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1 ona") as well as physisorbed proteins ("soft corona").
2 oteins forming what is known as the protein 'corona'.
3 Rosuvastatin Multinational Trial in HF-REF (CORONA).
4 statin Multinational Trial in Heart Failure (CORONA).
5 lease of magnetic energy stored in the Sun's corona.
6 the chemical composition of the SNA protein corona.
7 g a continuous layer visually appearing as a corona.
8 nostics for their presence in the nonflaring corona.
9 ydrophobic PPS core and PNIPAAM on the outer corona.
10 fic proteins that form the so-called protein corona.
11 ionic PGlu intermediate shell layer, and PEG corona.
12 ers with a 5kgmol(-1) methoxy-terminated PEG corona.
13 nsivity is endowed by a responsive polymeric corona.
14 % mannoside-terminated PEG chains in the PEG corona.
15 mechanisms in the Sun's outer atmosphere, or corona.
16 he inhomogeneous magnetic field of the solar corona.
17 ic particles akin to those seen in the solar corona.
18 the chromosphere but not, until now, in the corona.
19 a densely functionalized aptamer-displaying corona.
20 rresponding to radio wave propagation in the corona.
21 long the Sun's magnetic field lines into the corona.
22 erate the fast solar wind and heat the quiet corona.
23 or balance the radiative losses of the quiet corona.
24 the interface region between photosphere and corona.
25 is wave mode is sufficient to heat the solar corona.
26 of 50 to 150 kilometers per second into the corona.
27 - 12 gauss magnetic field measurement in the corona.
28 d size because of the formation of a protein corona.
29 metric poly(3-hexylthiophene) or polystyrene corona.
30 ) W m(-2)) is transferred onto the overlying corona.
31 iarm stars with boronic ester cores and PDMA coronas.
32 robrain natriuretic peptide (hazard ratio in CORONA, 1.50; 95% confidence interval, 1.17-1.92; P=0.00
33 ecreasing galectin-3 levels (hazard ratio in CORONA, 1.60; 95% confidence interval, 1.13-2.25; P=0.00
34 bsorb proteins to form 'nanoparticle-protein coronas', a process governed by molecular interactions b
36 planation for the composition of the protein corona, aiding in the development of safe and effective
38 e-art magnetohydrodynamic model of the solar corona and a model for the motion of emitting cometary t
39 er issues such as the formation of a protein corona and antibody multivalency interfere with the labe
40 to play a role in heating the million-degree corona and are associated with Alfvenic waves that help
43 s known about the atomistic structure of the corona and how it influences the phase behavior and prop
44 ausing energy exchange between the Sun's hot corona and its cool lower atmosphere remain poorly under
45 stigation of the temporal profile of protein corona and its evolution in biological matrices as well
46 The detailed morphology of the subgiant's corona and its possible interaction with its companion a
47 with lower HLB value, less dense hydrophilic corona and more hydrophobic core volume are efficient in
48 aining blocks with a homogeneous polystyrene corona and those with a patch-like polystyrene/poly(meth
49 ion region (between the chromosphere and the corona) and of the corona that reveal how Alfvenic motio
50 statin in Multinational Trial Heart Failure (CORONA) and the Gruppo Italiano per lo Studio della Sopr
51 old nanoparticle system packaged with a SipA corona, and found this bacterial mimic not only accumula
54 active sequences displayed from the particle corona, and the ability to easily encapsulate biologics
55 f NMs dictate the composition of the protein corona, and the toxicity of NMs and iv) NMs can affect s
56 in (44%) was comparable to that in the glans/corona, and type-specific positivity was observed betwee
57 f species-specific formation of biomolecular coronas, and this suggests that the use of representativ
59 is concluded that, regardless of the type of corona applied, CF(2)Br(2) reacts in air NTP via a commo
62 se To evaluate if the formation of a protein corona around ferumoxytol nanoparticles can facilitate s
64 ave profiled proteins forming the long-lived corona around silver nanoparticles (75 nm OECD reference
65 ntal data suggests that the microgels form a corona around the microspheres and induce a soft repulsi
67 a) chitosan nanoparticles, while it formed a corona around those composed of more densely cross-linke
69 e used to detect chemisorbed proteins ("hard corona") as well as physisorbed proteins ("soft corona")
71 served wave energy that is able to reach the corona based on observational constraints, which has imp
72 ofiles and to mechanistically understand the coronas' biological/ecological impact, we present a tier
73 sted of a N-(2-hydroxypropyl) methacrylamide corona block with pendent pyridyl disulfide groups for r
75 ufficient Poynting flux not only to heat the corona but also to originate the supersonic solar wind.
