This diagram illustrates the effects of floating a box ("inner") and how its "sibling" is forced below it due to the 'clear' property. A document window is shown, with 8 lines (numbered 1 to 8), each 24px high. Text before the "inner" box flows on lines 1 and halfway on line 2. The "inner" box has been floated to the right and occupies the second half of lines 3 and 4. ... The lines, as they appear in the image, contain: 1 Beginning of body contents. ... Inner contents" is blue. ...

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• Long description of example illustrating floating without clear
• Long description of example illustrating floating
• Long description for example illustrating absolute positioning

. The following pages show a few of the effects available with GIMP. This is by no means comprehensive; this is just an example of some of the effects possible. Many of these effects are created with plug-ins from the net . Check them out and enjoy. [ | Add Noise | Bleed | Edge Detect | Enhance | Lunarize | Pixelize | Relief | Shift | Solarize | Spread | ] . [ Tips Tricks Tutoriasl ]

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• The Name of the Plug-In: The ... Dialog Box
• Hands On; Texture Wrapping
• GIMP animations: merge-anim examples

... This thread uses PINTofALE to generate a simulated Chandra spectrum. ... define a DEM . ... pset marx .par ExposureTime=50000 OutputDir='sim_ marx ' \ ; GratingType='NONE' DetectorType=' ACIS-I ' SourceFlux=-1 \ ; SpectrumType='FILE' SpectrumFile='spec_ marx .dat' \ ; SourceType='POINT' DitherModel='INTERNAL' ; marx TSTART=2006.46 ; marx2fits sim_ marx / spec_ marx .evt ; dmextract infile= spec_ marx .evt[EVENTS][(x,y)=circle(4018,4141,10)] ; [bin pi=1:1024:1] outfile= spec_ ...

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• Doug Burke's Perl/S-Lang pages: Datatype examples
• Doug Burke's Perl/S-Lang pages: Structure examples
• Doug Burke's Perl/S-Lang pages: General examples

The example programs can be downloaded by clicking on the appropriate link, or can be copied from the directory $PHYTEACH/part_2/examples/ on the PWF Linux systems. The following are the programs referred to in self-study guide 2. page 11, projectile, projectile.f90 . ... page 34, simple subroutine example 1, swapmain.f90 . ... The following are the programs included in the Physics of Computational Physics handout. page 5, NAG Library information example, ex.f90 . ...

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• OptInt PmWiki : PmWiki / Wiki Style Examples
• OptInt PmWiki : PmWiki / Custom InterMap
• PPEUC Programme - Cosmic Microwave Background Workshop

Your Phase II Proposal and Using RPS2 . ... Exposure_Number: 1 Target_Name: HD12345 Config: HRS Opmode: ACQ Aperture: 2.0 Sp_Element: MIRROR-N1 Wavelength: Optional_Parameters: BRIGHT=RETURN, ! ... Number_of_Iterations: 1 Time_Per_Exposure: 13.5S Special_Requirements: ONBOARD ACQ FOR 2 Comments: STEP-TIME = 1.5 sec Exposure_Number: 2 Target_Name: HD12345 Config: HRS Opmode: ACQ/PEAKUP Aperture: 0.25 Sp_Element: MIRROR-N1 Wavelength: Optional_Parameters: SEARCH-SIZE=5 ! ...

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• Following the Road to Effective International Sharing of Astronomical
• GHRS Instrument Handbook
• Examples and Photometric Tests

... section 7.4 ) . If the detector map (a grid of positions used to calculate and flux weight the ARF: section 7.3 ) is either psf or flat , the map bounds and pixel size may be specified. ... The user can supply an external detector map instead (section 7.3.2 ), but the bounds must cover the regions. ... The following sub-sections show examples of usage. ... Example 4: Specifying an external detector map for an extended source . Example 5: Using an RMF dataset to specify the energy grid . ...

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• Dealing with MOS1 data in Timing Mode
• Examples.

These are very prominent absorption lines is most all galaxies. ... These pair of absorption lines will appear in all the spectra and they should be your principle source for determining the redshift. ... When this applet opens you will see an iconic representation of galaxies in the left hand side of the applet and a target area in the right side of the applet. ... Note: What you are doing in this excercise is identical to what Hubble did in the 1920's and you are using the same galaxies. ...

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• The Galaxy Gallery Page VII: Infrared Imaging
• Redshift Tutorial
• Conservation of Linear Momentum

... The variability of the spectrum of the optical component of the IR-source IRAS01005+7910 was discovered for the first time in the BTA spectra [1]. ... The spectral features include absorptions that form in near-photospheric layers, narrow envelope emissions, and emission-absorption profiles that form in photosphere-to-envelope transition layers (the wind). ... Discovery of spectral variation in the optical counterpart of IRAS01005+7910. ... Dashed line - envelope curve of all the SiII 5979 profiles ...

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This module illustrates many of the aspects of the Apache 1.2 API and, when used, demonstrates the manner in which module callbacks are triggered by the server. ... Source File: mod_example.c . ... The files in the src/modules/example directory under the Apache distribution directory tree are provided as an example to those that wish to write modules that use the Apache API. ... Example . ... Uncomment the "AddModule modules/example/mod_example" line near the bottom of the src/Configuration file. ...

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• Apache module mod_auth_anon.c
• Apache Tutorial: .htaccess files
• Mapping URLs to Filesystem Locations - Apache HTTP Server

... Suppose that a NS having a rotational magnetic   luminosity forms a binary system (with semi-major axis a ) with a normal star losing matter in the form of stellar wind (with a loss rate ). ... This means that while deriving the formula for a cavern in the general case, we must take into account the proximity of the normal star. ... It follows from the symmetry considerations that at the anterior point of the cavern (i.e. the point closest to the normal star), . ... If , the cavern is closed. ...

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• Transferring mag to erg/cm/s
• Effect of the Magnetic Field
• Evolutionary Scenarios of Binary Systems

... Previous: Background Fluctuation Analysis from the Multiscale Entropy . ... A new measure of information is defined which is based on noise modeling and incorporates resolution scale. Properties of this measure are discussed. ... Additionally it allows for image noise modeling, and subsequent noise removal. ... Hence information- and entropy-based processing technologies will be necessary for the effective design and implementation of large, future generation, image databases. ...

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• Modelling Spectro-photometric Characteristics of Eclipsing Binaries
• Spatial Structure of NGC 6822: An Example for Statistical Modeling of
• The SAX-LEGSPC Data Reduction and Analysis System: An Example of a Minimalist