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1 effective properties (density, bulk modulus, wavenumber).
2 a Scorpii) near 12.3 micrometers (811 to 819 wavenumbers).
3 -active modes shifted to significantly lower wavenumber.
4 on the solvent as well as on the excitation wavenumber.
5 o have the free-electron mass at much larger wavenumbers.
6 ver the full range of irradiation angles and wavenumbers.
7 hs, each corresponding to different incident wavenumbers.
8 wer CH stretching frequencies by hundreds of wavenumbers.
9 e optical path differences for the dispersed wavenumbers.
10 plays a pronounced positive signal at higher wavenumbers.
11 ration shifted characteristic peaks to lower wavenumbers.
13 the N-N stretching vibration occur at lower wavenumbers (1260-1020 cm(-1)) than in the binary phases
15 A weak infrared absorption feature near 4141 wavenumbers (2.415 micrometers) in the spectrum of WL5,
16 tion speed of 4-7 m/s predicted by theory; a wavenumber-2 or -3 structure for the planetary-scale, lo
17 governing surface stability over a range of wavenumbers 4-5 times larger than has previously been ob
25 are sensitive to the flagellar beat pattern wavenumber and even to the asymptotically small modellin
26 asymmetric waves of higher amplitude, lower wavenumber and frequency propagating down the flagellum
27 singly, this motion is dominated by a single wavenumber and persists throughout the observation perio
29 m head morphology and flagellar beat pattern wavenumber are conducted and reveal that stable surface
31 e threshold absorbance peak shifted to lower wavenumbers as film thickness increased, which is consis
33 l differences at the band ascribed to a high-wavenumber beta-sheet component near 1693 cm-1 and the b
34 rates that the most active species is a high wavenumber (ca. 1685 cm-1) carbonate that we associate d
36 to the aniline amine were plotted versus the wavenumber (cm(-1)) for the lambdamax of the emission pr
37 nformations divided into three groups at 750 wavenumbers (cm-1)(A-->B, F), 1000 cm-1 [A-->C(2)], and
38 on, using partial least square regression in wavenumber combination of 1086-1056, 1343-1333, 1507-145
39 hifted by approximately 110 cm(-1) to higher wavenumbers compared to the parent tetracyano complexes
40 n bonding, the Raman intensity of the higher-wavenumber component of the canonical Fermi doublet is g
41 he possibility of transfer of energy to high wavenumber components in the condensate spatial profile.
42 ce of the secondary responses depends on the wavenumber content of a perturbation and the activity le
43 the partitioning of energy as a function of wavenumber, controls the phenomenology of force generati
44 with theoretical models also retaining full wavenumber-dependence, we find an excellent fit of the e
47 interaction eigenvalue problem for the axial wavenumber, fluid pressure, and vibratory relative motio
48 alpha and IIbeta leads to a downshift in the wavenumber for both the alpha-helix and beta-strand band
49 pectrum was analyzed with SIMCA 2 at reduced wavenumbers for the classification of LF as well as BF s
52 lop a simultaneous fingerprint (FP) and high-wavenumber (HW) confocal Raman spectroscopy and (ii) to
53 rint (FP) spectra (800-1800 cm(-1)) and high-wavenumber (HW) Raman spectra (2800-3600 cm(-1)) from th
54 entation of the transnasal image-guided high wavenumber (HW) Raman spectroscopy to differentiate tumo
55 The position of each bar matches the peak wavenumber in the corresponding spectrum but is independ
56 shift in the cyano stretch of 1 to a higher wavenumber in trifluoroethanol, which is consistent with
57 l space with axes representing the digitized wavenumbers, into readily visualizable two and three-dim
59 height of swimming sperm to the beat pattern wavenumber is sufficient to suggest the possibility that
60 This relation can be characterized by the wavenumber k and the particle radius r using the paramet
61 all scales, and a transition near horizontal wavenumber k(t) = f/NH, where f is the Coriolis paramete
62 Nonlinear sampling of the interferograms in wavenumber (k) space degrades the depth-dependent signal
64 dvection is dominated by Coriolis forces for wavenumbers l < 60, with Rossby numbers smaller than app
66 a 25 mm radius hemisphere in terms of S/N at wavenumbers less than ca. 1400 cm(-1) despite the weaker
68 surface to absorb or reflect light is due to wavenumber matching requirements at the metal-sample int
69 the non-hydrogen-bonded phenoxyl, the lower-wavenumber member of the Fermi doublet loses most of its
70 an peak intensities of the higher- and lower-wavenumber members of the doublet) is diagnostic of spec
71 estimates for N, f, and H give a transition wavenumber near that observed, and numerical simulations
74 gher hydrophobicity with higher amplitude at wavenumber of 2874-2926 cm(-1) and 1731-1742 cm(-1) than
76 by plotting the absorption maxima versus the wavenumber of a Raman band found in the range 1610-1655
77 S)-NADD, there is an 11 cm-1 decrease in the wavenumber of the C4-D stretching band (nuC-D) and a 50%
78 le in tuning, the frequency variation of the wavenumber of the cochlear traveling wave was measured (
79 y predicted to be true for reductions in the wavenumber of the flagellum beat, but not universally so
80 infrared spectroscopy observes the change in wavenumber of the NO ligand band accompanying the isomer
82 rd propagation of planetary-scale waves with wavenumbers of 1 and 2, subsequently weakening the strat
84 patial information on NV electronic spins in wavenumber or 'k-space' followed by a fast Fourier trans
85 active phonons at approximately 100 and 300 wavenumbers pertaining to the lead-halide framework and
86 e an increase in CH(2) band heights and peak wavenumber positions indicated a further disordering of
87 1)) were analyzed, and band heights and peak wavenumber positions were assessed as a function of mono
88 o the full range of experimentally-available wavenumbers q, we extract the linear amplification rate
91 l differences in the CH region of HWVN (high-wavenumber) Raman spectra between melanoma and benign me
92 tion (QRA) of synoptic-scale waves with that wavenumber range becoming trapped within an effective mi
93 system acquired hyperspectral images in the wavenumber range of 102-2538 cm(-1) for a 25 x 25 mm(2)
96 in the range of 70-100nm, NIR spectra in the wavenumber range of 4000-7500cm(-1) and UV-Vis spectra i
97 laser source and the detection of a certain wavenumber range of the vibrational spectrum to differen
98 alth of information is contained in the high wavenumber range using 71 patients on a breast tissue mi
99 conformation spectra provide characteristic wavenumber ranges for the amide NH stretch fundamentals
101 e equally shifted for all materials to lower wavenumbers relative to its noninteracting value in carb
103 results based on Raman intensity variation, wavenumber shift, and linewidth broadening all give cons
105 und algorithm for optimal selection of a few wavenumbers, spectral phasor analysis provides a robust
106 ere for three recently introduced wavelength/wavenumber Standard Reference Materials (SRMs): SRM 2035
107 ponent suggests intensities at the following wavenumbers to be representative of nonplayable tapes: 1
108 the FT-IR chemical imaging, which has a high-wavenumber transmission window allowing measurement of t
109 smission mode with the same focus across all wavenumber values and simultaneous improvement in spatia
113 s obtained are in focus only at a particular wavenumber while they are defocused at other wavenumber
114 For beta-sheet content predictions, 580 wavenumbers within the amide I, II, A, and B and the C-H
115 alpha-helix content prediction utilized 120 wavenumbers within the amide I, II, A, B, and IV and the
116 y blotting and the acquisition of distance x wavenumber x intensity three-dimensional TLC-SERS plots.
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