data:solar_pmod

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data:solar_pmod [2016/11/17 12:04] – created jypeterdata:solar_pmod [2019/11/18 11:49] (current) – Replaced files links with sharebox links jypeter
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 The spectral grid is identical to the spectral grid used for the CMIP SSI data set for the The spectral grid is identical to the spectral grid used for the CMIP SSI data set for the
 wavelength longer than 120 nm. The SSI data have been scaled to match CMIP SSI in 1850. wavelength longer than 120 nm. The SSI data have been scaled to match CMIP SSI in 1850.
 +
 +Get the //Description of an alternative SSI dataset for PMIP// document in the [[#references|References]] section below for more information!
 +
 +===== Data file and format =====
  
 The data are available in simple text format with the description of the file structure in the The data are available in simple text format with the description of the file structure in the
-header. In addition we provide a FORTRAN routine to read the data and transform them to a+header 
 + 
 +  * file name = ''pmip4_corr_c14_v20160613.dat'' 
 + 
 +In addition we provide a {{:data:read_transfer_pmip_ssi.f90 |FORTRAN routine}} to read the data and transform them to a
 user defined spectral grid. user defined spectral grid.
  
 +===== References =====
 +
 +<WRAP center round tip 60%>
 +More details about this dataset can be found in the {{ :data:ssi_pmod_for_pmip_c14.pdf |Description of an alternative SSI dataset for PMIP document}}
 +</WRAP>
 +
 +  * Fontenla, J., O. White, P. Fox, E. Avrett, and R. Kurucz, Calculation of solar irradiances. I. Synthesis of the Solar Spectrum, The Astrophysical Journal, 518, 1, 480-499, 1999, [[http://iopscience.iop.org/article/10.1086/307258/meta|doi:10.1086/307258]]
 +  * Judge, P., G. Lockwood, R. Radick, G. Henry, A.I. Shapiro, W. Schmutz, and C. Lindsey, Confronting a solar irradiance reconstruction with solar and stellar data. Astronomy & Astrophysics, 544, A88, 6, 2012, [[http://www.aanda.org/articles/aa/abs/2012/08/aa18903-12/aa18903-12.html|doi:10.1051/0004-6361/201218903]]
 +  * Krivova, N. A., S. K. Solanki, M. Fligge, and Y. C. Unruh, Reconstruction of solar total and spectral irradiance variations in cycle 23: is solar surface magnetism the cause? Astron. Astrophys., 399, L1–L4, 2003, [[http://www.aanda.org/articles/aa/abs/2003/07/aaek061/aaek061.html|doi:10.1051/0004-6361:20030029]]
 +  * Shapiro, A. I.; Schmutz, W.; Schoell, M.; Haberreiter, M.; Rozanov, E. NLTE solar irradiance modeling with the COSI code, Astronomy and Astrophysics, 517, A48, 13, 2010, [[http://www.aanda.org/articles/aa/abs/2010/09/aa13987-09/aa13987-09.html|doi:10.1051/0004-6361/200913987]]
 +  * Shapiro, A. I.; Schmutz, W.; Rozanov, E.; Schoell, M.; Haberreiter, M.; Shapiro, A. V.; Nyeki, S. (SSR11), A new approach to long-term reconstruction of the solar irradiance leads to large historical solar forcing, Astronomy & Astrophysics, 529, A67, 8, 2011, [[http://www.aanda.org/articles/aa/abs/2011/05/aa16173-10/aa16173-10.html|doi:10.1051/0004-6361/201016173]]
 +  * Solanki, S., N. Krivova and J. Haigh, Solar irradiance variability and climate, Ann. Rev. Astron. Astrophys., 51, 311–351, 2013, [[http://www.annualreviews.org/doi/10.1146/annurev-astro-082812-141007|doi:10.1146/annurev-astro-082812-141007]]
 +  * Usoskin, I., Y. Gallet, F. Lopes, G. Kovaltsov, G. Hulot, Solar activity during the Holocene: the Hallstatt cycle and its consequence for grand minima and maxim. In press: Astron. Astrophys., 587, A150, 2016, [[http://www.aanda.org/articles/aa/abs/2016/03/aa27295-15/aa27295-15.html|doi:10.1051/0004-6361/201527295]]
 +
 +===== Download =====
 +
 +<WRAP center round info 60%>
 +Once you have downloaded the compressed text data file, you can use the command ''bzmore'' to have a quick look at its content without having to uncompress it! 
 +<code>  > bzmore pmip4_corr_c14_v20160411.dat.bz2
 +------> pmip4_corr_c14_v20160411.dat.bz2 <------
 +Annual mean SSI and TSI for PMIP provided by PMOD/WRC
 +Time period 850-1850
 +Number of years    1001
 +Number of spectral bins    3780
 +
 +Structure of the file
 +Start of the spectral bins in nm, format=(10(e12.4))
 +Length of the spectral bins in nm, format=(10(e12.4))
 +Year and TSI in W/m**2, format=(I4,1x,e12.4)
 +SSI in W/m**2/nm, format=(10(e12.4))
 +
 +  1.2000e+02  1.2100e+02  1.2200e+02  1.2300e+02  1.2400e+02  1.2500e+02  1.2600
 +e+02  1.2700e+02  1.2800e+02  1.2900e+02
 +  1.3000e+02  1.3100e+02  1.3200e+02  1.3300e+02  1.3400e+02  1.3500e+02  1.3600
 +e+02  1.3700e+02  1.3800e+02  1.3900e+02
 +</code>
 +</WRAP>
 +
 +If you want to download a file, click on the [[https://sharebox.lsce.ipsl.fr/index.php/s/Ci3D4lT1km7jXMs|PMIP4 PMOD_14C solar forcing data download link]] and then on the file you need.
 +
 +/* The files are currently protected by a password. Get in touch with [[johann.jungclaus@mpimet.mpg.de|Johann Jungclaus]] or [[pmip3web@lsce.ipsl.fr|Jean-Yves Peterschmitt]] if you need to access them. */
  
 +^ md5sum output ^ Data file ^ Size ^
 +| f48a9d042c0f7100dae17375d218c4e1 | pmip4_corr_c14_v20160411.dat.bz2 | 5.8 Mb |
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