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1) F10.7 Solar Radio Flux maxmize
Resource ID:spase://VSPO/NumericalData/DRAO/Solar.Radio.Flux/P1D
Start:1947-02-14 00:00:00 Observatory: Cadence:1 day
Stop:2016-09-14 08:00:05 Instrument: Resource:NumericalData
F10.7 cm (2800 MHz) solar radio flux observed at Ottowa (1947-1991) and now at Dominion Radio Astrophysical Observatory, Solar Radio Monitoring Program, National Research Council, Canada. Three flux measurements daily; cf. J. Geophys. Res., v. 92, p. 829, 1987

2) GOES X-ray Flux Plots maxmize
Resource ID:spase://VSPO/DisplayData/GOES/SXM/PLOTS
Start:2000-01-01 00:00:00 Observatory:GOES 8 Cadence:
Stop:2016-09-14 07:59:49 Instrument:GOES 8 Solar X-ray Monitor Resource:DisplayData
GOES X-ray plots from NOAA/SEC, 3-day plots of 5-min data

3) AGO P1 ICESTAR.Dayplot.Overview Dayplots maxmize
Resource ID:spase://VMO/DisplayData/ICESTAR/AGO.P1/ICESTAR.Dayplot.Overview/PT10S
Start:1996-01-01 00:00:00 Observatory:AGO P1 Cadence:10 seconds
Stop:2007-06-21 23:59:50 Instrument:AGO P1 Magnetometer Instrument Resource:DisplayData
AGO P1 ICESTAR.Dayplot.Overview Dayplots

4) AGO P2 ICESTAR.Dayplot.Overview Dayplots maxmize
Resource ID:spase://VMO/DisplayData/ICESTAR/AGO.P2/ICESTAR.Dayplot.Overview/PT10S
Start:1996-01-01 00:00:00 Observatory:AGO P2 Cadence:10 seconds
Stop:2007-06-21 23:59:50 Instrument:AGO P2 Magnetometer Instrument Resource:DisplayData
AGO P2 ICESTAR.Dayplot.Overview Dayplots

5) AGO P3 ICESTAR.Dayplot.Overview Dayplots maxmize
Resource ID:spase://VMO/DisplayData/ICESTAR/AGO.P3/ICESTAR.Dayplot.Overview/PT10S
Start:1996-01-01 00:00:00 Observatory:AGO P3 Cadence:10 seconds
Stop:1999-06-27 23:59:50 Instrument:AGO P3 Magnetometer Instrument Resource:DisplayData
AGO P3 ICESTAR.Dayplot.Overview Dayplots

6) AGO P4 ICESTAR.Dayplot.Overview Dayplots maxmize
Resource ID:spase://VMO/DisplayData/ICESTAR/AGO.P4/ICESTAR.Dayplot.Overview/PT10S
Start:1996-01-01 00:00:00 Observatory:AGO P4 Cadence:10 seconds
Stop:1998-12-01 23:59:50 Instrument:AGO P4 Magnetometer Instrument Resource:DisplayData
AGO P4 ICESTAR.Dayplot.Overview Dayplots

7) AGO P5 ICESTAR.Dayplot.Overview Dayplots maxmize
Resource ID:spase://VMO/DisplayData/ICESTAR/AGO.P5/ICESTAR.Dayplot.Overview/PT10S
Start:1997-01-01 00:00:00 Observatory:AGO P5 Cadence:10 seconds
Stop:2007-04-24 23:59:50 Instrument:AGO P5 Magnetometer Instrument Resource:DisplayData
AGO P5 ICESTAR.Dayplot.Overview Dayplots

8) AGO P6 ICESTAR.Dayplot.Overview Dayplots maxmize
Resource ID:spase://VMO/DisplayData/ICESTAR/AGO.P6/ICESTAR.Dayplot.Overview/PT10S
Start:1997-02-09 00:00:00 Observatory:AGO P6 Cadence:10 seconds
Stop:1999-03-13 23:59:50 Instrument:AGO P6 Magnetometer Instrument Resource:DisplayData
AGO P6 ICESTAR.Dayplot.Overview Dayplots

