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991.
Summary The analysis of spirits with a single stationary phase is still an unsolved problem; the two amyl alcohols, ethyl acetate
and acetal are not separated on a polar column, methanol and acetaldehyde coelute from an apolar column.
Trials with coupled columns of different polarities showed that optimum results were obtained with a 40 m capillary column,
comprising 6 m of Carbowax 20 M, 12 m of 1:1 Carbowax 20M:OV1 mixture and 30 m of PS 264.
Best results were achieved when a 1 m retention gap was used, injecting a small amount of sample and using a 7 cm syringe
needle. 相似文献
992.
The H2O and D2O chemical ionization (CI) mass spectra of selected methylhalides(CH3X, XF, CI) have been investigated at source temperatures from 330 to 500°K, and at total pressures from 01 to 1.1 Torr Hydronium (H3O+) ions, the reactant species formed that predominates in our source under these conditions, were found to promote a gas-phase nucleophilic substitution on the halogenated substrate by H2O, leading to CH3OH2+ (H2O)n (n = 0,1,2) ions. Occurrence of these substitution reactions, which are prevented under ICR conditions, provides direct evidence for contrasting ion reactivities under different experimental conditions, mainly due to the profound influence of the reaction environment on the formation of collision-stabilized intermediate species. 相似文献
993.
Estrella Escalona Platero Domenica Scarano Adriano Zecchina Giancarlo Meneghini Roberto De Franceschi 《Surface science》1996,350(1-3):113-122
The monolayer of CO molecules adsorbed at low temperature on highly sintered nickel oxide, gives rise to a very symmetric IR absorption band at 2136 cm−1 (θmax) with a full-width at half-maximum (FWHM) of 3.7 cm−1. This band shifts to higher frequenc upon decreasing the coverage, reaching the 2152 cm−1 value for θ→0. The observed shift is due to changes in the lateral interactions (dynamic and static) among the adsorbed molecules. The observed spectral simplicity implies that most of the adsorbed CO molecules occupy crystallographically identical sites with a similar environment. Moreover, the remarkably small half-width indicates that inhomogeneous broadening effects, due to surface defects, are very small and that NiO microcrystals behave as single crystals. The morphology of microcrystals has been studied by SEM, AFM and HRTEM techniques: it was concluded that the surface termination of the sample is mainly represented by the (100) and (111) faces. 相似文献
994.
Ionization potentials of small molecules are calculated by the MS Xα and LCAO Xα methods. The results are compared with the experimental values and the results of previous accurate calculations. The Xα method proves to be rather accurate and potentially superior to the HF method. Indication is found of a possible failure of the method in the fluoromethanes. The limitation of the MS Xα method is discussed. 相似文献
995.
Alberto Modelli Giuseppe Distefano Derek Jones Giancarlo Seconi 《Journal of Electron Spectroscopy and Related Phenomena》1983,31(1):63-73
The electron-transmission and He(I) photoelectron spectra of Si(CH3)3, Sn(CH3)3 and CH2Si(CH3)3 derivatives of thiophene and furan have been recorded. The first two substituents perturb the energies of the outer filled π orbitals and of the empty π* orbitals in opposite directions, causing a reduction of the HOMO/LUMO energy separation. The stabilization experienced by the π* MO's depends on their wavefunction coefficients at the site of substitution, and is attributed to interaction with low-lying empty orbitals of the substituent groups. The relatively small size (~ 0.4 eV) of this effect on the unoccupied ring MO's suggests that it should not appreciably affect the energy of the filled MO's.The strong conjugation between the π* unoccupied orbital of the nitro group and those of thiophene has also been investigated. 相似文献
996.
A combined pulse amplitude modulation (PAM) and pulse position modulation (PPM) technique is proposed and investigated as a feasible solution of the problem of line encoding in optical fibre communication systems. The basic idea is that of exploiting PAM and PPM jointly, to give rise to three different waveforms in one signalling period, without resorting to more than two signal levels. Some evaluations of the behaviour of this signalling format are reported in terms of coding efficiency, spectral density, timing information, and error probability. Alternative receiving schemes are also devised to improve system performance. 相似文献
997.
