
188 nveniently performed without use of an inert-atmosphere glovebox, as demonstrated across several case
190 packing conditions (cover brine, air or N(2) atmosphere) has been studied to preserve black ripe oliv
191 discharges to desired targets in the ambient atmosphere have been a subject of intense research effor
192 on CFCs, as unexplained source inputs to the atmosphere have been recently reported, and the potentia
193 t global mean rainfall increases in a warmer atmosphere; however, dynamical effects may result in mor
194 rocks to examine changes in the Late Archean atmosphere immediately prior to the Great Oxidation Even
195 gas transfer between soils or plants and the atmosphere in field settings where exogenous tracer appl
196 cks the fossil carbon and places it into the atmosphere, in longevity, as aerial carbon - carbon diox
197 n bionanoparticle interaction with a bipolar atmosphere induced, e.g., by a radioactive alpha-particl
198 do not form long-lived high-molecular-weight atmospheres; instead, they are lost to space alongside H
199 -time of the extratropical-tropical ocean-to-atmosphere interaction process, especially for the first
200 ese oscillations resulted from complex ocean-atmosphere interactions in the Nordic seas, caused by th
201 n global-scale models to better predict land-atmosphere interactions under future climate change.
202 wind effects and the associated fire-canopy-atmosphere interactions while considering prescribed bur
203 een local climate, vegetation, and ecosystem-atmosphere interactions, with likely local-to-regional i
208 agmatic pulse injected into the end-Triassic atmosphere is comparable to the amount of anthropogenic
209 quantifying the emissions of toxins into the atmosphere is crucial for evaluating the health conseque
210 seous exchange between the leaf and external atmosphere is governed by stomatal conductance (g(s)); t
214 We find that p-type doping in HCl/H(2)O atmosphere is related to the rearrangement of sulfur ato
215 em, metabolic gas exchange directly with the atmosphere is unlikely and could mostly occur through th
216 e that were formed with thick H(2)-dominated atmospheres lack high-molecular-weight atmospheres today
217 atological cycle may develop in the Amazonia atmosphere-land-ocean coupled system, favouring more ext
218 ple model of atmosphere evolution (including atmosphere loss to space, magma ocean crystallization, a
219 c aerosols at the most abundant sizes in the atmosphere (<1 mum) is analytically challenging, as hund
220 udy suggested that inert or inhibitor baking atmosphere may help prevent the Maillard reactions in ba
221 the database design accommodates other soil-atmosphere measurements (e.g. ecosystem respiration, cha
222 nthesis is being lost from ecosystems to the atmosphere more quickly over time, with important implic
225 ty, using a vegetation model (LPX) driven by Atmosphere-Ocean coupled General Climate Model climate r
226 lation (ENSO) is highly dependent on coupled atmosphere-ocean interactions and feedbacks, suggesting
234 onset and timing of the human impact on the atmosphere of the "roof of the world" remains poorly con
235 thium, sodium, potassium, and calcium in the atmosphere of the white dwarf Gaia DR2 43536074508603050
236 scenarios can be compared to observations of atmospheres of rocky exoplanets, potentially broadening
237 Pulse-like carbon dioxide release to the atmosphere on centennial time scales has only been ident
238 st) century, and the impact of extratropical atmosphere on the tropics has intensified during the pas
239 l billion years, implying that any remaining atmosphere on TOI-849b is likely to be enriched by water
240 cts of different pretreatment conditions and atmosphere on yield and oxidative stability of lipids fr
241 that in order to find high-molecular-weight atmospheres on warm exoplanets orbiting M-stars, we shou
244 full-spectrum simulated sunlight in ambient atmosphere, our unencapsulated and encapsulated cells re
246 acts of airborne bacteria found in the lower atmosphere over the Southern Ocean (SO) on the ecology o
249 PM(0.3) removal), low air resistance (<0.09% atmosphere pressure), high transparency (>82%), and rema
250 f Cu, Zr, and ZrCuAg alloy in a fluorine gas atmosphere provided by an in situ gas injection system (
251 he most abundant strong oxidant in the upper atmosphere, rather than O(2) But data from shock tube ex
252 individual and co-occurring chemicals in the atmosphere relate to altered expression of critical gene
253 of segregation for a given overpotential and atmosphere relevant to the operating conditions of perov
254 ce for oxygenic photosynthesis appeared, the atmosphere remained anoxic for hundreds of millions of y
256 radio terahertz wireless communication, the atmosphere reshapes terahertz pulses via group velocity
258 e controlled by partial equilibrium with the atmosphere resulting in relatively low DIC and high Omeg
260 mplacement of CAMP using the long-term ocean-atmosphere-sediment carbon cycle reservoir (LOSCAR) mode
261 on the path toward another Earth is to find atmospheres similar to those of Earth and Venus-high-mol
262 greatly impacted the composition of Earth's atmosphere since the evolution of oxygenic photosynthesi
267 is instead transported directly to the upper atmosphere, then dissociated by ions to produce atomic h
268 , freshwater, and marine ecosystems with the atmosphere, thereby regulating their size and reactivity
270 l energy, or the diffusion of CO(2) from the atmosphere through the stomata, and ultimately into the
271 ia oxidative C-C bond cleavage under an O(2) atmosphere to deliver the target molecules in high yield
272 ergy demands, as it can utilize CO(2) in the atmosphere to provide the required feedstocks for indust
276 equent occurrence of a high-molecular-weight atmosphere using a simple model of atmosphere evolution
277 )AlTaO(6))(0.7)} (LSAT) substrates in oxygen atmosphere using pulsed laser deposition technique.
279 e that lakes were constantly losing N to the atmosphere via denitrification and/or anammox, suggestin
280 similated via GPP is quickly returned to the atmosphere via respiration, we ask a critical question-c
281 f the extra carbon was emitted back into the atmosphere via several respiratory fluxes, with increase
282 dox profiles also suggest that Earth's early atmosphere was dominated by CO(2) and H(2)O, in contrast
285 at natural geological CH(4) emissions to the atmosphere were about 1.6 teragrams CH(4) per year, with
286 the lower atmosphere diffuses into the upper atmosphere where it is dissociated, producing atomic hyd
287 ed mainly in its elemental form Hg(0) to the atmosphere where it is oxidized to reactive Hg(II) compo
288 OA pollution sources in the offshore marine atmosphere, where continental and marine air pollutants
289 eleased from the target and ejected into the atmosphere, where it circulated the globe within a few h
290 ult from the transport of water to the upper atmosphere, where it is dissociated to hydrogen and esca
291 ures ranging from 100 million to 450 million atmospheres, where the understanding of white dwarf phys
292 sulfate aerosols and dust into Earth's upper atmosphere, which cooled and darkened the planet-a scena
294 t loss since 2000 warmed and dried the lower atmosphere, which reduced moisture recycling and resulte
295 ain photoproduct of Hg(II) photolysis in the atmosphere, which significantly increases the lifetime o
296 te is central to the chemical composition of atmospheres while factors such as planetary mass, therma
297 he deleterious influences of isoprene on the atmosphere, while sustaining woody biomass production in
299 iently enhance carbon sequestration from the atmosphere with a rate as high as 8 [Formula: see text]
300 evealed(4) an extended, X-ray-bright gaseous atmosphere with a virial temperature of 60 million Kelvi