Package: Spectra
Authors: RforMassSpectrometry Package Maintainer [cre], Laurent Gatto [aut] (https://orcid.org/0000-0002-1520-2268), Johannes Rainer [aut] (https://orcid.org/0000-0002-6977-7147), Sebastian Gibb [aut] (https://orcid.org/0000-0001-7406-4443), Jan Stanstrup [ctb] (https://orcid.org/0000-0003-0541-7369), Nir Shahaf [ctb]
Last modified: 2023-10-24 14:38:15.825743
Compiled: Tue Oct 24 19:10:51 2023

1 Introduction

The Spectra package provides a scalable and flexible infrastructure to represent, retrieve and handle mass spectrometry (MS) data. The Spectra object provides the user with a single standardized interface to access and manipulate MS data while supporting, through the concept of exchangeable backends, a large variety of different ways to store and retrieve mass spectrometry data. Such backends range from mzML/mzXML/CDF files, simple flat files, or database systems.

This vignette provides general examples and descriptions for the Spectra package. Additional information and tutorials are available, such as SpectraTutorials, MetaboAnnotationTutorials, or also in (Rainer et al. 2022).

2 Installation

The package can be installed with the BiocManager package. To install BiocManager use install.packages("BiocManager") and, after that, BiocManager::install("Spectra") to install Spectra.

3 General usage

Mass spectrometry data in Spectra objects can be thought of as a list of individual spectra, with each spectrum having a set of variables associated with it. Besides core spectra variables (such as MS level or retention time) an arbitrary number of optional variables can be assigned to a spectrum. The core spectra variables all have their own accessor method and it is guaranteed that a value is returned by it (or NA if the information is not available). The core variables and their data type are (alphabetically ordered):

acquisitionNum integer(1): the index of acquisition of a spectrum during a MS run.
centroided logical(1): whether the spectrum is in profile or centroid mode.
collisionEnergy numeric(1): collision energy used to create an MSn spectrum.
dataOrigin character(1): the origin of the spectrum’s data, e.g. the mzML file from which it was read.
dataStorage character(1): the (current) storage location of the spectrum data. This value depends on the backend used to handle and provide the data. For an in-memory backend like the MsBackendDataFrame this will be "<memory>", for an on-disk backend such as the MsBackendHdf5Peaks it will be the name of the HDF5 file where the spectrum’s peak data is stored.
intensity numeric: intensity values for the spectrum’s peaks.
isolationWindowLowerMz numeric(1): lower m/z for the isolation window in which the (MSn) spectrum was measured.
isolationWindowTargetMz numeric(1): the target m/z for the isolation window in which the (MSn) spectrum was measured.
isolationWindowUpperMz numeric(1): upper m/z for the isolation window in which the (MSn) spectrum was measured.
msLevel integer(1): the MS level of the spectrum.
mz numeric: the m/z values for the spectrum’s peaks.
polarity integer(1): the polarity of the spectrum (0 and 1 representing negative and positive polarity, respectively).
precScanNum integer(1): the scan (acquisition) number of the precursor for an MSn spectrum.
precursorCharge integer(1): the charge of the precursor of an MSn spectrum.
precursorIntensity numeric(1): the intensity of the precursor of an MSn spectrum.
precursorMz numeric(1): the m/z of the precursor of an MSn spectrum.
rtime numeric(1): the retention time of a spectrum.
scanIndex integer(1): the index of a spectrum within a (raw) file.
smoothed logical(1): whether the spectrum was smoothed.

For details on the individual variables and their getter/setter function see the help for Spectra (?Spectra). Also note that these variables are suggested, but not required to characterize a spectrum. Also, some only make sense for MSn, but not for MS1 spectra.

3.1 Creating `Spectra` objects

The simplest way to create a Spectra object is by defining a DataFrame with the corresponding spectra data (using the corresponding spectra variable names as column names) and passing that to the Spectra constructor function. Below we create such an object for a set of 3 spectra providing their MS level, olarity but also additional annotations such as their ID in HMDB (human metabolome database) and their name. The m/z and intensity values for each spectrum have to be provided as a list of numeric values.

library(Spectra)

spd <- DataFrame(
    msLevel = c(2L, 2L, 2L),
    polarity = c(1L, 1L, 1L),
    id = c("HMDB0000001", "HMDB0000001", "HMDB0001847"),
    name = c("1-Methylhistidine", "1-Methylhistidine", "Caffeine"))

## Assign m/z and intensity values.
spd$mz <- list(
    c(109.2, 124.2, 124.5, 170.16, 170.52),
    c(83.1, 96.12, 97.14, 109.14, 124.08, 125.1, 170.16),
    c(56.0494, 69.0447, 83.0603, 109.0395, 110.0712,
      111.0551, 123.0429, 138.0662, 195.0876))
spd$intensity <- list(
    c(3.407, 47.494, 3.094, 100.0, 13.240),
    c(6.685, 4.381, 3.022, 16.708, 100.0, 4.565, 40.643),
    c(0.459, 2.585, 2.446, 0.508, 8.968, 0.524, 0.974, 100.0, 40.994))

sps <- Spectra(spd)
sps

## MSn data (Spectra) with 3 spectra in a MsBackendMemory backend:
##     msLevel     rtime scanIndex
##   <integer> <numeric> <integer>
## 1         2        NA        NA
## 2         2        NA        NA
## 3         2        NA        NA
##  ... 18 more variables/columns.

Alternatively, it is possible to import spectra data from mass spectrometry raw files in mzML/mzXML or CDF format. Below we create a Spectra object from two mzML files and define to use a MsBackendMzR backend to store the data (note that this requires the mzR package to be installed). This backend, specifically designed for raw MS data, keeps only a subset of spectra variables in memory while reading the m/z and intensity values from the original data files only on demand. See section Backends for more details on backends and their properties.

fls <- dir(system.file("sciex", package = "msdata"), full.names = TRUE)
sps_sciex <- Spectra(fls, source = MsBackendMzR())
sps_sciex

## MSn data (Spectra) with 1862 spectra in a MsBackendMzR backend:
##        msLevel     rtime scanIndex
##      <integer> <numeric> <integer>
## 1            1     0.280         1
## 2            1     0.559         2
## 3            1     0.838         3
## 4            1     1.117         4
## 5            1     1.396         5
## ...        ...       ...       ...
## 1858         1   258.636       927
## 1859         1   258.915       928
## 1860         1   259.194       929
## 1861         1   259.473       930
## 1862         1   259.752       931
##  ... 33 more variables/columns.
## 
## file(s):
## 20171016_POOL_POS_1_105-134.mzML
## 20171016_POOL_POS_3_105-134.mzML

The Spectra object sps_sciex allows now to access spectra data from 1862 MS1 spectra and uses MsBackendMzR as backend (the Spectra object sps created in the previous code block uses the default MsBackendMemory).

3.2 Accessing spectrum data

As detailed above Spectra objects can contain an arbitrary number of properties of a spectrum (so called spectra variables). The available variables can be listed with the spectraVariables method:

spectraVariables(sps)

##  [1] "msLevel"                 "rtime"                  
##  [3] "acquisitionNum"          "scanIndex"              
##  [5] "dataStorage"             "dataOrigin"             
##  [7] "centroided"              "smoothed"               
##  [9] "polarity"                "precScanNum"            
## [11] "precursorMz"             "precursorIntensity"     
## [13] "precursorCharge"         "collisionEnergy"        
## [15] "isolationWindowLowerMz"  "isolationWindowTargetMz"
## [17] "isolationWindowUpperMz"  "id"                     
## [19] "name"

spectraVariables(sps_sciex)

##  [1] "msLevel"                  "rtime"                   
##  [3] "acquisitionNum"           "scanIndex"               
##  [5] "dataStorage"              "dataOrigin"              
##  [7] "centroided"               "smoothed"                
##  [9] "polarity"                 "precScanNum"             
## [11] "precursorMz"              "precursorIntensity"      
## [13] "precursorCharge"          "collisionEnergy"         
## [15] "isolationWindowLowerMz"   "isolationWindowTargetMz" 
## [17] "isolationWindowUpperMz"   "peaksCount"              
## [19] "totIonCurrent"            "basePeakMZ"              
## [21] "basePeakIntensity"        "ionisationEnergy"        
## [23] "lowMZ"                    "highMZ"                  
## [25] "mergedScan"               "mergedResultScanNum"     
## [27] "mergedResultStartScanNum" "mergedResultEndScanNum"  
## [29] "injectionTime"            "filterString"            
## [31] "spectrumId"               "ionMobilityDriftTime"    
## [33] "scanWindowLowerLimit"     "scanWindowUpperLimit"

