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r615 r704 71 71 <TH> </TH> 72 72 </TR> 73 <TR><TH BGCOLOR="#F0F0F0" rowspan= 2>Utilities:</TH>73 <TR><TH BGCOLOR="#F0F0F0" rowspan=3>Utilities:</TH> 74 74 <TH><A Href="liveplot.html">LIVEPLOT</A></TH> 75 75 <TH><A Href="liveplot.html">BKGEDIT</A></TH> … … 79 79 <TH><A Href="#WIDPLT">WIDPLT</A></TH> 80 80 <TH><A Href="#ABSPLT">ABSPLT</A></TH> 81 <TH><A Href="#INSTEDIT">INSTEDIT</A></TH> 82 </TR> 83 <TR> 81 84 <TH><A Href="gsas2cif.html">CIF export</A></TH> 85 <TH> </TH> 86 <TH> </TH> 82 87 </TR> 83 88 <TR><TH BGCOLOR="#F0F0F0">Installation Notes:</TH> … … 268 273 to save screen space. 269 274 <P> 270 <img src="powpref4a.gif" align=left >275 <img src="powpref4a.gif" align=left alt="EXPGUI Screen snapshot"> 271 276 Once the GSAS program has finished, if the program has modified 272 277 the .EXP file, … … 287 292 This file is deleted when the GSAS program completes. 288 293 <P> 289 <img src="lock.gif" align=left >294 <img src="lock.gif" align=left alt="EXPGUI Screen snapshot"> 290 295 In Windows-9x, the <a Href="expgui_Win_readme.html#Winexec">Winexec</a> 291 296 package is used to execute a command that creates a DOS window. … … 463 468 <P> 464 469 WIDPLT and ABSPLT both use the <A href="#blt">BLT</A> graphics package. 470 </DL></DL> 471 472 <br clear=all> 473 <a name="INSTEDIT"></a> 474 <H3>D.6 INSTEDIT</H3> 475 <DL><DL> 476 477 The INSTEDIT utility is used to edit or create an instrument parameter file. 478 At this time it can only be used to edit files for 479 constant-wavelength data. The utility can be started from the "Edit File" 480 button in the 481 <A HREF="expgui3.html#AddHist">"Add New Histogram"</A> dialog, or from the 482 the "instedit" option in the Powder menu. In the latter case, the user 483 is given the chance to select an input file. If no file is selected, 484 a new, empty, file is created. An example INSTEDIT window appears below. 485 <P> 486 <img SRC="instedit1.gif" align=RIGHT alt="EXPGUI Screen snapshot"> 487 <br clear=all> 488 <P> 489 Note that an instrument parameter file is used for a single type of data, 490 as is selected by the menu button at the top of the window. 491 However, multiple sets of parameters may be included in a 492 file, to be used for example with differing operating modes for the 493 instrument. Each set of parameters is called a bank in GSAS terminology. 494 The radiobuttons on the top of the window are used to select 495 which bank's parameters will be viewed. 496 The "Add Bank" button adds an additional bank to the file. 497 <P> 498 The parameters are described briefly below, but in more depth in the 499 GSAS manual (for example, pages 158-166 for profile parameters and 500 page 221-223 for the details of the instrument parameter file.) 501 <P> 502 <H5>Bank Parameters</H5> 503 The parameters available for each bank are: 504 <DL> 505 <DT>Title<DD>This probably has no real use. 506 <DT>Instrument Name<DD>This string is used for creation of CIFs. It is 507 best if this name is unique for each instrument. 508 <DT>Primary Wavelength<DD>Note, this value is set automatically when 509 the radiation type is selected 510 <DT>Zero Correction<DD>This is the shift to be applied to 2theta 511 values in centidegrees (degrees/100). This value should probably be 512 near zero for Debye-Scherrer geometry instruments (unless known from 513 calibration) and will almost always be fixed at zero 514 for Bragg-Brentano geometry. 515 <DT> 516 </DL> 517 <I>X-ray only parameters</I> 518 <DL> 519 <DT>Radiation type<DD>Used with x-rays. The value set here 520 determines the anomolous dispersion (f' and f'' values) used. 521 <DT>Monochromatic/Dual<DD>Used with x-rays. Set to dual when Kalpha1, Kalpha2 522 radiation is present. 523 <DT>Secondary Wavelength<DD>Used in "dual" wavelength mode. 524 Note, this value is set automatically when the radiation type is selected 525 <DT>Wavelength Ratio<DD>Typically 0.5 for typical K alpha 1,2 instruments, 526 <<I>i.e.</I>when K alpha 1 is double the intensity of K alpha 2. 527 <DT>Polarization Correction<DD>There are three modes for this, where the 528 first two modes work similarly. The first mode ("Diffracted Beam") 529 is most common. The third mode ("None") is used when 530 Lorentz-polaraization corrections are applied to the data prior to its input 531 to GSAS. See page 144-145 in the GSAS manual for more information on these 532 corrections. 533 <DT>Polarization Ratio<DD>In "Diffracted Beam" mode: 534 typically 0.5 for lab instruments without monochromators and higher for 535 instruments with a diffracted beam; the value depends on the monochromator 536 take-off angle. Typically slightly below unity (0.9-0.98) for synchrotron 537 instruments. Ask the instrument scientist for the appropriate value. 538 </DL> 539 <P> 540 Each bank in the instrument parameter file has one or more sets of 541 profile parameters associated. Set number 1 is the default loaded 542 when a histogram is added. Increase the number of sets 543 using the "Add profile" button. Select the optimal profile type 544 for use with your data for this set, but for most flexibility, define 545 default values for all useful profile types (type 1 is of use only for 546 CW neutron work) and set these values from fitting a standard with 547 minimal broodening. Note that profiles can be read from a GSAS experiment 548 file using the "Import profile", which raises a dialog 549 such as the one below. 550 <P> 551 <img SRC="instedit2.gif" align=RIGHT alt="EXPGUI Screen snapshot"> 552 <br clear=all> 553 465 554 466 555 </DL></DL> … … 469 558 <a name="ConvertUnix"></a> 470 559 <a name="ConvertWin"></a> 471 <h3>D. 6File Conversions</h3>560 <h3>D.7 File Conversions</h3> 472 561 <DL><DL> 473 562 <P> … … 489 578 <br clear=all> 490 579 <a name="Composition"></a> 491 <h3>D. 7Compute Composition</h3>580 <h3>D.8 Compute Composition</h3> 492 581 <DL><DL> 493 582 The composition box shows the unit cell and asymmetric unit composition … … 498 587 <br clear=all> 499 588 <a name="DeleteHistoryRecords"></a> 500 <h3>D. 8Delete History Records</h3>589 <h3>D.9 Delete History Records</h3> 501 590 <DL><DL> 502 591 Every time a GSAS program (including EXPGUI) is run, an entry is added to … … 545 634 This routine is used to copy coordinates, unit cell parameters and space group 546 635 information from other GSAS experiment (.EXP) files. 636 <DT><B>MSI .xtl format</B><DD> 637 <a HREF="#ExportMSI">see below</a> 638 <DT><B>PLATON .spf (Standard Parameter File) format</B><DD> 639 <a HREF="#ExportSPF">see below</a> 640 547 641 </DL></DL> 548 642
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