R satellites

Figure 5.4 Part of the microwave spectmm of cyanodiacetylene. (The many satellite transitions in each group are due to the molecule being in not only the zero-point vibrational state but also a multitude of excited vibrational states.) (Reproduced, with permission, from Alexander, A. J., Kroto, H. W. and Walton, D. R. M., J. Mol. Spectrosc., 62, 175, 1967)...

Spencer, R. W., and Christy, J. R. (1992). Precision and Radiosonde Validation of Satellite Gridpoint Temperature Anomalies, Part 11 A Tropospheric Retrieval and Trends during 1979-90. Jonmai ofChmute 5 858-866. 

By measuring the relative intensities of satellite and main lines, the population ratio is obtained, if it can be assumed that the dipole moment and line strength is not appreciably different in the two cases. From the population ratio R, the energy interval AE is obtained from the Boltzmann law i.e.,... 

Myneni, R. B., Los, S. O. and Tucker, C. J. (1996). Satellite-based identification of linked vegetation index and sea surface temperature anomaly areas from 1982-1990 for Africa, Australia and South America, Geophys. Res. Lett. 23, 729-732. 

Stadler H, Skritek P, Sommer R et al (2008) Microbiological monitoring and automated event sampling at karst springs using LEO-satellites. Water Sci Technol 58 899-909... 

Consider drops of different sizes in a mixture exposed to a 2D extensional flow. The mode of breakup depends on the drop sizes. Large drops (R > Caa,tal/xcy) are stretched into long threads by the flow and undergo capillary breakup, while smaller drops (R Cacri,oV/vy) experience breakup by necking. As a limit case, we consider necking to result in binary breakup, i.e., two daughter droplets and no satellite droplets are produced on breakup. The drop size of the daughter droplets is then... 

Upon breakup, the filament breaks into a set of primary or mother drops whose sizes are, to a first approximation, proportional to R. The size of drops produced when the filament breaks can then be obtained from the distribution of R. Each mother drop produced upon breakup carries a distribution of satellites of diminishing size for example, each mother drop of radius r has associated with it one large satellite of radius r, two smaller satellites of radius i 2 four satellites of radius r(3), and so on. For breakup at rest, the distribution of smaller drops is a unique function of the viscosity ratio. 

Ge, J.P., Zhang, Q., Zhang, T.R. and Yin, Y.D. (2008) Core-satellite nanocomposite catalysts protected by a porous silica shell controllable reactivity, high stability, and magnetic recyclability. Angewandte Chemie International Edition, 47 (46), 8924-8928. 

An exception to this rule arises in the ESR spectra of radicals with small hyperfine parameters in solids. In that case the interplay between the Zeeman and anisotropic hyperfine interaction may give rise to satellite peaks for some radical orientations (S. M. Blinder, J. Chem. Phys., 1960, 33, 748 H. Sternlicht,./. Chem. Phys., 1960, 33, 1128). Such effects have been observed in organic free radicals (H. M. McConnell, C. Heller, T. Cole and R. W. Fessenden, J. Am. Chem. Soc., 1959, 82, 766) but are assumed to be negligible for the analysis of powder spectra (see Chapter 4) where A is often large or the resolution is insufficient to reveal subtle spectral features. The nuclear Zeeman interaction does, however, play a central role in electron-nuclear double resonance experiments and related methods [Appendix 2 and Section 2.6 (Chapter 2)]. 

Predictions we will only see the abundance trend in the one satellite that finally settles in a torus at our R the abundance trends will differ depending on the potential well of the satellite, it must be largish and not a dSph no age gap between thin and thick disk as thin disk is accreted also at early times Observations tight trends in kinematically selected samples so far all studied thick disk stars are older than thin disk stars... 

Cayrel R., Spite M., et al. 2005, ESO Astrophysics Symposia Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites , S. Randich and L. Pasquini eds. (this book). 

The EPR spectrum of 7 (R=CF3) AsFr, salt in S02, consisted of a central binomial septet due to coupling of 6 equivalent F atoms with one set of weak 33S satellites. Although trithiolylium cations contain two inequivalent sets of sulfur nuclei, only one set of 33S satellites were observed. Further studies with 7 (R=C02Me) however managed to resolve the 33S satellite into two components in 1 2 intensity ratio, consistent with the structure of a 1,2,3-trithiolylium radical cation.92... 

Rs Radar slant range from the satellite to the antenna footprint at range R... 

Because of the l/r dependence, the exchange interaction rapidly decreases with an increase in the difference between the principal quantum numbers of the impaired electrons and the core vacancy. Thus multiplet splitting is negligible in the Is spectra of paramagnetic transition metal compounds. On the other hand, shake-up intensity is essentially independent of the core level involved. Hence one can distinguish between shake-up and multiplet satellites by changing the principal quantum number of the core electron ionized76. ... 

Bidigare, R.R., and C.C. Trees. 2000. HPLC phytoplankton pigments Sampling, laboratory methods, and quality assurance procedures. Pp. 154-161 in Ocean Optics Protocols for Satellite Ocean Color Sensor Validation, Revision 2, J. Mueller and G. Fargion, eds., NASA Technical Memorandum 2000-209966. 

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