76 d not only to highlight the presence of this corona, but also to estimate its apparent thickness to a
78 L1) and coronal steric effects (via the PtBA corona chain length in the P segment, L2 related to the
79 namely coronal steric effects (via the PtBA corona chain) and attractive interaction strength (via t
80 PFS cylinders with a residual percentage of corona chains dependent on the photoirradiation time.
83 icelles with variable and spatially distinct corona chemistries, including amphiphilic nanostructures
84 ecific interactions between the nanoparticle-corona complex and the cell surface including triggering
89 his study explores the importance of protein corona composition for nanoparticle recognition by coelo
94 ischemic systolic heart failure enrolled in CORONA (Controlled Rosuvastatin Multinational Study in H
95 ardiac dysfunction and prognosis measured in CORONA (Controlled Rosuvastatin Multinational Trial in H
96 nt of Reduction in Mortality and Morbidity], CORONA [Controlled Rosuvastatin Multinational Trial in H
97 shown that the formation of protein-graphene corona could effectively reduce its cytotoxicity; howeve
98 -coil BCPs in solution and selective micelle corona cross-linking, we have created short (about 130 n
100 The structure and composition of the protein corona depends on the synthetic identity of the nanomate
101 sequently, we will discuss about the protein corona derived from blood with foci on the physiochemica
102 o reliably and easily estimate the detergent corona diameter and select the smallest size, critical f
106 of a solid needle which is commonly used for corona discharge creation, helping us to have direct axi
113 nerates up to +/-5 kV dc voltage to ignite a corona discharge plasma in air for up to 12 h of continu
114 omena linked to negative ionization, such as corona discharge, arcing, and electrospray destabilizati
115 ile nanocarriers with methoxy-terminated PEG coronas do not associate with cells, regardless of size.
116 ptake, a 1.8kgmol(-1) methoxy-terminated PEG corona does not sufficiently protect the nanocarriers fr
117 11 W3 (Lovejoy) passed deep within the solar corona, effectively probing a region that has never been
118 Therein, the C blocks form the stabilizing corona emanating from B compartments, which in turn resi
119 body) so that the composition of the protein corona evolves over time, iii) the physico-chemical char
120 polycyclic granulomas with large lymphocytic coronas, extensive emperipolesis of lymphocytes within m
121 ompared to nanoparticles without a dense PEG corona following local administration by either manual i
122 ld, we introduce the potential impact of the corona for NM-microbiome-(human)host interactions and th
123 main of thrombomodulin (TM) onto the micelle corona for the local generation of activated protein C,
126 nsional oligonucleotide structure on protein corona formation, we studied the identity and quantity o
127 gion of the proteins is then surrounded by a corona formed by these molecules, ensuring a hydrophilic
128 lythiophene block copolymer with a different corona-forming block to the resulting nanofibers led to
130 on of the composition and ratio of core- and corona-forming polymers (indirectly tuning PEGylation de
131 orporated BMA in both the polyplex core- and corona-forming polymers, resulting in robust endosomolys
133 oly(ferrocenyldimethylsilane) (PFS) block, a corona-forming segment of poly(2-vinylpyridine) (P2VP),
136 r sodium-specific fluorescence visualized by CoroNa-Green, a sodium-specific fluorophore, than the wi
137 The structural homology of the daffodil corona has remained a source of debate throughout the hi
139 ntities and amounts of the proteins in this "corona" have been thoroughly examined, the spatial arran
140 nteraction with the NP surface form a "hard" corona (HC), which is believed to mediate NP interaction
141 may influence the composition of the protein corona (i.e. they encounter different proteins on their
142 delivery is the quick formation of a protein corona (i.e., protein adsorbed on the nanoparticle surfa
146 comet C/2011 N3 (SOHO) within the low solar corona in five wavelength bands in the extreme ultraviol
147 totoxicity, pointing to the role of protein "corona" in conferring the biological impact of amyloidog
150 images and serial sections demonstrate that corona initiation occurs late in development, after the