The two Spectra contain a different set of variables: besides "msLevel", "polarity", "id" and "name", that were specified for the Spectra object sps, it contains more variables such as "rtime", "acquisitionNum" and "scanIndex". These are part of the core variables defining a spectrum and for all of these accessor methods exist. Below we use msLevel and rtime to access the MS levels and retention times for the spectra in sps.

msLevel(sps)

## [1] 2 2 2

rtime(sps)

## [1] NA NA NA

We did not specify retention times for the spectra in sps thus NA is returned for them. The Spectra object sps_sciex contains many more variables, all of which were extracted from the mzML files. Below we extract the retention times for the first spectra in the object.

head(rtime(sps_sciex))

## [1] 0.280 0.559 0.838 1.117 1.396 1.675

Note that in addition to the accessor functions it is also possible to use $ to extract a specific spectra variable. To extract the name of the compounds in sps we can use sps$name, or, to extract the MS levels sps$msLevel.

sps$name

## [1] "1-Methylhistidine" "1-Methylhistidine" "Caffeine"

sps$msLevel

## [1] 2 2 2

We could also replace specific spectra variables using either the dedicated method or $. Below we specify that all spectra in sps represent centroided data.

sps$centroided <- TRUE

centroided(sps)

## [1] TRUE TRUE TRUE

The $ operator can also be used to add arbitrary new spectra variables to a Spectra object. Below we add the SPLASH key to each of the spectra.

sps$splash <- c(
    "splash10-00di-0900000000-037d24a7d65676b7e356",
    "splash10-00di-0900000000-03e99316bd6c098f5d11",
    "splash10-000i-0900000000-9af60e39c843cb715435")

This new spectra variable will now be listed as an additional variable in the result of the spectraVariables function and we can directly access its content with sps$splash.

Each spectrum can have a different number of mass peaks, each consisting of a mass-to-charge (m/z) and associated intensity value. These can be extracted with the mz or intensity functions, each of which return a list of numeric values.

mz(sps)

## NumericList of length 3
## [[1]] 109.2 124.2 124.5 170.16 170.52
## [[2]] 83.1 96.12 97.14 109.14 124.08 125.1 170.16
## [[3]] 56.0494 69.0447 83.0603 109.0395 110.0712 111.0551 123.0429 138.0662 195.0876

intensity(sps)

## NumericList of length 3
## [[1]] 3.407 47.494 3.094 100 13.24
## [[2]] 6.685 4.381 3.022 16.708 100 4.565 40.643
## [[3]] 0.459 2.585 2.446 0.508 8.968 0.524 0.974 100 40.994

Peak data can also be extracted with the peaksData function that returns a list of numerical matrices with peak variables such as m/z and intensity values. Which peak variables are available in a Spectra object can be determined with the peaksVariables function.

peaksVariables(sps)

## [1] "mz"        "intensity"

These can be passed to the peaksData function with parameter columns to extract the peak variables of interest. By default peaksData extracts m/z and intensity values.

pks <- peaksData(sps)
pks[[1]]

##          mz intensity
## [1,] 109.20     3.407
## [2,] 124.20    47.494
## [3,] 124.50     3.094
## [4,] 170.16   100.000
## [5,] 170.52    13.240

Note that we would get the same result by using the as method to coerce a Spectra object to a list or SimpleList:

as(sps, "SimpleList")

## List of length 3

The spectraData function returns a DataFrame with the full data for each spectrum (except m/z and intensity values), or with selected spectra variables (which can be specified with the columns parameter). Below we extract the spectra data for variables "msLevel", "id" and "name".

spectraData(sps, columns = c("msLevel", "id", "name"))

## DataFrame with 3 rows and 3 columns
##     msLevel          id              name
##   <integer> <character>       <character>
## 1         2 HMDB0000001 1-Methylhistidine
## 2         2 HMDB0000001 1-Methylhistidine
## 3         2 HMDB0001847          Caffeine

Spectra are one-dimensional objects storing spectra, even from different files or samples, in a single list. Specific variables have thus to be used to define the originating file from which they were extracted or the sample in which they were measured. The data origin of each spectrum can be extracted with the dataOrigin function. For sps, the Spectra created from a DataFrame, this will be NA because we did not specify the data origin:

dataOrigin(sps)

## [1] NA NA NA

dataOrigin for sps_sciex, the Spectra which was initialized with data from mzML files, in contrast, returns the originating file names:

head(basename(dataOrigin(sps_sciex)))

## [1] "20171016_POOL_POS_1_105-134.mzML" "20171016_POOL_POS_1_105-134.mzML"
## [3] "20171016_POOL_POS_1_105-134.mzML" "20171016_POOL_POS_1_105-134.mzML"
## [5] "20171016_POOL_POS_1_105-134.mzML" "20171016_POOL_POS_1_105-134.mzML"

The current data storage location of a spectrum can be retrieved with the dataStorage variable, which will return an arbitrary string for Spectra that use an in-memory backend or the file where the data is stored for on-disk backends:

dataStorage(sps)

## [1] "<memory>" "<memory>" "<memory>"

head(basename(dataStorage(sps_sciex)))

## [1] "20171016_POOL_POS_1_105-134.mzML" "20171016_POOL_POS_1_105-134.mzML"
## [3] "20171016_POOL_POS_1_105-134.mzML" "20171016_POOL_POS_1_105-134.mzML"
## [5] "20171016_POOL_POS_1_105-134.mzML" "20171016_POOL_POS_1_105-134.mzML"

Certain backends (such as the MsBackendMemory and MsBackendDataFrame) support also additional peaks variables. At present, these must already be present when the backend gets initialized. In future a dedicated function allowing to add peaks variables will be available. Below we thus first extract the full data (including peaks variables) from the sps spectra object and add a column "peak_anno" with peak annotations for each individual peak. Importantly, for peak variables, a value needs to be assigned to each individual peak, even it it is NA (the lengths of the new peak variable must match lengths of mz or intensity, i.e. the number of peaks per spectrum).

## Extract the full data from a spectrum
spd <- spectraData(sps, columns = union(spectraVariables(sps),
                                        peaksVariables(sps)))
## Add a new column with a *annotation* for each peak
spd$peak_anno <- list(c("a", NA_character_, "b", "c", "d"),
                      c("a", "b", "c", "d", "e", "f", "g"),
                      c("a", "b", "c", "d", "e", "f", "g", "h", "i"))
## lengths have to match:
lengths(spd$peak_anno)

## [1] 5 7 9

lengths(spd$mz)

## [1] 5 7 9

The parameter peaksVariables (currently only available for the backendInitialize method of MsBackendMemory and MsBackendDataFrame) allows to define which of the columns from an input data contain peaks variables (in our case "mz", "intensity" and the additional "peak_anno" column).

sps2 <- Spectra(spd, backend = MsBackendMemory(),
                peaksVariables = c("mz", "intensity", "peak_anno"))
peaksVariables(sps2)

## [1] "mz"        "intensity" "peak_anno"

Full peak data can be extracted with the peaksData function that has a second parameter columns allowing to define which peak variables to return. Below we extract the peak data for the second spectrum.

peaksData(sps2, columns = peaksVariables(sps2))[[2L]]

##       mz intensity peak_anno
## 1  83.10     6.685         a
## 2  96.12     4.381         b
## 3  97.14     3.022         c
## 4 109.14    16.708         d
## 5 124.08   100.000         e
## 6 125.10     4.565         f
## 7 170.16    40.643         g

We can also use the peaksData to extract the values for individual peak variables.

## Peak annotations for the first spectrum
peaksData(sps2, "peak_anno")[[1L]]

##   peak_anno
## 1         a
## 2      <NA>
## 3         b
## 4         c
## 5         d

## Peak annotations for the second spectrum
peaksData(sps2, "peak_anno")[[2L]]

##   peak_anno
## 1         a
## 2         b
## 3         c
## 4         d
## 5         e
## 6         f
## 7         g

Peak variables can also be extracted using the $ method:

sps2$peak_anno

## [[1]]
## [1] "a" NA  "b" "c" "d"
## 
## [[2]]
## [1] "a" "b" "c" "d" "e" "f" "g"
## 
## [[3]]
## [1] "a" "b" "c" "d" "e" "f" "g" "h" "i"

Similar to spectra variables it is also possible to replace values for existing peaks variables using the $<- function.

