ASM */ ;/* CHANGING OF THE BYTE SEQUENCE FOR LONG */ ;/* */ ;/******************************************************************/ CODESEG_TEXT SEGMENT WORD PUBLIC 'CODE' CODESEG_TEXT ENDS _ DATA SEGMENT WORD PUBLIC ' DATA ' _ DATA ENDS CONST SEGMENT WORD PUBLIC ' CONST ' CONST ENDS _ BSS SEGMENT WORD PUBLIC ' BSS ' _ BSS ...

... Create a list widget. listw_bind . ... void listw_bind (KListWidget list, KPixCanvas canvas) . ... Only one list widget may be bound per pixel canvas. void listw_destroy (KListWidget list) . ... void listw_get_attributes (KListWidget list, .. ... The attribute notify function will be called whenever the list widget attributes are changed (see listw_set_attributes ). ... flag listw_PROTO_position_func (KListWidget list, unsigned int index, unsigned int event_code, void *e_info, void **f_info) . ...

Appendix B: The Effects of Thermal Changes on the "Absolute" Position of the Secondary . ... I will use the same nomenclature for the rod forces here as I used in Appendix A. In Appendix A, the axial force balance equation at the horizon was shown to be . ... The quantity that we really wish to derive is , where is the rod elongation at some initial epoch (i.e. when the rods were first tensioned) and where is the rod elongation at some later time after the rod temperatures had changed. ...

OptInt PmWiki . ... Tech Meet 16 . ... Page History | ... MROI Delay Line Design Contract . ... Return to Tech Meet 16 ( Edit ) . ... MF/XS Investigate possible ways of clamping camera cable and assess any extra space needed . XS Make 3d drawing for NMT based on 2011-05-17 layout showing changes to space envelopes that we are requesting . ... Right-angle layout unsuitable even with shorter f lens . ... Happy with concept for baseplate, kinematic supports and pin position under final fold mirror . ...

... Count Rate Ratio (cr_ratio) . Introduction of a tabular file, that describes the differences between expected count rates and the count rates measured in orbit. ... The change involve a new entry in the 'models' section of RGASIM : rgasim begin models begin MYMODEL begin : lincoordFile RGS_coordinates_file.CCF end : end : end . Exploiting the LINCOORD files as described above, the location of these simluators in the telescope frame are no longer described in the configuration files of SciSim. ...

Next: Semi-major axis change Up: Change of Binary Parameters: Previous: Change of Binary Parameters: . The mass of the star that loses matter is . Accordingly, the mass of the accreting star is . where is the accretion rate   of the captured matter. ... In the case of compact accretors, we require the rate of their mass increase to be limited by the accretion energy output equal to the critical Eddington luminosity   . ...

... The previous example, Chapter 12, "Expanding Colored Squares Example," illustrates how to expand and contract the clipping region of a layer without changing the wrapping width of the layer. This example illustrates how to capture mouse events so that the user can make a layer's wrapping width wider or narrower by dragging the mouse. ... how to capture mouse events for a layer . how to change the wrapping width of a layer by using the load() function . ... Capturing Events for the Layer . ...

Next: Catalog Construction Up: Observations and Analysis Previous: Source Detections . ... It was assumed that the highest signal gives the most likely position of the source. ... Comparing the summed map with the maps from the individual energy ranges, the one which produced the smallest error box was chosen to represent the source position, as long as was greater than 4, a level chosen to reflect a reasonable degree of confidence in the detection. ...

... In the above example, the second region uses the global coordinate system (PHYSICAL by default). ... Supported systems include: name description ---- ----------- PHYSICAL pixel coords of original file using LTM/LTV IMAGE pixel coords of current file FK4, B1950 sky coordinate systems FK5, J2000 sky coordinate systems GALACTIC sky coordinate systems ECLIPTIC sky coordinate systems ICRS currently same as J2000 LINEAR linear wcs as defined in file In addition, two mosaic coordinate ...

... A couple of new tasks have also been added; including, SAACLEAN to the NICMOS package, 'tweakshifts' to the DITHER package and a Python interface to SExtractor. Updated or New Tasks: ===================== 1. NEW TASKS: - 'tweakshifts' added to the DITHER package: This prototype version of 'tweakshifts' provides an automated interface for computing residual shifts between input exposures being combined using MultiDrizzle or PyDrizzle. ... Changes to CALSTIS: - Updated to Version 2.19. ...

... Class . ... PREV CLASS NEXT CLASS . FRAMES NO FRAMES All Classes . ... FIELD | ... METHOD . DETAIL: FIELD | ... public interface IJEventListener . ... Field Summary . static int . ... Field Detail static final int FOREGROUND_COLOR_CHANGED . ... Constant Field Values . static final int BACKGROUND_COLOR_CHANGED . ... static final int COLOR_PICKER_CLOSED . ... static final int LOG_WINDOW_CLOSED . ... static final int TOOL_CHANGED . ... Method Detail void eventOccurred (int eventID) . ...

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 ]). ...

... Bad Astronomy . ... I think I will break from my usual format of Bad Astronomy/ Good Astronomy by saying that the way we define seasons currently is not strictly bad, but I feel (in my opinion!) that it could be better. The definition of when the seasons begin is at the moment of solstice or equinox; that is, winter (in the north) starts on December 22 nd and summer starts on June 22 nd . ... Now imagine breaking up the Sun's 46 degree up-and-down yearly swing into 1 day intervals. ...

Modules | ... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Developer Documentation . ... This is a first attempt at writing the lessons I learned when trying to convert the mod_mmap_static module to Apache 2.0. ... create per-server config structures */ . ... merge per-server config structures */ . ... Questions on how to manage the Apache HTTP Server should be directed at either our IRC channel, #httpd, on Freenode, or sent to our mailing lists . ...

The 2.6 kernel contains a long list of changes which affect device driver writers. As part of the task of porting the Linux Device Drivers sample code to 2.6, your humble LWN Kernel Page author is producing a set of articles describing the changes which must be made. ... November 25, 2003) The entire set of articles has been updated to reflect the 2.6.0-test10 kernel. ... Timekeeping changes (November, 2003; 2.6.0-test9); changes to how the kernel manages time and time-related events. ...

Astronomy Discussion Forums . Forums: . Atm ћ Astrophotography ћ Blackholes ћ Blackholes2 ћ CCD ћ Celestron ћ Domes ћ Education . ... Discussion Forums . ... Note The Change . Forum List | ... Post Message | ... www.astronomy.net . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

An Ancient Universe: How Astronomers Know the Vast Scale of Cosmic Time . THE CHANGING UNIVERSE: EVOLUTION HAPPENS! ... Luckily nature has left a wide range of clues about evolution for us - at every scale of the universe - which we can uncover with some good astronomical detective work. a) Changes in the Solar System . ... An Ancient Universe - Table of Contents . ... The Universe: An Overview | ... The Changing Universe - Changes in the Solar System - Changes in Stars - Changes in the Universe | ...