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1) Solar Data at Meudon and Tarbes via BASS 2000 maxmize
Resource ID:spase://VSPO/NumericalData/BASS2000/SolarData
Start:1989-12-01 00:00:00 Observatory:Meudon Cadence:
Stop:2016-09-14 07:59:52 Instrument:Meudon Spectroheliograph Resource:NumericalData
Multiple solar data products held at Meudon and Tarbes sites in France, via the BASS (Base de donnees Solaire Sol) 2000 web site. Included are Nancay radioheliograph data, Meudon spectroheliograph data, THEMIS data and Pic du Mida coronagraph data

2) BBSO solar images maxmize
Resource ID:spase://VSPO/DisplayData/BBSO/IM
Start:1991-02-01 00:00:00 Observatory: Cadence:
Stop:2016-09-14 07:59:49 Instrument: Resource:DisplayData
Big Bear Solar Observatory (BBSO) solar images of the following types or sources: broadband, Calcium II K line, Dopplergram, H alpha, Vectomagnetogram components I, Q, U and V, white light, He I line (10830 A), He I D3 line (5876 A o), He I D3 line (5876 A), Ca I line (6103 A), IR camera

3) CALLISTO Solar Spectrogram FITS files maxmize
Resource ID:spase://VWO/NumericalData/CALLISTO/FAS.PT0.25S
Start:2002-09-07 12:08:00 Observatory: Cadence:
Stop:2016-09-14 08:00:15 Instrument: Resource:NumericalData
This dataset contains solar dynamic spectrogram FITS files of the CALLISTO spectrometer data from the e-Callisto network of stations. The FITS file is composed of four parts: the ASCII-format header, the binary spectrum and two BIN tables. One table is for the time axis and the other for the frequency axis. FITSvfiles contain the keyword BUNIT in the primary header. If the BUNIT = 'SFU', then data are calibrated. If the BUNIT = 'digits', then data are raw data without any calibration. The naming convention for each file is of the form: STATION_YYYYMMDD_HHMMSS_CODE.fit.gz where STATION is a variable length station name and following the Date (YYYYMMDD) and UT time (HHMMSS) CODE is a two digit number that is an individual description of the front-end of the system. From the website http://e-callisto.org - The CALLISTO spectrometer is a programmable heterodyne receiver built in the framework of IHY2007 and ISWI by former Radio and Plasma Physics Group (PI Christian Monstein) at ETH Zurich, Switzerland. The main applications are observation of solar radio bursts and rfi-monitoring for astronomical science, education and outreach. The instrument natively operates between 45 and 870 MHz using a modern, commercially available broadband cable-TV tuner CD1316 having a frequency resolution of 62.5 KHz. The data obtained from CALLISTO are FIT-files with up to 400 frequencies per sweep. The data are transferred via a RS-232 cable to a computer and saved locally. Time resolution is 0.25 sec at 200 channels per spectrum (800 pixels per second). The integration time is 1 msec and the radiometric bandwidth is about 300 KHz. The overall dynamic range is larger than 50 dB. For convenient data handling several IDL- and Python-routines were written. Many CALLISTO instruments have already been deployed, including: 5 spectrometers in India (2 in Ooty, 1 in Gauribidanur, 1 in Pune, 1 in Ahmedabad), one in Badary near Irkutsk, Russian Federation, two in South Korea, three in Australia (Perth, Melbourne and Heathcote), two in Hawaii, two in Mexico, one in Costa Rica, two in Brazil, three in Mauritius, four in Ireland, one in Czech Republic, two in Mongolia, four in Germany, two in Alaska, two in Kazakhstan, one in Cairo, one in Nairobi, one in Sri Lanka, three in Trieste, one in Hurbanovo/Slovakia, two in Belgium, two in Finland, 8 in Switzerland, one in Sardinia, two in Spain, 5 in Malaysia, two in Indonesia, one in Scotland/UK one in Roztoky/Slovakia, one in Peru, one in Rwanda, one in Pakistan, one in Denmark, one in Japan and one in South Africa. Through the IHY/UNBSSI and ISWI instrument deployment program, CALLISTO is able to continuously observe the solar radio spectrum for 24h per day through all the year. All Callisto spectrometers together form the e-Callisto network. Callisto in addition is dedicated to do radio-monitoring within its frequency range with 13,200 channels per spectrum. The frequency range can be expanded to any range by switching-in a heterodyne up- or a down-converter. Instrument deployment including education and training of observers was financially supported by SNF, SSAA, NASA, Institute for Astronomy and North-South Center of ETH Zurich and a few private sponsors.

