Hydrology Measurements

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Transcription:

Hydrology Measurements Stefan Uhlenbrook Introduction to Isotope Hydrology

Introduction to Isotope Hydrology Stefan Uhlenbrook, Ph, MSc, habil. Professor of Hydrology UNESCO-IHE Institute for Water Education and elft University of Technology The Netherlands E-mail: s.uhlenbrook@unesco-ihe.org s.uhlenbrook@tudelft.nl

Introduction of the Lecturer Hydrologist originally from Freiburg, Germany MSc, Ph and habilitation in Freiburg In elft, the Netherlands, since January 2005: Professor of Hydrology at UNESCO-IHE, elft Since November 2009: part-time professor for experimental hydrology at TU elft Working experiences mainly in catchments in Germany, Austria, USA, East Africa, sub-saharan Africa, Vietnam, Iran and Palestine, and recently some other more humid places i.e. Thailand and Malaysia) experimentalist and modeler

Sources of course notes and further information Books: Kendall and Mconnell Eds.) 1998: Isotope Tracers in Catchment Hydrology, Elsevier Kaess Ed.), 1998: Tracing Techniques in Geohydrology, - Rotterdam Balkema Mook, W. G. 2001): Environmental Isotopes in the Hydrological Cycle- Principles and Applications. UNESCO-IAEA, IHP Publications. free at the web!) Aggarwal P.K., Gat J.R., Foehlich K.F.O., 2005: Isotopes in the water cycle. Springer, 381 p. Clark, I.. and Fritz, P.:Environmental isotopes in hydrogeology. Lewis Publishers, 1997 Jeff Mconnell s web page: www.cof.orst.edu/cof/fe/watershd/shortcourses.php Carol Kendall s web page: http://wwwrcamnl.wr.usgs.gov/isoig/res/ Isotope Hydrology Section: http://www-naweb.iaea.org/napc/ih/index.html Global Network for Isotopes in Precipitation: http://www-naweb.iaea.org/napc/ih/gnip/ihs_gnip.html Isotope and Geochemistry web page: http://www.eeb.cornell.edu/isogeochem/. I am sure there is more available!

Acknowledgements for some of the material used in this course Prof. Chris Leibundgut, Univ. of Freiburg, Germany i.e. general, artificial tracers) Prof. Jeff Mconnell, Oregon State Univ., Corvallis, USA i.e. isotope tracers) r. Jens Lange i.e. general, artificial tracers, case studies) r. oug Burns, USGS, USA i.e. isotope tracers) r. Pardeep Agarwall, IAEA, Vienna, Austria i.e. isotope tracers) r. Axel Suckow, IAEA, Vienna, Austria i.e. radioactive tracers) r. Paul Königer i.e. artificial tracers). many others are not mentioned! sorry, but my references are sometimes incomplete!!

Remember the basic hydrological questions that tracers can help address Where does runoff originate in a catchment? How long has water resided in different hydrological storages? How fast does water move in different hydrological storages? How does groundwater and surface water interact? What biogeochemical processes affect water chemistry? Questions relevant for isotope hydrology What are the rates of these biogeochemical processes?

Isotope tracers Can provide information about climatic conditions also paleoclimatology) Some isotopes 18 O, 2 H, 3 H) behave conservatively during transport as they are part of the water molecule, thus they reflect mixing and transport processes Identification of source and movement of water Identification of dynamics of hydrologic processes Isotope contents of ice in Antarctica help to understand previous climates

this course! efinitions Atoms of the same element that have a different number of neutrons, and therefore a different mass Examples: oxygen 16 O, 17 O, 18 O hydrogen H, 2 H = deuterium, ), 3 H = tritium, T) Superscript is the mass number and reflects the sum of protons and neutrons sometimes written as O-18 or 18-O) Stable isotopes do not decay, for example 2 H or 18 O Radioactive unstable) isotopes decay to more stable forms at a known rate, for example 3 H decays to 3 He General distinction: Isotope Hydrology: 18 O, 2 H, 3 H, components of the water molecule i.e. age dating, mixing, runoff sources and flow paths, groundwater/surface water interactions, climate indicator, ) Isotope Biogeochemistry: 15 N, 13 C, 34 S, etc. i.e. biogeochemical processes)

16 8 O Isotope basics Mass number = protons + neutrons) 8 protons positive), 8 electrons negative), 8 neutrons neutral) Atomic number = protons) - Protons and neutrons in the nucleus have approximately the same weight - Electrons negative charge) are lighter and are located in electron shells 18 O 8 protons, 8 electrons, 10 neutrons 8 - Nuclides with same atomic number i.e. an element) but different mass number are called isotopes - 92 natural elements have more than 1000 stable and radioactive isotopes

Some common environmental isotopes Source: Kendall, 1998

Natural abundance ratios are very small Element Isotope Abundance %) Ratio Hydrogen 1 H 99.985 2 H ) 0.015 150.022 e-6 Carbon 12 C 98.892 13 C 1.108 112.04 e-4 Oxygen 16 O 99.759 17 O 0.037 370.894 e-6 18 O 0.204 2044.928 e-6

Isotope units Stable isotope compositions water sample) of low mass elements such as O, H, C, N, and S are expressed in delta units δ) expressed as the deviation from a standard std) in parts per thousand o / oo or per mil) Example: δ 18 O o / oo ) = [ 18 O/ 16 O)sample / 18 O/ 16 O)std] 1) 1000 positive value means sample ratio is greater than std. negative value means sample ratio is less than std.