3.3 Filtering, subsetting and merging

Apart from classical subsetting operations such as [ and split, a set of filter functions are defined for Spectra objects (for detailed help please see the ?Spectra help). Filter and subset functions either reduce the number of spectra within a Spectra object, or affect the number of peaks (by either aggregating or subset) within each spectrum. Filter functions affecting the total number of spectra are:

filterAcquisitionNum: retains spectra with certain acquisition numbers.
filterDataOrigin: subsets to spectra from specific origins.
filterDataStorage: subsets to spectra from certain data storage files.
filterEmptySpectra: removes spectra without mass peaks.
filterMzRange: subsets spectra keeping only peaks with an m/z within the provided m/z range.
filterIsolationWindow: keeps spectra with the provided mz in their isolation window (m/z range).
filterMsLevel: filters by MS level.
filterPolarity: filters by polarity.
filterPrecursorIsotopes: identifies precursor ions (from fragment spectra) that could represent isotopes of the same molecule. For each of these spectra groups only the spectrum of the monoisotopic precursor ion is returned. MS1 spectra are returned without filtering.
filterPrecursorMaxIntensity: filters spectra keeping, for groups of spectra with similar precursor m/z, the one spectrum with the highest precursor intensity. All MS1 spectra are returned without filtering.
filterPrecursorMzRange: retains (MSn) spectra with a precursor m/z within the provided m/z range.
filterPrecursorMzValues: retains (MSn) spectra with precursor m/z value matching the provided value(s) considering also a tolerance and ppm.
filterPrecursorCharge: retains (MSn) spectra with speified precursor charge(s).
filterPrecursorScan: retains (parent and children) scans of an acquisition number.
filterRt: filters based on retention time range.

Filter functions that return the same number of spectra, but affect/subset the peaks data (m/z and intensity values) within each spectrum are:

combinePeaks: groups peaks within each spectrum based on similarity of their m/z values and combines these into a single peak per peak group.
deisotopeSpectra: deisotopes each individual spectrum keeping only the monoisotopic peak for peaks groups of potential isotopologues.
filterIntensity: filter each spectrum keeping only peaks with intensities meeting certain criteria.
filterMzRange: subsets peaks data within each spectrum keeping only peaks with their m/z values within the specified m/z range.
filterPrecursorPeaks: removes peaks with either an m/z value matching the precursor m/z of the respective spectrum (with parameter mz = "==") or peaks with an m/z value larger or equal to the precursor m/z (with parameter mz = ">=").
filterMzValues: subsets peaks within each spectrum keeping or removing (all) peaks matching provided m/z value(s) (given parameters ppm and tolerance).
reduceSpectra: filters individual spectra keeping only the largest peak for groups of peaks with similar m/z values.

In the example below we select all spectra measured in the second mzML file and subsequently filter them to retain spectra measured between 175 and 189 seconds in the measurement run.

fls <- unique(dataOrigin(sps_sciex))
file_2 <- filterDataOrigin(sps_sciex, dataOrigin = fls[2])
length(file_2)

## [1] 931

sps_sub <- filterRt(file_2, rt = c(175, 189))
length(sps_sub)

## [1] 50

In addition, Spectra support also subsetting with [. Below we perform the filtering above with [ -based subsetting.

sps_sciex[sps_sciex$dataOrigin == fls[2] &
          sps_sciex$rtime >= 175 &
          sps_sciex$rtime <= 189]

## MSn data (Spectra) with 50 spectra in a MsBackendMzR backend:
##       msLevel     rtime scanIndex
##     <integer> <numeric> <integer>
## 1           1   175.212       628
## 2           1   175.491       629
## 3           1   175.770       630
## 4           1   176.049       631
## 5           1   176.328       632
## ...       ...       ...       ...
## 46          1   187.768       673
## 47          1   188.047       674
## 48          1   188.326       675
## 49          1   188.605       676
## 50          1   188.884       677
##  ... 33 more variables/columns.
## 
## file(s):
## 20171016_POOL_POS_3_105-134.mzML

The equivalent using filter function is shown below, with the added benefit that the filtering is recorded in the processing slot.

sps_sciex |>
    filterDataOrigin(fls[2]) |>
    filterRt(c(175, 189))

## MSn data (Spectra) with 50 spectra in a MsBackendMzR backend:
##       msLevel     rtime scanIndex
##     <integer> <numeric> <integer>
## 1           1   175.212       628
## 2           1   175.491       629
## 3           1   175.770       630
## 4           1   176.049       631
## 5           1   176.328       632
## ...       ...       ...       ...
## 46          1   187.768       673
## 47          1   188.047       674
## 48          1   188.326       675
## 49          1   188.605       676
## 50          1   188.884       677
##  ... 33 more variables/columns.
## 
## file(s):
## 20171016_POOL_POS_3_105-134.mzML
## Processing:
##  Filter: select data origin(s) /home/biocbuild/bbs-3.18-bioc/R/site-library/msdata/sciex/20171016_POOL_POS_3_105-134.mzML [Tue Oct 24 19:10:53 2023]
##  Filter: select retention time [175..189] on MS level(s) 1 [Tue Oct 24 19:10:53 2023]

Note that the use of the filter functions might be more efficient for some backends, depending on their implementation, (e.g. database-based backends could translate the filter function into a SQL condition to perform the subsetting already within the database).

Multiple Spectra objects can also be combined into a single Spectra with the c or the concatenateSpectra function. The resulting Spectra object will contain an union of the spectra variables of the individual objects. Below we combine the Spectra object sps with an additional object containing another MS2 spectrum for Caffeine.

caf_df <- DataFrame(msLevel = 2L, name = "Caffeine",
                    id = "HMDB0001847",
                    instrument = "Agilent 1200 RRLC; Agilent 6520 QTOF",
                    splash = "splash10-0002-0900000000-413259091ba7edc46b87",
                    centroided = TRUE)
caf_df$mz <- list(c(110.0710, 138.0655, 138.1057, 138.1742, 195.9864))
caf_df$intensity <- list(c(3.837, 32.341, 0.84, 0.534, 100))

caf <- Spectra(caf_df)

Next we combine the two objects.

sps <- concatenateSpectra(sps, caf)
sps

## MSn data (Spectra) with 4 spectra in a MsBackendMemory backend:
##     msLevel     rtime scanIndex
##   <integer> <numeric> <integer>
## 1         2        NA        NA
## 2         2        NA        NA
## 3         2        NA        NA
## 4         2        NA        NA
##  ... 20 more variables/columns.
## Processing:
##  Merge 2 Spectra into one [Tue Oct 24 19:10:53 2023]

The resulting object contains now the data for all 4 MS2 spectra and an union of all spectra variables from both objects.

spectraVariables(sps)

##  [1] "msLevel"                 "rtime"                  
##  [3] "acquisitionNum"          "scanIndex"              
##  [5] "dataStorage"             "dataOrigin"             
##  [7] "centroided"              "smoothed"               
##  [9] "polarity"                "precScanNum"            
## [11] "precursorMz"             "precursorIntensity"     
## [13] "precursorCharge"         "collisionEnergy"        
## [15] "isolationWindowLowerMz"  "isolationWindowTargetMz"
## [17] "isolationWindowUpperMz"  "id"                     
## [19] "name"                    "splash"                 
## [21] "instrument"

The second object had an additional spectra variable instrument that was not present in sps and all the spectra in this object will thus get a value of NA for this variable.

sps$instrument

## [1] NA                                    
## [2] NA                                    
## [3] NA                                    
## [4] "Agilent 1200 RRLC; Agilent 6520 QTOF"

Sometimes not all spectra variables might be required (e.g. also because many of them are empty). This might be specifically interesting also for Spectra containing the data from very large experiments, because it can significantly reduce the object’s size in memory. In such cases the selectSpectraVariables function can be used to retain only specified spectra variables.

