Pubs.GISS: Ingersoll and Miller 1986: Motions in the interiors and atmospheres of

Pubs.GISS: Rossow et al. 1980: Cloud morphology and motions from Pioneer Venus images Go to Main

Pubs.GISS: Zahn et al. 1974: Nonlinear cellular motions in Poiseuille channel flow Go to Main Content

JAS-D-14-0139.1. Application of an isentropic analysis of convective motions to a

effects on climate sensitivity. The dependence of cumulus mass flux on vertical motions, and the

components of Earth's weather and climate. They are produced by atmospheric motions across a very

for the first two shear modes. The behavior of particle motions for different

movement of the atmospheric fluid as a superposition of motions occurring on different scales

of the turbulent nature of the atmospheric and oceanic motions that transport heat and

a record of significant residual fluctuations apparently indicative of varying vertical motions. Regular oscillations over pressure

with a passive scalar from two spanwise dye slots to distinguish between fluid motions originating in the

black hole is its gravitational mass, which is discernible through its effect on macroscopic bodies (orbital motions) or microscopic bodies (compressional

the neglect of coupling between the translational and internal motions. Recently, we have shown

of ozone an attempt is made to combine the mean meridional motions and the

weak dynamic regime or large in a multilayered haze complex, if stronger vertical motions exist. Denser precipitating cloud

105<1337:ACOEAD>2.0.CO;2. The contribution of small-scale motions to the

the edge of the nuclear disk. The equations of motions are then quite simple

ISS) began observing Saturn in early February 2004. From analysis of cloud motions through early October 2004

the underlying convection, the thermal-wind balance of observed cloud-top motions implies a mapping

with a passive scalar from two spanwise dye slots to distinguish between fluid motions originating in the

vertical earth movements, and geographically uneven distribution of long-term records. Crustal motions introduce a major

lines arise; the hydrogen lines have very broad wings, corresponding to Doppler motions of ±2500

the concentration in ice nuclei, the vigor of vertical motions and precipitation

technique, we investigate the influence of coagulation, sedimentation and turbulent motions on the observed

of shapes, sizes and albedos allows their use as tracers of theatmospheric motions in the

be an important water vapor sink). Rather, it is likely that the same transient motions that produce the

the evolution of their cloud properties over their lifetimes, and their motions. The results

for O stars compared with B stars; and, in binary systems, slower apsidal motions, closer rotational-revolutional synchronism

near the boundaries for large Rayleigh numbers and large horizontal scale motions. The linear

and description at Planetary Photojournal. (Image credit: NASA/JPL/Space Science Institute) Jet streams are motions in an

8 , 1035-1038, doi:10.1029/GL008i010p01035. Limaye, S.S., and V.E. Suomi, 1981: Cloud motions on Venus: Global structure

Rev. , 44 , 191-240, doi:10.1007/BF00200817. Ingersoll, A.P., and R.L. Miller , 1986: Motions in the

Genio , S.S. Limaye, L.D. Travis , and P.H. Stone, 1980: Cloud morphology and motions from Pioneer Venus images

152806. Zahn, J.-P., J. Toomre, E.A. Spiegel, and D.O. Gough, 1974: Nonlinear cellular motions in Poiseuille

massive stars . Astrophys. J. , 214 , 809-811, doi:10.1086/155310. White, R.E., 1977: Microturbulence, systematic motions, and line

Coupled Isotopic Model Simulations Kirstie Lynn Stramler The Influence of Synoptic Atmospheric Motions on the Arctic

2966.2005.09720.x. Stramler, K.L. , 2006: The Influence of Synoptic Atmospheric Motions on the Arctic

42 , 49-91, doi:10.1080/03091928808208858. 1986 Ingersoll, A.P., and R.L. Miller , 1986: Motions in the