4) CCMC: Solar Model Results maxmize
Resource ID:spase://VSPO/NumericalData/CCMC/Solar-Model/Results
Start: Observatory: Cadence:
Stop: Instrument: Resource:NumericalData
Results of runs of solar models (MAS, PFSS) at CCMC

5) CORONAS-F Full Sun XUV Spectroscopy Imaging (SPIRIT) Data maxmize
Resource ID:spase://VSPO/NumericalData/CORONAS-F/SPIRIT/PT5M
Start:2001-07-01 00:00:00 Observatory:CORONAS-F Cadence:5 minutes
Stop:2004-12-31 23:59:00 Instrument:Full Sun XUV Spectroscopy Imaging (SPIRIT) Resource:NumericalData
Data from the Full Sun XUV Spectroscopy Imaging (SPIRIT) onboard CORONAS-F.

6) Callisto Quicklook Solar Spectrogram Plots maxmize
Resource ID:spase://VWO/DisplayData/Callisto/FAS.PT15M
Start:2002-09-07 12:08:00 Observatory: Cadence:
Stop:2016-09-14 08:00:14 Instrument: Resource:DisplayData
This dataset contains solar dynamic spectrogram PNG plots of the Callisto spectrometer data from the e-Callisto network of stations. Each plot spans 15 minutes. The naming convention for each file is of the form: STATION_YYYYMMDD_HHMMSS_CODE.fit.gz.png where STATION is a variable length station name and following the Date (YYYYMMDD) and UT time (HHMMSS) CODE is a two digit number that is an individual description of the front-end of the system. From the website http://e-callisto.org - The CALLISTO spectrometer is a programmable heterodyne receiver built in the framework of IHY2007 and ISWI by former Radio and Plasma Physics Group (PI Christian Monstein) at ETH Zurich, Switzerland. The main applications are observation of solar radio bursts and rfi-monitoring for astronomical science, education and outreach. The instrument natively operates between 45 and 870 MHz using a modern, commercially available broadband cable-TV tuner CD1316 having a frequency resolution of 62.5 KHz. The data obtained from CALLISTO are FIT-files with up to 400 frequencies per sweep. The data are transferred via a RS-232 cable to a computer and saved locally. Time resolution is 0.25 sec at 200 channels per spectrum (800 pixels per second). The integration time is 1 msec and the radiometric bandwidth is about 300 KHz. The overall dynamic range is larger than 50 dB. For convenient data handling several IDL- and Python-routines were written. Many CALLISTO instruments have already been deployed, including: 5 spectrometers in India (2 in Ooty, 1 in Gauribidanur, 1 in Pune, 1 in Ahmedabad), one in Badary near Irkutsk, Russian Federation, two in South Korea, three in Australia (Perth, Melbourne and Heathcote), two in Hawaii, two in Mexico, one in Costa Rica, two in Brazil, three in Mauritius, four in Ireland, one in Czech Republic, two in Mongolia, four in Germany, two in Alaska, two in Kazakhstan, one in Cairo, one in Nairobi, one in Sri Lanka, three in Trieste, one in Hurbanovo/Slovakia, two in Belgium, two in Finland, 8 in Switzerland, one in Sardinia, two in Spain, 5 in Malaysia, two in Indonesia, one in Scotland/UK one in Roztoky/Slovakia, one in Peru, one in Rwanda, one in Pakistan, one in Denmark, one in Japan and one in South Africa. Through the IHY/UNBSSI and ISWI instrument deployment program, CALLISTO is able to continuously observe the solar radio spectrum for 24h per day through all the year. All Callisto spectrometers together form the e-Callisto network. Callisto in addition is dedicated to do radio-monitoring within its frequency range with 13,200 channels per spectrum. The frequency range can be expanded to any range by switching-in a heterodyne up- or a down-converter. Instrument deployment including education and training of observers was financially supported by SNF, SSAA, NASA, Institute for Astronomy and North-South Center of ETH Zurich and a few private sponsors.

