Circular polarization of sunlight reflected by planetary atmospheres

Multiple scattering calculations are performed in order to investigate the nature of the circular polarization of sunlight reflected by planetary atmospheres. Contour diagrams as a function of size parameter and phase angle are made for the integrated light from a spherical but locally plane-parallel atmosphere of spherical particles. To investigate the origin of the circular polarization, results are also computed for second-order scattering and for a simpler semiquantitative model of scattering by two particles. Observations of the circular polarization of the planets are presently too meager for accurate deduction of cloud particle properties. However, certain very broad constraints can be placed on the properties of the dominant cloud particles on Jupiter and Saturn. The cloud particle size and refractive index deduced for the Jupiter clouds by Loskutov, Morozhenko, and Yanovitskii from analyses of the linear polarization are not consistent with the circular polarization. The few available circular polarization observations of Venus are also examined.     

Construction of a genomic DNA library with a TA vector and its application in cloning of the phytoene synthase gene from the cyanobacteriumSpirulina platensis M-135

INTRODUCTIONThesignalproaningschemeofmostpnsentsonarsyStasuChaseChosounder,fishfinder,etc.,deteCtsthesignaIsaanrdingt0theamPlitudethasholdafterthefilter.However,inacomplicatalandfrequenhychangingunderotCfacousticalchanne,thesta-bilityandreiabilityofthiskindofsonarsySteIndroeshamlyasanysySthenoisewhleadt0anindedion.AmplitudefaderesultingfromstrongsignalfluCtuationcauseslossofdata.InsomesyStetnS,suchasndnelocatingsonar,highrangingamCyisneded,soasinglededionschernecann0tadapttoit.Resul…     

Propagation Speed of a Magnetic Flux-tube Soliton with Electric Current

We present some results of a magnetic flux-tube soliton propagating along a current loop surrounded by a weakly ionized plasma, by using a 3-D Neutral-MHD simulation code. When the velocity of mass flows outside the current loop exceeds about 0.6_A, the magnetic pulse behaves as an isolated string wave which is called a curved soliton, propagating with a velocity less than that one of exterior mass flow. The propagation speed of the magnetic flux-tube soliton is studied by changing the intensity of the electric current along the flux tube, which usually cannot be observed directly. It is found that the soliton speed decreases proportionally to the increment of the electric current, and the speed is independent of the direction of the electric current. We can estimate the current intensity inside a magnetic flux-tube soliton by observations of the soliton speed and the external plasma flow velocity. These results should be compared with recent high-resolution observations of moving magnetic features (MMFs) observed near sunspots.