Cosmic-Ray Fluxes Present and Past

Slides:



Advertisements
Similar presentations
10 Be 06NOV2012 Kelly Hughes. How is it produced? Cosmic Ray Spallation: – 10 Be results from 16 O being bombarded with highly energetic cosmic rays Muon-reduced.
Advertisements

Cosmic Ray Using for Monitoring and Forecasting Dangerous Solar Flare Events Lev I. Dorman (1, 2) 1. Israel Cosmic Ray & Space Weather Center and Emilio.
New Production Rate Estimates for In Situ Cosmogenic 14 C Cronus-Earth/EU Workshop, Vancouver, July Bailey Dugan, Nathaniel Lifton, A.J. Timothy.
Paul Evenson, Waraporn Nuntiyakul,
Global Warming and Climate Sensitivity Professor Dennis L. Hartmann Department of Atmospheric Sciences University of Washington Seattle, Washington.
Towards a European Infrastructure for Lunar Observatories Bremen, Wednesday 23 rd March 2005 A 3D cosmic ray detector on the Moon X. Moussas University.
Cosmic Induced Backgrounds D. Reyna Argonne National Lab.
A particularly obvious example of daily changing background noise level Constructing the BEST High-Resolution Synoptic Maps from MDI J.T. Hoeksema, Y.
1 Trends and Anomalies in Southern Hemisphere OH Inferred from 12 Years of 14 CO Data Martin Manning, Dave Lowe, Rowena Moss, Gordon Brailsford National.
Millstone Hill ISR, June 14-18, Ti, June 14-18, 2004.
Cosmic-Ray Fluxes Present and Past Nathaniel Lifton, Marek Zreda, Darin Desilets, John Clem  Background  Objectives  Present-Day Fluxes  Instrumental.
A particularly obvious example of daily changing background noise level Constructing the BEST High-Resolution Synoptic Maps from MDI J.T. Hoeksema, Y.
“How Have Glaciers Behaved in Patagonia in the Past?” with Dr. Michael Kaplan Dr. Michael J Passow Originally presented 25 Oct 2014.
Solar Irradiance Variability Rodney Viereck NOAA Space Environment Center Derived Total Solar Irradiance Hoyt and Schatten, 1993 (-5 W/m 2 ) Lean et al.,
First Results on Solar Irradiance Variability from PROBA2/LYRA/SWAP R. Kariyappa (guest investigator), S. T. Kumar, M. Dominique, D. Berghmans, L. Dame,
Radiation conditions during the GAMMA-400 observations:
Maciej Sliwinski A review of 4 studies
Development of energy-dependent scaling for cosmic-ray neutron intensities and for in- situ cosmogenic nuclide production rates Marek Zreda - Arizona Devendra.
Cosmogenic Dating.  A group of isotopic methods of age determination based on accumulation of certain nuclides, which are produced only in the top few.
October 24, 2012 G 610 – Climate of the Holocene Presenter: Erin Dunbar Assistant: Jesse Senzer.
Ground Level Enhancement of May 17, 2012 Observed at South Pole SH21A-2183 Takao Kuwabara 1,3 ; John Bieber 1 ; John Clem 1,3 ; Paul Evenson 1,3 ; Tom.
The Merton Report an AIMES/IGBP-ESA partnership As Earth System science advances and matures, it must be supported by robust and integrated observation.
Causes of Climate Change Over the Past 1000 Years Thomas J. Crowley Presentation by Jessica L. Cruz April 26, 2001.
Metrics for quantification of influence on climate Ayite-Lo Ajovan, Paul Newman, John Pyle, A.R. Ravishankara Co-Chairs, Science Assessment Panel July.
Ground level enhancement of the solar cosmic rays on January 20, A.V. Belov (a), E.A. Eroshenko (a), H. Mavromichalaki (b), C. Plainaki(b), V.G.