7) SMEI Imagery of CME's maxmize
Resource ID:spase://VSPO/DisplayData/Coriolis/SMEI/IMAGES
Start:2003-03-31 00:00:00 Observatory:Coriolis Cadence:
Stop:2016-09-14 07:59:48 Instrument:Solar Mass Ejection Imager (SMEI) Resource:DisplayData
Images and movies from the Solar Mass Ejection Imager (SMEI) flown on the USAF Coriolis spacecraft

8) Australian Space Weather Services Culgoora Observatory Spectrograms maxmize
Resource ID:spase://VWO/DisplayData/Culgoora/DS.GIF.PT12H
Start:1992-11-14 20:12:33 Observatory:Culgoora Cadence:
Stop:2016-09-14 08:00:14 Instrument:Culgoora Solar Radiospectrograph Resource:DisplayData
Culgoora and Learmonth Observatories dynamic spectrogram plots display frequency in MHz on the vertical axis and time in UT on the horizontal axis. Each plot spans local daylight hours with time resolution of 3 seconds. The frequency range is 18 - 1800 MHz for Culgoora spectrogams and 25 - 180 MHz for Learmonth spectrograms. The intensity values are color coded and are expressed as relative logarithmic units (0 to 255). The Culgoora spectrograms consist of 4 frequency bands: 18-57, 57-180, 180-570 570 -1800 MHz and Learmonth has 2 bands: 25-75, 75-180 MHz. The two Learmonth bands are each divided into 400 frequency steps. Culgoora spectrograph data is available since November 1992, Learmonth data since June 2000.

9) 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

10) Evans Solar Facility Spectroheliographs maxmize
Resource ID:spase://VSPO/NumericalData/EvansSolarFacility/Spectroheliograph/PT86400S
Start:1996-02-05 00:00:00 Observatory:Evans Solar Facility Cadence:86400 seconds
Stop:1999-05-28 00:00:00 Instrument:Evans Solar Facility (ESF) Spectroheliograph Resource:NumericalData
Daily Solar Full Disk Spectroheliographs at 6563A and 3934A taken at John W. Evans Solar Facility

11) GOES SXI Solar X-Ray Images maxmize
Resource ID:spase://VSPO/NumericalData/GOES/12/SXI/PT60.00S
Start:2001-08-16 00:00:00 Observatory:GOES 12 Cadence:60.00 seconds
Stop:2016-09-14 08:00:05 Instrument:GOES 12 Solar X-Ray Imager Resource:NumericalData
GOES SXI Solar X-Ray Images in FITS format

12) 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

13) GONG Solar Data from BBSO maxmize
Resource ID:spase://VSPO/NumericalData/Ground/BBSO/GONG/PT86400S
Start:2001-03-14 00:00:00 Observatory:BBSO Cadence:86400 seconds
Stop:2016-09-14 08:00:05 Instrument:Global Oscillation Network Group (GONG) at BBSO Resource:NumericalData
GONG (Global Oscillations Network Group) helioseismology data from Big Bear Solar Observatory, LOS_velocity and LOS_magnetic field data, 6768 A.

14) GONG Solar Data from Cerro Tololo maxmize
Resource ID:spase://VSPO/NumericalData/Ground/CTIO/GONG/PT86400S
Start:2001-04-20 00:00:00 Observatory:CTIO Cadence:86400 seconds
Stop:2016-09-14 08:00:05 Instrument:Global Oscillation Network Group (GONG) at CTIO Resource:NumericalData
GONG (Global Oscillations Network Group) helioseismology data from Cerro Tololo Observatory, LOS_velocity and LOS_magnetic field data, 6768 A.