9) McMurdo ICESTAR.Dayplot.Overview Dayplots maxmize
Resource ID:spase://VMO/DisplayData/ICESTAR/McMurdo/ICESTAR.Dayplot.Overview/PT10S
Start:1995-11-29 00:00:00 Observatory:McMurdo Cadence:10 seconds
Stop:2007-06-21 23:59:50 Instrument:McMurdo Magnetometer Instrument Resource:DisplayData
McMurdo ICESTAR.Dayplot.Overview Dayplots

10) McMurdo Photometer PT10S Data maxmize
Resource ID:spase://VMO/NumericalData/ICESTAR/McMurdo/Photometer/PT10S
Start:2003-04-10 00:00:00 Observatory:McMurdo Cadence:10 seconds
Stop:2006-07-18 23:59:50 Instrument:McMurdo Photometer Instrument Resource:NumericalData
McMurdo Photometer PT10S data; Station Id: MCM; ICESTAR Channels (15) 630 nm and (16) 427.8 nm photometer levels both expressed in units of KiloRaylieghs (kR).

11) South Pole ICESTAR.Dayplot.Overview Dayplots maxmize
Resource ID:spase://VMO/DisplayData/ICESTAR/South.Pole/ICESTAR.Dayplot.Overview/PT10S
Start:1986-01-01 00:00:00 Observatory:South Pole Cadence:10 seconds
Stop:2007-06-21 23:59:50 Instrument:South Pole Magnetometer Instrument Resource:DisplayData
South Pole ICESTAR.Dayplot.Overview Dayplots

12) South Pole Photometer PT10S Data maxmize
Resource ID:spase://VMO/NumericalData/ICESTAR/South.Pole/Photometer/PT10S
Start:2003-04-10 00:00:00 Observatory:South Pole Cadence:10 seconds
Stop:2006-07-18 23:59:50 Instrument:South Pole Photometer Instrument Resource:NumericalData
South Pole Photometer PT10S data; Station Id: SPA; ICESTAR Channels (15) 630 nm and (16) 427.8 nm photometer levels both expressed in units of KiloRaylieghs (kR).

13) LISIRD supplied Composite Lyman Alpha maxmize
Resource ID:spase://VSPO/NumericalData/LASP/LISIRD/Composite/Lyman.Alpha/P1D
Start:1947-01-01 00:00:00 Observatory:SORCE Cadence:1 day
Stop:2016-09-14 08:00:05 Instrument:Solar Stellar Irradiance Comparison Experiment (SOLSTICE) Resource:NumericalData
This data product contains daily irradiance levels (photons/s/cm**2) of solar Lyman alpha (121.5 nm) radiation from multiple spacecraft and modelling sources, including AE-E/ESUM, SME/SUVM, UARS/SOLSTICE, TIMED/SEE and SORCE/SOLSTICE spacecraft and F10.7 and Mg models. Data are available from 1947 to near-current, both graphically and, in txt/csv format, digitally, from the LISIRD interface at U.Colorado/LASP.

14) LISIRD supplied Composite Solar Spectral Irradiance maxmize
Resource ID:spase://VSPO/NumericalData/LASP/LISIRD/Composite/Solar.Spectra.Irradiance/P1D
Start:1978-11-08 00:00:00 Observatory:NOAA 9 Cadence:1 day
Stop:2005-08-01 00:00:00 Instrument:SBUV/2 Resource:NumericalData
This data product contains daily-averaged solar spectra over the UV range 120-400 nm in 1 nm bins from multiple spacecraft, including SME, Nimbus 7 SBUV, NOAA 9 and 11 SBUV/2, UARS SUSIM and UARS SOLSTICE. Data are available from 1978-Nov-08 to 2005-Aug-01. Data include irradiances and their absolute and long-term uncertainties. Data are available both as a zipped text data file and as an IDL save file via LISIRD at LASP. The data set was created by Matthew DeLand of SSAI.

