CRONUS-Eart-Earth Annual Meeting 2007 Berkeley, California, 8-9 December CRONUS-Earth Meeting Minutes Saturday, December 8, 2007 Attendees Fred Phllips Tim Jull Greg Balco Bob Reedy Janet Sisterson Alice Doughty Meredith Kelly Aaron Putnam Mike Kaplan Marian Scott Lisa Majkowski Katrin Mai Kees Welton Marek Zreda Darin Desilets Kuni Nishiizumi Nat Lifton Brian Borchers Bailey Dugan Brent Goering David Argento Shasta Marrero Enriqueta Barrera Jonathan (Kuni’s student) Missing John Gosse (delayed in transit) Tibor Dunai (missed flight) Marc Caffee (Antarctica) Joerg Shaefer (baby expected) Mark Kurz (Antarctica) Bob Finkel (France) John Stone (Antarctica) Meeting began at 12:45. Housekeeping (Nishiizumi) • Conference center housekeeping (history of conference center, restrooms, drinks, tour of Kuni’s clean lab later in the day). Welcome (Phillips) • Change in format of meeting. • Time to think in terms of how individual efforts will contribute to global project goals. • Standardized reporting. NSF Perspective (Barrera) • Group invited to ask questions. • Pleased with the success of program (leadership, participation, organization, results). • Looking forward to February information meeting. • International connection brings a lot of attention to NSF. • Other earth science community news – new/future projects will find role for cosmogenic nuclides (Critical Zone Observatories, climate change studies). • NSF trend to develop observatories. • CRONUS-Earth work will feed into work in plans for the next ten years. • Future support: o no new funding in 2008 (flat or down). o Earth Scope is the priority. o Submit annual report soon – need to get funds before money gets reallocated to Earth Scope (before end of January). • Number of positions available at the NSF: o Earth Science Division Director -would like to have someone in surface earth processes. Apply for position or share the announcment. Closes at end of January. o Positions available with Enriqueta – biology, geomorphology. • Geosciences and geoinformatics – CRONUS-Earth needs to develop a compellation of databases with standardized terminology. • Questions: o What are three observatories? NSF had funds for allocated for 2 two observatories and supported the third from the core program –UC Merced (located in the Sierra Nevada), U Colorado Boulder, Penn State (Susquehanna). Observatories open for collaboration. Researchers can apply for additional funding to work at these laboratories. o If observatories and CRONUS-Earth are taking large amounts of money from the core program, will this change the nature of how NSF funds smaller research projects? CRONUS-Earth and observatories have a finite life (five years). Last year, program budget increased by 20%. Makes up for prior under-funding. However, Earth Scope and NEON are long term, with infrastructure funding coming from Congress. Eventually, the NSF will have to support these long term projects, maybe from core program. Waters Programs is important because it includes surficial processes. because it includes surficial processes. Action item: Submit annual reports before end of January. Issue 1: Improvement of accuracy of cross-sections Geological calibration Moderator: Phillips Overview (Phillips) • Production rate – measure it empirically or measure energy dependant cross- sections and integrate. • We have funds for processing of samples. • Sampling on schedule except for Hawaii (need additional radiocarbon samples, permitting issues). • Slower than expected on analyses due to change in procedure. All rock now ground at central site and homogenized, then aliquots sent to individual investigators – slow process. • John Stone is working on the borehole in Antarctica. • Mid to high latitudes are utility for basic production rate calculations Low latitudes (high altitude) used for scaling. • Questions: o Purpose of Peru elevation transect? Provides low altitude sample. o Getting samples from Joe Licciardi and John Gosse’s Wind River sites to do duplicates? Fred will contact Joe and John. o Are there radiocarbon samples from Hawaii flows? Yes. o What were the initial criteria for calibration sites? Geology had to be well known, age control on site, and evidence of boulder erosion rates. Action item: Contact Licciardi and Stone for samples. Action item: Need to develop criteria for sites -minimum number of samples must agree before site is identified as calibration data set and the role of investigator site knowledge/judgment. Action item: Need to get field/lab evidence for “wacko” sites -should try to say why site is not correlating. Sample submission forms (Majkowski) • An online form for requesting reimbursement for sample preparation (and analysis, in the case of noble gas samples) will soon be up and running on the NMT website. Please review the prototype online sample form and give feedback. feedback. • Suggested amendments: o Drop-down list of sample sites o Blank option to enter different sample site o Option to select multiple nuclides simultaneously for single sample o Require