3.4 Data manipulations

Some analyses require manipulation of the mass peak data (i.e. the m/z and/or intensity values). One example would be to remove all peaks from a spectrum that have an intensity lower than a certain threshold. Below we perform such an operation with the replaceIntensitiesBelow function to replace peak intensities below 10 in each spectrum in sps with a value of 0.

sps_rep <- replaceIntensitiesBelow(sps, threshold = 10, value = 0)

As a result intensities below 10 were set to 0 for all peaks.

intensity(sps_rep)

## NumericList of length 4
## [[1]] 0 47.494 0 100 13.24
## [[2]] 0 0 0 16.708 100 0 40.643
## [[3]] 0 0 0 0 0 0 0 100 40.994
## [[4]] 0 32.341 0 0 100

Zero-intensity peaks (and peaks with missing intensities) can then be removed with the filterIntensity function specifying a lower required intensity level or optionally also an upper intensity limit.

sps_rep <- filterIntensity(sps_rep, intensity = c(0.1, Inf))

intensity(sps_rep)

## NumericList of length 4
## [[1]] 47.494 100 13.24
## [[2]] 16.708 100 40.643
## [[3]] 100 40.994
## [[4]] 32.341 100

The filterIntensity supports also a user-provided function to be passed with parameter intensity which would allow e.g. to remove peaks smaller than the median peak intensity of a spectrum. See examples in the ?filterIntensity help page for details.

Note that any data manipulations on Spectra objects are not immediately applied to the peak data. They are added to a so called processing queue which is applied each time peak data is accessed (with the peaksData, mz or intensity functions). Thanks to this processing queue data manipulation operations are also possible for read-only backends (e.g. mzML-file based backends or database-based backends). The information about the number of such processing steps can be seen below (next to Lazy evaluation queue).

sps_rep

## MSn data (Spectra) with 4 spectra in a MsBackendMemory backend:
##     msLevel     rtime scanIndex
##   <integer> <numeric> <integer>
## 1         2        NA        NA
## 2         2        NA        NA
## 3         2        NA        NA
## 4         2        NA        NA
##  ... 20 more variables/columns.
## Lazy evaluation queue: 2 processing step(s)
## Processing:
##  Merge 2 Spectra into one [Tue Oct 24 19:10:53 2023]
##  Signal <= 10 in MS level(s) 2 set to 0 [Tue Oct 24 19:10:53 2023]
##  Remove peaks with intensities outside [0.1, Inf] in spectra of MS level(s) 2. [Tue Oct 24 19:10:53 2023]

It is possible to add also custom functions to the processing queue of a Spectra object. Such a function must take a peaks matrix as its first argument, have ... in the function definition and must return a peaks matrix (a peaks matrix is a numeric two-column matrix with the first column containing the peaks’ m/z values and the second the corresponding intensities). Below we define a function that divides the intensities of each peak by a value which can be passed with argument y.

## Define a function that takes a matrix as input, divides the second
## column by parameter y and returns it. Note that ... is required in
## the function's definition.
divide_intensities <- function(x, y, ...) {
    x[, 2] <- x[, 2] / y
    x
}

## Add the function to the procesing queue
sps_2 <- addProcessing(sps_rep, divide_intensities, y = 2)
sps_2

## MSn data (Spectra) with 4 spectra in a MsBackendMemory backend:
##     msLevel     rtime scanIndex
##   <integer> <numeric> <integer>
## 1         2        NA        NA
## 2         2        NA        NA
## 3         2        NA        NA
## 4         2        NA        NA
##  ... 20 more variables/columns.
## Lazy evaluation queue: 3 processing step(s)
## Processing:
##  Merge 2 Spectra into one [Tue Oct 24 19:10:53 2023]
##  Signal <= 10 in MS level(s) 2 set to 0 [Tue Oct 24 19:10:53 2023]
##  Remove peaks with intensities outside [0.1, Inf] in spectra of MS level(s) 2. [Tue Oct 24 19:10:53 2023]

Object sps_2 has now 3 processing steps in its lazy evaluation queue. Calling intensity on this object will now return intensities that are half of the intensities of the original objects sps.

intensity(sps_2)

## NumericList of length 4
## [[1]] 23.747 50 6.62
## [[2]] 8.354 50 20.3215
## [[3]] 50 20.497
## [[4]] 16.1705 50

intensity(sps_rep)

## NumericList of length 4
## [[1]] 47.494 100 13.24
## [[2]] 16.708 100 40.643
## [[3]] 100 40.994
## [[4]] 32.341 100

Alternatively we could define a function that returns the maximum peak from each spectrum (note: we use the unname function to remove any names from the results):

max_peak <- function(x, ...) {
    unname(x[which.max(x[, 2]), , drop = FALSE])
}

sps_2 <- addProcessing(sps_rep, max_peak)
lengths(sps_2)

## [1] 1 1 1 1

intensity(sps_2)

## NumericList of length 4
## [[1]] 100
## [[2]] 100
## [[3]] 100
## [[4]] 100

Each spectrum in sps_2 thus contains only a single peak. The parameter spectraVariables of the addProcessing function allows in addition to define spectra variables that should be passed (in addition to the peaks matrix) to the user-provided function. This would enable for example to calculate neutral loss spectra from a Spectra by subtracting the precursor m/z from each m/z of a spectrum (note that there would also be a dedicated neutralLoss function to perform this operation more efficiently). Our tool example does not have precursor m/z values defined, thus we first set them to arbitrary values. Then we define a function neutral_loss that calculates the difference between the precursor m/z and the fragment peak’s m/z. In addition we need to ensure the peaks in the resulting spectra are ordered by (the delta) m/z values. Note that, in order to be able to access the precursor m/z of the spectrum within our function, we have to add a parameter to the function that has the same name as the spectrum variable we want to access (in our case precursorMz).

sps_rep$precursorMz <- c(170.5, 170.5, 195.1, 195.1)

neutral_loss <- function(x, precursorMz, ...) {
    x[, "mz"] <- precursorMz - x[, "mz"]
    x[order(x[, "mz"]), , drop = FALSE]
}

We have then to call addProcessing with spectraVariables = "precursorMz" to specify that this spectra variable is passed along to our function.

sps_3 <- addProcessing(sps_rep, neutral_loss,
                       spectraVariables = "precursorMz")
mz(sps_rep)

## NumericList of length 4
## [[1]] 124.2 170.16 170.52
## [[2]] 109.14 124.08 170.16
## [[3]] 138.0662 195.0876
## [[4]] 138.0655 195.9864

mz(sps_3)

## NumericList of length 4
## [[1]] -0.0200000000000102 0.340000000000003 46.3
## [[2]] 0.340000000000003 46.42 61.36
## [[3]] 0.0123999999999853 57.0338
## [[4]] -0.886400000000009 57.0345

As we can see, the precursor m/z was subtracted from each m/z of the respective spectrum. A better version of the function, that only calculates neutral loss spectra for MS level 2 spectra would be the neutral_loss function below. Since we are accessing also the spectrum’s MS level we have to call addProcessing adding also the spectra variable msLevel to the spectraVariables parameter. Note however that the msLevel spectra variable is by default renamed to spectrumMsLevel prior passing it to the function. We have thus to use a parameter called spectrumMsLevel in the neutral_loss function instead of msLevel.

neutral_loss <- function(x, spectrumMsLevel, precursorMz, ...) {
    if (spectrumMsLevel == 2L) {
        x[, "mz"] <- precursorMz - x[, "mz"]
        x <- x[order(x[, "mz"]), , drop = FALSE]
    }
    x
}
sps_3 <- addProcessing(sps_rep, neutral_loss,
                       spectraVariables = c("msLevel", "precursorMz"))
mz(sps_3)

## NumericList of length 4
## [[1]] -0.0200000000000102 0.340000000000003 46.3
## [[2]] 0.340000000000003 46.42 61.36
## [[3]] 0.0123999999999853 57.0338
## [[4]] -0.886400000000009 57.0345

Using the same concept it would also be possible to provide any spectrum-specific user-defined value to the processing function. This variable could simply be added first as a new spectra variable to the Spectra object and then this variable could be passed along to the function in the same way we passed the precursor m/z to our function above.