15) Proba 2 LYRA List of Solar Flares maxmize
Resource ID:spase://VSPO/NumericalData/PROBA2/LYRA/Flarelist/PT24H
Start:2010-01-06 00:00:00 Observatory:PROBA2 Cadence:24 hours
Stop:2016-09-14 07:59:51 Instrument:Proba 2 Sun Watcher using APS detectors and Image Processing (SWAP) Resource:NumericalData
This dataset contains daily lists of solar flares observed by the Large Yield RAdiometer (LYRA) onboard Proba 2. The lists recorded the begin, peak, and end time of each flare (1-minute averages), its class of intensity, and the region. The purpose of the list is to get an overview of the flares that LYRA observes and relate them to class, begin, max, etc. according to GOES. Besides listing the values in ASCII format, each file also provides a plot.

16) Proba 2 LYRA Raw Time Series maxmize
Resource ID:spase://VSPO/NumericalData/PROBA2/LYRA/Level_1/PT24H
Start:2011-11-30 00:00:00 Observatory:PROBA2 Cadence:24 hours
Stop:2016-09-14 07:59:51 Instrument:Proba 2 Sun Watcher using APS detectors and Image Processing (SWAP) Resource:NumericalData
This dataset contains level 1 times series from the Large Yield RAdiometer (LYRA) onboard Proba 2. It comprises a set of metadata and uncalibrated daily solar irradiance measured in four selected ultraviolet bands: the Lyman-alpha line at 121.6 nm, the 200-220 nm Herzberg continuum range, the 17-80 nm aluminium filter range and the 6-20 nm zirconium filter range. The data are in FITS format.

17) Proba 2 LYRA Calibrated Time Series maxmize
Resource ID:spase://VSPO/NumericalData/PROBA2/LYRA/Level_2/PT24H
Start:2010-01-06 00:00:00 Observatory:PROBA2 Cadence:24 hours
Stop:2016-09-14 07:59:51 Instrument:Proba 2 Sun Watcher using APS detectors and Image Processing (SWAP) Resource:NumericalData
This dataset contains level 2 calibrated times series from the Large Yield RAdiometer (LYRA) onboard Proba 2. It comprises a set of metadata and calibrated daily solar irradiance measured in four selected ultraviolet bands: the Lyman-alpha line at 121.6 nm, the 200-220 nm Herzberg continuum range, the 17-80 nm aluminium filter range and the 6-20 nm zirconium filter range. The data are in FITS format.

18) Proba 2 LYRA Level 3 Calibrated Time Series maxmize
Resource ID:spase://VSPO/NumericalData/PROBA2/LYRA/Level_3/PT60S
Start:2010-01-06 00:00:00 Observatory:PROBA2 Cadence:60 seconds
Stop:2016-09-14 07:59:51 Instrument:Proba 2 Sun Watcher using APS detectors and Image Processing (SWAP) Resource:NumericalData
This dataset contains level 3 calibrated times series from the Large Yield RAdiometer (LYRA) onboard Proba 2 that are averaged to the minute. It comprises a set of metadata and calibrated solar irradiance measured in four selected ultraviolet bands: the Lyman-alpha line at 121.6 nm, the 200-220 nm Herzberg continuum range, the 17-80 nm aluminium filter range and the 6-20 nm zirconium filter range. The data are in FITS format.

19) Proba 2 LYRA Daily PNG Files of Calibrated Time Series maxmize
Resource ID:spase://VSPO/DisplayData/PROBA2/LYRA/Level_4/PT24H
Start:2010-01-15 00:00:00 Observatory:PROBA2 Cadence:24 hours
Stop:2016-09-14 07:59:48 Instrument:Proba 2 Sun Watcher using APS detectors and Image Processing (SWAP) Resource:DisplayData
This dataset contains daily PNG files of calibrated time series from the Large Yield RAdiometer (LYRA) onboard Proba 2. Data are averaged to one minute. Time series of solar irradiance are displayed in all four ultraviolet channels: the Lyman-alpha line at 121.6 nm, the 200-220 nm Herzberg continuum range, the 17-80 nm aluminium filter range and the 6-20 nm zirconium filter range.