password to access sample form o Update lab costs o Add noble gas, U Arizona to lab selection o Generate figures for labs to invoice o Add data from other tests (XRF, etc.) Action item: Make changes to form. Action item: Check laboratory costs. Action item: Go live by January 15, 2008. Action item: Enter all previously analyzed samples. Promontory Point • Some samples have good agreement with a couple of outliers have seen this several times). Outliers may not be biased but quantitatively different. • Slightly over-estimating age. • Suggestion – start making duplicates within own lab. Could be a homogenization problem or different rock type. • Questions: o Are there radiocarbon dates? Bonneville well constrained, Tab Hill not as well controlled. Tabernacle Hill • 3He has good agreement. • Slightly over-estimating age Scotland • Pleased with convergence of Scotland, Antarctica and Bonneville production rate. • Questions: o Getting PPT and Scotland samples? Contact Marc Caffee. o The assumption is 11.6 at Younger Dryas – is this a correct correlation? Any independent age control? Some are radiocarbon dated. Closely regional. Beetle temperatures. o Any effort to reproduce Scotland chronology? Would need to re-core bogs. Don’t have money in budget. o Brent has some Norway sites (well-constrained) within Younger Dryas (varves and ash) – could these be compared to Scotland? o Are supplemental funds available for additional Scotland work? Potentially but think it through this very carefully. Calibration dollars are on track. Action item: Fred to send out Marc’s report on Scotland. Fred to send out Marc’s report on Scotland. New England (Balco) • Location – Littleton, NH. • Boulder sheets lie within varve stratigraphy. Age well constrained. • See website http://depts.washington.edu/cosmolab/littleton/Littleton_report.html • Collected seven good samples Antarctic Core (Phillips for Stone) • Questions: o Status of drilling? Moving ahead. John has funding from Polar Program. He is making connections with New Zealand drillers. Moderator: Sisterson Laboratory X-sections (Sisterson/Caffee/Nishiizumi) • Kuni to receive Janet’s samples within the next year. Kuni will need to look at activities and determine when he can do them. • Tim has some low level samples. Measurements (Nishiizumi) • Questions: o Will Kuni be going again next year? Yes, he will do 200, maybe 300. Physics-based modeling (Reedy) • Methods for computing neutron fluxes are well-benchmarked but it is having good values for the production cross-sections that are the key to the ultimate production rates. • Clem found uncertainty in nitrogen x-section. • Quantity stuff gives a dataset that can be used – can this be used to tell which cross-sections that are problematic? By time the problems are identified, it is too late. Really need neutron cross-sections. Not possible to model neutron cross- sections from proton cross-sections. At high enough energy, over 100 MeV, they kind of look the same (looking at the effect) – but for many reactions, this is not true. Can get an estimate but it may not be physical. • Bob needs input for parameterizing the cosmic ray flux at the top of the atmosphere. • Questions: o What does Brian need to in order to end up with better estimates for terrestrial rates? Bob can provide production at poles (with no-geomagnetic cutoff) within a +/10% uncertainty and +/-10% uncertainty on neutron cross-sections. Brian would like other locations at different latitudes and longitudes for scaling. o What about inputting geomag variability to see what happens at top of atmosphere? Nat says there are estimates from neutron studies. Action item: Bob needs input for parameterizing the cosmic ray flux at the top of the atmosphere. Action item: Bob can provide Brian with production at poles (with no-geomagnetic cutoff) within a +/-10% uncertainty and +/-10% uncertainty on neutron cross-sections. Parameter optimization modeling (Borchers) • Issues with result duplication – 36Cl, some PPT 10Be issues. • Should compile information so that we can see where this issue is happening. • CRONUS-Earth could hold workshop for users to bring in all data and talk about the problems. • Users haven’t gotten to the point of multiple samples (culture and cash). • Need to develop formal protocol for duplicates. • Site samples with variability indicate that there is something different in the geology. But what about different results from the same boulder? Must start at the beginning to understand where variability initiates. Need to do all steps on every sample. • Brian can’t do calculations until uncertainty is decided. He wants to have production rate calculated from neutron flux cross-sections with uncertainties next to geologic production rates to compare. He cannot come up with one big combination without unbiased estimates and uncertainties. • Bob cannot provide this information because it is very difficult to calculate the neutron flux cross-sections uncertainties. They are at least 10%. He cannot provide rigorous numbers. • Questions: o Could K and Ca be measured in solution after sample is dissolved? Yes. o What about inputting geomag variability to see what happens at top of atmosphere? Nat says there are estimates from neutron studies. Business Meeting (Phillips) Meeting began at 17:30. Fred Phillips chaired the meeting. Item 1: Election of three members for Steering Committee (can be new or existing members could continue by vote of acclamation). Current Steering Committee: Phillips, Jull, Kurtz, Schaefer, Borchers, Stone, Lifton. Greg Balco motioned to retain current committee. Bob Reddy seconded. All said aye. Item 2: Where to hold the next annual meeting. 