Another example for spectra processing potentially helpful for spectral matching against reference fragment spectra libraries would be a function that removes fragment peaks with an m/z matching the precursor m/z of a spectrum. Below we define such a function that takes the peaks matrix and the precursor m/z as input and evaluates with the closest function from the MsCoreUtils whether the spectrum contains peaks with an m/z value matching the one of the precursor (given tolerance and ppm). The returned peaks matrix contains all peaks except those matching the precursor m/z.

library(MsCoreUtils)
remove_precursor <- function(x, precursorMz, tolerance = 0.1, ppm = 0, ...) {
    if (!is.na(precursorMz)) {
        keep <- is.na(closest(x[, "mz"], precursorMz, tolerance = tolerance,
                             ppm = ppm, .check = FALSE))
        x[keep, , drop = FALSE]
    } else x
}

We can now again add this processing step to our Spectra object. As a result, peaks matching the precursor m/z (with tolerance = 0.1 and ppm = 0) will be removed.

sps_4 <- addProcessing(sps_rep, remove_precursor,
                       spectraVariables = "precursorMz")

peaksData(sps_4) |> as.list()

## [[1]]
##          mz intensity
## [1,] 124.20    47.494
## [2,] 170.16   100.000
## 
## [[2]]
##          mz intensity
## [1,] 109.14    16.708
## [2,] 124.08   100.000
## [3,] 170.16    40.643
## 
## [[3]]
##            mz intensity
## [1,] 138.0662       100
## 
## [[4]]
##            mz intensity
## [1,] 138.0655    32.341
## [2,] 195.9864   100.000

As a reference, the original peak matrices are shown below.

peaksData(sps_rep) |> as.list()

## [[1]]
##          mz intensity
## [1,] 124.20    47.494
## [2,] 170.16   100.000
## [3,] 170.52    13.240
## 
## [[2]]
##          mz intensity
## [1,] 109.14    16.708
## [2,] 124.08   100.000
## [3,] 170.16    40.643
## 
## [[3]]
##            mz intensity
## [1,] 138.0662   100.000
## [2,] 195.0876    40.994
## 
## [[4]]
##            mz intensity
## [1,] 138.0655    32.341
## [2,] 195.9864   100.000

Note that we can also perform a more relaxed matching of m/z values by passing a different value for tolerance to the function:

sps_4 <- addProcessing(sps_rep, remove_precursor, tolerance = 0.6,
                       spectraVariables = "precursorMz")
peaksData(sps_4) |> as.list()

## [[1]]
##         mz intensity
## [1,] 124.2    47.494
## 
## [[2]]
##          mz intensity
## [1,] 109.14    16.708
## [2,] 124.08   100.000
## 
## [[3]]
##            mz intensity
## [1,] 138.0662       100
## 
## [[4]]
##            mz intensity
## [1,] 138.0655    32.341
## [2,] 195.9864   100.000

Since all data manipulations above did not change the original intensity or m/z values, it is possible to restore the original data. This can be done with the reset function which will empty the lazy evaluation queue and call the reset method on the storage backend. Below we call reset on the sps_2 object and hence restore the data to its original state.

sps_2_rest <- reset(sps_2)

intensity(sps_2_rest)

## NumericList of length 4
## [[1]] 3.407 47.494 3.094 100 13.24
## [[2]] 6.685 4.381 3.022 16.708 100 4.565 40.643
## [[3]] 0.459 2.585 2.446 0.508 8.968 0.524 0.974 100 40.994
## [[4]] 3.837 32.341 0.84 0.534 100

intensity(sps)

## NumericList of length 4
## [[1]] 3.407 47.494 3.094 100 13.24
## [[2]] 6.685 4.381 3.022 16.708 100 4.565 40.643
## [[3]] 0.459 2.585 2.446 0.508 8.968 0.524 0.974 100 40.994
## [[4]] 3.837 32.341 0.84 0.534 100

Finally, for Spectra that use a writeable backend, such as the MsBackendMemory, MsBackendDataFrame or MsBackendHdf5Peaks, it is possible to apply the processing queue to the peak data and write that back to the data storage with the applyProcessing function. Below we use this to make all data manipulations on peak data of the sps_rep object persistent.

length(sps_rep@processingQueue)

## [1] 2

sps_rep <- applyProcessing(sps_rep)
length(sps_rep@processingQueue)

## [1] 0

sps_rep

## MSn data (Spectra) with 4 spectra in a MsBackendMemory backend:
##     msLevel     rtime scanIndex
##   <integer> <numeric> <integer>
## 1         2        NA        NA
## 2         2        NA        NA
## 3         2        NA        NA
## 4         2        NA        NA
##  ... 20 more variables/columns.
## Processing:
##  Merge 2 Spectra into one [Tue Oct 24 19:10:53 2023]
##  Signal <= 10 in MS level(s) 2 set to 0 [Tue Oct 24 19:10:53 2023]
##  Remove peaks with intensities outside [0.1, Inf] in spectra of MS level(s) 2. [Tue Oct 24 19:10:53 2023]
##  ...1 more processings. Use 'processingLog' to list all.

Before applyProcessing the lazy evaluation queue contained 2 processing steps, which were then applied to the peak data and written to the data storage. Note that calling reset after applyProcessing can no longer restore the data.

3.5 Visualizing `Spectra`

The Spectra package provides the following functions to visualize spectra data: - plotSpectra: plot each spectrum in Spectra in its own panel. - plotSpectraOverlay: plot multiple spectra into the same plot.

Below we use plotSpectra to plot the 4 spectra from the sps object using their names (as provided in spectra variable "name") as plot titles.

plotSpectra(sps, main = sps$name)

It is also possible to label individual peaks in each plot. Below we use the m/z value of each peak as its label. In the example we define a function that accesses information from each spectrum (z) and returns a character for each peak with the text that should be used as label. Parameters labelSrt, labelPos and labelOffset define the rotation of the label text and its position relative to the x and y coordinates of the peak.

plotSpectra(sps, main = sps$name,
            labels = function(z) format(mz(z)[[1L]], digits = 4),
            labelSrt = -30, labelPos = 2, labelOffset = 0.1)

These plots are rather busy and for some peaks the m/z values are overplotted. Below we define a label function that will only indicate the m/z of peaks with an intensity higher than 30.

mzLabel <- function(z) {
    z <- peaksData(z)[[1L]]
    lbls <- format(z[, "mz"], digits = 4)
    lbls[z[, "intensity"] < 30] <- ""
    lbls
}
plotSpectra(sps, main = sps$name, labels = mzLabel,
            labelSrt = -30, labelPos = 2, labelOffset = 0.1)

Sometimes it might be of interest to plot multiple spectra into the same plot (e.g. to directly compare peaks from multiple spectra). This can be done with plotSpectraOverlay which we use below to create an overlay-plot of our 4 example spectra, using a different color for each spectrum.

cols <- c("#E41A1C80", "#377EB880", "#4DAF4A80", "#984EA380")
plotSpectraOverlay(sps, lwd = 2, col = cols)
legend("topleft", col = cols, legend = sps$name, pch = 15)

Lastly, plotSpectraMirror allows to plot two spectra against each other as a mirror plot which is ideal to visualize spectra comparison results. Below we plot a spectrum of 1-Methylhistidine against one of Caffeine.

plotSpectraMirror(sps[1], sps[3])

The upper panel shows the spectrum from 1-Methylhistidine, the lower the one of Caffeine. None of the peaks of the two spectra match. Below we plot the two spectra of 1-Methylhistidine and the two of Caffeine against each other matching peaks with a ppm of 50.

par(mfrow = c(1, 2))
plotSpectraMirror(sps[1], sps[2], main = "1-Methylhistidine", ppm = 50)
plotSpectraMirror(sps[3], sps[4], main = "Caffeine", ppm = 50)

See also ?plotSpectra for more plotting options and examples.