20) Proba 2 LYRA 3-Day PNG Files of Calibrated Time Series maxmize
Resource ID:spase://VSPO/DisplayData/PROBA2/LYRA/Level_4B/PT72H
Start:2010-01-15 00:00:00 Observatory:PROBA2 Cadence:72 hours
Stop:2016-09-14 07:59:48 Instrument:Proba 2 Sun Watcher using APS detectors and Image Processing (SWAP) Resource:DisplayData
This dataset contains 3-day calibrated quicklook PNG files of calibrated time series from the Large Yield RAdiometer (LYRA) onboard Proba 2. Data are averaged to one minute. Time series of solar irradiance are displayed in two of the ultraviolet channels: the 17-80 nm aluminium filter range and the 6-20 nm zirconium filter range.

21) SDO/EVE Data Products at LASP/U.Colo maxmize
Resource ID:spase://VSPO/NumericalData/SDO/EVE/PT10S
Start:2010-05-20 00:00:00 Observatory:SDO Cadence:10 seconds
Stop:2016-09-13 08:00:05 Instrument:EVE Resource:NumericalData
The EVE (Extreme Ultraviolet Variability Experiment) Principal Investigator site at U. Colorado's Laboratory for Atmospheric and Space Physics (LASP) archives, and provides multiple access paths to, a variety of SDO(Solar Dynamics Observatory)/EVE digital and display solar images, as well as to tools for selecting and analyzing data. Data include Ka band and S band irradiances, and spectra, at various calibration levels and at product-dependent time resolutions ranging between 0.25s and 1 min.

22) SNOE Daily Integrated Values of 2 to 7 nm Solar Soft X-ray Irradiance maxmize
Resource ID:spase://VSPO/NumericalData/SNOE/SXP/2-7nm_Irradiance/PT1D
Start:1998-03-11 00:00:00 Observatory:Student Nitric Oxide Explorer (SNOE) Cadence:24 hours
Stop:2000-10-01 00:00:00 Instrument:SNOE Solar X-ray Photometer, 0.2-3.5A Resource:NumericalData
This data set was provided by the PI team and contains daily values of the integrated solar X-ray irradiance (2-7 nm) as measured by the SNOE Solar X-ray Photometer. The data cover the time period March 11, 1998 to October 1, 2000 and are given in ASCII format. Irradiances are given as measured at the spacecraft and adjusted to 1 A.U. Also included are the 10.7 cm solar radio flux (daily and 81-day average) measured at Ottawa, Canada and Lyman Alpha photon fluxes measured by the UARS SOLSTICE instrument.

23) SORCE 6-hr and 1-day Solar Spectral Irradiance maxmize
Resource ID:spase://VSPO/NumericalData/SORCE/SSI/PT6H
Start:2003-03-02 00:00:00 Observatory:SORCE Cadence:6 hours
Stop:2016-09-14 08:00:04 Instrument:Spectral Irradiance Monitor (SIM) Resource:NumericalData
SORCE 6-hour and daily Solar Spectral Irradiance data from SIM, SOLSTICE and XPS instruments, covering 1-34 nm (XPS) and 115-2000 nm

24) SORCE TIM 6-hr and 1-day Total Solar Irradiance maxmize
Resource ID:spase://VSPO/NumericalData/SORCE/TIM/PT6H
Start:2003-03-02 00:00:00 Observatory:SORCE Cadence:6 hours
Stop:2016-09-14 08:00:04 Instrument:Total Irradiation Monitor (TIM) Resource:NumericalData
SORCE TIM 6-hour and daily Total Solar Irradiance Data

25) TIMED SEE Level2A EGS Solar Irradiance Data maxmize
Resource ID:spase://VITMO/NumericalData/TIMED/SEE/L2A_EGS
Start:2002-02-08 00:00:00 Observatory:TIMED Cadence:
Stop:2016-09-12 07:58:11 Instrument:Solar EUV Experiment (SEE) Resource:NumericalData
The EUV Grating Spectrograph (EGS) aboard SEE performs measurements of the Sun for about 3 minutes every orbit (97 minutes) which usually gives 14-15 measurements per day. The Level 2A data is time averaged over each measurement, after being 1-AU corrected and removing flares. The 1-AU correction is provided.

