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pmip3:wg:degla:bc:ghg [2015/02/17 19:14]
ruza
pmip3:wg:degla:bc:ghg [2015/10/21 13:40]
ruza
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    More info here: http://​wiki.splitbrain.org/​plugin:​discussion */    More info here: http://​wiki.splitbrain.org/​plugin:​discussion */
        
-/* ~~DISCUSSION|Discussion on core experiment ​design~~ *+~~DISCUSSION|Discussion on core experiment ​greenhouse gases~~
  
 ====== Last Deglaciation Greenhouse Gases ====== ====== Last Deglaciation Greenhouse Gases ======
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 [[pmip3:​wg:​degla:​bc:​core|Go back]] to the main core experiment design page. \\ [[pmip3:​wg:​degla:​bc:​core|Go back]] to the main core experiment design page. \\
 [[pmip3:​wg:​degla:​index|Go back]] to the main working group page. \\ [[pmip3:​wg:​degla:​index|Go back]] to the main working group page. \\
-Please note, this page is a work in progress and is not ready for discussion yet. \\ 
 \\  \\ 
 Please use the //​Discussion//​ section below to specifically comment on the choice of __greenhouse gases__ for the core experiment. \\ Please use the //​Discussion//​ section below to specifically comment on the choice of __greenhouse gases__ for the core experiment. \\
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 The composite record (EPICA Dome C, Vostok and Taylor Dome) from [[http://​www.nature.com/​nature/​journal/​v453/​n7193/​full/​nature06949.html | Lüthi et al. (2008)]]<​sup>​[1]</​sup>​ provides CO<​sub>​2</​sub>​ data spanning 800 ka to present. ​ The composite record (EPICA Dome C, Vostok and Taylor Dome) from [[http://​www.nature.com/​nature/​journal/​v453/​n7193/​full/​nature06949.html | Lüthi et al. (2008)]]<​sup>​[1]</​sup>​ provides CO<​sub>​2</​sub>​ data spanning 800 ka to present. ​
-The data will be provided on the timescale of [[http://​www.clim-past.net/​9/​1733/​2013/​cp-9-1733-2013.html | Veres et al. (2013)]]<​sup>​[2]</​sup>​\\+The data will be provided on the AICC2012 ​timescale of [[http://​www.clim-past.net/​9/​1733/​2013/​cp-9-1733-2013.html | Veres et al. (2013)]]<​sup>​[2]</​sup>​\\
 \\ \\
-**Comparison of CO2 records and the PMIP3 LGM** ((Plot produced by Lauren Gregoire, Feb 2015)) \\+**Comparison of CO2 records and the PMIP3 LGM:** ((Plot produced by Lauren Gregoire, Feb 2015)) \\
 {{ http://​homepages.see.leeds.ac.uk/​~earri/​pmip_deglac/​CO2_comparison.png?​ | Comparison of CO2 }}  {{ http://​homepages.see.leeds.ac.uk/​~earri/​pmip_deglac/​CO2_comparison.png?​ | Comparison of CO2 }} 
-In particular, note how the new AICC2012<​sup>​[2]</​sup>​ age model affects the timing of the record and the '​LGM'​ CO<​sub>​2</​sub>​ value; now 188 ppm compared to 185 ppm in PMIP3. There are also differences in timing ​with the [[http://​www.nature.com/​nature/​journal/​v514/​n7524/​full/​nature13799.html | Marcott et al. (2014)]] record.\\+In particular, note how the new AICC2012<​sup>​[2]</​sup>​ age model affects the timing of the record and the '​LGM' ​(21 ka; vertical dashed line) CO<​sub>​2</​sub>​ value; now 188 ppm compared to 185 ppm in PMIP3. There are also differences in timing ​and in the LGM value compared to the higher resolution ​[[http://​www.nature.com/​nature/​journal/​v514/​n7524/​full/​nature13799.html | Marcott et al. (2014)]]<​sup>​[3]</​sup> ​record.\\
 \\ \\
-We are proposing to use the composite record of [[http://​www.nature.com/​nature/​journal/​v453/​n7193/​full/​nature06949.html | Lüthi et al. (2008)]]<​sup>​[1]</​sup>​. \\+We are proposing to use the composite record of [[http://​www.nature.com/​nature/​journal/​v453/​n7193/​full/​nature06949.html | Lüthi et al. (2008)]]<​sup>​[1]</​sup>​; as per the magenta and red lines. \\
  
 \\ \\
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 ===== Methane ===== ===== Methane =====
  