15) GONG Solar Data from Learmonth maxmize
Resource ID:spase://VSPO/NumericalData/Ground/Learmonth/GONG/PT86400S
Start:2001-04-30 00:00:00 Observatory:Learmonth Cadence:86400 seconds
Stop:2016-09-14 08:00:05 Instrument:Global Oscillation Network Group (GONG) at Learmonth Resource:NumericalData
GONG (Global Oscillations Network Group) helioseismology data from Learmonth Observatory, LOS_velocity and LOS_magnetic field data, 6768 A.

16) Mauna Loa Solar Observatory ACOS/CHIP LOS_Velocity Images maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/ACOS/CHIP/LOS-Velocity.Images
Start:1996-04-20 00:00:00 Observatory:MLSO Cadence:
Stop:2016-09-14 08:00:05 Instrument:MLSO_ACOS Resource:NumericalData
Mauna Loa Solar Observatory (MLSO) solar line-of-sight velocity images (dopplergrams) and movies from the Chromospheric Helium Imaging Photometer (CHIP, 1083.0 nm) of the Advanced Coronal Observing System (ACOS). As of early 2005, VSO used 'chp' rather than 'CHIP'.

17) Mauna Loa Solar Observatory ACOS/CHIP Images maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/ACOS/CHIP/Solar.Images
Start:1996-04-20 00:00:00 Observatory:MLSO Cadence:
Stop:2016-09-14 08:00:05 Instrument:MLSO_ACOS Resource:NumericalData
Mauna Loa Solar Observatory (MLSO) solar images and movies from the Chromospheric Helium Imaging Photometer (CHIP, 1083.0 nm) of the Advanced Coronal Observing System (ACOS). As of early 2005, VSO used 'chp' rather than 'CHIP'.

18) Mauna Loa Solar Observatory ACOS/MK4 Images maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/ACOS/MK4/Solar.Images
Start:1998-10-01 00:00:00 Observatory:MLSO Cadence:
Stop:2016-09-14 08:00:05 Instrument:MLSO_ACOS Resource:NumericalData
Mauna Loa Solar Observatory (MLSO) solar coronal images and movies in white light polarization brightness from the Mark-IV (Mk4) instrument of the Advanced Coronal Observing System (ACOS)

19) Solar Imagery from Mauna Loa Solar Observatory at HAO maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/ACOS/Solar.Images
Start:1980-01-01 00:00:00 Observatory:MLSO Cadence:
Stop:2016-09-14 08:00:05 Instrument:MLSO_ACOS Resource:NumericalData
Mauna Loa Solar Observatory (MLSO) solar images and movies from the Advanced Coronal Observing System (ACOS), the Experiment for Coordinated Helioseismic Observations (ECHO) and the Precision Solar Photometric Telescope (PSPT). ACOS includes the Chromospheric Helium Imaging Photometer (CHIP, 1083.0 nm), H-alpha prominence and solar disk monitor (PICS, 656.2 nm), and the Mk4 K-coronameter (sees white light K-corona from 1.12 to 2.79 solar radii). ECHO observes oscillations in solar surface radial velocities. PSPT observes the solar disk in three bandpasses: 605-610 nm (red), 408-412 nm (blue) and 393 nm (Ca II K). Some MLSO data contribute to the GONG program.

20) GONG Solar Data from MLSO maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/GONG/PT86400S
Start:2001-06-16 00:00:00 Observatory:MLSO Cadence:86400 seconds
Stop:2016-09-14 08:00:05 Instrument:Global Oscillation Network Group (GONG) at MLSO Resource:NumericalData
GONG (Global Oscillations Network Group) helioseismology data from Mauna Loa Solar Observatory, LOS_velocity and LOS_magnetic field data, 6768 A.

21) GONG Solar Data from El Teide maxmize
Resource ID:spase://VSPO/NumericalData/Ground/TEIDE/GONG/PT86400S
Start:2001-07-30 00:00:00 Observatory:TEIDE Observatory Cadence:86400 seconds
Stop:2016-09-14 08:00:05 Instrument:Global Oscillation Network Group (GONG) at TEIDE Resource:NumericalData
GONG (Global Oscillations Network Group) helioseismology data from El Teide Observatory, LOS_velocity and LOS_magnetic field data, 6768 A.