26) TIMED SEE Level2A XPS Solar Irradiance Data maxmize
Resource ID:spase://VITMO/NumericalData/TIMED/SEE/L2A_XPS
Start:2002-01-22 00:00:00 Observatory:TIMED Cadence:
Stop:2016-09-12 07:58:11 Instrument:Solar EUV Experiment (SEE) Resource:NumericalData
The 12 X-Ray Photometers (XP) aboard SEE perform full-disk irradiance measurements of the Sun for about 3 minutes every orbit (97 minutes) which usually gives 14-15 measurements per day. 8 of the XPs produce XUV signals (more info on XP coatings) and one other XP provides a hydrogen Lyman-alpha measurement (121.5 nm). The XPS Level 2A data is time averaged over each measurement, after being 1-AU corrected and removing flares. The 1-AU correction is provided.

27) TIMED SEE Level2B EGS Occultations Data maxmize
Resource ID:spase://VITMO/NumericalData/TIMED/SEE/L2B_EGS
Start:2002-04-25 00:00:00 Observatory:TIMED Cadence:
Stop:2014-09-14 07:58:11 Instrument:Solar EUV Experiment (SEE) Resource:NumericalData
The EUV Grating Spectrograph (EGS) aboard SEE performs measurements of the Sun for about 3 minutes every orbit (97 minutes) which usually gives 14-15 measurements per day. 4x per year, in-between direct solar measurements, the SEE instrument has opportunities to observe the solar irradiance transmitted through the atmosphere. The Level 2B EGS Occultation data is time averaged over each measurement and divided by the average of the previous and next solar observations. The EGS resolution is about 0.4 nm, but the data product is sampled at 0.1 nm with valid data ranging from ~27-190 nm.

28) TIMED SEE Level2 EGS Solar Irradiance Data maxmize
Resource ID:spase://VITMO/NumericalData/TIMED/SEE/L2_EGS
Start:2002-02-08 00:00:00 Observatory:TIMED Cadence:
Stop:2016-09-12 07:58:11 Instrument:Solar EUV Experiment (SEE) Resource:NumericalData
The EUV Grating Spectrograph (EGS) aboard SEE performs measurements of the Sun for about 3 minutes every orbit (97 minutes) which usually gives 14-15 measurements per day. The Level 2 data is time averaged over the entire day, after being 1-AU corrected and removing flares. The 1-AU correction is provided.

29) TIMED SEE Level2 XPS Solar Irradiance Data maxmize
Resource ID:spase://VITMO/NumericalData/TIMED/SEE/L2_XPS
Start:2002-01-22 00:00:00 Observatory:TIMED Cadence:
Stop:2016-09-12 07:58:11 Instrument:Solar EUV Experiment (SEE) Resource:NumericalData
The 12 X-Ray Photometers (XP) aboard SEE perform full-disk irradiance measurements of the Sun for about 3 minutes every orbit (97 minutes) which usually gives 14-15 measurements per day. 8 of the XPs produce XUV signals (more info on XP coatings) and one other XP provides a hydrogen Lyman-alpha measurement (121.5 nm). The XPS Level 2 data is time averaged over the entire day, after being 1-AU corrected and removing flares. The 1-AU correction is provided.

30) TIMED SEE Level 3 Solar Irradiance Data maxmize
Resource ID:spase://VITMO/NumericalData/TIMED/SEE/L3
Start:2002-01-22 00:00:00 Observatory:TIMED Cadence:
Stop:2016-09-12 07:58:11 Instrument:Solar EUV Experiment (SEE) Resource:NumericalData
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.