In-Situ Chlorine-36 Nicole Dix HWR 696T. Outline  Introduction  Production Mechanisms  Sample Collection Methods  Laboratory Analysis  Applications.
Cosmogenic Isotopes: Production Rates Matt Baillie HWR 696T 2/26/04.
Cosmic rays at sea level. There is in nearby interstellar space a flux of particles—mostly protons and atomic nuclei— travelling at almost the speed of.
Neutron Monitor Community Workshop—Honolulu, Hawaii
David Argento (some aspects of) cosmogenic nuclide production.
The objective of the CRONUS-Earth Project is to simultaneously address the various uncertainties affecting the production and accumulation of in-situ cosmogenic.
February 7, Long Term Decline of South Pole Neutron Monitor Counting Rate – A Possible Magnetospheric Interpretation Paul Evenson, John Bieber,
The objective of the CRONUS-Earth Project is to simultaneously address the various uncertainties affecting the production and accumulation of in-situ cosmogenic.
Goal of Stochastic Hydrology Develop analytical tools to systematically deal with uncertainty and spatial variability in hydrologic systems Examples of.
Preliminary validation of computational procedures for a New Atmospheric Ionizing Radiation (AIR) model John M. Clem, Giovanni De Angelis, Paul Goldhagen.
Muon-induced neutron background at Boulby mine Vitaly A. Kudryavtsev University of Sheffield UKDMC meeting, ICSTM, London, 27 June 2002.
Update on the analysis of muon angular distributions in equatorial coordinates F.Riggi Dept. of Physics and INFN, Catania.
FLUKA Muon Calculations For Electronic Applications
Cosmogenic Muon Background
Paul Evenson University of Delaware
Observation of cosmogenic nuclide Be-7 concentrations in the air at Bangkok and trajectory analysis of global air-mass motion S. Suzuki , H. Sakurai ,
Physics-Based Modeling Robert Reedy (UNM), Kyeong Kim (U. Ariz
South Pole Ice model Dmitry Chirkin, UW, Madison.
IceCube: Multiwavelength Approach to
V2.0 minus V2.5 RSAS Tangent Height Difference Orbit 3761
INTEGRAL Satellite on Oct 28th 2003
Development of a GLE Alarm System Based Upon Neutron Monitors
Department of Space Physics: Detached Laboratory at Lomnický štít (LS)
The ROLO Lunar Calibration System Description and Current Status
Neutron backgrounds in KamLAND
Validation of Satellite-derived Lake Surface Temperatures
John Kelley for the IceCube Collaboration
CH. 4 THE RESEARCH PROCESS
Carbon dating Carbon has 3 isotopes: 12C – stable 13C – stable
In-Situ Chlorine-36 Nicole Dix HWR 696T.
Cosmogenic Isotope Dating Overview
University of Delaware
Records of Cosmogenic Isotope Production Rates
Daya Bay Neutrino Experiment
Chapter 4B: SOLAR IRRADIATION CALCULATION
13-2 The Age of the Earth Modern Biology.
Simulation of 14C production rates for the troposphere and stratosphere in weak geomagnetic intensity at 26,000 yr BP 1 Graduate School of Science and.
Masters Thesis Proposal by Eric W. Portenga
Instrumental Surface Temperature Record
Determining long term erosion rates in Panama
PHYS 5326 – Lecture #7 Improvements in Sin2qW
EGU 2018, Vienna, 13 April 2018; abstract EGU
Intae Yu Sungkyunkwan University (SKKU), Korea KNO 2nd KNU, Nov
Analysis of GLAST Balloon Experiment Data
EGU 2018, Vienna, 8 April 2018; abstract EGU
Presentation transcript:

