2.4.1 spase://CNES/NumericalData/CDPP-AMDA/TIMED/SEE/timed-see-l3 daily averages daily averages / level3 / flares excluded 2024-05-23T02:24:26Z SEE Level 3 OVERVIEW: The Solar EUV Experiment (SEE) is comprised of two science components: * the EUV Grating Spectrograph (EGS) component covers the wavelength range from approximately 26 to 190 nm * the X-Ray Photometer System (XPS) component covers the wavelength range from approximately 0.5 to 34 nm Level 3 data has flares removed, is useful for long-term climatological study. Users that wish to publish the results derived from TIMED data should normally offer co-authorship to the PI or his/her designated team member. Co-authorship may be declined. Appropriate acknowledgement to institutions, personnel, and funding agencies should be given. spase://CNES/Person/CDPP-AMDA/T.Woods PrincipalInvestigator Dataset description http://lasp.colorado.edu/data/timed_see/level3/README_SEE_L3_012.TXT timed-see-flux PartOf EUV / X ray spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi timed-see-l3 Web Service to this product using the HAPI interface. CSV Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers. spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA Web application https://amda.cdpp.eu Access to Data via CDPP/AMDA Web application. CSV VOTable CDF PNG Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers. http://lasp.colorado.edu/data level3 spase://CNES/Instrument/CDPP-AMDA/TIMED/SEE Irradiance 2002-01-22T12:00:00Z 2024-05-19T12:00:00Z PT24H Earth.NearSurface.Ionosphere SEE Level 3 data files contain one daily averaged solar irradiance spectrum in 1 nm intervals extracted from the EGS Level 2 and XPS Level 2 data products. Shortward of 27 nm, a solar model is scaled to match the XPS broadband data. SEE Level 3 data files also contain 38 emission lines extracted from EGS Level 2 spectra, and the XPS Level 2 diode irradiances. For normal operations, SEE observes the Sun for about 3 minutes every orbit (97 minutes), which usually gives 14-15 measurements per day. The SEE Level 3 data are time averaged over the entire day, after applying corrections for atmospheric absorption, degradation, flare removal, and to 1 AU. flux : spectra timed_sp_daily Merged median solar irradiance for XPS and EGS flux at 1nm bins W/m**2/nm Spectrogram -1 Photon EnergyFlux flux : lines timed_ln_daily Integrated median spectral line irradiance W/m**2/nm TimeSeries -1 Photon EnergyFlux