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data:data_analysis_manual [2024/10/25 15:36]
Terje Fredvik [Data products]
data:data_analysis_manual [2026/08/24 16:48] (current)
Peter Young [Find data] added event list links
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 The data levels, FITS files, and headers are described in The data levels, FITS files, and headers are described in
-  * The [[https://​spice-wiki.ias.u-psud.fr/​lib/​exe/​fetch.php/​public:​spice-uio-dpdd-0002-2.1-data_product_description_document_spicefits_.pdf|Data ​Products ​Description Document]] (DPDD)+  * The {{ :​public:​spice-uio-dpdd-0002-2.2-data_product_description_document_spicefits_all_accepted.pdf |Data Product ​Description Document (DPDD) ​version 2.2}}
   * The LLDPDD for the Low-Latency (LL) files   * The LLDPDD for the Low-Latency (LL) files
  
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   * Accessible through IDL/SSW and Python/Fido   * Accessible through IDL/SSW and Python/Fido
   * FIXME As of 2024-03-29, the SPICE files on VSO are old files from release 3.0 only   * FIXME As of 2024-03-29, the SPICE files on VSO are old files from release 3.0 only
 +
 +Event lists:
 +  * [[public:​eventlists:​flares|Flares]]
 +  * [[public:​eventlists:​prominences|Prominences]]
  
 ===== Tips and Advice on Analyzing SPICE Data ===== ===== Tips and Advice on Analyzing SPICE Data =====
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 | d->​get\_number\_windows() ​     | No. of spectral windows ​               | | d->​get\_number\_windows() ​     | No. of spectral windows ​               |
 | d->​get\_window\_data(i,/​load) ​ | Extract a data window ​                 | | d->​get\_window\_data(i,/​load) ​ | Extract a data window ​                 |
-| d->​get\_lambda\_vector(i) ​     | Get wavelength vector for the window ​                 |+| d->​get\_lambda\_vector(i) ​     | Get wavelength vector for the window ​  | 
 +| d->​get\_time\_vector(i) ​       | Get the mid-time for each exposure ​    |
 | d->​get\_header(i) ​             | Extract a data window header ​          | | d->​get\_header(i) ​             | Extract a data window header ​          |
 | d->​get\_window\_id(i) ​         | Get the data window ID                 | | d->​get\_window\_id(i) ​         | Get the data window ID                 |
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 Links: Links:
 +  * Python quicklook tool: [[https://​pypi.org/​project/​spiceitup/​|SPICE-IT-UP]].
   * Example with [[:​data:​data_analysis_manual:​sunraster|with sunraster]].   * Example with [[:​data:​data_analysis_manual:​sunraster|with sunraster]].
   * Tutorial about [[https://​git.ias.u-psud.fr/​spice/​data-analysis-club/​-/​blob/​main/​20230516-coordinates/​coordinates.ipynb|plotting and coordinates transforms]]   * Tutorial about [[https://​git.ias.u-psud.fr/​spice/​data-analysis-club/​-/​blob/​main/​20230516-coordinates/​coordinates.ipynb|plotting and coordinates transforms]]
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 ==== Line fitting ==== ==== Line fitting ====
  
-=== Using EIS fitting software ​for SPICE === +For IDL Gaussian ​fitting software, please check: **[[data:line_fitting_idl|IDL software for emission line fitting]]**.
- +
-The routine spice\_getwindata returns a "​windata"​ structure in a form compatible with the eis\_auto\_fit suite of routines for Hinode/EIS. Further information on these routines is given in [[https://​doi.org/​10.5281/​zenodo.6339584 +
-|EIS Software Note 15]]. The mask spectra fitting routines (Case 2 in the document) do not currently work with SPICE, however.+
  
-The EIS software enable a number of operations to be performed on windata structuresas described in [[https://sohoftp.nascom.nasa.gov/solarsoft/hinode/eis/doc/eis_notes/21_WINDATA/eis_swnote_21.pdf|EIS Software Note 21]]. For example, eis\_bin\_windata allows spatial binning of the rasters.+Fitting in Python can be done with any fitting libraryincluding ​[[https://docs.astropy.org/​en/​stable/​modeling/​|astropy.modelling]]. From astropy 7.0, there is a user-friendly way of doing the fitting in parallel ([[https://github.com/aperiosoftware/parallel-modeling-examples/blob/main/spice/​Final_Tutorial.ipynb|tutorial]] by Stuart Mumford).
  
-If you have problems running ​the EIS software on SPICE data, please contact ​[[https://science.gsfc.nasa.gov/sed/bio/peter.r.young|Dr. Peter Young]].+This is used by the [[https://pypi.org/project/pycfit/|PyCFIT]] library, which provides a GUI for fitting the different components.
  
 === Line window width and spectral tilt === === Line window width and spectral tilt ===
data/data_analysis_manual.1729863413.txt.gz · Last modified: 2024/10/25 15:36 by Terje Fredvik