152 pattern of the C-class gene NbAGAMOUS in the corona is more similar to that of the stamens than that
157 iew, we discuss the formation of the protein corona, its structure and composition, and its influence
158 of apolipoprotein AI (ApoAI) from Si NP hard coronas, leaving unaltered the dispersion physicochemica
159 t target the detection of airborne analytes, Corona/lens-based-collection provides a new path to achi
160 We engineered nanomedicine with the stealth corona made up of densely packed bone seeking ligand, al
163 segments provides a promising route to core-corona nanoparticles (micelles) with a wide range of pot
165 emically matched MSNP and highlights protein corona neutrality as an important design consideration w
166 timing and magnitude of upward motion to the corona observed 29 s after the event onset in 171 A by t
170 lts), which is ascribed to an accretion disk corona of energetic particles akin to those seen in the
173 observed that i) the composition of protein corona of NMs is likely to be dictated by their route of
174 nigma typically invoke the deposition in the corona of nonthermal energy generated by magnetoconvecti
177 ombination, our results demonstrate that the corona of the daffodil N. bulbocodium exhibits stamen-li
183 phine ligands immobilized within the soluble coronas of block copolymer micelles is found to induce i
184 low-degree nodes surrounded by hierarchical coronas of hubs, and are uncovered only through the opti
185 , we show that acquisition of a coating, or "corona", of NOM alters the hydrodynamic and electrokinet
190 We find that the presence of a serum protein corona on the tip strongly modifies the interaction as i
191 results demonstrate that the effects of NOM coronas on nanoparticle properties and interactions with
192 to other triblock comicelles with different coronas on the central or end segment where "cross" supe
194 ct of circumcision was stronger at the glans/corona (OR, 0.47; 95% CI, 0.37-0.60) and urethra (OR, 0.
195 a short time scale, described as a "dynamic" corona, others with higher affinity and long-lived inter
196 nteractions lead to the formation of protein coronas, particle wrapping, intracellular uptake and bio
199 l environments, NPs are coated by a 'protein corona' (PC), critically affecting physiological and the
201 In this work, we applied a new technique, corona phase molecular recognition (CoPhMoRe), to identi
202 tube by chemical adsorption, also form a new corona phase that exhibits highly selective recognition
203 f human blood proteins, revealing a specific corona phase that recognizes fibrinogen with high select
204 e transition also changes the observed SWCNT corona phase, modulating the recognition of riboflavin.
206 nic HPV, specifically localized to the glans/corona, possibly because of its proximity to the foreski
208 While a 5kgmol(-1) methoxy-terminated PEG corona prevents non-specific uptake, a 1.8kgmol(-1) meth
211 present study, a method to differentiate the corona proteins based on their relative dissociation rat
212 ong enough to penetrate into the Sun's inner corona provide information on the solar atmosphere and m
213 rls showed persistently lower FA in anterior corona radiata (ACR) (group, P = .04; group x age x sex,
215 dal cingulate (M4) motor regions through the corona radiata (CR), internal capsule (IC) and crus cere
216 (CC), superior longitudinal fasciculus (LF), corona radiata (CR), internal capsule (IC) and external
218 internal capsule, callosal isthmus, and the corona radiata (p=0.04 for FIQ and p=0.01 for PIQ, corre
219 -0.02 (P = .02); MD, beta = -0.01 (P = .03)] corona radiata and external capsule [right FA, beta = 0.
221 tions of the corpus callosum and beyond (eg, corona radiata and inferior longitudinal fasciculus) acr
222 tropy than control subjects in the posterior corona radiata and the optic radiation (P < 0.002).
223 ant differences also emerged in the anterior corona radiata as well as in white matter underlying the
227 matter (in corpus callosum, cingulum bundle, corona radiata, and superior fronto-occipital fasciculus
228 ingulum, fornix, stria terminalis, posterior corona radiata, and superior longitudinal fasciculus in
229 lum, fornix, and stria terminalis, posterior corona radiata, and superior longitudinal fasciculus.