5th Annual Meeting will be held prior to AGU (December 13-14). Need to organize community outreach meeting to present appropriate results and protocols for public comment. Kuni requested to reserve SSL conference room for next year. Save GSA for final year. Item 3: Goldschmidt Conference Is it possible to organize a meeting for 2008 Goldschmidt (Vancouver, July 13-18)? Need to try to organize something with CRONUS-EU (project ending soon). Item 4: Additional topics that need more work? Trying to understand the sources of variability in sample-to-sample analyses. Once intercalibration results are in, CRONUS-Earth can hold a workshop on those plus calibrations results and a program to sample and analyze samples to reduce uncertainty. Workshop should be limited to those researchers who have had issues (must be careful about attendees). Unsure about timing. Needs to be in 2008 (last samples by March 2008). Meeting adjourned at 18:15. Saturday, December 8, 2007 Attendees Fred Phllips Tim Jull Greg Balco Bob Reedy Janet Sisterson Alice Doughty Meredith Kelly Aaron Putnam Mike Kaplan Marian Scott Lisa Majkowski Katrin Mai Kees Welton Marek Zreda Darin Desilets Kuni Nishiizumi Nat Lifton Brian Borchers Bailey Dugan Brent Goering David Argento Shasta Marrero Enriqueta Barrera John Gosse Tom Lowell Peter Vermeesch Shasta Marrero Enriqueta Barrera John Gosse Tom Lowell Peter Vermeesch Missing Tibor Dunai (missed flight) Marc Caffee (Antarctica) Joerg Shaefer (baby expected) Mark Kurz (Antarctica) Bob Finkel (France) John Stone (Antarctica) Meeting began at 08:55. Issue 2: Improvement of accuracy of scaling Moderator: Lifton Interpretation of neutron monitor measurements (Lifton for Clem) • Clem initially funded for two years. According to Enriqueta, there is no problem with getting two more years in the present form of proposal that Clem submitted. He must reapply after first year. Not funded yet but in process. • Issue with neutron monitors – may over-correct. Neutron flux increases with altitude. Clem is checking latitude and altitude variations. • Questions: o How can we check the neutron flux modeling (effects of uncertainty in 14N cross-sections) with actual data? Nat will check with Clem. Not a lot of data out there on nitrogen. There may be differences in binding energies of nitrogen and it may be incorrect to scale form 12C. o Has Clem only done it with FLUKA model? Not sure. There is a new model – MCNPX. The scaling effects will be less because you don’t scale from sea level to the top of the atmosphere. Action item: Nat will check with Clem about the neutron flux modeling (effects of uncertainty in 14N cross-sections). Geomagnetic secular variation/trajectory modeling (Lifton) • CALS7K.2 model. CRONUS-Earth has no calibration data for 50 ka but CRONUS-EU does. Katrin has some 51 ka – 300 ka samples from Canary Islands. Tibor sent Nat images from Canary Islands and a volcano in South America. • Questions: o Why does CALS7K.2 have a longitudinal effect? It could be because it is non-linear. The difference may be computational. o VADM data -why SINT-800 not SINT-2000? Nobody believes the SINT-2000 values. Cathy Constable indicates that there may be problems with way that the volcanics were calibrated. o How accurate are the time-integrated 14C at sea level (when using this model in the web calculator)? Given the quality of the calibration dataset, cannot distinguish between scaling schemes. Present calibration set will be able to distinguish the scaling scheme that is correct (at least Lal vs. neutron monitor). Geological scaling activities (Lifton) Saturated 14C • New number difference due to changes in sample processing (increased to 3-4 days of etching). If you keep etching longer, do you see convergence of values? The problem is that grain size eventually gets too small. • Need to decide on atmospheric pressure for all calibration sites. • Joerg has pressure data for Tibet. • Desilets now has non-neutron monitor based-model (?meaning unclear?). • Questions: o How old are the saturated Chile samples? About 100 ka. o Have you considered rock surface uplift? No because only seeing the last 20 ka. o Have you read the James Divers paper on how the atmosphere compresses? Not yet. o To take non-dipole component information back, is there a way to use stochastic modeling to move it back in time using 7 ka record? Constable is extending model back 10 ka. She is using