SIMS Map of MOS 1298 Crater 1

Impact feature information

SIMS Images

Below are the SIMS images of this feature. A thumbnail image overview is available, too. The analysis was performed on 04-14-1992. The following mass numbers were imaged:
16, 23, 24, 27, 28, 39, 40, 48, 52, 56, 56, 58, 63, 64, 107

Analytical Conditions:

These parameters directly affect spectrometer signal intensities.

Primary beam:

Secondary beam:


Image 1, O (Mass 16)

signal intensity scale: 0 -> 416; scale bars are 50 micrometers

--------------------------------------------------------------------------------
Element Comments
--------------------------------------------------------------------------------
16O	Primary ion species.
--------------------------------------------------------------------------------
NOTE: An asterisk (*) means that these species were in fact observed on Hi-Res
      Mass Spectra of a particular mass on the Standard.

Image Conditions

These parameters directly affect image intensities.

Image 2, Mass 23 (Na)

signal intensity scale: 0 -> 213; scale bars are 50 micrometers

--------------------------------------------------------------------------------
			% isotopic	Resolution
Element Interferents	abundance	  (m/Dm)	Comments
--------------------------------------------------------------------------------
23Na	30SiO2+ 	  3.10		  -4222 	not resolvable, low
							abundance. Na distri-
							bution had to be non-co-
							incident with high con-
							centration of the Si
							distribution for a
							positive ID. Looked for
							NaH (not resolvable from
							12C2) and/or NaO (not
							resolvable from 27AlC)
							in samples with high Si.
	*46Ti2+,46Ca2+			   <1776	resolved
--------------------------------------------------------------------------------
NOTE: An asterisk (*) means that these species were in fact observed on Hi-Res
      Mass Spectra of a particular mass on the Standard.

Image Conditions

These parameters directly affect image intensities.

Image 3, Mass 24 (Mg)

signal intensity scale: 0 -> 226; scale bars are 50 micrometers

--------------------------------------------------------------------------------
					Resolution
Element Interferents			  (m/Dm)	Comments
--------------------------------------------------------------------------------
24Mg   *48Ti2+,48Ca2+,*23NaH+,12C2	   <2731	resolved
--------------------------------------------------------------------------------
NOTE: An asterisk (*) means that these species were in fact observed on Hi-Res
      Mass Spectra of a particular mass on the Standard.

Image Conditions

These parameters directly affect image intensities.

Image 4, Al (Mass 27)

signal intensity scale: 0 -> 6389; scale bars are 50 micrometers

NOTE: CHANNEL PLATE GAIN AND PRIMARY BEAM CURRENT WAS REDUCED SUBSTANTIALLY
      ON Aluminum SUBSTRATES.
--------------------------------------------------------------------------------
			% isotopic	Resolution
Element Interferents	abundance	  (m/Dm)	Comments
--------------------------------------------------------------------------------
27Al   *26MgH		 11.0		  +3042 	moderate abundance,
							idenitfied Al line if
							sample with low Al
	54Cr2+,*13C15N,*12C2H3,54Fe2+	   <2298	resolved
--------------------------------------------------------------------------------
NOTE: An asterisk (*) means that these species were in fact observed on Hi-Res
      Mass Spectra of a particular mass on the Standard.

Image Conditions

These parameters directly affect image intensities.

Image 5, Si (Mass 28)

signal intensity scale: 0 -> 4376; scale bars are 50 micrometers

NOTE: USED 28SI ON NON-SI SUBSTRATES.
--------------------------------------------------------------------------------
					Resolution
Element Interferents			  (m/Dm)	Comments
--------------------------------------------------------------------------------
28Si   *56Fe2+,*27AlH,*12CO,12C2H4	   <2957	resolved
--------------------------------------------------------------------------------
NOTE: An asterisk (*) means that these species were in fact observed on Hi-Res
      Mass Spectra of a particular mass on the Standard.

Image Conditions

These parameters directly affect image intensities.

Image 6, Mass 39 (K)

signal intensity scale: 0 -> 320; scale bars are 50 micrometers

--------------------------------------------------------------------------------
					Resolution
Element Interferents			  (m/Dm)	Comments
--------------------------------------------------------------------------------
39K    *27AlC,23NaO,12C3H3		   <2190	resolved
--------------------------------------------------------------------------------
NOTE: An asterisk (*) means that these species were in fact observed on Hi-Res
      Mass Spectra of a particular mass on the Standard.

Image Conditions

These parameters directly affect image intensities.

Image 7, Ca (Mass 40)

signal intensity scale: 0 -> 271; scale bars are 50 micrometers

--------------------------------------------------------------------------------
			% 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.

Image Conditions

These parameters directly affect image intensities.

Image 8, Mass 48 (unidentified)

signal intensity scale: 0 -> 129; scale bars are 50 micrometers

--------------------------------------------------------------------------------
			% isotopic	Resolution
Element Interferents	abundance	  (m/Dm)	Comments
--------------------------------------------------------------------------------
48Ti	96Mo2+		 16.5		 +11,000	not resolvable, presence
							unlikely
	48Ca		  0.185 	 +10,000	not resolvable, very low
							abundance, Ti must be
							non-coincident with Ca,
							looked at 47Ti line
       *47TiH		  7.29		  +4123 	appears as a small peak
							on the right slope of
							the 48Ti peak
       *24Mg2+,48O3,24MgC2,12C4 	   <2167	resolved
--------------------------------------------------------------------------------
NOTE: An asterisk (*) means that these species were in fact observed on Hi-Res
      Mass Spectra of a particular mass on the Standard.

