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Two MATLAB programs for computing paleo-elevations
and burial ages from paired-cosmogenic nuclides
Pierre-Henri Blard, Maarten Lupker, Moïse Rousseau, Jim Tesson
To cite this version:
Pierre-Henri Blard, Maarten Lupker, Moïse Rousseau, Jim Tesson. Two MATLAB programs for
computing paleo-elevations and burial ages from paired-cosmogenic nuclides. MethodsX, Elsevier,
2019, 6, pp.1547-1556. �10.1016/j.mex.2019.05.017�. �hal-02377566�
Method
article
Two
MATLAB
programs
for
computing
paleo-elevations
and
burial
ages
from
paired-cosmogenic
nuclides
Pierre-Henri
Blard
a,b,*
,
Maarten
Lupker
c,
Moïse
Rousseau
d,
Jim
Tesson
aa
CentredeRecherchesPétrographiquesetGéochimiques(CRPG),UMR7358,CNRS-UniversitédeLorraine, 15rueNotreDamedesPauvres,54500Vandoeuvre-lès-Nancy,France
bLaboratoiredeGlaciologie,DGES-IGEOS,UniversitéLibredeBruxelles,1050Bruxelles,Belgium c
ETHZürich-GeologicalInstitute,Sonnegstrasse5,8092Zürich,Switzerland
d
ResearchInstituteonMinesandEnvironment(RIME)UQAT-Polytechnique,Montréal,Canada ABSTRACT
Methodsbasedoncosmic-rayproducednuclidesarekeytoimproveourunderstandingoftheEarthsurface dynamic.Measuringmultiplecosmogenicnuclidesinthesamerocksamplehasagreatpotential,butdata interpretationrequiresrigorousandoftencomplexmathematicaltreatments.Inordertomakeprogressonthis topic,thispaperpresentstwoeasy-to-useMATLAB©programspermittingtoderiveinformationfrompairsof
cosmogenicnuclides(26Al-10Beor10Be-21Ne)measuredinrocksamplesthathavebeenexposedtocosmicraysin
thepast:“Paleoaltitude.m”and“Burial.m”Codesavailablehereassupplementarymaterial.
“Paleoaltitude.m” computes paleoelevations from a sample whose burial age is known. This new paleoaltimetrymethod is presented in detail in Blard et al.[1]. The present article also develops the mathematicalapproach.
Sincetheelevationofexposuremayaffecttheaccuracyofaburialage[1],thesecondMATLAB©script“Burial. m”isdesignedtocomputeburialagesfrom26Al-10Beor10Be-21Nepairs,takingintoaccountthepositionofa
sample(elevationandlatitude)duringitspreburialexposurehistory.
©2019PublishedbyElsevierB.V.ThisisanopenaccessarticleundertheCCBY-NC-NDlicense(http:// creativecommons.org/licenses/by-nc-nd/4.0/).
ARTICLE INFO
Methodname:Cosmogenicnuclides,Paleoaltimetry,Burialage Keywords:Cosmogenicnuclides,10
Be,26
Al,21
Ne,MATLAB,Paleoelevation,Continuousexposure,Steadyerosion,Burialages
Articlehistory:Received19March2019;Accepted16May2019;Availableonline25June2019
*Correspondingauthorat:CentredeRecherchesPétrographiquesetGéochimiques(CRPG),UMR7358,CNRS-Universitéde Lorraine,15 rueNotreDamedesPauvres,54500Vandoeuvre-lès-Nancy,France.
E-mailaddress:pierre-henri.blard@univ-lorraine.fr(P.-H.Blard). https://doi.org/10.1016/j.mex.2019.05.017
2215-0161/© 2019 Published by ElsevierB.V. This is an open access articleunder the CC BY-NC-ND license(http:// creativecommons.org/licenses/by-nc-nd/4.0/).
MethodsX6(2019)1547–1556
ContentslistsavailableatScienceDirect
MethodsX
SpecificationsTable
SubjectArea: EarthandPlanetarySciences
Morespecificsubjectarea: geochemistry;geochronology;cosmogenicnuclides;26
Al;10
Be;21
Ne Methodname: cosmogenicnuclides;paleoaltimetry;burialage
Nameandreferenceof originalmethod
P.-H.Blard,M.Lupker,M.Rousseau-Paired-cosmogenicnuclidepaleoaltimetry–Earthand PlanetaryScienceLetters,2019.doi.org/https://doi.org/10.1016/j.epsl.2019.03.005. Resourceavailability 2Matlabscriptswiththispaper:“Paleoaltitude.m”and“Burial.m”Codesavailablehereas
supplementarymaterial.