δ 18 O values in nature Ice from glaciers of Arctic, Antarctica and Greenland Ocean Meerwasser water Niederschlag Precipitation water Bodenwasser Soil water Grundwasser Groundwater Rhein River Rhine water Geothermal geothermale water Wasser Magmatic magmatische water Wasser Metamorphic metamorphe water Wasser -50-40 -30-20 -10 0 10 20 30 Light δ 18 O[ V-SMOW] Heavy Source: CLARK & FRITZ 1997); extended with data from Leibundgut 2002)

Additional units 3 H expressed as Tritium Units TU), one TU = 1 tritium atom per 10 18 H atoms 1 TU = 0.119 Bq = 7.1 decays per minute in 1 liter water [dpm/l] 3 H may also be expressed as pci/l where 1 TU = 3.2 pci/l 14 C expressed as percent of modern carbon pmc) Many heavy isotopes are expressed as an absolute ratio, for example 87 Sr/ 86 Sr

Isotope fractionation Phenomenon whereby the isotopic composition of an element in a given compound or ion changes during the transition of the element from one compound or physical state to another Proportions of isotopes will change during chemical or biological reactions and phase changes Mass dependent: depend on the mass difference between isotopes Non-mass dependent: depend on the structure of the nucleus Fractionation is temperature dependent; stronger fractionation for phase change during low temperatures Isotopic composition can shift even if there are no large changes in phase liquid/gas); for example, soil water in contact with soil gas of a different isotopic composition

Evaporation and condensation change of phase) The condensate becomes enriched in the heavy isotope 18 O, 2 H) relative to the vapor uring evaporation/melting the remaining water water/ice) becomes heavier enriched in heavy isotopes) Rain becomes progressively lighter as storms move inland from the ocean Evaporation is strongly affected by humidity the higher the humidity, the smaller the change in δ 18 O and δ during evaporation Net effect of evaporation and condensation produces a meteoric water line

Evaporation and condensation effects

Controls of the spatial variation of δ 18 O and δ in precipitation Apparent Temperature Effect precipitation becomes heavier as temperature increases, δ 18 O +0.5 / o C Amount Effect rainout creates progressively lighter precipitation during an event Evaporation Effect precipitation may evaporate as it falls, especially through dry air, becomes heavier Altitude Effect precipitation becomes lighter with increasing elevation on windward side of mountains 18 O: -0.15 to 0.5%0/100 meters : -1.5 to -4%0/100 meters Continental Effect precipitation becomes progressively lighter inland from moisture source

Temperature effect Source: IAEA

Altitude effect Source: IAEA

Seasonal effects southern Germany) Source: IAEA Source: IAEA

Continental effect http://www.sahra.arizona.edu/programs/isotopes/oxygen.html

Amount effect better: intra-storm variability!) Source: IAEA

Heavy Latitudinal effect Light 90 0 latitude 0 0 Source: IAEA

Spatial variations in the USA Why are patterns of δ 18 O and δ so similar? Source: Kendall and Coplen, 2001

GNIP IAEA) Gew-jährl. O18-Werte für Europa [ V-SMOW] Source: IAEA

Taking water samples for isotope analysis 18 O, and 3 H) No evaporation from the sample bottle No evaporation from precipitation sampler dry bottles, no mixing with old water pumping of fresh groundwater from wells samples volumes depend on the device, usually 100 ml are enough for 18 O and up to one liter for 3 H danger of fractionation!

Global Network of Isotopes in Precipitation GNIP) Source: IAEA - IAEA National Networks H-3 only new closed Precipitation sampler

Information available at the GNIP database 183 active stations in 53 countries The Isotope Hydrology Laboratory of IAEA is currently performing isotope analyses of about 30 % of the collected precipitation samples; 33 other labs are involved Available are isotope data H-2, O-18, H-3), basic meteorological variables type and amount of precipitation, surface air temperature and vapour pressure) 88,000 records from 700 stations located in 101 countries First data of tritium was collected in 1953 First data of stable isotopes were collected in 1960

Global isotopic composition of precipitation Source: IAEA

Generalization Isotopic composition of precipitation Consistent average compositions over time and space Annual cycle of compositional changes heavy in summer and light in winter; becomes muted towards equator Large variation among storms Often considerable variability within storms Snow often plots along lines of higher d-excess than rain Storms derived from different storms tracks may have consistently different meteoric water lines