22) GONG Solar Data from Udaipur maxmize
Resource ID:spase://VSPO/NumericalData/Ground/Udaipur/GONG/PT86400S
Start:2001-10-25 00:00:00 Observatory:Udaipur Cadence:86400 seconds
Stop:2016-09-14 08:00:05 Instrument:Global Oscillation Network Group (GONG) at Udaipur Resource:NumericalData
GONG (Global Oscillations Network Group) helioseismology data from Udaipur Observatory, LOS_velocity and LOS_magnetic field data, 6768 A.

23) Hinode data (all-inclusive) via Project Page or DARTS maxmize
Resource ID:spase://VSPO/NumericalData/Hinode/PT1M
Start:2006-10-01 00:00:00 Observatory:Hinode Cadence:1 minute
Stop:2016-09-14 08:00:04 Instrument:Solar Optical Telescope Resource:NumericalData
A wealth of Hinode movie, image and digital data are accessible via links from the NASA/MSFC Project web page and from the DARTS data archive in Japan. Data are from all three instruments, the Solar Optical Telescope (SOT), the X-Ray Telescope (XRT) and the EUV Imaging Spectrometer (EIS)

24) Solar Radio Spectrograms at Zurich maxmize
Resource ID:spase://VSPO/NumericalData/IA/Zurich/BENZ
Start:1978-05-29 00:00:00 Observatory: Cadence:
Stop:2016-09-14 07:59:49 Instrument: Resource:NumericalData
Solar radio spectrograms and other products at the Institute of Astronomy, ETH Zurich Switzerland

25) JSPO Solar Image Data maxmize
Resource ID:spase://VSPO/NumericalData/JSPO/MOTH/PT3600.00S
Start:2003-01-01 00:00:00 Observatory:JSPO Cadence:3600.00 seconds
Stop:2003-01-20 00:00:00 Instrument:MOTH Magneto Optical filters at Two Heights Resource:NumericalData
Jeffreys South Pole Observatory (JSPO) solar intensity and LOS_velocity data at 5890A and 7699A

26) KSO Ca II K Solar Images maxmize
Resource ID:spase://VSPO/DisplayData/KSO/KANZ/CaIIK
Start:2010-07-31 00:00:00 Observatory:KSO Cadence:
Stop:2016-09-14 07:59:48 Instrument:KANZ (VSO notation) Resource:NumericalData
Ca II K solar imagery from Kanzelhoehe Solar Observatory (KSO), Austria

27) KSO H-alpha Solar Images maxmize
Resource ID:spase://VSPO/DisplayData/KSO/KANZ/H-alpha
Start:2000-01-20 00:00:00 Observatory:KSO Cadence:
Stop:2016-09-14 07:59:48 Instrument:KANZ (VSO notation) Resource:NumericalData
H-alpha solar imagery from Kanzelhoehe Solar Observatory (KSO), Austria

28) KSO Whitelight Solar Images maxmize
Resource ID:spase://VSPO/DisplayData/KSO/KANZ/Whitelight
Start:2007-07-02 00:00:00 Observatory:KSO Cadence:
Stop:2016-09-14 07:59:48 Instrument:KANZ (VSO notation) Resource:NumericalData
Whitelight solar imagery from Kanzelhoehe Solar Observatory (KSO), Austria

29) KPVT 512-ch magnetograph solar intensity data maxmize
Resource ID:spase://VSPO/NumericalData/KittPeak/Magnetograph/INTENS/PT3600S
Start:1974-05-02 00:00:00 Observatory:Kitt Peak Cadence:3600 seconds
Stop:1993-02-03 00:00:00 Instrument:512-channel magnetograph Resource:NumericalData
Kitt Peak Vacuum Telescope (KPVT) 512-channel magnetograph solar visible and near-IR intensity data