Methoddetails
This article presents two Matlab© programs, “Paleoaltitude.m” and “Burial.m”, and their mathematicaldescriptions.Thesetwogeologicalapplicationsarebasedonthemeasurementofa cosmogenicnuclidespair(26Al-10Beor10Be-21Ne)inrocksthathavebeenexposedtocosmicraysin thegeologicalpast(upto>10millionyears ago)(Fig.1).Thepaleoaltimetrymethodis newand describedin[1].Theburialagemethodisalreadywidelyused(e.g.[2]);themainnoveltyofthescript “Burial.m”istotakeintoaccountthespatialpositionofthesample(latitudeandelevation)inthe calculationoftheburialage[1].Codesavailablehereassupplementarymaterial.
Program1-“Paleoaltitude.m”:Thisscriptcomputestheelevationofarocksamplesinwhicha pairofcosmogenicnuclideswithdifferenthalf-lives(26Al-10Beand10Be-21Ne)wasmeasured.Inthe caseofancientexposures,theburialagehastobeknownandbeaccountedforradioactivedecay.
Program2-“Burial.m”:Thiscodecomputesthedurationsincearockwasburiedfrom cosmic-rays.Altitudeandlatitudeatwhichthepaleo-exposureoccurredhavetobeknown.Botharenecessary inputoftheprogram.
By default, the code includes sea level high latitude production rates computed from the worldwidedatabaseavailableintheCREpcalculator(crep.crpg.cnrs-nancy.fr,ICE-Ddatabase;[3])and theproductionparameterssummarizedin[1].
Theseprogramsweredesignedandoptimizedwiththe2018aversionofMatlab©.Somefunctions couldbeunavailableiftheprogramsarerunwithanolderversionofMatlab©.Alldefaultparameters usedinthecodesarethosedefinedintheTable1ofBlardetal.[1].
Program1:“Paleoaltitude.m”–Computationofpaleoaltitudeofexposure
Thephysicalprinciplesofthisnewpaleoaltimetrymethodarepresentedinthemainarticle[1].
TutorialoftheMatlab©script:“Paleoaltitude.m”
Tousetheprogram,usersmustloadthefunctionfileintheirMatlab©workspaceandrunthe "Paleoaltitude.m"script.Awindowwithclickablebuttonsisthendisplayed.
Necessaryinputdata(intheformof.csvor.xlsxspreadsheets)are: Column1:Samplename
Column2:Latitude()
Column3:Presentaltitude(m) Column4:Burialage(Ma)
Columns5and6:Nuclide11s(at.g1)
Columns7and8:Nuclide21s(at.g1)
Typesofnuclides(10Be,26Alor21Ne)mustbedefinedusingtheinteractivebox.Itisimportantto checkthat thecorrectnuclidesareloadedbelowthecorrespondingheaders. Oncedataarecorrectly uploaded,usersmaypushthe"1-Calculate elevations"buttontostart thecalculations. Itis also
possibletopushthe"2-Plot" buttontodisplaythedatain a twocosmogenicnuclidesdiagram (26Al/10Bevs10Beor10Be/21Nevs21Ne).Oncethefigureisdisplayed,specificsamplesorsub-dataset maybeselectedandplotted.Fig.2showsanexampleofsuchaplotthatpermitstocomparedatawith theoreticalexposurecurvesatvariouselevations(bydefault,theprogramplotssurface exposure curvesfor0,2000and4000melevations).
Outputresults(in.csv): Column1:Samplename.
Columns2to4:H(m),H_min(m),H_max(m)-Mean,minimumandmaximumelevationcomputedassumingcontinuous exposure(noerosion).SeeBlardetal.[1]forcomplementaryinformation.
Columns5and6:Tint1s(Ma)-Integrationtimeoverwhichaltitudeiscomputedassumingcontinuousexposure(noerosion).
TintiscomputedfromEq.(7)inBlardetal.[1],usingthenuclidehavingtheshortesthalf-life(26Alor10Be)andthescalingfactor
ofthecomputedelevation.