Vincenzo Barone Francesco Lelj Nino Russo Giancarlo Abbate 《Solid State Communications》1984,49(9):925-928
The MNDO semiempirical method has been used to study the structure of the (111) surface of diamond-like crystals employing two model clusters. Numerical results are in agreement with previous computations for the small X4H9 clusters and become very similar to experimental data when employing the larger X9H15 clusters. These latter clusters allow also the study of surface reconstruction. Our results suggest that the Haneman model of 2 × 1 reconstruction could be equally valid for silicon and diamond, but in the latter case the difference in vertical shifts is too small to be experimentally observed. 相似文献
998.
Summary The cosmic-ray power spectral density in the frequency band (5·10−8÷1·10−5) Hz has been estimated from data of mid- and high-latitude neutron monitors and low latitude ion chamber data. The power
spectral density in the band (1·10−11÷1·10−8) Hz for mid-latitude neutron data has been inferred from sunspot records. The spectra show an overallf
−2 behaviour with a plateau in the band (5·10−7÷1·10−6) Hz which we show to be due mainly to the Forbush decreases. The solar-rotation peaks are explained by the recurrence effect
of the same Forbush decreases. The spectra during solar maxima and minima have similar behaviour but differ by a factor of
10 in magnitude. Some anomalies and peaks in the spectrum may be attributed to semi-annual, annual and biannual waves.
Riassunto Si calcola una stima della densità spettrale di potenza dei raggi cosmici nella banda di frequenze (5·10−8÷1·10−5) Hz, facendo uso dei dati di stazioni con monitori di neutroni alle medie e alte latitudini e di stazioni con camere di ionizzazione alle basse latitudini. La densità spettrale di potenza nella banda (10−11÷10−8) Hz per le stazioni con monitori di neutroni alle medie latitudini è dedotta dalla serie delle macchie solari. Gli spettri mostrano una distribuzione generale della potenza del tipof −2 con un plateau nella banda (5·10−7÷10−6) Hz che si mostra essere dovuto principalmente alle decrescite d'intensità di tipo Forbush. I picchi in corrispondenza dei periodi di rotazione solare sono spiegati come dovuti alla ricorrenza di questi stessi eventi. Lo spettro di potenza durante i periodi di massima e minima attività solare mostra la stessa distribuzione in frequenza ma differisce di un fattore 10 in grandezza. Alcune anomalie e picchi nello spettro sono attribuiti all'onda annuale e semiannuale della intensità dei raggi cosmici.
Резюме Оценивается спектральная плотность космических лучей в области частот (5·10−8÷10−5) Гц, используя данные с нейтронных мониторов, расположенных на станциях на средних и высоких широтах, и данные с ионизационных камер, расположенных на станциях на низких широтах. Спектральная плотность в области (10−11÷10−8) Гц, с нейтронных мониторов на средних широтах, выводится из регистрации солнечных пятен. Полученные спектры обнаруживают обшую зависимость типаf −2 с плато в области (5·10−7÷10−6) Гц, которое, должно быть, связано с убываниями Форбуша. Пики, соответствующие периоду вращения Солнца, объясняются как рекуррентные эффекты убываний Форбуша. Спектр в течение периодов максимумов и минимумов солнечной активности обнаруживает аналогичное частотное поведение, но отличается в 10 раз по величине. Некоторые аномалии и пики в спектре могут быть приписаны полугодичным, годичным и двух-годичным волнам интенсивности космических лучей.相似文献
999.
Summary We report the design criteria and performance characteristics of a hollow-cathode tube developed especially for high-resolution
Doppler-free laser spectroscopy. It is simple to construct and is easily demountable. Narrow homogeneous line widths of refractory
and highly reactive-element transitions have been observed by applying intermodulated detection scheme.
To speed up publication, the authors of this paper have agreed to not receive the proofs for correction. 相似文献
1000.