. Florence, Rome. September 1999: page 31 . a33. Ponte Vecchio, as seen from ponte S. Trinita. previous page | title page | jump to normal size | index | next page

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• Florence, Rome. September 1999: page 36
• Florence, Rome. September 1999: page 113
• Florence, Rome. September 1999: page 148

Astronomy Picture of the Day . Mars to Appear Normal this August . ... 8.08.2005 . ... August . ... August 2005 . ... 2005 2006 . ... NASA Web Site Statements, Warnings, and Disclaimers . NASA Official: Jay Norris. ... A service of: LHEA at NASA / GSFC . ... U. Based on Astronomy Picture Of the Day . Publications with keywords: Mars . Publications with words: Mars . ... Opportunity at Santa Maria Crater . ... Intrepid Crater on Mars . ... A Dark Dune Field in Proctor Crater on Mars . ...

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• XWare > APOD

... September 18, 1996 . Stars in the Infrared Sky . ... Explanation: What if you could see infrared light ? Because this light is less absorbed by dust than visible light, you could peer into the center of our Milky Way Galaxy. The stars there are normally hidden from direct view by the interstellar dust clouds which line the Galactic plane. ... Interplanetary dust , which tends to lie along the plane of our own solar system, scatters sunlight and emits radiation at these wavelengths too. ...

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. Visitors of my Home Page: . љ . Back to Home Page . Personal information . Alexander Konovalenko alex.kono@mailcity.com

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... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...

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... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

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