Columns7to9:H_erosion(m),H_min_Erosion(m),H_max_Erosion(m)-Mean,minimumandmaximumelevationcomputed assumingsteadystateerosion.SeeBlardetal.[1]forcomplementaryinformation.
Columns10and11:Erosion1s(m.Ma1).Erosionisherecomputedconsideringthespallogenicproductiononlyandthe preburial10
Beconcentration,usingEq.(14)inLal[4].
Columns12and13:Tint1s(Ma)-Integrationtimeoverwhichaltitudeiscomputedassumingsteadystateerosion.Tintis
computedfromEq.(7)inBlardetal.[1],usingthenuclidehavingtheshortesthalf-life(26
Alor10
Be)andthespatialscaling factorofthecomputedelevation.
Resultsmaybeexportedintheformofa.csvspreadsheetbyclickingthebutton"Export".
Mathematicaldescriptionoftheprogramusedin“Paleoaltitude.m”tocomputepaleo-elevationsandtheir associateduncertainties
ForanuclideX,
l
Xistheradioactivedecayconstant(yr1),PX(at.g1.yr1)theSLHLproduction rate,NXandD
NX(at.g1)themeasuredconcentrationwithitsuncertainty.l
Y,PY,NYandD
NYarethe variablesspecifictothenuclideY.Inthecaseofpaleo-exposedmaterial,NXandNYarefirstcorrectedforradioactivedecaysincethe burialinitiation(tburial):
NX ¼NX present
elXtburial ð1aÞNY ¼NY present
elYtburial ð1bÞHere,itisassumedthatthereisnoinheritanceduetopre-exposureandthataltitudehasremained constantduringexposure.
FortwocosmogenicradioactivenuclidesXandYwithdifferenthalf-lives
l
Xandl
Y,suchasl
X<l
Y: NX¼ fPXl
Xþme
1eðlXþmeÞt ð2aÞ NY¼ fPYl
Yþme
1eðlYþmeÞt ð2bÞ In Eqs. (2a) and (2b), t(yr) is thepreburial exposure duration, f(dimensionless) the spatial productionratescalingfactor,m
(cm1)therockabsorptioncoefficient(m
=r
/L
,withr
thedensityin g.cm-3andL
theattenuationlengthing.cm-2)ande
(cm.yr1)theerosionrate.Continuousexposurecase(
e
=0m.Ma1)In the following, thevariables A, B,
D
A,D
Band r are defined as: A ¼ lYNYPY , B¼ lXNX PX ,
D
A¼ lYDNY PY ,D
B¼ lXDNX PX andr¼ lX lYwithr<1Fig.1.Synopticdescriptionofthetwomethodsforthe26
Al-10
Bepair. Case1:Burialageisknownandpaleoaltitudescanbecomputed.
Exactsolution. SolvingtheYnuclideEq.(2b)fortandsubstituteitinXEq.(2a)leadsto:
0¼ff 1Af r
B ð3aÞ
Fig.2. Exampleofapairednuclidesplotrealizedusingthe“Plot”functionofthe“Paleoaltitude.m”program.Shownisthe
10Be-21NedatasetfromtheAtacamadesert,Chile,SouthAmerica,reviewedin[1].Dataarefrom([7–11]).
Fig.3. Graphicaldescriptionofthemathematicalmethodusedtocomputeelevationsandtheirassociatedpositiveand negativeuncertainties.Exampleofatwo-radioactivenuclideinversionwiththe26Al-10Bepairwitha5%analyticalerror(1s)
(lightorangeellipse).Solidlines:continuousexposure.Dashedlines:steady-statedenudation.Redshadedboxes:upperand lowerforbiddenareas.
t¼1
l
Y ln 1A f ð3bÞ(3b)canalsobewrittenwiththeXnuclide.Bothequationsneedtosatisfytheconditionf>max(A,B). Eq.(3a)hasnoanalyticalsolutionforfandmustbenumericallysolved.Forthis,thefunctiongthatis decreasingontheinterval]A,1[canbedefinedasfollow:
gðxÞ¼xx 1Ax r
B ð4aÞ
gðfÞ¼0 ð4bÞ
Toensuretheexistenceofthesolutionf,thefollowingconditionsneedtobesatisfied: lim
A g¼AB>0 ð5aÞ
lim
1 g¼rAB<0 ð5bÞ
(5a)and(5b)conditionsaresatisfiedwhenthesampledoesnotplotinthelowerorupperforbidden areas(Fig.3).