231 onal anisotropy (optic radiations, posterior corona radiata, and the splenium region of the corpus ca
233 al superior longitudinal fasciculi, superior corona radiata, anterior thalamic radiations, and poster
234 of internal capsule, superior and posterior corona radiata, bilateral external capsule and the right
235 d increases in MD in the bilateral posterior corona radiata, bilateral superior longitudinal fascicul
236 was whole-brain FA in parts of the anterior corona radiata, external capsule, and cerebellum (P<0.05
237 9) evidenced higher FA in the right superior corona radiata, higher FA and AD in bilateral corticospi
238 or G carrier genotypes in the left and right corona radiata, left uncinate fasciculus, left inferior
239 ood ADHD in the right superior and posterior corona radiata, right superior longitudinal fasciculus,
240 tracts, specifically within right posterior corona radiata, right tapetum, and bilateral corpus call
241 um of corpus callosum, anterior and superior corona radiata, superior longitudinal and inferior front
242 in patients with NMO, mainly located in the corona radiata, uncinate fasciculus, corpus callosum, op
249 iffusivities in superior (SCR) and posterior corona radiatae (PCR) (group x age x sex, P = .002; grou
250 splenium of corpus callosum, left posterior corona radiate/posterior thalamic radiate, right superio
252 atmospheric pressure were investigated in a corona reactor energized by +dc, -dc, or +pulsed high vo
253 uced contraction of the poly(ethylene oxide) corona, reducing steric resistance between vesicles and,
254 ave been thought to reside in the peripheral corona region of the kinetochore, distal to microtubule
256 onent of the nanoparticle-associated protein corona renders the associated nanomaterials susceptible
258 evious observations of Alfvenic waves in the corona revealed amplitudes far too small (0.5 km s(-1))
259 tography from the Cold War-era 'Gambit' and 'Corona' satellite surveillance systems (1965-1969) with
260 le granulomas with subtle/absent lymphocytic coronas, sclerosis of the surrounding tissue, and polymo
261 he SAXS data were well-fitted by a detergent corona shaped in an elliptical toroid around the crystal
263 uch breaks also happened before the onset of corona, so they cannot be used as an adequate indicator
267 odel of the n-dodecyl beta-d-maltopyranoside corona surrounding aquaporin-0, the most abundant membra
268 D-Zwilch-ZW10 (RZZ) complex builds a fibrous corona that assembles on mitotic kinetochores before MT
269 is paradigm shifted for the chromosphere and corona that constitute the outer atmosphere, which is no
270 y bind to NMs, forming a protein/biomolecule corona that critically affects the NMs' (patho)biologica
272 interface region between the surface and the corona that is highly sensitive to the coronal heating m
273 tudy, we characterize changes in the protein corona that occur as DOTAP-based lipoplexes are formulat
275 at possess a dense polyethylene glycol (PEG) corona that prevents them from being trapped by adhesion
276 the chromosphere and the corona) and of the corona that reveal how Alfvenic motions permeate the dyn
277 he acquisition of a surface coating (protein corona) that is determined by the route of entry and phy
278 interface between the Sun's photosphere and corona, the chromosphere and transition region play a ke
280 m its spectrum), the high temperature of the corona (though the reason for the high temperature remai
283 ained magnetohydrodynamic model of the solar corona to calibrate heliospheric reconstructions based s
284 olyester layer for drug loading, a polar PEO corona to provide biocompatibility, and three different
286 h the right proportion of the flexible alkyl corona to the rigid core, mesomorphic behavior of one co
287 eric layers, i.e., the transition region and corona, to high temperatures is a long-standing problem
288 in a subset of 1452 patients enrolled in the CORONA trial, which included patients with HF, aged >/=6
289 statin Multinational Trial in Heart Failure (CORONA) trial (n=1329), and at baseline and at 6 months
291 erging zoonotic viruses, including SARS-like corona viruses, henipaviruses, and lyssaviruses, underst
295 idly coated by proteins, forming a so-called corona which may strongly modify their interaction with
297 riers protected by a hydroxyl-terminated PEG corona with J774 cells is size dependent, while nanocarr
298 s or spicules is accelerated upward into the corona, with much of the plasma heated to temperatures b
299 ed from magnetic reconnection in the tenuous corona, would cause a direct perturbation of the dense p
300 s from worm-like SES CCMs with a homogeneous corona yields triblock co-micelles almost quantitatively
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