This document is intended to familiarize you with the basics of the content of this archive. It contains comments and general notes on the archival process, data formats used, and part of an example SIMS data sheet. You may access this information directly through the list shown below.
Information on possible data loss or access problems
Although the SIMS data, SIMS thumbnail, bargraph, and profile data sheets
were mostly created by computer software and have therefore presumably
working hyperlinks, the data acquisition and archival process was performed by
humans susceptible to errors. The following list summarizes some of the
problems that may affect this archive's content.
Standard filenames, pathnames, file extensions
and -formats
The main archival activity consisted in the conversion of file formats from a SIMS-machine specific format to a format that could hold additional information, entering information from notebooks and verifying and re-verifying this data. A lot of time has been spent on element classification using information from notebooks and preocedures that are not explicitly stored in this database. During the archival activity, the author generated more than 11000 lines of C code, mostly during the first eight weeks of the six-month archival process.
This archive still contains data with rather "raw" character. Results based on this data were, however, published elsewhere before, too. The main purpose of this archive is to provide access to data that might not be further analyzed by the IDE team due to budget constraints. Hopefully, this data will be used before similar experiments are proposed.
All data in the archive came from
If your html client software (e.g. Mosaic) crashes when trying to access a SIMS data page, you may try the one of the following:
Given below are the SIMS images of this feature.
A thumbnail image overview is available, too.
The analysis was performed on 04-20-1992. The following mass numbers were
imaged:
16, 23, 24, 27, 28, 39, 40, 48, 52, 56, 56, 58, 63, 64, 107
This list is generated directly from the SIMS image file. Sometimes, mass numbers that had no counts were skipped by the operator, which is usually noted in the general comments in the previous section. This means that a particular species was not seen.
Missing values are marked using a question mark. Although sometimes an educated guess could have been made to assume a value, the author decided against it as this seemed not suitable for an archive. Hint: Look for analyses performed chronologically before or after the analyses you may want to guess the value for as it is relatively safe to assume that procedures did not change significantly during subsequent analyses.
Contrast diaphragm had alwas a constant value of 3 and image pixel size was 256 by 256 16-Bit for all analyses. Note that you have to correct the aspect ratio of the images if you want to have undistorted images. Convert the image to a 256 by 212 pixel image for geometrically correct images.
The ion image is available as a TIFF image by clicking on the image. Notes:
signal intensity scale: 0 -> 189; scale bars are 50 micrometers
The table below a ion image lists all relevant mass interferences for
this particular mass. The instrument was operated at a mass resolution of
at least 3000, which is the reason why interfering species which need
resolutions less than 3000 are not individually listed in this table. For
"uncommon" masses this table is not given.
-------------------------------------------------------------------------------- % isotopic Resolution Element Interferents abundance (m/Dm) Comments -------------------------------------------------------------------------------- 40Ca 40K 0.012 +28,000 not resolvable, very low abundance. 39KH 93.1 +4470 not resolvable, used 44Ca (SiO resolvable interference) or non- coinci-dence with K dis- tribution *28SiC,*24MgO,27Al13C, <2993 resolved 12C2O,12C3H4 -------------------------------------------------------------------------------- NOTE: An asterisk (*) means that these species were in fact observed on Hi-Res Mass Spectra of a particular mass on the Standard.
Only identifiable masses with the same channel plate gain value and ID may be displayed. The plot shows data points with Relative Sensitivity Factors for both material implanted in a silicon matrix and material implanted in a lunar analog glass matrix applied to them. When comparing the values of the data file available for this feature with the data of another feature, all instrument and image acquisition parameters must be the same to make any quantitative comparison of these two features. The values in the data file are shift-corrected pixel counts summed over the entire area inside the box and divided by the box area. 48Ti signals are corrected for 48Ca (0.185abundance, not resolvable). Please refer to the element classification information for the interpretation of this plot.