Uncertaintypropagation. Since Eqs. (4a) and (4b) cannot be analytically solved,the confidence interval[f,f+]canbedeterminedbydefiningthefunction
D
gthatdescribestheuncertaintyattached tothegfunction.D
gisamonotonedecreasingfunction.Thus,f-andf+,thenegativeandpositive boundariesoff,canbecomputedbyfindingtherootsofgD
gandg+D
g:D
gðxÞ¼ ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi@
gðxÞ@
AD
A 2 þ@
g@
ðxÞ BD
B 2 s ¼ ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi rD
A 1A x r1 " #2 þD
B2 v u u t ð6aÞ ðgD
gÞðfÞ¼0 ð6bÞ ðgþD
gÞfþ ¼0 ð6cÞMaximumelevationandupperforbiddenzone
f+existswhenthefollowingconditionissatisfied.Thisconditionrequiresthattheuppervalueof thesolutionrangeremainsbelowtheupperforbiddenarea(Fig.3):
lim 1ðgþ
D
gÞ¼rABþ ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi r2D
A2þD
B2 q <0 ð7ÞMinimumelevationandlowerforbiddenzone
Theminimumelevationfcanbecomputedifthecondition(5b)issatisfied,whichleadstothe followingcondition: lim 1ðg
D
gÞ¼rAB ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi r2D
A2þD
B2 q <0 ð8aÞMoreoverlimAðg
D
gÞ¼1.Thus,(g-D
g)needtobenotmonotonictoensuretheexistenceoff:9
x02A;1; gðx0Þ>0 and 8x>x0:@
g
D
gð Þ
Whenasampleisclosetothelowerforbiddenarea,reachingthelimitsofconditions(8a)and(8b),itis still possibletodefinea limitvaluefor f, correspondingtoa samplethatstands justabovethe forbiddenarea.Thislimitvalueisdeterminedbytheequilibriumbetweenproductionandradioactive decay,anditisherecomputedas:
f¼maxðA;BÞ ð9Þ
Steady-stateerosioncase(t->1)
Normal case. For long exposure durations (t >> 1/(
l
+m
e
)), Eqs.(2a) and (2b) become time-independent.SolvingEq.(2b)form
e
andsubstituteitinEq.(2a)thenleadsto:f¼NXNYð
l
Xl
YÞPXNYPYNX ð10aÞ
me
¼fPYNY
l
Y ð10bÞBecausef>0and
m
e
>0,Eqs.(10a)and(10b)leadtothethreefollowingconditions,where(11a)and(11b)areequivalenttothe(5a)and(5b)conditions: NY NX> PY
l
X PXl
Y ð11aÞ PXNYPYNX<0 ð11bÞ f>maxðA;BÞ ð11cÞTheclassicaluncertaintypropagationformulacanherebeusedtocomputeanalyticalsolutionsfor f-andf+,[f-,f+]beingtheone-sigmaconfidenceinterval:
D
f¼l
Yl
X ðPXNYPYNXÞ2ð12aÞ
fþ¼fþ
D
f ð12bÞf¼f
D
f ð12cÞParticularcaseoflargeerosion. f+andfshouldbeconsideredcarefullywhenerosionislargebecause
D
ftendstoinfinityinthiscase.ThereforeD
fcanbelargerthanf,resultinginanegativef-.Sinceitis requiredthatf>maxðA;BÞ,f-canhoweverbedefinedinanycaseby:f¼maxðA;B;f
D
fÞ ð13ÞNoteonsampleslyingintheforbiddenzone. Whenasampleisintheupperforbiddenzone,theupper uncertaintyf+doesnotexist,f<0,andf-canbeestimatedasfollow:
f¼maxðA;BÞ ð14Þ
Whenasampleisinthelowerforbiddenzone,fdoesnotexistand
me
<0.f+couldthusbedefinedas theminimumelevationwhichensureapositiveerosion:fþ¼maxðA;BÞ ð15Þ
Program2:“Burial.m”–Calculationofburialages TutorialoftheMatlab©script:“Burial.m”
Tousetheprogram,usersmustloadthefunctionfileintheirMatlab©workspaceandrunthe "Burial.m"script.Awindowwithclickablebuttonsisthendisplayed.
