Differences
This shows you the differences between two versions of the page.
| Next revision | Previous revision Next revision Both sides next revision | ||
|
data:solar [2016/07/28 10:23] jypeter created |
data:solar [2016/11/17 10:11] jypeter Removed the references to past2k |
||
|---|---|---|---|
| Line 4: | Line 4: | ||
| You will find on this page some of the boundary condition data that you have to use for | You will find on this page some of the boundary condition data that you have to use for | ||
| * [[exp_design: | * [[exp_design: | ||
| - | * [[exp_design: | ||
| Please make sure to read the [[# | Please make sure to read the [[# | ||
| Line 10: | Line 9: | ||
| Get in touch with the following people if you have questions: | Get in touch with the following people if you have questions: | ||
| - | | [[johann.jungclaus@mpimet.mpg.de|Johann Jungclaus]] | Last Millennium, past2k | + | | [[johann.jungclaus@mpimet.mpg.de|Johann Jungclaus]] | Last Millennium | |
| | [[krivova@mps.mpg.de|Natalia Krivova]] | Details on the SATIRE-based data sets | | | [[krivova@mps.mpg.de|Natalia Krivova]] | Details on the SATIRE-based data sets | | ||
| | [[Tania.Egorova@pmodwrc.ch|Tania Egorova]] | Details on the PMOD-based data set | | | [[Tania.Egorova@pmodwrc.ch|Tania Egorova]] | Details on the PMOD-based data set | | ||
| Line 33: | Line 32: | ||
| ==== Data ==== | ==== Data ==== | ||
| + | * [[data: | ||
| + | * [[data: | ||
| - | SOLAR_FORCING_SATIRE_14C (link to the data page, below) | ||
| - | |||
| - | SOLAR_FORCING_SATIRE_10Be | ||
| - | |||
| - | SOLAR_FORCING_PMOD_14C | ||
| - | |||
| - | |||
| - | |||
| - | Data page: (lets just start with the default page) | ||
| - | |||
| - | ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ | ||
| - | |||
| - | The PMIP4-CMIP6 SOLAR_FORCING_SATIRE_14C | ||
| - | |||
| - | The file contains solar spectral irradiance based on 14C and the SATIRE-M model for the last 9000 years (6754.5 BC to December 2015). Two versions are provided, one (*_fc.txt) with an adaptation of the spectral irradiance to the CMIP6 historical forcing, and one (*_nfc.txt) without such re-scaling. The data set scaled to the CMIP6 historical forcing is the recommended forcing for the PMIP4-CMIP6 “tier-1” past1000 experiment. | ||
| - | |||
| - | |||
| - | Data files | ||
| - | |||
| - | The data are provided in simple text format. The files contain the SSI reconstruction using SATIRE-M based on 14C isotopes. | ||
| - | |||
| - | The file structure is as follows: | ||
| - | 1st array: wavelength array in [nm], listing the center of each wavelength bin. | ||
| - | 2nd array: wavelength bin in [nm], listing the bin width of each wavelength bin. | ||
| - | 3rd array: time in [year] (floating numbers). | ||
| - | 4th array: SSI reconstruction in [W m-2 nm-1]. SSI is average SSI in corresponding bin. | ||
| - | |||
| - | We provide following code (IDL) to read the .txt file and calculate TSI: | ||
| - | |||
| - | ; | ||
| - | ;N=69235 for 14C reconstruction | ||
| - | ;N=61595 for 10Be reconstruction | ||
| - | header=strarr(12) | ||
| - | satire_wl=dblarr(1070) | ||
| - | satire_dwl=dblarr(1070) | ||
| - | time=dblarr(N) | ||
| - | SSI=dblarr(1070, | ||
| - | |||
| - | openr, | ||
| - | | ||
| - | | ||
| - | | ||
| - | | ||
| - | | ||
| - | close,1 | ||
| - | |||
| - | TSI=dblarr(N) | ||
| - | FOR i=0L,N-1 DO TSI[i]=TOTAL(satire_dwl*SSI[*, | ||
| - | ; | ||
| - | |||
| - | |||
| - | Download | ||
| - | |||
| - | link to the .tar.gz file | ||