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data:data_analysis_manual [2023/11/10 09:19]
Terje Fredvik [Data products]
data:data_analysis_manual [2024/01/17 16:26]
Peter Young [Units and uncertainties]
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   * ''​EAR\_TDEL'':​ light travel time difference between Sun centre to Spacecraft and Sun centre to Earth (seconds)   * ''​EAR\_TDEL'':​ light travel time difference between Sun centre to Spacecraft and Sun centre to Earth (seconds)
  
-The full list of keywords is given in the [[https://​spice.ias.u-psud.fr/​spice-data/documents/SPICE-UIO-DPDD-0002-1.4-Data_Product_Description_Document.pdf|DPDD]] - search for "Solar ephemeris keywords"​.+The full list of keywords is given in the [[https://​spice-wiki.ias.u-psud.fr/​lib/exe/fetch.php/​public:​spice-uio-dpdd-0002-1.8-data_product_description_document_spicefits_.pdf|DPDD]] - search for "Solar ephemeris keywords"​.
  
 Users should make sure to correct the SPICE observing times for EAR\_TDEL in order to compare with observations from Earth-orbiting spacecraft. This is especially important for highly-dynamic structures such as flares or CMEs. Users should make sure to correct the SPICE observing times for EAR\_TDEL in order to compare with observations from Earth-orbiting spacecraft. This is especially important for highly-dynamic structures such as flares or CMEs.
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 ==== Units and uncertainties ==== ==== Units and uncertainties ====
  
-The data cube (returned by the SSW object method ''​get\_window\_data''​ or by the Python ''​astropy''​ or ''​sunraster''​ libraries) of the SPICE level-2 files contains spectral radiances in units of W/m²/s/sr/nm. The wavelength vector has units of nm. To convert a radiance in W/m²/s/sr to erg/​cm²/​s/​sr,​ it is necessary to multiply by 1000.+The data cube (returned by the SSW object method ''​get\_window\_data''​ or by the Python ''​astropy''​ or ''​sunraster''​ libraries) of the SPICE level-2 files contains spectral radiances in units of W/​m²/​sr/​nm. The wavelength vector has units of nm. To convert a radiance in W/m²/sr to erg/​cm²/​s/​sr,​ it is necessary to multiply by 1000.
  
 Uncertainties on the spectral radiances can be obtained with: Uncertainties on the spectral radiances can be obtained with:
data/data_analysis_manual.txt · Last modified: 2024/03/29 14:21 by eric buchlin