Award Abstract # 0345595
Collaborative Research: A Proposal for the Cosmic-Ray Produced Nuclide Systematics on Earth (CRONUS-Earth) Project

NSF Org: EAR
Division Of Earth Sciences
Recipient: WOODS HOLE OCEANOGRAPHIC INSTITUTION
Initial Amendment Date: March 8, 2005
Latest Amendment Date: March 3, 2009
Award Number: 0345595
Award Instrument: Continuing Grant
Program Manager: Enriqueta Barrera
EAR
 Division Of Earth Sciences
GEO
 Directorate for Geosciences
Start Date: March 1, 2005
End Date: February 28, 2011 (Estimated)
Total Intended Award Amount: $0.00
Total Awarded Amount to Date: $308,673.00
Funds Obligated to Date: FY 2005 = $88,382.00
FY 2006 = $70,379.00

FY 2007 = $22,379.00

FY 2008 = $57,919.00

FY 2009 = $69,614.00
History of Investigator:
  • Mark Kurz (Principal Investigator)
    mkurz@whoi.edu
Recipient Sponsored Research Office: Woods Hole Oceanographic Institution
266 WOODS HOLE RD
WOODS HOLE
MA  US  02543-1535
(508)289-3542
Sponsor Congressional District: 09
Primary Place of Performance: Woods Hole Oceanographic Institution
266 WOODS HOLE RD
WOODS HOLE
MA  US  02543-1535
Primary Place of Performance
Congressional District:
09
Unique Entity Identifier (UEI): GFKFBWG2TV98
Parent UEI:
NSF Program(s): Petrology and Geochemistry,
Instrumentation & Facilities,
Geobiology & Low-Temp Geochem,
Geomorphology & Land-use Dynam
Primary Program Source: app-0107 
app-0106 

01000910DB NSF RESEARCH & RELATED ACTIVIT

01000809DB NSF RESEARCH & RELATED ACTIVIT

app-0105 
Program Reference Code(s): 0000, OTHR
Program Element Code(s): 157300, 158000, 729500, 745800
Award Agency Code: 4900
Fund Agency Code: 4900
Assistance Listing Number(s): 47.050

ABSTRACT

Terrestrial- in situ- cosmogenic nuclide (TCN) methods for surface exposure dating and other
earth-science applications were first demonstrated in 1986. During the subsequent 17 years these methods have developed into versatile and indispensable tools in many fields of modern Earth Sciences, including paleoclimatology, geomorphology, tectonics, hydrology, and volcanology. The TCN that have been demonstrated to be widely applicable are 3H, 10Be, 14C, 21Ne, 26Al, and 36Cl. This rapid development has been facilitated by methodological progress, including improvements in sampling strategies, sample preparation procedures and analyses of cosmogenic nuclides (by accelerator mass spectrometry (AMS) and noble gas mass spectrometry). In order to remain at the cutting edge of the earth sciences the accuracy of TCN methods must be significantly improved. However, it is the consensus of practitioners in the field that further developments are instead moving toward an impasse. This limitation is imposed, not by methodological considerations, but rather by incomplete understanding of the fundamental physical processes, and by lack of rigorous intercomparability between different investigators and methods. The global distribution of cosmogenic nuclide production depends on a number of interrelated factors, and these
factors must be simultaneously controlled in order to arrive at the equations and parameters that accurately define production rates at all points, and over geological time. This task is far beyond the capability of any individual investigator.