Cosmic-Ray Fluxes Present and Past Nathaniel Lifton, Marek Zreda, Darin Desilets, John Clem Background Objectives Present-Day Fluxes Instrumental Measurements Modeling Time-Integrated Fluxes In Situ 14C in Saturated Surfaces CRONUS-Earth

Background Production Rates Well-Established at Few Sites Scaling Models Predict Production Rates Elsewhere Current Scaling Models Based on Modern Cosmic-Ray Measurements Lal, 1991; Stone, 2000; Dunai, 2000, 2001; Desilets & Zreda, 2003; Lifton et al., in prep Neutron Monitors (NM) Other Instruments/Techniques Problems Need to Tie CR Measurements to CN Production in Rocks Limited Empirical Testing of Models Over Millenial Time Scales Scarcity of Samples of Well-Established Age CRONUS-Earth

Objectives Relate NM Measurements to CN Production Rates Global NM Network Data, Published Surveys CRONUS-Earth

Global Neutron Monitor Network CRONUS-Earth

Global Neutron Monitor Network CRONUS-Earth

Objectives Relate NM Measurements to CN Production Rates Global NM Network Data, Published Surveys Selected Low-Energy Neutron Detector Measurements Using NM Data as a Basis for CN Scaling Can a Single Scaling Model Apply to the Entire Neutron Energy Spectrum? Detailed NM Response to Secondary Cosmic Rays? NMs More Sensitive to High Energies Are Rocks as Well? Physically Relate NM Response and CN Production in Rock Test Scaling Models over Millenial Time Scales In Situ 14C in Saturated Surfaces CRONUS-Earth

Present-Day Fluxes Measurements (Zreda, Desilets) Modeling (Zreda, Desilets, Clem) CRONUS-Earth

Time-Integrated Scaling From In Situ 14C Production Rates Short Half-Life 5,730 yr Secular Equilibrium by About 25 kyr Insensitive to Moderate Erosion Rates Many Geomorphic Settings Suitable for Production Rate Determinations CRONUS-Earth

In Situ Cosmogenic 14C (In Situ 14C) Extract From Quartz Opportunity for Thorough Empirical Testing of Scaling Models Integrated Over Millenial Time Scales CRONUS-Earth

Existing Altitude Transects CRONUS-Earth

In Situ 14C Production Rate Scaling Produced by Nucleons and Muons 83% spallation, 15% slow muon, 2% fast muon (Heisinger et al, 2002) Preliminary Antarctic Data Suggest Low Muogenic Production CRONUS-Earth

Antarctic Altitude Transect CRONUS-Earth

In Situ 14C Production Rate Scaling Produced by Nucleons and Muons 83% spallation, 15% slow muon, 2% fast muon (Heisinger et al, 2002) Preliminary Antarctic Data Suggest Low Muogenic Production Scale to SL, High Latitude Time-integrated production rate Account for geomagnetic and solar variability Test atmospheric models Test For Bias With Sample Altitude and Latitude CRONUS-Earth

Identifying Scaling Model Biases CRONUS-Earth

Uncertainties Scatter in Preliminary Data CRONUS-Earth

Observed Scatter CRONUS-Earth

Uncertainties Scatter in Preliminary Data Low Values = Geologic Factors Address with Many Analyses High Values = Inadequate Pretreatment? Identify and Minimize Lab Sources of Scatter Different Workers Different Sample Prep Techniques Different Degrees of Etching? Objective Indicator of Etching Amount Ba, Al, Zr? CRONUS-Earth

Stepwise Dissolution CRONUS-Earth

Uncertainties Scatter in Preliminary Data Low Values = Geologic Factors Address with Many Analyses High Values = Inadequate Pretreatment? Identify and Minimize Lab Sources of Scatter Different Workers Different Sample Prep Techniques Different Degrees of Etching? Objective Indicator of Etching Amount Ba, Al, Zr? Spallogenic/Muogenic Production Proportions Antarctic Altitude Transect 5-10 m Drill Cores from Geological Calibration CRONUS-Earth

Timeline and Deliverables Year 1 Identify Global Sample Set for Saturated 14C Analysis Already Collected by Other Investigators Evidence for 14C Saturation Stable/Long-Lived CN Data Geomorphic/Geologic Indicators Years 1-5 Analyses Year 5 Results Compared with Other CRONUS Data Geomagnetic & Solar Variation Effects Atmospheric Effects Spallogenic/Muogenic Production Incorporate into Parameter Estimation Model Write Papers CRONUS-Earth

Geological Calibration Lake Bonneville Shorelines

Lake Bonneville, Utah

Tabernacle Hill

Bonneville & Provo Shorelines