pmip3:design:lm:index
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pmip3:design:lm:index [2009/02/09 15:50] – Added warning and moved the 'Goto [exp]' at the top of the page jypeter | pmip3:design:lm:index [2010/02/12 15:55] – Added link to 8k2 jypeter | ||
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- | ~~DISCUSSION~~ | + | ~~DISCUSSION:closed~~ |
- | //Go to =>// [ [[pmip3: | + | < |
+ | //Go to =>// [ [[pmip3: | ||
====== Last Millennium Experimental Design ====== | ====== Last Millennium Experimental Design ====== | ||
- | <note warning> | + | <note warning> |
+ | |||
+ | The basic principle is that we should strive to include all relevant transient forcings over this period if the functionality exists in the model, noting that conformability with the CMIP5 controls and 20th Century transient is crucial. | ||
===== Boundary conditions ===== | ===== Boundary conditions ===== | ||
+ | ==== Summary of Last Millennium boundary conditions ==== | ||
+ | |||
+ | ^ ^ | ||
+ | | Orbital parameters | ||
+ | | Date of vernal equinox | ||
+ | | Trace gases | Annually varying (850-1850) ([[index# | ||
+ | | Volcanic Aerosols | ||
+ | | Solar irradiance | ||
+ | | | ||
+ | | Aerosols | ||
+ | | Vegetation | ||
+ | | Ice sheets | ||
+ | | Topography and coastlines | ||
+ | |||
+ | Please use the [[index# | ||
===== Initial conditions ===== | ===== Initial conditions ===== | ||
+ | ===== Additional information ===== | ||
+ | |||
+ | ==== Total Solar Irradiance ==== | ||
+ | |||
+ | |||
+ | The following figure (click to get the full-size image) has been provided by [[johann.jungclaus@zmaw.de|Johann Jungclaus]] (MPI-M Hamburg) | ||
+ | |||
+ | {{: | ||
+ | |||
+ | Time series of TSI (Wm-2) from 800AD to 2000. For the COSMOS (MPI-M) | ||
+ | Millennium simulations (black curve), a 11 year cycle was added for consistency over the | ||
+ | entire period. | ||
+ | |||
+ | Notes: We will impose an 11 year cycle on pre-sunspot reconstructions for consistency of the spectrum of natural variability. Additionally, | ||
+ | |||
+ | Candidate reconstructions: | ||
+ | |||
+ | ==== Volcanic Forcings ==== | ||
+ | |||
+ | Issues: compatability of eff. rad, zonality, height distribution with modern satellite (Sato) data. | ||
+ | |||
+ | Candidate datasets: Crowley, Ammann - differences in thresholds for significant eruptions, peak forcing etc. Need merged/ | ||
+ | |||
+ | ==== Reconstructed evolution of trace gases ==== | ||
+ | |||
+ | The evolution of CO< | ||
+ | |||
+ | |||
+ | ==== Orbital forcing ==== | ||
+ | |||
+ | The following orbital parameters parameters should be used, if they are not internally calculated. | ||
+ | |||
+ | Note: calculation from Berger (1978), annually varying. | ||
+ | |||
+ | === Precomputed table === | ||
+ | |||
+ | The {{: | ||
+ | [[gschmidt@giss.nasa.gov|Gavin Schmidt]] (GISS). | ||
+ | |||
+ | === Linear regressions === | ||
+ | |||
+ | Over the period 0-2100 CE, the parameters are well approximated by the following linear regressions: | ||
+ | |||
+ | ^ Parameter | ||
+ | | ECC | 0.017475 - 0.000000382 * Year | | ||
+ | | OBL | 23.697 | ||
+ | | PERI-180 | ||
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[ [[pmip3: | [ [[pmip3: | ||
[ [[pmip3: | [ [[pmip3: | ||
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pmip3/design/lm/index.txt · Last modified: 2010/09/16 14:38 by jypeter