spherical harmonic models to take it back further. o Have you considered that samples from the Andes boulders may have been covered for a short time by ash? How persistent would it be? Could be multiple times but would be relative to location. In situ 14C Lab (Goehring) • Questions: o How can you check snow cover? Will be able to tell from 14C data. Canaries (Lifton) • Stone collected Holocene lavas, CRONUS-EU has Holocene and older lavas. • Questions: o What are the age controls? Radiocarbon. And Christopher Columbus saw it erupting in 1492. Quelccaya & Peru altitude transect (Kelly) (Kelly) • Erosion problem associated with late Holocene. • Potential to test the energy dependent scaling using 10Be. But to make a rigorous test, would need similar samples from sea level. May not be a high energy-low energy thing, may be neutron monitor bias due to dipole. • Difficult to get a very old minimum (calibrated). If minimum radiocarbon is 9 ka, then don’t have calibration site. No, not a problem because you don’t need to get that close because of scaling schemes. • Questions: o Is there a potential to get good radiocarbon ages from this setting? Yes, a lot of continuous peat deposits. o Can we be glacial geologists and say that this is a Younger Dryas moraine? No! Must have data supporting this. o What will you have to do to get minimum ages? Will have to core. o Would like to get an attitude transect for 14C – any thoughts? There are exposed higher bedrock ridges but they are highly eroded. o What about going up from sea level? It is a long way from Lima. Could do the altitude transect on the west side. o How humid is the climate starting at Lima? Not that humid. A better transect may be in Chile. o Is there a potential for snow cover? Not really, it’s very windy. Action item: Meredith will research potential altitude transects for Fred. Andes site (Kaplan) • Questions: o Are the errors due to scaling or are they analytical errors? Analytical. Secondary sites and possibilities (Breque, Iceland, Sierra Nevada, Zuni Bandera, Asian transect, Namibia, others?) • Have money in budget for two TBA sites. New Zealand (Doughty/Putnam) • Some disagreement about precision of data and degree of error (not within one sigma). Turkey Transect (Zreda) • No dates on the dome (dates from ash flow). Could potentially be a problem. • Low energy component may be over-estimated, resulting in 20% difference from radiocarbon dates. Maybe should use Fred’s unpublished production rate. • Other potential problem -sensitivity to any uncertainty in nucleogenic computation. • Questions: o How many ppm Cl? 1000. Artificial targets (Zreda/Kurz) • Questions: o What is going on with Lal targets? Prepared toxic targets – could not get permission to put on sites. Lal is working on new targets. These targets will only take a few months of exposure. Lal has exposed some targets at White Mountains and at sea level in La Jolla. He is currently analyzing them and will know if his procedures are good. o Does the difference between targets on ground and on roof have any boundary effects? It should not affect high-energy neutrons. Could model to take this into account. Rooftop placement was due to security. o Will these samples freeze? Probably not. 10Be behavior will be different if water freezes. Freeze-melt could be very bad. o How much 10Be in the plastic? Kuni has found 10Be in water blanks. Kuni suggested measuring this first. Marek thinks not much 10Be. Could put a carboy under ground for three years. Artificial targets (Vermeesch) • Questions: o Where was 4500 m site? Monte Rosa. Artificial targets – action item: Put a 10Be blank carboy under ground for three years Issue 3: Improvement in accuracy of analytical measurements Moderator: Jull Standards and intercomparison (Jull/Scott) • Need Low Al quartz for 26Al sample. This could be difficult. • Questions: o Where does 36Cl fit into this? Does Shasta have material? Yes, collected limestone. Send it to Tim when it is ready and it will be used for second round. Need evidence that it’s homogeneous and chemical composition. Need a minimum of 8 aliquots. o Original recommendation was to use 5 grams etched with three HF treatments. Do you mind if they do more? You can etch it again but need to document that this was done. o Who has done petrography/geochemistry on quartz? Are there inclusions (rutile)? Tables with this data are available upon request from Tim. o Why did you do as much preprocessing? To test that component. o Kuni feels that there are problems with the previous sample (not good). Can there be better sample for Phase 2? Trying to identify some new samples. Work in process. Need to produce table of lab results. Need meeting to present all data. Rationale – trying to identify which part is problem – sample or processing. o What is the difference producing variability? Could be the splitting. Action item: Finalize acquisition and preparation of second suite of samples. Action item: Set timeline and distribute samples. Action item: Await results (distribute in April 2008, deadline for results December 2008). Action item: Analysis of Phase 1 results by June 2008 (prior to Goldschmidt). 