30) KPVT 512-ch magnetograph LOS_magnetic field data maxmize
Resource ID:spase://VSPO/NumericalData/KittPeak/Magnetograph/LOSMAG/PT3600S
Start:1974-02-01 00:00:00 Observatory:Kitt Peak Cadence:3600 seconds
Stop:1993-04-10 00:00:00 Instrument:512-channel magnetograph Resource:NumericalData
Kitt Peak Vacuum Telescope (KPVT) 512-channel magnetograph solar near-IR LOS_magnetic field data

31) KPVT SPMG solar intensity data maxmize
Resource ID:spase://VSPO/NumericalData/KittPeak/Spectromagnetograph/INTENS/PT3600S
Start:1992-04-19 00:00:00 Observatory:Kitt Peak Cadence:3600 seconds
Stop:2003-02-22 00:00:00 Instrument:Spectromagnetograph Resource:NumericalData
Kitt Peak Vacuum Telescope (KPVT) spectromagnetograph (SPMG) visible and near-IR intensity data

32) KPVT SPMG LOS_magnetic field data maxmize
Resource ID:spase://VSPO/NumericalData/KittPeak/Spectromagnetograph/LOSMAG/PT3600S
Start:1992-04-21 00:00:00 Observatory:Kitt Peak Cadence:3600 seconds
Stop:2003-09-21 00:00:00 Instrument:Spectromagnetograph Resource:NumericalData
Kitt Peak Vacuum Telescope (KPVT) spectromagnetograph (SPMG) line-of-sight solar magnetic field data

33) NSO/KP Coronal Hole Maps maxmize
Resource ID:spase://VSPO/DisplayData/KittPeak/VacuumTelescope/P27D
Start:1989-09-12 00:00:00 Observatory:Kitt Peak Cadence:27 days
Stop:2002-03-30 00:00:00 Instrument:Kitt Peak Vacuum Telescope (KPVT) Resource:DisplayData
These are PDF files organized as one plot (one file) per 27.27 day Carrington rotation. The files are determined from 1083 nm He I observations made at Kitt Peak.

34) 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.

35) 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.

36) Australian Space Weather Services Learmonth Observatory Spectrograms maxmize
Resource ID:spase://VWO/DisplayData/Learmonth/DS.GIF.PT12H
Start:2000-06-16 05:00:00 Observatory:Learmonth Cadence:
Stop:2016-09-14 08:00:14 Instrument:Learmonth Solar Radiospectrograph Resource:DisplayData
Culgoora and Learmonth Observatories dynamic spectrogram plots display frequency in MHz on the vertical axis and time in UT on the horizontal axis. The time span for each plot varies, generally spanning local day time hours with time resolution of 3 seconds. The frequency range is 18 - 1800 MHz for Culgoora spectrogams and 25 - 180 MHz for Learmonth spectrograms. The intensity values are color coded and are expressed as relative logarithmic units (0 to 255). The Culgoora spectrograms consist of 4 frequency bands: 18-57, 57-180, 180-570 570 -1800 MHz and Learmonth has 2 bands: 25-75, 75-180 MHz. The two Learmonth bands are each divided into 400 frequency steps. Culgoora spectrograph data is available since November 1992, Learmonth data since June 2000.

37) Nobeyama Radioheliograph Images and Data maxmize
Resource ID:spase://VSPO/NumericalData/NOB_RH/NORH/PT60S
Start:1992-07-01 00:00:00 Observatory:NOB_RH Cadence:60 seconds
Stop:2016-09-14 07:59:51 Instrument:NORH Resource:NumericalData
Nobeyama Radioheliograph images, movies, data, several products, 17 and 34 GHz, polarization; resolutions between 1-min and 1 day

38) OAC H-alpha Solar Images maxmize
Resource ID:spase://VSPO/DisplayData/OAC/OACT/H-ALPHA
Start:2002-02-26 00:00:00 Observatory:OAC Cadence:
Stop:2016-09-14 07:59:49 Instrument:OACT (VSO notation) Resource:DisplayData
H-alpha solar imagery from Osservatorio Astrofisica di Catania (OAC), Sicily, Italy

