Next: Scattering properties Up: Polarization properties (transmitted radiation) Previous: Linear polarization: wavelength dependence . Traditionally, the main problem considered in connection with circular interstellar polarization is the meaning of the wavelength where changes the sign . ... This is also demonstrated by Fig. 19 (lower panel) which shows the wavelength dependence of the factors of linear and circular polarization for particles of magnetite as was done by Shapiro ([ 1975 ]). ...

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... B.1 New functionality . ... B.3 Semantic changes from CSS1 . ... CSS2 builds on CSS1 and all valid CSS1 style sheets are valid CSS2 style sheets. The changes between the CSS1 specification (see [CSS1] ) and this specification fall into three groups: new functionality, updated descriptions of CSS1 functionality, and changes to CSS1. ... Several internationalization features, including list numbering styles , support for bidirectional text , and support for language-sensitive quotation marks . ...

... The following tables summarize basic properties of the two echelle gratings. ... At the center of each order, the dispersion is 3.0 km s-1 per diode, at the long-wavelength end of each order it is 2.9 km s-1 per diode, and at the short-wavelength end of each order it is 3.1 km s-1 per diode. ... The figure below shows the echelle blaze function (also known as the "Ripple Function") in the form of sensitivity relative to the peak of the blaze as the product of wavelength and order number. ...

... AstroGrid Registry . ... 1.DB client and WebDav . ... If you are using the recommended xml database eXist (which also is bundled up with the registry). ... Also it supports WebDav which allows you to connect various Applications like XMLSpy or Oxygen as well as your typical File Manager normally support WebDav meaning you can view the whole database just like any other network drive on your system. ... ex: http://software.astrogrid.org/schema/vo-resource-types/VOResource/v1.0/VOResource.xsd . ...

Next: V652HER AND MERGED BINARY Up: EXTREME HELIUM STARS: PULSATION Previous: MASSES . Although pulsations in EHes appear to be ubiquitous, it is not possible to summarize their properties with a single definition. ... The first discovery of pulsation in an EHe was made by Landolt (1975), who discovered a 0.1day photometric period in V652Her, and by Hill et al. (1981), who measured the radial velocity curve and demonstrated the variations were due to radial pulsation. ... 1987, Jeffery et al. ...

... You are here: start €Ё difx €Ё tip_and_tricks . ... Add svn properties to source files . Get IPP version 7 to play nice with mpifxcorr . ... This should never be called for DiFX data. ... The following template should be modified to reflect the path base = /home/swc/difx/intel/ipp/7.0.1.084/ia32 Name: ipp Description: Intel Performance Primitives Requires: Version: 7.0.1.084 Libs: -L${base}/lib/ia32 -L${base}/ipp/lib/ia32 -lipps -lippvm -lippcore -liomp5 Cflags: -I${base}/ipp/include . ...

... 2009: Europa Lander: Science Goals and Experiments Introduction Europa's complex surface is the consequence of physical processes in the ice shell and in the deep interior. ... Tidal deformation induces pressure changes and therefore may drive currents in the ocean. ... This allows for the determination of the ice shell thickness. cold brittle ice thin ice layer completely frozen ocean Europa's Response to Tidal Forcing h 2 Elastic response of the ice shell. ...