3.6 Aggregating spectra data

The Spectra package provides the combineSpectra function that allows to aggregate multiple spectra into a single one. The main parameters of this function are f, which defines the grouping of the spectra, and FUN which allows to define the function that performs the actual aggregation. The default aggregation function is combinePeaksData (see ?combinePeaksData for details) that combines multiple spectra into a single spectrum with all peaks from all input spectra (with additional paramter peaks = "union"), or peaks that are present in a certain proportion of input spectra (with parameter peaks = "intersect"; parameter minProp allows to define the minimum required proportion of spectra in which a peak needs to be present. Below we use this function to combine the spectra for 1-methylhistidine and caffeine into a single spectrum for each compound. We use the spectra variable $name, that contains the names of the compounds, to define which spectra should be grouped together.

sps_agg <- combineSpectra(sps, f = sps$name)

As a result, the 4 spectra got aggregated into two.

plotSpectra(sps_agg, main = sps_agg$name)

By default, all peaks present in all spectra are reported. As an alternative, by specifying peaks = "intersect" and minProp = 1, we could combine the spectra keeping only peaks that are present in both input spectra.

sps_agg <- combineSpectra(sps, f = sps$name, peaks = "intersect", minProp = 1)
plotSpectra(sps_agg, main = sps_agg$name)

This results thus in a single peak for 1-methylhistidine and none for caffeine - why? The reason for that is that the difference of the peaks’ m/z values is larger than the default tolerance used for the peak grouping (the defaults for combinePeaksData is tolerance = 0 and ppm = 0). We could however already see in the previous section that the reported peaks’ m/z values have a larger measurement error (most likely because the fragment spectra were measured on different instruments with different precision). Thus, we next increase the tolerance and ppm parameters to group also peaks with a larger difference in their m/z values.

sps_agg <- combineSpectra(sps, f = sps$name, peaks = "intersect",
                          minProp = 1, tolerance = 0.2)
plotSpectra(sps_agg, main = sps_agg$name)

Whether in a real analysis we would be OK with such a large tolerance is however questionable. Note: which m/z and intensity is reported for the aggregated spectra can be defined with the parameters intensityFun and mzFun of combinePeaksData (see ?combinePeaksData for more information).

While the combinePeaksData function is indeed helpful to combine peaks from different spectra, the combineSpectra function would in addition also allow us to provide our own, custom, peak aggregation function. As a simple example, instead of combining the spectra, we would like to select one of the input spectra as representative spectrum for grouped input spectra. combineSpectra supports any function that takes a list of peak matrices as input and returns a single peak matrix as output. We thus define below a function that calculates the total signal (TIC) for each input peak matrix, and returns the one peak matrix with the largest TIC.

#' function to select and return the peak matrix with the largest tic from
#' the provided list of peak matrices.
maxTic <- function(x, ...) {
    tic <- vapply(x, function(z) sum(z[, "intensity"], na.rm = TRUE),
                  numeric(1))
    x[[which.max(tic)]]
}

We can now use this function with combineSpectra to select for each compound the spectrum with the largest TIC.

sps_agg <- combineSpectra(sps, f = sps$name, FUN = maxTic)
plotSpectra(sps_agg, main = sps_agg$name)

3.7 Comparing spectra

Spectra can be compared with the compareSpectra function, that allows to calculate similarities between spectra using a variety of methods. compareSpectra implements similarity scoring as a two-step approach: first the peaks from the pair of spectra that should be compared are matched (mapped) against each other and then a similarity score is calculated on these. The MAPFUN parameter of compareSpectra defines the function to match (or map) the peaks between the spectra and parameter FUN specifies the function to calculate the similarity. By default, compareSpectra uses MAPFUN = joinPeaks (see ?joinPeaks for a description and alternative options) and FUN = ndotproduct (the normalized dot-product spectra similarity score). Parameters to configure these functions can be passed to compareSpectra as additional parameter (such as e.g. ppm to define the m/z-relative tolerance for peak matching in joinPeaks).

Below we calculate pairwise similarities between all spectra in sps accepting a 50 ppm difference of peaks’ m/z values for being considered matching.

compareSpectra(sps, ppm = 50)

##           1         2         3         4
## 1 1.0000000 0.1380817 0.0000000 0.0000000
## 2 0.1380817 1.0000000 0.0000000 0.0000000
## 3 0.0000000 0.0000000 1.0000000 0.1817149
## 4 0.0000000 0.0000000 0.1817149 1.0000000

The resulting matrix provides the similarity scores from the pairwise comparison. As expected, the first two and the last two spectra are similar, albeit only moderately, while the spectra from 1-Methylhistidine don’t share any similarity with those of Caffeine. Similarities between Spectra objects can be calculated with calls in the form of compareSpectra(a, b) with a and b being the two Spectra objects to compare. As a result a n x m matrix will be returned with n (rows) being the spectra in a and m (columns) being the spectra in b.

The above similarity was calculated with the default (normalized) dot-product, but also other similarity scores can be used instead. Either one of the other metrics provided by the MsCoreUtils could be used (see ?MsCoreUtils::distance for a list of available options) or any other external or user-provided similarity scoring function. As an example, we use below the spectral entropy similarity score introduced in (Y et al. 2021) and provided with the msentropy package. Since this msentropy_similarity function performs also the mapping of the peaks between the compared spectra internally (along with some spectra cleaning), we have to disable that in the compareSpectra function using MAPFUN = joinPeaksNone. To configure the similarity scoring we can pass all additional parameters of the msentropy_similarity (see ?msentropy_similarity) to the compareSpectra call. We use ms2_tolerance_in_ppm = 50 to set the tolerance for m/z-relative peak matching (equivalent to ppm = 50 used above) and ms2_tolerance_in_da = -1 to disable absolute tolerance matching.

library(msentropy)

## Loading required package: Rcpp

compareSpectra(sps, MAPFUN = joinPeaksNone, FUN = msentropy_similarity,
               ms2_tolerance_in_ppm = 50, ms2_tolerance_in_da = -1)

##           1         2         3         4
## 1 1.0000000 0.3002225 0.0000000 0.0000000
## 2 0.3002225 1.0000000 0.0000000 0.0000000
## 3 0.0000000 0.0000000 1.0000000 0.5144764
## 4 0.0000000 0.0000000 0.5144764 1.0000000

Note also that GNPS-like scores can be calculated with MAPFUN = joinPeaksGnps and FUN = MsCoreUtils::gnps. For additional information and examples see also (Rainer et al. 2022) or the SpectraTutorials tutorial.

Another way of comparing spectra would be to bin the spectra and to cluster them based on similar intensity values. Spectra binning ensures that the binned m/z values are comparable across all spectra. Below we bin our spectra using a bin size of 0.1 (i.e. all peaks with an m/z smaller than 0.1 are aggregated into one binned peak.

sps_bin <- Spectra::bin(sps, binSize = 0.1)

All spectra will now have the same number of m/z values.

lengths(sps_bin)

## [1] 1400 1400 1400 1400

Most of the intensity values for these will however be 0 (because in the original spectra no peak for the respective m/z bin was present).

intensity(sps_bin)

## NumericList of length 4
## [[1]] 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 ... 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0
## [[2]] 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 ... 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0
## [[3]] 0.459 0 0 0 0 0 0 0 0 0 0 0 0 0 0 ... 0 0 0 0 0 40.994 0 0 0 0 0 0 0 0 0
## [[4]] 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 ... 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 100

We’re next creating an intensity matrix for our Spectra object, each row being one spectrum and columns representing the binned m/z values.

intmat <- do.call(rbind, intensity(sps_bin))

We can now identify those columns (m/z bins) with only 0s across all spectra and remove these.

zeros <- colSums(intmat) == 0
intmat <- intmat[, !zeros]
intmat

##       [,1]  [,2]  [,3]  [,4]  [,5]  [,6]  [,7]   [,8]  [,9] [,10] [,11] [,12]
## [1,] 0.000 0.000 0.000 0.000 0.000 0.000 0.000  0.000 3.407 0.000 0.000 0.000
## [2,] 0.000 0.000 0.000 6.685 4.381 3.022 0.000 16.708 0.000 0.000 0.000 0.000
## [3,] 0.459 2.585 2.446 0.000 0.000 0.000 0.508  0.000 0.000 8.968 0.524 0.974
## [4,] 0.000 0.000 0.000 0.000 0.000 0.000 0.000  0.000 0.000 3.837 0.000 0.000
##      [,13]  [,14] [,15] [,16]   [,17] [,18]   [,19] [,20]  [,21] [,22]
## [1,]     0 47.494 3.094 0.000   0.000 0.000 100.000 13.24  0.000     0
## [2,]   100  0.000 0.000 4.565   0.000 0.000  40.643  0.00  0.000     0
## [3,]     0  0.000 0.000 0.000 100.000 0.000   0.000  0.00 40.994     0
## [4,]     0  0.000 0.000 0.000  32.341 1.374   0.000  0.00  0.000   100

The associated m/z values for the bins can be extracted with mz from the binned Spectra object. Below we use these as column names for the intensity matrix.

colnames(intmat) <- mz(sps_bin)[[1L]][!zeros]

This intensity matrix could now for example be used to cluster the spectra based on their peak intensities.

heatmap(intmat)

As expected, the first 2 and the last 2 spectra are more similar and are clustered together.