10Be half-life (Nishiizumi) • Papers need to report the standard used. Reviewers need to ask for the standard and enforce reporting the standard. • Questions: o What to do with samples measured relative to NIST standard (with the 2 half lives)? Examples of bad use of half-life are in the literature. Watch out for incorrectly reported data. We haven’t produced much data for CRONUS before the identification of this problem so this issue should be considered for all future data. o Measurement uncertainties are working their way into the uncertainty. How should this be treated for the community? Other communities report their findings for a standard, but we can’t do that. Must pass this information onto the community. Official notice to editors of relevant journals about this problem (may or may not work) Parameter optimization modeling (what do we need?) (Borchers) • You have to believe in the uncertainties that are reported. • Calculator: must provide the people using it some advice on the uncertainties that will be used (should be used) • Encourage people to have a standard reporting format. Make sure that people report the raw data so that things can be recalculated in the future. Action item: Intercomparison between labs (AMS labs not all the same). Need to address all these labs. Action item: ID more samples to use for inter-comparison. Action item: Workshop on this topic with all the people who contributed. Issue 4: A common interpretation platform A common interpretation platform Moderator: Balco CRONUS-Earth Web Calculator (Balco) • Updates on the end-user software. • Issues to discuss: 1. What do do for resource allocation? Maintenance? Long-term solution? 2. iCRONUS vs online calculator? Overlap? Transparency of end product to assimilation of overall project results? 3. Planning issues for integration of online/end-user services with internal data- assimilation effort (especially WRT uncertainties). 4. Serious attention to databases? All the databases need to interconnect and that we can all share and exchange. • Current issues: 1. Be-10 stds and half-life? How do we help people get the correct results based on their data? 2. How and when do we update the calibration data set (include TAB or PPT). • It is still important to report the original data. The community may use this to calculate two different reported age/results on a common platform. • He3 calculator: (grad student PhD for CRONUS) developing calculator. Greg predicts opposition. Compositional variability of target is a contentious issue. Will add to website when done. ACE (Zreda) • Changes: web-based application changed to stand-alone application. Software will be done December -January. • Transparent code, modular (use what you need. Example: sea level correction, put in box, if you don’t want to correct for it, take it out). • Differ with this group on how production rates and scaling should be handled. This is a tool for people to use to “explore the cosmogenic universe”, not necessarily saying that it is better or worse than something else, but just giving them the tool. • Paper will be published summer 2008 announcing software, then another with details later. • Nothing is hard-wired; everything is customizable. The calibration set will be selectable. Any changes in the code will recalibrate automatically. The version numbers will be tagged with what has changed. You can always undo changes. • Depth profiles will be handled (high energy will use neutron attenuation length). Cosmocalc • The paper is online in g-cubed: Cosmocalc: An Excel add-in. • Install Cosmocalc from cosmocalc.googlepages.com • Calculates: scaling factors, shielding factor, snow shielding, thickness correction, banana plots, age-erosion rate, burial exposure, burial erosion, (some calcs do Monte Carlo), can convert lat/long/inclination. Fully customizable on hidden page. Implicit calibration: based on sites. page. Implicit calibration: based on sites. • Doesn’t do paleomagnetic corrections (too big, not user friendly). No thermal neutrons. Not ready for 36Cl, 14C. Can specify half-life. Parameter optimization modeling (interfacing with Web Calc / uncertainty calcs)(Borchers) (3:15-3:30 pm) Parameter optimization modeling (interfacing with Web Calc / uncertainty calcs) (Borchers) • Question: o If you have only one common interpretation platform, how do you know if you have any error? In the calibration process, if you can fit you data, it is a good indication that the code is working. No validation yet if the Matlab code is working correctly. General review and discussion Tibor to provide update on Cronus-EU data sets. Should be available autumn next year. Action item: Get list from Fred. Joint Meeting • Goldschmidt would work well, however it may be a bit early (won’t have all the data). Link data discussion to major meeting in 2009. Could consider having it in Vienna. CRONUS Website (Caffee by proxy) Action item: Link to calculator. Action