-The EPICA Dome C record from [[http://​www.nature.com/​nature/​journal/​v453/​n7193/​full/​nature06950.html | Loulergue et al. (2008)]]<​sup>​[3]</​sup>​ provides CH<​sub>​4</​sub>​ data also spanning 800 ka to present. +The EPICA Dome C record from [[http://​www.nature.com/​nature/​journal/​v453/​n7193/​full/​nature06950.html | Loulergue et al. (2008)]]<​sup>​[4]</​sup>​ provides CH<​sub>​4</​sub>​ data also spanning 800 ka to present. 
-The data will be provided on the timescale of [[http://​www.clim-past.net/​9/​1733/​2013/​cp-9-1733-2013.html | Veres et al. (2013)]]<​sup>​[2]</​sup>​ \\+The data will be provided on the AICC2012 ​timescale of [[http://​www.clim-past.net/​9/​1733/​2013/​cp-9-1733-2013.html | Veres et al. (2013)]]<​sup>​[2]</​sup>​\\
 \\ \\
-**EPICA Dome C and the PMIP3 LGM** ((Plot produced by Lauren Gregoire, ​Feb 2015)) \\ +**EPICA Dome C and the PMIP3 LGM** ((Plot produced by Lauren Gregoire, ​April 2015)) \\ 
-{{ http://​homepages.see.leeds.ac.uk/​~earri/​pmip_deglac/​CH4.png| EPICA Dome C CH4 }} \\+{{ :pmip3:​wg:​degla:​bc:​ch4.png | EPICA Dome C CH4 }} \\ 
 +Also note how the new AICC2012<​sup>​[2]</​sup>​ age model affects the '​LGM'​ (21 ka; vertical dashed line) CH<​sub>​4</​sub>​ value.\\
  
 +\\
  
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- 
 ===== Nitrous Oxide ===== ===== Nitrous Oxide =====
  
-Work in progress! ​\\ \\+The TALDICE record from [[http://​www.sciencedirect.com/​science/​article/​pii/​S0012821X10006023 | Schilt et al. (2010)]]<​sup>​[5]</​sup>​ provides N<​sub>​2</​sub>​O data spanning 140 ka to present. 
 +The data will be provided on the AICC2012 timescale of [[http://​www.clim-past.net/​9/​1733/​2013/​cp-9-1733-2013.html | Veres et al. (2013)]]<​sup>​[2]</​sup>​.\\ 
 +\\ 
 +**TALDICE and the PMIP3 LGM** ((Plot produced by Lauren Gregoire, Feb 2015)) \\ 
 +{{ http://​homepages.see.leeds.ac.uk/​~earri/​pmip_deglac/​N2O.png?​ | TALDICE N2O }} \\ 
 +The old PMIP3 '​LGM'​ (21 ka; vertical dashed line) CH<​sub>​4</​sub>​ value, probably remains representative of the glacial period for the model spin-up, although the 21 ka value for the transient run will be lower, as per the record above. \\ 
 + 
 +\\
  
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-===== Points ​To Discuss ​=====+===== Points ​to discuss ​=====
  