Image Conditions

These parameters directly affect image intensities.

Image 9, Mass 52 (unidentified)

signal intensity scale: 0 -> 94; scale bars are 50 micrometers

--------------------------------------------------------------------------------
			% isotopic	Resolution
Element Interferents	abundance	  (m/Dm)	Comments
--------------------------------------------------------------------------------
52Cr	28Si24Mg,*40CaC,26Mg2,		   <2420	resolved
	25MgAl,40KC,28SiC2
--------------------------------------------------------------------------------
NOTE: An asterisk (*) means that these species were in fact observed on Hi-Res
      Mass Spectra of a particular mass on the Standard.

Image Conditions

These parameters directly affect image intensities.

Image 10, Mass 56 (Fe)

signal intensity scale: 0 -> 182; scale bars are 50 micrometers

NOTE: 28Si2 and 40CaO are not resolvable among themselves and appear as
      one peak to the right of the 56Fe peak.
--------------------------------------------------------------------------------
			% isotopic	Resolution
Element Interferents	abundance	  (m/Dm)	Comments
--------------------------------------------------------------------------------
56Fe
 --AND--
56Si2	55MnH		 99.9		  +5118 	not resolvable, unlikely
							to be present without Fe
       *28Si2,44CaC,*40CaO,29SiAl,	   <2956	resolved
	40KO,32SC2,24MgO2,C4H6
--------------------------------------------------------------------------------
NOTE: An asterisk (*) means that these species were in fact observed on Hi-Res
      Mass Spectra of a particular mass on the Standard.

Image Conditions

These parameters directly affect image intensities.

Image 11, Si2 (Mass 56)

signal intensity scale: 0 -> 414; scale bars are 50 micrometers

NOTE: 28Si2 and 40CaO are not resolvable among themselves and appear as
      one peak to the right of the 56Fe peak.
--------------------------------------------------------------------------------
			% isotopic	Resolution
Element Interferents	abundance	  (m/Dm)	Comments
--------------------------------------------------------------------------------
56Fe
 --AND--
56Si2	55MnH		 99.9		  +5118 	not resolvable, unlikely
							to be present without Fe
       *28Si2,44CaC,*40CaO,29SiAl,	   <2956	resolved
	40KO,32SC2,24MgO2,C4H6
--------------------------------------------------------------------------------
NOTE: An asterisk (*) means that these species were in fact observed on Hi-Res
      Mass Spectra of a particular mass on the Standard.

Image Conditions

These parameters directly affect image intensities.

Image 12, Mass 58 (unidentified)

signal intensity scale: 0 -> 185; scale bars are 50 micrometers

NOTE: THIS IMAGE IS MOST LIKELY A COMBINATION OF 58Si2, Si2H, Si2H2,
      FeH, and (only if present) 58Ni.

NOTE: Ni MUST be NON-COINCIDENT with Fe AND Si (unlikely if it is
      present) for POSITIVE, QUANTITATIVE IDENTIFICATION. It should
      be possible to identify Ni using measured responses for non-
      resolvable interferences and their parent elemental isotopes
--------------------------------------------------------------------------------
			% isotopic	Resolution
Element Interferents	abundance	  (m/Dm)	Comments
--------------------------------------------------------------------------------
58Ni	58Fe		  0.33		 -28,000	not resolvable, very low
							(68.3%) abundance
	57FeH		  2.19		  +7352 	not resolvable, low
							abundance
	58Si2		  5.92		  +3777 	not resolvable
--------------------------------------------------------------------------------
NOTE: An asterisk (*) means that these species were in fact observed on Hi-Res
      Mass Spectra of a particular mass on the Standard.

Image Conditions

These parameters directly affect image intensities.

Image 13, Mass 63 (unidentified)

signal intensity scale: 0 -> 95; scale bars are 50 micrometers

--------------------------------------------------------------------------------
			% isotopic	Resolution
Element Interferents	abundance	  (m/Dm)	Comments
--------------------------------------------------------------------------------
63Cu	62NiH		  3.66		  +9578 	not resolvable, Cu must
							be non-co-incident with Ni
							for positive identifi-
							cation
      * 47TiO		  7.26		  +3684 	not resolvable, Cu must
							be non-coincident with Ti
							for positive identifi-
							cation
	39KC2,27AlC3,C5H3		   <1844	resolved
--------------------------------------------------------------------------------
NOTE: An asterisk (*) means that these species were in fact observed on Hi-Res
      Mass Spectra of a particular mass on the Standard.

Image Conditions

These parameters directly affect image intensities.

Image 14

Black image; no counts at this mass.


Image 15

Black image; no counts at this mass.


Mass Ratio Plot

The image displayed below shows the area (79,70 to 157,150) and the image (number 1, mass 16) that was used to compute mass ratios.

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.


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Klaus G. Paul, 7-12-1994