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Nathan C. Hearn Tomasz Plewa R. Paul Drake Carolyn Kuranz 《Astrophysics and Space Science》2007,307(1-3):227-231
We present two- and three-dimensional simulations involving Richtmyer–Meshkov and Rayleigh-Taylor instabilities run with the
adaptive mesh refinement code, flash. Variations in the rate of mixing layer growth due to dimensionality, perturbation modes,
and simulation resolution are explored. These simulations are designed for detailed comparisons with experiments run on the
Omega laser to gain understanding of the mixing processes and to prepare for validation of the Flash code. 相似文献
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Crustal structure of central Tibet as derived from project INDEPTH wide-angle seismic data 总被引:6,自引:0,他引:6
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Soft X-rays (0.1–0.8 keV) from the region including the Oph dark cloud were observed with the SAS-3 low-energy X-ray telescope. No X-ray absorption by the cloud was observed. This indicates that the diffuse component of soft X-rays in this region is mostly from the foreground of the Oph cloud which is located at a distance of 160–200 pc. 相似文献
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Elizabeth H. Hearn 《Geophysical Journal International》2003,155(3):753-777
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W.M. Irvine Z. Abraham M. AHearn W. Altenhoff Ch. Andersson J. Bally W. Batrla A. Baudry D. Bockelée-Morvan G. Chin J. Crovisier I. de Pater D. Despois L. Ekelund E. Gerard T. Hasegawa C. Heiles J.M. Hollis A. Wootten 《Icarus》1984,60(1):215-220
Detections and upper limits to the continuum emission (1 ≤ λ ≤6 cm) and spectral line emission (OH, CO, CS, HCN, HCO+, CN, CH3CN, CH3C2H, NH3, H2O, HC3N, CH3CH2CN) are reported from radio observations of Comets 1983d and 1983e. Comparison is made with observations of CN at optical wavelengths. These results may be useful in planning future cometary observations. 相似文献