SUBROUTINE GDSD_WFITS(FILNAM,KEY,LEVEL,FREC,ERROR) *@subroutine gdsd_wfits(character,character,integer,character,integer) *#>gdsd_wfits.dc2 *Subroutine: GDSD_WFITS * *Purpose: Write FITS-type descriptor item * *File: gdsd_wfits.shl * *Category: GDS * *Author: J.P. Terlouw * *Use: CALL GDSD_WFITS ( file_id, *name, level, record, *error ) * * file_id = file identifier, CHARACTER * * name = name of FITS item. ... 4 CALL GDS___CHECK(BOOLER,ERROR_I,ERROR,*RETURN) BOOLER=FREC_I(1:10).EQ.' ...

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. While using vi to edit an existing file, you are actually working on a copy of the file that is held in a temporary buffer . If you invoked vi with a new filename, (or no file name) the contents of the file only exist in this buffer. Saving a file writes the contents of this buffer to the permanent file, replacing its contents. You can write the buffer to a new file or to some other file. You can also decide not to write the contents of the buffer, and leave your original file unchanged.

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... Corresponding authors will receive an e-mail with a PDF file of paged proof for checking and correction. The file can be read and edited using Adobe Acrobat Reader (version 9 and higher) which can be free downloaded via the Internet ( http://get.adobe.c om/reader/ ). ... You can use text correction tools to make corrections (after selecting the necessary text fragment). ... For users of Adobe Reader 9: . ... to insert text without replacing the existing text, use the "Insert text at cursor" tool. ...

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This section of library contains information about "classic" Star Catalogs. ... For a Henry Draper Catalog 272149 stars have received a total of 531,211 identifications in 7 сatalogs: . 270456 - in Astrographic Catalogue ( "Carte du Ciel", 4M), . 251943 - in Guide Stars Catalog (GSC), . ... A file with information on the components of 1788 of multiple systems in catalog HDEC (3681 component, or a combination thereof, with 4054 recording). ... A file with information about 21971 variable stars. ...

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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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