@article {904,
	title = {"Spectrum-only" assignment of core-penetrating and core-nonpenetrating Rydberg states of calcium monofluoride},
	journal = {Canadian Journal of Chemistry-Revue Canadienne De Chimie},
	volume = {82},
	number = {6},
	year = {2004},
	note = {ISI Document Delivery No.: 861XATimes Cited: 3Cited Reference Count: 38},
	month = {Jun},
	pages = {791-803},
	type = {Article},
	abstract = {Rydberg states of calcium monofluoride in the n* = 17-20 region have been observed by ionization-detected optical-optical double-resonance spectroscopy via the D(2)Sigma(+) v = 1 intermediate state. All members of the six core-penetrating Rydberg series in the n* = 17-20 region and several components of the 17f and 17g core-nonpenetrating Rydberg states have been assigned. While the assignment of core-penetrating Rydberg states is straightforward without use of an effective Hamiltonian model, "spectrum-only" assignment of core-nonpenetrating states is complicated because strong l-uncoupling causes the core-nonpenetrating states to evolve rapidly from Hund{\textquoteright}s case (b) to Hund{\textquoteright}s case (d) coupling. We describe "spectrum-only" assignment procedures, developed in the spirit of Gerhard Herzberg, that can be used to assign optical-optical double-resonance spectra of core-penetrating and core-nonpenetrating Rydberg states using only information contained in the spectrum rather than predictions derived from an effective Hamiltonian model. The ambiguities that arise in the assignment of each class of states are discussed in detail.},
	keywords = {ANGULAR-MOMENTUM STATES, AUTOIONIZATION, CaF, DECAY DYNAMICS, electric quadrupole moment, EXCITED-STATES, HIGHER, IONIZATION, laser spectroscopy, MAGNETIC-FIELD, NO, QUANTUM-DEFECT THEORY, Rydberg states, TRIPLE-RESONANCE SPECTROSCOPY},
	isbn = {0008-4042},
	url = {<Go to ISI>://000224450700014},
	author = {Kay, J. J. and Byun, D. S. and Clevenger, J. O. and Jiang, X. and Petrovi, V. S. and Seiler, R. and Barchi, J. R. and Merer, A. J. and Field, R. W.}
}
@article {4882,
	title = {Structure formation in dipolar fluids driven by rotating fields},
	journal = {Journal of Chemical Physics},
	volume = {112},
	number = {22},
	year = {2000},
	note = {ISI Document Delivery No.: 319MVTimes Cited: 9Cited Reference Count: 18},
	month = {Jun},
	pages = {9828-9833},
	type = {Article},
	abstract = {The influence of rotating fields on strongly interacting dipolar fluids is investigated using molecular dynamics and Brownian dynamics simulations. Both one-component and two-component systems are considered. It is shown that under certain conditions rotating fields can induce spatial layering in these systems. This behavior is similar to that recently observed in experimental studies of electrorheological and magnetorheological fluids. The binary mixture results are particularly interesting. It is shown that components that differ only in their moments of inertia can be separated by adjusting the frequency of the applied field. (C) 2000 American Institute of Physics. [S0021-9606(00)50822-8].},
	keywords = {BIAXIAL FIELD, COMPOSITES, DROPLET, DYNAMICS, MAGNETIC-FIELD, SIMULATION},
	isbn = {0021-9606},
	url = {<Go to ISI>://000087346500019},
	author = {Murashov, V. V. and Patey, G. N.}
}
@article {3810,
	title = {Nonthermal escape of the atmospheres of Venus, Earth, and Mars},
	journal = {Reviews of Geophysics},
	volume = {34},
	number = {4},
	year = {1996},
	note = {ISI Document Delivery No.: VU919Times Cited: 37Cited Reference Count: 188},
	month = {Nov},
	pages = {483-505},
	type = {Review},
	abstract = {Atmospheric loss from planetary atmospheres is an important geophysical problem with implications for planetary evolution. This is a multidisciplinary research field that requires an expertise in a wide range of subjects including statistical mechanics, fluid mechanics, plasma physics, collision theory, and surface science. This paper is a review of the current state of our understanding of atmospheric loss from the terrestrial planets. A detailed discussion is provided of the basic concepts required to understand the processes occurring in the high-altitude portion of a planetary atmosphere referred to as the exosphere. Light atomic species with sufficient translational energy can escape from an atmosphere. The translational energy required for escape could be thermal energy and proportional to the ambient temperature or the result of some collisional processes energizing the species above thermal energies. These collisional processes, which include charge exchange and dissociative recombination between energetic ions, neutrals, and electrons, are referred to as nonthermal escape processes. We highlight the similarities and differences in the important escape mechanisms on the terrestrial planets and comment on application of these mechanisms to evolutionary theories of the terrestrial atmospheres. The emphasis in this paper is directed toward the need to consider the exosphere as collisional.},
	keywords = {CHARGE-EXCHANGE, dissociative recombination, FRACTIONATION, HOT OXYGEN GEOCORONA, MAGNETIC-FIELD, MAGNETOHYDRODYNAMIC MODEL, MARTIAN ATMOSPHERE, mass, MULTISPECIES, NITROGEN-ATOMS, SOLAR-WIND INTERACTION, ULTRAVIOLET SPECTROMETER EXPERIMENT},
	isbn = {8755-1209},
	url = {<Go to ISI>://A1996VU91900004},
	author = {Shizgal, B. D. and Arkos, G. G.}
}