Necessaryinputdata(intheformof.csvor.xlsxspreadsheet)are: Column1:Samplename
Column2:Latitude()
Column3:Altitude(m)
Columns4and5:Nuclide11s(at.g1) Columns6and7:Nuclide21s(at.g1).
Nuclides(10Be,26Alor21Ne)mustbedefinedusingtheinteractivebox.Itisimportanttocheckthat thecorrectnuclidesareloadedbelowthecorrespondingheaders.Oncedataarecorrectlyuploaded,users maypushthe"1-Calculateburialages"buttontostartcalculations.Itisalsopossibletopushthe"2 -Plot"buttontodisplaythedatainatwocosmogenicnuclidesdiagram(26Al/10Bevs10Beor10Be/21Nevs 21Ne).Notethattheplotfunctionbecomesfunctionalonlyafterthecalculationofburialages.Oncethe figureisdisplayed,itispossibletoselectspecificsamplesandplotasub-datasetonly.Fig.4showsan exampleofsuchaplot.
Aftercalculations,resultsmaybeexportedintheformofa.csvspreadsheetbyclickingthebutton "Export".
Outputresults(in.csv): Column1:Samplename
Columns2,3and4:T_Burial(Ma),-1s(Ma),+1s(Ma).BurialageiscomputedsolvingEq.(16)forthe26
Al-10
BepairandEq.(17) forthe10
Be-21
Nepair.Theonesigmaconfidenceinterval[-1s,+1s]iscomputedfromthestatisticaldistributionofthesolutions obtainedfromaMonteCarlosimulation(104
draws).
Columns5and6:Preburialerosion1s(m.Ma1).ErosioniscalculatedusingEq.(14)in[4],consideringonlythespallogenic
productionandthepreburial10Beconcentration.
Columns7and8:Preburialexposureduration1s(ka).Equivalentsurfaceexposuretimeiscomputedassumingnoerosion, usingEqs.(8a)and(8b)in[1].Calculationusesthe21
Neconcentrationinthecaseofthe(10
Be-21
Ne)pairand10
Beinthecaseof the(26
Al-10
Be)pair.
Mathematicaldescriptionofthealgorithmusedinthe“Burial.m”code
Inthisversion,the“Burial.m”programassumesthattwogeologicalconditionsaresatisfied:1) beforeburial,thematerialhadreachedsteady-stateerosionand2)theburialwasinstantaneousand deepenoughtoensuretheabsenceofpost-burialproduction.Inthiscase,theequationlinkingthe burialagetburialandthemeasuredcosmogenicnuclideconcentrationsN1andN2is:
P1 N1 el1tburialP2 N2 el2tburial¼
l
1l
2 f ð16ÞSinceEq.(16)hasnoanalyticalsolution,ithastobenumericallysolvedtodeterminetburial.In practice,the“Burial.m”programcallsthe“Burial26Al_10Ne.m”functionthatsolvesEq.(16)usinga MonteCarloapproach.Bydefault,104randomdrawsarerealized,assuming10Beand26Alfollowthe normal distributions (N10,
s
10) and (N26,s
26), where N10 and N26 (at.g1) are the measuredconcentrations,
s
10ands
26(at.g1)theironesigmaanalyticaluncertainties.Thisequationishere appliedinthecaseofthe26Al-10Bepair.Fortheparticularcaseofthe10Be-21Nepair,Eq.(16)simplifiesandcanbeanalyticallysolved: tburial¼1
l
ln N10 P10 P21 N21þl
10 f ð17Þ Thefunction“Burial10Be_21Ne.m”usesEq.(17)tocomputetburial.Tokeepcalculationssimple,pre-burialerosion(Columns4and5)isherecomputedconsidering thespallogenic production only. Notehoweverthat theneglection of muogenic productionmay underestimatethecorrecterosionratesbyupto30%(e.g.[5,6]).Ifpreburialerosionisfasterthan 100m.Ma1,neglectingthemuogenicproductionmayleadtounderestimatethecomputedburial agesby~100to200ka.
Acknowledgements
WearegratefultoGregBalco,DerekFabelandtwoanonymousreviewersfortheirconstructive commentsthatpermittedtoimprovetheMatlab©scriptsandtheearlierversionofthemanuscript. ThisisCRPGcontributionn2690.
AppendixA.Supplementarydata
Codescanbedownloadedhere:https://doi.org/10.1016/j.mex.2019.05.017.