39) OBSPM H-alpha Solar Images maxmize
Resource ID:spase://VSPO/DisplayData/OBSPM/H-ALPHA
Start:2004-10-22 00:00:00 Observatory:OBSPM Cadence:
Stop:2016-09-14 07:59:49 Instrument:OBSPM Heliograph Resource:DisplayData
H-alpha solar imagery from OBservatoire Solaire de Paris a Meudon (OBSPM)

40) PICARD SODISM Level 1 Data maxmize
Resource ID:spase://SMWG/NumericalData/PICARD/SODISM/Level1/PT1M
Start:2010-07-01 00:00:00 Observatory:PICARD Cadence:1 minute
Stop:2013-03-31 23:59:00 Instrument:SOlar Diameter Imager and Surface Mapper (SODISM) Resource:NumericalData
Solar images are available from the SOlar Diameter Imager and Surface Mapper (SODISM) onboard the Picard space mission from the middle ultraviolet to the near infrared in five narrow spectral bands centered at 215.0, 393.37, 535.7, 607.1, and 782.2 nm. Various products are available, including limb image for helioseismology (HL), macros pixel image for helioseismology (HMP), dark current - full image (CO), dark current - limb image (LCO), limb image for diameter (DL), solar rotation full image (RS), and stellar calibration (ES).

41) 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.

42) 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.

43) 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.

44) 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.

45) 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.

46) 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.

47) Proba 2 SWAP Daily Solar Average Intensities maxmize
Resource ID:spase://VSPO/NumericalData/PROBA2/SWAP/EUV/Avg_Intensities/PT24H
Start:2009-11-20 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 Proba 2 dataset contains daily intensities of the solar corona averaged over the SWAP (Sun Watcher using Active Pixel System detector and Image Processing) Field of View in calibrated images. Images are sampled near 17.4 nm every minute by the Extreme UltraViolet (EUV) imager, showing how the sun’s corona changes and evolves over time. Due to its large viewing angle, PROBA2 sees a region of the corona not seen by the other solar satellites, including the ESA/NASA Solar and Heliospheric Observatory (SOHO), and NASA's Solar Dynamics Observatory (SDO).

48) Proba 2 SWAP Daily Solar Movies maxmize
Resource ID:spase://VSPO/DisplayData/PROBA2/SWAP/EUV/Daily_Movies/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 Proba 2 SWAP (Sun Watcher using Active Pixel System detector and Image Processing) dataset contains daily movies of the solar corona. Images are sampled near 17.4 nm every minute by the Extreme UltraViolet (EUV) imager, showing how the sun’s corona changes and evolves over time. Due to its large viewing angle, PROBA2 sees a region of the corona not seen by the other solar satellites, including the ESA/NASA Solar and Heliospheric Observatory (SOHO), and NASA's Solar Dynamics Observatory (SDO).

49) Proba 2 SWAP Raw Solar Images maxmize
Resource ID:spase://VSPO/NumericalData/PROBA2/SWAP/EUV/Level_0/PT24H
Start:2009-11-30 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 Proba 2 SWAP (Sun Watcher using Active Pixel System detector and Image Processing) dataset contains level 0 raw data of the solar corona. Images are sampled near 17.4 nm every minute by the Extreme UltraViolet (EUV) imager, showing how the suns corona changes and evolves over time. Each LV0 FITS file contains an image in digital numbers (DN) and all the information that is required to analyze it, but at the same time it restricts this information to that subset which is stable over time and will not require reprocessing when a new understanding of the instrument performance becomes available.

50) Proba 2 SWAP Calibrated Solar EUV Images maxmize
Resource ID:spase://VSPO/NumericalData/PROBA2/SWAP/EUV/Level_1/PT1M
Start:2011-11-30 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 1 calibrated images from the Sun Watcher using Active Pixel System detector and Image Processing (SWAP) onboard Proba 2. Images of the solar corona are sampled near 17.4 nm every minute by the Extreme UltraViolet (EUV) imager and corrected for all known instrumental defects, with the image data in exposure-normalized units (DN/s/pixel). The resulting FITS file is the reference science product that does not require the user to use any proprietary software.

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