3.8 Exporting spectra

Spectra data can be exported with the export method. This method takes the Spectra that is supposed to be exported and the backend (parameter backend) which should be used to export the data and additional parameters for the export function of this backend. The backend thus defines the format of the exported file. Note however that not all MsBackend classes might support data export. The backend classes currently supporting data export and its format are: - MsBackendMzR (Spectra package): export data in mzML and mzXML format. Can not export all custom, user specified spectra variables. - MsBackendMgf (MsBackendMgf package): exports data in Mascot Generic Format (mgf). Exports all spectra variables as individual spectrum fields in the mgf file. - MsBackendMsp (MsBackendMsp): exports data in NIST MSP format. - MsBackendMassbank (MsBackendMassbank) exports data in Massbank text file format.

In the example below we use the MsBackendMzR to export all spectra from the variable sps to an mzML file. We thus pass the data, the backend that should be used for the export and the file name of the result file (a temporary file) to the export function (see also the help page of the export,MsBackendMzR function for additional supported parameters).

fl <- tempfile()
export(sps, MsBackendMzR(), file = fl)

To evaluate which of the spectra variables were exported, we load the exported data again and identify spectra variables in the original file which could not be exported (because they are not defined variables in the mzML standard).

sps_im <- Spectra(backendInitialize(MsBackendMzR(), fl))
spectraVariables(sps)[!spectraVariables(sps) %in% spectraVariables(sps_im)]

## [1] "id"         "name"       "splash"     "instrument"

These additional variables were thus not exported. How data export is performed and handled depends also on the used backend. The MsBackendMzR for example exports all spectra by default to a single file (specified with the file parameter), but it allows also to specify for each individual spectrum in the Spectra to which file it should be exported (parameter file has thus to be of length equal to the number of spectra). As an example we export below the spectrum 1 and 3 to one file and spectra 2 and 4 to another.

fls <- c(tempfile(), tempfile())
export(sps, MsBackendMzR(), file = fls[c(1, 2, 1, 2)])

A more realistic use case for mzML export would be to export MS data after processing, such as smoothing (using the smooth function) and centroiding (using the pickPeaks function) of raw profile-mode MS data.

3.9 Changing backends

In the previous sections we learned already that a Spectra object can use different backends for the actual data handling. It is also possible to change the backend of a Spectra to a different one with the setBackend function. We could for example change the (MsBackendMzR) backend of the sps_sciex object to a MsBackendMemory backend to enable use of the data even without the need to keep the original mzML files. Below we change the backend of sps_sciex to the in-memory MsBackendMemory backend.

print(object.size(sps_sciex), units = "Mb")

## 0.4 Mb

sps_sciex <- setBackend(sps_sciex, MsBackendMemory())
sps_sciex

## MSn data (Spectra) with 1862 spectra in a MsBackendMemory backend:
##        msLevel     rtime scanIndex
##      <integer> <numeric> <integer>
## 1            1     0.280         1
## 2            1     0.559         2
## 3            1     0.838         3
## 4            1     1.117         4
## 5            1     1.396         5
## ...        ...       ...       ...
## 1858         1   258.636       927
## 1859         1   258.915       928
## 1860         1   259.194       929
## 1861         1   259.473       930
## 1862         1   259.752       931
##  ... 33 more variables/columns.
## Processing:
##  Switch backend from MsBackendMzR to MsBackendMemory [Tue Oct 24 19:11:00 2023]

With the call the full peak data was imported from the original mzML files into the object. This has obviously an impact on the object’s size, which is now much larger than before.

print(object.size(sps_sciex), units = "Mb")

## 53.2 Mb

The dataStorage spectrum variable has now changed, while dataOrigin still keeps the information about the originating files:

head(dataStorage(sps_sciex))

## [1] "<memory>" "<memory>" "<memory>" "<memory>" "<memory>" "<memory>"

head(basename(dataOrigin(sps_sciex)))

## [1] "20171016_POOL_POS_1_105-134.mzML" "20171016_POOL_POS_1_105-134.mzML"
## [3] "20171016_POOL_POS_1_105-134.mzML" "20171016_POOL_POS_1_105-134.mzML"
## [5] "20171016_POOL_POS_1_105-134.mzML" "20171016_POOL_POS_1_105-134.mzML"

3.10 Parallel processing notes

Most functions on Spectra support (and use) parallel processing out of the box. Peak data access and manipulation methods perform by default parallel processing on a per-file basis (i.e. using the dataStorage variable as splitting factor). Spectra uses BiocParallel for parallel processing and all functions use the default registered parallel processing setup of that package (see ?bpparam() for more information).

Note however that some backends (e.g. those using connections to SQL databases such as MsBackendMassbank, MsBackendSql) do not support parallel processing because the database connection can not be shared across processes. The backendBpparam function allows to evaluate whether a Spectra object (or in fact its used MsBackend class) supports a certain parallel processing setup. Calling backendBpparam on a Spectra with a backend that does not support parallel processing would (should) return SerialParam(), always. Below we create an empty Spectra object and test whether that supports parallel processing.

tmp <- Spectra()
backendBpparam(tmp)

## class: MulticoreParam
##   bpisup: FALSE; bpnworkers: 4; bptasks: 0; bpjobname: BPJOB
##   bplog: FALSE; bpthreshold: INFO; bpstopOnError: TRUE
##   bpRNGseed: ; bptimeout: NA; bpprogressbar: FALSE
##   bpexportglobals: TRUE; bpexportvariables: FALSE; bpforceGC: FALSE
##   bpfallback: TRUE
##   bplogdir: NA
##   bpresultdir: NA
##   cluster type: FORK

The backend (in this case a MsBackendMemory thus supports parallel processing. We can also specifically test this for individual backends (and parallel setups):

backendBpparam(MsBackendDataFrame(), SnowParam(2))

## class: SnowParam
##   bpisup: FALSE; bpnworkers: 2; bptasks: 0; bpjobname: BPJOB
##   bplog: FALSE; bpthreshold: INFO; bpstopOnError: TRUE
##   bpRNGseed: ; bptimeout: NA; bpprogressbar: FALSE
##   bpexportglobals: TRUE; bpexportvariables: TRUE; bpforceGC: FALSE
##   bpfallback: TRUE
##   bplogdir: NA
##   bpresultdir: NA
##   cluster type: SOCK

4 Backends

Backends allow to use different backends to store mass spectrometry data while providing via the Spectra class a unified interface to use that data. This is a further abstraction to the on-disk and in-memory data modes from MSnbase (Gatto, Gibb, and Rainer 2020). The Spectra package defines a set of example backends but any object extending the base MsBackend class could be used instead. The default backends are:

MsBackendMemory: the default backend to store data in memory. Due to its design the MsBackendMemory provides fast access to the peaks matrices (using the peaksData function) and is also optimized for fast access to spectra variables and subsetting. Since all data is kept in memory, this backend has a relatively large memory footprint (depending on the data) and is thus not suggested for very large MS experiments.
MsBackendDataFrame: the mass spectrometry data is stored (in-memory) in a DataFrame. Keeping the data in memory guarantees high performance but has also, depending on the number of mass peaks in each spectrum, a much higher memory footprint.
MsBackendMzR: this backend keeps only general spectra variables in memory and relies on the mzR package to read mass peaks (m/z and intensity values) from the original MS files on-demand.
MsBackendHdf5Peaks: similar to MsBackendMzR this backend reads peak data only on-demand from disk while all other spectra variables are kept in memory. The peak data are stored in Hdf5 files which guarantees scalability.

All of the above mentioned backends support changing all of their their spectra variables, except the MsBackendMzR that does not support changing m/z or intensity values for the mass peaks.