 Please think about the following points and add any comments on these or any other aspects of the experiment design to the discussion section below: [Topics will be added here as they are raised below or by email.] Please think about the following points and add any comments on these or any other aspects of the experiment design to the discussion section below: [Topics will be added here as they are raised below or by email.]
-  * With the new AICC2012<​sup>​[2]</​sup>​ age model, the LGM values for CO<​sub>​2</​sub>​ and CH<​sub>​4</​sub>​ are inaccurate, as can be seen from the plots above. Do we need a new PMIP LGM definition for these greenhouse gases in accordance with the records? \\ \\ +  ​* **RESOLVED** With the new AICC2012<​sup>​[2]</​sup>​ age model, the LGM values for CO<​sub>​2</​sub><​sup>​[1]</​sup> and CH<​sub>​4</​sub><​sup>​[4]</​sup> are inaccurate, as can be seen from the plots above. Do we need a new PMIP LGM definition for these greenhouse gases in accordance with the records? ​**DECISION (Oct 2015): We have used the new, up to date CO<​sub>​2</​sub>​ (188 ppm) and CH<​sub>​4</​sub>​ (375 ppb) values for our LGM equilibrium-type 21 ka spinup. We do not know what the LGM group'​s decision will be.**\\ \\ 
-  * N<​sub>​2</​sub>​O values take a dive in the lead up to 21 ka. The PMIP3 value of 200 ppb looks fairly representative of the LGM state, even though this is a bit higher than the actual 21 ka value. We recommend that groups spin-up with 200 ppb N<​sub>​2</​sub>​O,​ and begin the transient simulation from 21 ka in the record (as shown in the plot above). ​ \\ \\ +  ​* **RESOLVED** N<​sub>​2</​sub>​O<​sup>​[1]</​sup> ​values take a dive in the lead up to 21 ka. The PMIP3 value of 200 ppb looks fairly representative of the LGM state, even though this is a bit higher than the actual 21 ka value. We recommend that groups spin-up with 200 ppb N<​sub>​2</​sub>​O,​ and begin the transient simulation from 21 ka in the record (as shown in the plot above). ​**DECISION (Oct 2015): We have stuck with the old, more representative N<​sub>​2</​sub>​O value of 200 ppb. However, the transient '​spinup'​ 26-21 ka and the transient run (21-9 ka) should use the chronologically accurate values, as plotted above. We do not know what the LGM group'​s decision will be.** \\ \\ 
-  * Should the core experiment use the [[http://​www.nature.com/​nature/​journal/​v514/​n7524/​full/​nature13799.html | Marcott et al. (2014)]]<​sup>​[4]</​sup>​ CO<​sub>​2</​sub>​ records? \\ For example, these newer data are higher resolution than [[http://​www.nature.com/​nature/​journal/​v453/​n7193/​full/​nature06949.html | Lüthi et al. (2008)]]<​sup>​[1]</​sup>,​ but are restricted to 23-9 ka. Therefore more consistency may be be gained from using the older [[http://​www.nature.com/​nature/​journal/​v453/​n7193/​full/​nature06949.html | Lüthi et al. (2008)]]<​sup>​[1]</​sup>​ CO<​sub>​2</​sub>​ records, if longer simulations are planned by groups. Also, CH<​sub>​4</​sub>​ and N<​sub>​2</​sub>​O data are not yet available in such high resolution.\\ \\+  ​* **RESOLVED** Should the core experiment use the [[http://​www.nature.com/​nature/​journal/​v514/​n7524/​full/​nature13799.html | Marcott et al. (2014)]]<​sup>​[3]</​sup>​ CO<​sub>​2</​sub>​ records? \\ For example, these newer data are higher resolution than [[http://​www.nature.com/​nature/​journal/​v453/​n7193/​full/​nature06949.html | Lüthi et al. (2008)]]<​sup>​[1]</​sup>,​ but are restricted to 23-9 ka. Therefore more consistency may be be gained from using the older [[http://​www.nature.com/​nature/​journal/​v453/​n7193/​full/​nature06949.html | Lüthi et al. (2008)]]<​sup>​[1]</​sup>​ CO<​sub>​2</​sub>​ records, if longer simulations are planned by groups. Also, CH<​sub>​4</​sub>​ and N<​sub>​2</​sub>​O data are not yet available in such high resolution. ​**DECISION (Oct 2015): We have chosen to use the older data from [[http://​www.nature.com/​nature/​journal/​v453/​n7193/​full/​nature06949.html | Lüthi et al. (2008)]]<​sup>​[1].** \\ \\\\ \\
  
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   - Lüthi, D. et al. High-resolution carbon dioxide concentration record 650,​000–800,​000 years before present. Nature 453, 379–382 (2008).   - Lüthi, D. et al. High-resolution carbon dioxide concentration record 650,​000–800,​000 years before present. Nature 453, 379–382 (2008).
   - Veres, D. et al. The Antarctic ice core chronology (AICC2012): an optimized multi-parameter and multi-site dating approach for the last 120 thousand years. Clim Past 9, 1733–1748 (2013). 10, 297–317 (1991). ​   - Veres, D. et al. The Antarctic ice core chronology (AICC2012): an optimized multi-parameter and multi-site dating approach for the last 120 thousand years. Clim Past 9, 1733–1748 (2013). 10, 297–317 (1991). ​
 +  - Marcott, S. A. et al. Centennial-scale changes in the global carbon cycle during the last deglaciation. Nature 514, 616–619 (2014).
   - Loulergue, L. et al. Orbital and millennial-scale features of atmospheric CH4 over the past 800,​000 years. Nature 453, 383–386 (2008).   - Loulergue, L. et al. Orbital and millennial-scale features of atmospheric CH4 over the past 800,​000 years. Nature 453, 383–386 (2008).
-  - MarcottS. A. et al. Centennial-scale changes in the global carbon cycle during the last deglaciationNature 514616619 (2014).\\ \\+  - Schilt, A. et al. Atmospheric nitrous oxide during the last 140,000 years. Earth Planet. Sci. Lett3003343 (2010).\\ \\
  
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pmip3/wg/degla/bc/ghg.txt · Last modified: 2015/10/21 13:42 by ruza