Global Meteoric Water Line GMWL) When precipitation samples from all around the world are plotted in δ vs. δ 18 O space, they form an approximate line really a band or narrow oval of data). Harmon Craig 1961): δ²h = 8 * δ 18 O + 10 Slope of 8 close to the ratio of equilibrium fractionation factors of H and O isotopes at 25 30 o C, and that produced by Rayleigh condensation of rain at 100% humidity Y-intercept is 10 due to kinetic enrichment of in evaporating ocean water called deuterium excess d

elta Global Meteoric Water Line 40 0-40 -80-120 -160 δ = 8 δ 18 O + 10 Craig formula from 1961) -30-20 -10 0 elta O-18 euterium excess, d New, more precise formula from IAEA 2004 based on GNIP data): δ 2 H = 8.17 ±0.07) δ 18 O + 11.27±0.65) VSMOW

euterium Excess, d Value changes with climate cooler, more humid areas have smaller d values Examples: Global mean = +10 North America = +6 Mediterranean = +22 New Zealand = -0.3 euterium excess can sometimes be used to identify water that was recharged during a different climatic regime

GNIP IAEA) euterium Exzess Source: IAEA

Mean values of precipitation water and its position at the meteoric water line Meteoric water line warm regions cold regions Source: IAEA

Meteoric water line contains much information Northern Wisconsin, USA Source: Kendall, 2001

Evaporation lines Source: IAEA

/ 18 O-relation at the lake of Neusiedel, Switzerland Precipitation Lake water Source: IAEA

Interpretation of MWL: Groundwater isotopic composition Plug flow system, low dispersion Avg. Precip. Summer recharge δ Winter recharge Well mixed system, high dispersion ifferent origin, glacial melt water? δ 18 O

Use LMWL in large rivers Agarwaal et al., 2002

Overview of some LMWLs From: E. Mazor 1997) Chemical and isotopic groundwater hydrology. M. ekker, New York, 413pp; and Clark & Fritz, 1997, 6. Region Meteoric line ) Global meteoric line) δ 2 H = 8δ 18 O + 10 Northern hemisphere continental) δ 2 H = 8.1 ± 1)δ 18 O + 11 ± 1) Mediterranean or Middle East) δ 2 H = 8δ 18 O + 22 Maritime Alps April 1976) δ 2 H = 8.0 ± 0.1)δ 18 O + 12.1 ± 1.3) Maritime Alps October 1976) δ 2 H = 7.9 ± 0.2)δ 18 O + 13.4 ± 2.6) Northeastern Brazil δ 2 H = 6.4δ 18 O + 5.5 Northern Chile δ 2 H = 7.9δ 18 O + 9.5 Tropical Islands δ 2 H = 4.6 ± 0.4)δ 18 O + 0.1 ± 1.6)

Meteoric Water Line MWL): Generalizations Source: IAEA

eveloping your own LMWL Good rules of thumb 1. Each site has its own LMWL 2. Need to collect all precipitation for at least 2-3 years at a site to get a good average value for recharge 3. o not interpolate LMWL or averages from the data for the closest IAEA or other station but compare with IAEA data) 4. There is lots of spatial and temporal variation in the isotopic composition of precipitation 5. The GMWL or LMWL is not a tight line they are many lines that fit through an ellipse of data points uncertainty)

eveloping your own LMWL Good rules of thumb 6. Evaporation causes samples to plot below the MWL 7. Recharge water can be very different from average rainfall 8. Samples easily fractionate in poor quality bottles; use ones with good caps. Wrap in tape or dip in paraffin for long-term storage 9. Samples archive well; collect more samples than you need, and analyze them in groups

Why do waters differ from isotopic composition of precipitation? Evaporation of surface waters, interception Seasonal recharge unequal distribution over the year) Time lag, waters might reflect past precipitation Precipitation sampling site may not be representative of basin elevation, temp., etc.) Mixing of different water components different groundwater, soil water etc.) amping of the seasonal fluctuations due to dispersion in the system

ata from European rivers The anube is a mixture of many other rivers Agarwaal et al., 2002

Take home messages Stable and unstable radioactive) isotopes 2 H, 18 O and 3 H, respectively) of water molecule are natural inputs into the hydrological cycle and behave conservatively Isotope fractionation due to phase changes or biogeochemical processes All precipitation data can be summarized to MWL 2 H vs. 18 O http://bit.ly/pjippa diagram), but LMWL can vary from this Samples at the MWL can be interpreted as summer-winter precipitation, evaporation effects etc. There are temperature-, altitude-, amount-, seasonal-, latitudinal-, and continental effects Need of a specialized laboratory but number is increasing; incl. TU elft, UNESCO-IHE) Much data is available at the IAEA GNIP, GNIR etc)