References
[1]P.-H.Blard,M.Lupker,M.Rousseau,Paired-cosmogenicnuclidepaleoaltimetry,EarthPlanet.Sci.Lett.515(2019)271–282, doi:http://dx.doi.org/10.1016/j.epsl.2019.03.005.
Fig.4.Exampleofapairednuclidesplotrealizedusingthe“Plot”functionofthe“Burial.m”program.Shownisthe26
Al-10
Be datasetfromcavesilico-clasticsedimentsburiedinthecavesoftheAriègeregion,Pyrénées,France(Sartégou[12],PhDThesis).
[2]D.E.Granger,P.F.Muzikar,Datingsedimentburialwithinsitu-producedcosmogenicnuclides:Theory,techniques,and limitations,EarthPlanet.Sci.Lett.188(2001)269–281,doi:http://dx.doi.org/10.1016/S0012-821X(01)00309-0. [3]L.Martin,P.-H.Blard,G.Balco,J.Lave,R.Delunel,N.Lifton,V.Laurent,TheCREpprogramandtheICE-Dproductionrate
calibrationdatabase:afullyparameterizableandupdatedonlinetooltocomputecosmic-rayexposureages,Quat. Geochronol.38(2017)25–49,doi:http://dx.doi.org/10.1016/j.quageo.2016.11.006.
[4]D.Lal,Cosmicraylabelingoferosionsurfaces:insitunuclideproductionratesanderosionmodels,EarthPlanet.Sci.Lett. 104(1991)424–439,doi:http://dx.doi.org/10.1016/0012-821X(91)90220-C.
[5]M.Lupker,P.H.Blard,J.Lavé,C.France-Lanord,L.Leanni,N.Puchol,J.Charreau,D.Bourlès,10,EarthPlanet.Sci.Lett.333
(2012)146–156,doi:http://dx.doi.org/10.1016/j.epsl.2012.04.020. [6]G.Balco,Productionratecalculationsforcosmic-ray-muon-produced10
Beand26
Albenchmarkedagainstgeological calibrationdata,Quat.Geochronol.39(2017)150–173,doi:http://dx.doi.org/10.1016/j.quageo.2017.02.001.
[7]F.Kober,S.Ivy-Ochs,F.Schlunegger,H.Baur,P.W.Kubik,R.Wieler,Denudationratesandatopography-drivenrainfall thresholdinnorthernChile:multiplecosmogenicnuclidedataandsedimentyieldbudgets,Geomorphology83(2007)97– 120,doi:http://dx.doi.org/10.1016/j.geomorph.2006.06.029.
[8]K.Nishiizumi,M.W.Caffee,R.C.Finkel,G.Brimhall,T.Mote,RemnantsofafossilalluvialfanlandscapeofMioceneagein theAtacamadesertofnorthernChileusingcosmogenicnuclideexposureagedating,EarthPlanet.Sci.Lett.237(2005) 499–507,doi:http://dx.doi.org/10.1016/j.epsl.2005.05.032.
[9]C.J.Placzek,A.Matmon,D.E.Granger,J.Quade,S.Niedermann,Evidenceforactivelandscapeevolutioninthehyperarid Atacamafrommultipleterrestrialcosmogenicnuclides,EarthPlanet.Sci.Lett.295(2010)12–20,doi:http://dx.doi.org/ 10.1016/j.epsl.2010.03.006.
[10]B.Ritter,S.A.Binnie,F.M.Stuart,V.Wennrich,T.J.Dunai,EvidenceformultiplePlio-Pleistocenelakeepisodesinthe hyperaridAtacamadesert,Quat.Geochronol.44(2018)1–12,doi:http://dx.doi.org/10.1016/j.quageo.2017.11.002. [11]B.Ritter,F.M.Stuart,S.A.Binnie,A.Gerdes,V.Wennrich,T.J.Dunai,Neogenefluviallandscapeevolutioninthehyperarid
coreoftheAtacamadesert,Sci.Rep.8(2018)13952,doi:http://dx.doi.org/10.1038/s41598-018-32339-9.
[12]A.Sartégou,-ÉvolutionMorphogéniqueDesPyrénéesOrientales:ApportsDesDatationsDeSystèmesKarstiquesÉtagés ParLesNucléidesCosmogéniquesEtLaRPE.PhDThesis,UniversitédePerpignan,2017NNT:2017PERP0044.