31) TIMED SEE Level 3A Solar Irradiance Data maxmize
Resource ID:spase://VITMO/NumericalData/TIMED/SEE/L3A
Start:2002-01-22 00:00:00 Observatory:TIMED Cadence:
Stop:2016-09-12 07:58:11 Instrument:Solar EUV Experiment (SEE) Resource:NumericalData
SEE Level 3A data files contain each measurements averaged solar irradiance spectrum in 1 nm intervals extracted from the EGS Level 2A and XPS Level 2A data products. Shortward of 27 nm, a solar model is scaled to match the XPS broadband data. SEE Level 3A data files also contain 38 emission lines extracted from EGS Level 2A spectra, and the XPS Level 2A 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 3A data are time averaged over each measurement, after applying corrections for atmospheric absorption, degradation, flare removal, and to 1-AU.

32) TIMED SEE Level 4 XPS Modeled Solar Irradiance Data maxmize
Resource ID:spase://VITMO/NumericalData/TIMED/SEE/L4_XSP
Start:2002-01-22 00:00:00 Observatory:TIMED Cadence:
Stop:2016-09-12 07:58:11 Instrument:Solar EUV Experiment (SEE) Resource:NumericalData
The SEE XPS Level 4 data are derived from the XPS Level 1 data products. The XPS Level 4 processing algorithm uses reference CHIANTI spectral models to generate a higher spectral resolution (0.1 nm) estimate of the solar XUV irradiance by scaling the model reference spectra to match the XPS photometer currents (signal). The CHIANTI Quiet Sun (QS) spectrum and Active Region (AR) spectrum are used with a scaling of the AR spectrum to match the minimum signal on each day, and then a CHIANTI isothermal flare spectrum is scaled to match the signal above the daily minimum signal. The flare temperature is determined from the ratio of the GOES XRS 0.1-0.8 nm irradiance to the GOES XRS 0.05-0.4 nm irradiance. These scaling factors, flare temperature, and resulting model spectrum in the 0-40 nm range in 0.1 nm intervals are in the XPS Level 4 data product for every measurement made by XPS photometer #1 or #2 (0.1-7 nm band). A SEE XPS Level 4 data product is produced for each UT day, and these daily products are also merged into three different full mission data files: daily averages (24-hour) orbit averages (3-min about every 97 min) 1-minute averages (but with only about 3% duty cycle) The XPS Level 4 result in 0.1 nm intervals is also compressed into 1-nm intervals for use in the SEE Level 3 and Level 3A data products. On-orbit instrument characterization is an ongoing effort, and the SEE team checks photometer degradation using redundant channels and underflight calibration rockets whose payload includes TIMED SEE prototype instruments. The accuracy of the XPS Level 1 irradiance is 12%-26%, photometer dependent. There is additional uncertainty for applying the spectral model for the XPS Level 4 irradiances, and this estimated accuracy is 30% for the integrated XUV irradiance. The spectral distribution in the XPS Level 4 is from the CHIANTI model and not from direct measurements from XPS, a set of broadband photometers. The spectral distribution above 27 nm has been validated with the TIMED SEE EGS (27-190 nm, 0.4 nm resolution) measurements, so there is good confidence in the spectral distribution shortward of 27 nm.

33) Ulysses GRB data via CDAWeb maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/SWICS/GSFC/SPDF/GRB/PT5M
Start:1990-11-10 00:02:30 Observatory:Ulysses Cadence:5 minutes
Stop:2006-12-31 00:00:00 Instrument:Solar Wind Ion Composition Spectrometer (GLG/SWICS) Resource:NumericalData
This data set from the Ulysses Gammay-Ray Bursts experiment contains 5-minute resolution filtered averages of cosmic gamma ray and solar X-Ray count rates. Count rate units are c/s. See Astron. Astrophys. Suppl. Ser., 92(2), 401-410, 1992 for more information.

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