item: Send a list of things that people would like. Marc has someone to implement the suggestions Action item: Want revision on the logo. Spend some money on website design (check with Paul Bierman). Action item: Need option to upload photos. Action item: Need searchable database. EarthScope (Gosse) • Geochronologists have database that they want to make available -queryable, spatial geochronology (Geo Earth Scope and Earth Chem Projects). • Have been as to do this for Ur/Th/He – exactly what we’re talking about. Click for what has been done or check the whole database. • Hosted at U Kansas (Doug Walker). • Wants from us (in next 6 months) to come up with a set of protocols, a set of challenges, things that we want from the database, how to interface, how to query, right now – wants current data. Action item: John will send out email to CRONUS and Cronus-EU. To start, John will send around a proposal about what should be in our database, how to interface, how to query. They want to put files attached to each sample, Ur/Th -photo’s of zircons with measurements. Action item: Eventually, Doug Walker would come to CRONUS workshop or we could go to U Kansas for 2-3 day meeting. Action item: Enriqueta – although Doug Walker suggested that he would do the databases, CRONUS-Earth should dictate how the database should be built. Not sure if his money includes cosmogenic nuclides. John will send out email to CRONUS and Cronus-EU. To start, John will send around a proposal about what should be in our database, how to interface, how to query. They want to put files attached to each sample, Ur/Th -photo’s of zircons with measurements. Action item: Eventually, Doug Walker would come to CRONUS workshop or we could go to U Kansas for 2-3 day meeting. Action item: Enriqueta – although Doug Walker suggested that he would do the databases, CRONUS-Earth should dictate how the database should be built. Not sure if his money includes cosmogenic nuclides. Overview on Geological Calibration progress and future plans (Phillips/Lifton) • Production rates summary: o Where we are – calibration sampling program on target. Collected 2/3 of total samples. Good tropical sight (high altitude). Only thing lagging is Hawaii – problem with analyzing samples already obtained, permits. o Preliminary results for 36Cl and 10Be – certain samples have poor variability. Need to work with Brian about more systematic ways of analyzing samples to identify variability. Sample analyses running slowly. All calibration site samples must be analyzed by this time next year (can decide if we need another site). o Intercomparison is an important component of this program. Must do the intercomparison samples in timely manner. Time-consuming analyses plus crush, sieve, homogenize at Purdue takes a lot of time. Most of those are done – most people have most of the samples that they need. o Make it a process to run replicates of a certain percent of samples – Brian to help develop protocol. Processes seem very different at the various labs. People need to talk about this. o Can’t have a recipe that covers everything (samples can be different). o Intercomparison – will publish without names, but it would be easier to figure out happened if we knew…to diagnose the problem. The geologic calibration samples paid for by CRONUS are public. For 10Be, no names until problem is identified. o Kuni noted that the same sample with the same standard changes over time. Action item: Hawaii sampling. Action item: Need to work with Brian about more systematic ways of analyzing samples to identify variability. Action item: Brian to help develop protocol to run replicates of a certain percent of samples. Nat: • Standstill on neutron monitor modeling (Clem) but back on track. • Geologic calibration 14C – will go headway with three sites in hand. • Sat. 14C high altitude looks good. Don’t know what to make of sea level high latitude plots – still some scatter. • Temporal spatial distribution of nuclides – headway in coming year. • Making progress on geomag corrections. Action item: Neutron measurement and targets – need to get more He target out this year. Lal should get his stuff out. And Pieter. Tim: • Have initial intercomparison set out. Action item: Trying to identify additional samples. Second batch by April. Action item: First intercomparison batch completed by June 2008 (for Goldschmidt). Action item: Workshop at Goldschmidt. Problems with AMS standards. Look at all stages of process to see where there are inconsistencies. Action item: Need to provide the user communities with standard issues. Kuni – will paper have specific recipe? Yes, so that people can identify where they went wrong. Action item: Must follow through with analyzing intercomparison samples. Reminder now – MARIAN. Greg: • Not doing too bad but stalled. Action item: Need professional construction, maintenance and housing of website. Action item: Fred will work with Brian to see if 36Cl can come online. Action item: Possible stand alone Al/Be matlab module. Meeting Adjourned 4:58 PM