In order to achieve this next, necessary, step the CRONUS-Earth Project is proposed. The project
has the following goals: (i) to establish a rigorous basis for intercomparison between measurement of different nuclides and by different investigators, (ii) to provide a firm linkage between cosmic-ray physics and the systematics of the TCN produced by the cosmic rays, and (iii) to produce generally-accepted formulations and parameters for calculation of TCN production. The ultimate goal is to advance the precision and accuracy of all TCN methods from its current range of ~10% to 20% toward a 5% level. This project is envisioned as an international, collaborative effort. CRONUS-Earth consists of six major components: (i) A methodological intercomparison, including sample preparation as well as analytical measurement. (ii) Spatial/temporal distribution of cosmic-ray fluxes, through "mining" existing neutron monitor datasets, modeling of neutron monitor responses, and measurement of saturated in situ 14C altitude/latitude profiles. (iii) Emplacement of artificial targets for 3He, 21Ne, 10Be, 32P and 36Cl production, to link contemporary cosmic-ray fluxes to production rates and scaling factors. (iv) Measurement of production cross-sections using laboratory neutron beams. (v) A numerical modeling effort to integrate the
observations and to calculate the effects of past geomagnetic and paleoclimatic changes on cosmogenic nuclide production. (vi) Geological calibration of nuclide production rates, based on independently-dated surfaces worldwide. These will be classified by quality into primary calibration sites and secondary, or "verification", sites that will be used to test the overall production-rate model. These six components comprise a synergistic and coordinated approach to a problem that is clearly beyond the scope of individuals and small research teams. We propose a consortium approach to managing the project, involving multiple investigators, annual meetings to monitor progress, compile data, and exchange with the community, rapid electronic distribution of results, and integration of the final products through a project office charged with disseminating the results to the community. A linked CRONUS-Europe proposal has been submitted to the EU and will be closely coordinated with CRONUS-Earth.

The CRONUS-Earth Project will address the NSF intellectual merit review criterion through
establishing an improved, quantitative, physically-based, understanding of TCN production and
accumulation that can be applied to solve a wide variety of problems in the earth sciences. The Project will address the broader impacts criterion by providing formulations, parameters, and computer codes that will constitute an intellectual infrastructure enabling more consistent, accurate, and widespread application of TCN methods in the earth sciences. Furthermore, the Project will provide a basis for a more formal and organized future approach to promoting consistency in application of TCN methods, such as committees to provide recommended values for parameters. Finally, it will include a component to directly involve undergraduates, and especially minority students, in research in aspects of earth science related to CRONUS.

PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH

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J.M. Licciardi, M.D. Kurz, J.M. Curtice "Cosmogenic 3He production rates from Holocene lava flows in Iceland" Earth and Planetary Science Letters , v.246 , 2006 , p.241
Ackert, RP; Becker, RA; Singer, BS; Kurz, MD; Caffee, MW; Mickelson, DM "Patagonian glacier response during the late glacial-holocene transition" SCIENCE , v.321 , 2008 , p.392 View record at Web of Science 10.1126/science.115721
Anslow, FS; Clark, PU; Kurz, MD; Hostetler, SW "Geochronology and paleoclimatic implications of the last deglaciation of the Mauna Kea Ice Cap, Hawaii" EARTH AND PLANETARY SCIENCE LETTERS , v.297 , 2010 , p.234 View record at Web of Science 10.1016/j.epsl.2010.06.02
Bockheim, JG; Kurz, MD; Soule, SA; Burke, A "Genesis of Active Sand-filled Polygons in Lower and Central Beacon Valley, Antarctica" PERMAFROST AND PERIGLACIAL PROCESSES , v.20 , 2009 , p.295 View record at Web of Science 10.1002/ppp.66
C.L. Denoncourt, J.M. Licciardi, J.O.Stone, R.C. Finkel, M.D. Kurz "Calibration of Cosmogenic 36Cl production rates from Holocene lava flows in Iceland" EOS Trans AGU , v.86 , 2005 , p.F23
DeLaeter, J. and M.D. Kurz "Alfred Nier and the sector field mass spectrometer" Journal of Mass Spectrometry , v.41 , 2006 , p.847
Goehring, BM; Kurz, MD; Balco, G; Schaefer, JM; Licciardi, J; Lifton, N "A reevaluation of in situ cosmogenic He-3 production rates" QUATERNARY GEOCHRONOLOGY , v.5 , 2010 , p.410 View record at Web of Science 10.1016/j.quageo.2010.03.00
M.D. Kurz, S. Rowland, J. Curtice, A. Saal, T. Naumann "Eruption rates at Fernandina volcano, Galapagos archipelago, from cosmogenic helium in surficial lava flows." EOS Trans AGU , v.86 , 2005 , p.F31

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