With the example below we load the data from a single mzML file and use a MsBackendHdf5Peaks backend for data storage. The hdf5path parameter allows us to specify the storage location of the HDF5 file.

library(msdata)
fl <- proteomics(full.names = TRUE)[5]

sps_tmt <- Spectra(fl, backend = MsBackendHdf5Peaks(), hdf5path = tempdir())
head(basename(dataStorage(sps_tmt)))

## [1] "TMT_Erwinia_1uLSike_Top10HCD_isol2_45stepped_60min_01.mzML.h5"
## [2] "TMT_Erwinia_1uLSike_Top10HCD_isol2_45stepped_60min_01.mzML.h5"
## [3] "TMT_Erwinia_1uLSike_Top10HCD_isol2_45stepped_60min_01.mzML.h5"
## [4] "TMT_Erwinia_1uLSike_Top10HCD_isol2_45stepped_60min_01.mzML.h5"
## [5] "TMT_Erwinia_1uLSike_Top10HCD_isol2_45stepped_60min_01.mzML.h5"
## [6] "TMT_Erwinia_1uLSike_Top10HCD_isol2_45stepped_60min_01.mzML.h5"

A (possibly incomplete) list of R packages providing additional backends that add support for additional data types or storage options is provided below:

MsBackendMgf: support for import/export of mass spectrometry files in mascot generic format (MGF).
MsBackendMsp: allows to import/export data in NIST MSP format. Extends the MsBackendDataFrame and keeps thus all data, after import, in memory.
MsBackendMassbank (package MsBackendMassbank): allows to import/export data in MassBank text file format. Extends the MsBackendDataFrame and keeps thus all data, after import, in memory.
MsBackendMassbankSql (package MsBackendMassbank): allows to directly connect to a MassBank SQL database to retrieve all MS data and variables. Has a minimal memory footprint because all data is retrieved on-the-fly from the SQL database.
MsBackendSql: stores all MS data in a SQL database and has thus a minimal memory footprint.
MsBackendCompDb (package CompoundDb): provides access to spectra data (spectra and peaks variables) from a CompDb database. Has a small memory footprint because all data (except precursor m/z values) are retrieved on-the-fly from the database.
MsBackendRawFileReader: implements a backend for reading MS data from Thermo Fisher Scientific’s raw data files using the manufacturer’s NewRawFileReader .Net libraries. The package generalizes the functionality introduced by the rawrr package, see also (Kockmann and Panse 2021).
MsBackendHmdbXml (package MsbackendHmdb): allows import of MS data from xml files of the Human Metabolome Database (HMDB). Extends the MsBackendDataFrame and keeps thus all data, after import, in memory.
MsBackendTimsTof (package MsBackendTimsTof: allows import of data from Bruker TimsTOF raw data files (using the opentimsr R package).
MsBackendWeizMass (package MsBackendWeizMass: allows to access MS data from WeizMass MS/MS spectral databases.

5 Handling very large data sets

The Spectra package was designed to support also efficient processing of very large data sets. Most of the functionality do not require to keep the full MS data in memory (specifically, the peaks data, i.e., m/z and intensity values, which represent the largest chunk of data for MS experiments). For some functions however the peaks data needs to be loaded into memory. One such example is the lengths function to determine the number of peaks per spectra that is calculated (on the fly) by evaluating the number of rows of the peaks matrix. Backends such as the MsBackendMzR perform by default any data processing separately (and eventually in parallel) by data file and it should thus be safe to call any such functions on a Spectra object with that backend. For other backends (such as the MsBackendSql or the MsBackendMassbankSql) it is however advised to process the data in a chunk-wise manner using the spectrapply function with parameter chunkSize. This will split the original Spectra object into chunks of size chunkSize and applies the function separately to each chunk. That way only data from one chunk will eventually be loaded into memory in each iteration enabling to process also very large Spectra objects on computers with limited hardware resources. Instead of a lengths(sps) call, the number of peaks per spectra could also be determined (in a less memory demanding way) with spectrapply(sps, lengths, chunkSize = 5000L). In that way only peak data of 5000 spectra at a time will be loaded into memory.

6 Session information

sessionInfo()

## R version 4.3.1 (2023-06-16)
## Platform: x86_64-pc-linux-gnu (64-bit)
## Running under: Ubuntu 22.04.3 LTS
## 
## Matrix products: default
## BLAS:   /home/biocbuild/bbs-3.18-bioc/R/lib/libRblas.so 
## LAPACK: /usr/lib/x86_64-linux-gnu/lapack/liblapack.so.3.10.0
## 
## locale:
##  [1] LC_CTYPE=en_US.UTF-8       LC_NUMERIC=C              
##  [3] LC_TIME=en_GB              LC_COLLATE=C              
##  [5] LC_MONETARY=en_US.UTF-8    LC_MESSAGES=en_US.UTF-8   
##  [7] LC_PAPER=en_US.UTF-8       LC_NAME=C                 
##  [9] LC_ADDRESS=C               LC_TELEPHONE=C            
## [11] LC_MEASUREMENT=en_US.UTF-8 LC_IDENTIFICATION=C       
## 
## time zone: America/New_York
## tzcode source: system (glibc)
## 
## attached base packages:
## [1] stats4    stats     graphics  grDevices utils     datasets  methods  
## [8] base     
## 
## other attached packages:
##  [1] msdata_0.41.0       msentropy_0.1.4     Rcpp_1.0.11        
##  [4] MsCoreUtils_1.14.0  IRanges_2.36.0      Spectra_1.12.0     
##  [7] ProtGenerics_1.34.0 BiocParallel_1.36.0 S4Vectors_0.40.0   
## [10] BiocGenerics_0.48.0 BiocStyle_2.30.0   
## 
## loaded via a namespace (and not attached):
##  [1] jsonlite_1.8.7         compiler_4.3.1         BiocManager_1.30.22   
##  [4] Biobase_2.62.0         rhdf5filters_1.14.0    magick_2.8.1          
##  [7] parallel_4.3.1         cluster_2.1.4          jquerylib_0.1.4       
## [10] yaml_2.3.7             fastmap_1.1.1          R6_2.5.1              
## [13] knitr_1.44             MASS_7.3-60            bookdown_0.36         
## [16] bslib_0.5.1            rlang_1.1.1            cachem_1.0.8          
## [19] xfun_0.40              fs_1.6.3               sass_0.4.7            
## [22] cli_3.6.1              Rhdf5lib_1.24.0        magrittr_2.0.3        
## [25] digest_0.6.33          ncdf4_1.21             mzR_2.36.0            
## [28] MetaboCoreUtils_1.10.0 rhdf5_2.46.0           clue_0.3-65           
## [31] evaluate_0.22          codetools_0.2-19       rmarkdown_2.25        
## [34] tools_4.3.1            htmltools_0.5.6.1

References

Gatto, Laurent, Sebastian Gibb, and Johannes Rainer. 2020. “MSnbase, Efficient and Elegant R-Based Processing and Visualization of Raw Mass Spectrometry Data.” Journal of Proteome Research, September. https://doi.org/10.1021/acs.jproteome.0c00313.

Kockmann, Tobias, and Christian Panse. 2021. “The rawrr R Package: Direct Access to Orbitrap Data and Beyond.” Journal of Proteome Research. https://doi.org/10.1021/acs.jproteome.0c00866.

Rainer, Johannes, Andrea Vicini, Liesa Salzer, Jan Stanstrup, Josep M. Badia, Steffen Neumann, Michael A. Stravs, et al. 2022. “A Modular and Expandable Ecosystem for Metabolomics Data Annotation in R.” Metabolites 12 (2): 173. https://doi.org/10.3390/metabo12020173.

Y, Li, Kind T, Folz J, Vaniya A, Mehta Ss, and Fiehn O. 2021. “Spectral Entropy Outperforms MS/MS Dot Product Similarity for Small-Molecule Compound Identification.” Nature Methods 18 (12). https://doi.org/10.1038/s41592-021-01331-z.

Description and usage of Spectra objects

24 October 2023

1 Introduction

2 Installation

3 General usage

3.1 Creating `Spectra` objects

3.2 Accessing spectrum data

3.3 Filtering, subsetting and merging

3.4 Data manipulations

3.5 Visualizing `Spectra`

3.6 Aggregating spectra data

3.7 Comparing spectra

3.8 Exporting spectra

3.9 Changing backends

3.10 Parallel processing notes

4 Backends

5 Handling very large data sets

6 Session information

References

Description and usage of Spectra objects

24 October 2023

1 Introduction

2 Installation

3 General usage

3.1 Creating Spectra objects

3.2 Accessing spectrum data

3.3 Filtering, subsetting and merging

3.4 Data manipulations

3.5 Visualizing Spectra

3.6 Aggregating spectra data

3.7 Comparing spectra

3.8 Exporting spectra

3.9 Changing backends

3.10 Parallel processing notes

4 Backends

5 Handling very large data sets

6 Session information

References

3.1 Creating `Spectra` objects

3.5 Visualizing `Spectra`