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1) AIM/CIPS noctilucent cloud images and movies, etc. maxmize
Resource ID:spase://VSPO/NumericalData/AIM/CIPS/PT90M
Start:2007-06-01 00:00:00 Observatory:AIM Cadence:90 minutes
Stop:2016-09-14 08:00:04 Instrument:AIM Cloud Imaging and Particle Size experiment Resource:NumericalData
AIM/CIPS (Cloud Imaging and Particle Size) data are available in multiple processing levels: 1a (calibrated and geolocated albedo); 1b (map- projected albedo at 5km x 5km resolution); 1c (same as 1b, but with Rayleigh scattering background subtracted); 2 (imagery for 15 orbit- specific strips per day, built from 1c data); 3a (daily "daisies" built as composites over level 2 data); 3b (seasonal movies built from level 3a data); 4 (cloud properties such as ice water content and particle radius extracted from lower level data). Data files for levels 2, 3a and 4 are accessible from http://aim.hamptonu.edu/sds/cal_index_aim.php?instrument=cips, with level 2 and 4 data as gzipped netCDF's and level 3a imagery in PNG format. Brief descriptions of data levels, browse imagery, and links to fuller data documentation files at LASP are available from http://aim.hamptonu.edu/library/documentation/instruments/cips/cips_docs.html Data are available over each polar region about 4 months each year, during that region's summer.(

2) Akebono ATV auroral images maxmize
Resource ID:spase://VSPO/DisplayData/Akebono/ATV/PT3H
Start:1989-04-12 00:00:00 Observatory:Akebono Cadence:3 hours
Stop:1990-02-28 00:00:00 Instrument:Akebono Auroral TV Imagery(ATV) Resource:NumericalData
These Akebono ATV auroral images are available at somewhat irregular time intervals. There are also a few brief movies of various types of auroral forms.

3) 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

4) 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

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) 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

7) DE 1 Spin-Scan Auroral Imager UV Images maxmize
Resource ID:spase://VSPO/NumericalData/DE1/SAI/PT3M
Start:1981-09-23 00:00:00 Observatory:Dynamics Explorer 1 Cadence:3 minutes
Stop:1991-02-18 00:00:00 Instrument:DE 1 Spin-Scan Auroral Imager Resource:NumericalData
This data set contains ultraviolet images in quasi-logarithmically compressed counts from the vacuum ultraviolet imaging photometer of the Spin-Scan Auroral Imager (SAI) flown on DE 1. The time resolution was 3 to 12 minutes per image. Also included are the GCI position vector, velocity vector and spin axis of the spacecraft. Data are available in CDF format from CDAWeb.

8) 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

9) 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

10) 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.

11) 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.

12) 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.

13) 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'.

14) 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)

15) Mauna Loa Solar Observatory PICS and DPM Images maxmize
Resource ID:spase://VSPO/NumericalData/Ground/MaunaLoaSO/ACOS/PICS-DPM/Solar.Images
Start:1994-02-02 00:00:00 Observatory:MLSO Cadence:
Stop:2016-09-14 08:00:05 Instrument:MLSO_ACOS Resource:NumericalData
Mauna Loa Solar Observatory (MLSO) H-alpha solar disk and limb images and movies from the Polarimeter for Inner Coronal Studies (PICS) and the Digital Prominence Monitor (DPM) that PICS replaced in September, 1997. PICS is part of the Advanced Coronal Observing System (ACOS). As of early 2005, VSO used 'dpm' for both DPM and PICS.

16) 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.

17) 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.

18) 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.

19) 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.

20) 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)

21) IMAGE EUV Key Parameters: Ion Images maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/EUV/PT600S
Start:2000-03-28 00:00:00 Observatory:IMAGE Cadence:
Stop:2005-12-18 00:00:00 Instrument:Extreme Ultraviolet Imager (EUV) Resource:DisplayData
IMAGE EUV Key Parameters, Ion Images, 10-min resolution

22) IMAGE FUV SI plots of O/N2 Ratios maxmize
Resource ID:spase://VEPO/DisplayData/IMAGE/FUV/SI/O_N2_Ratios
Start:2000-05-24 00:00:00 Observatory:IMAGE Cadence:2 minutes
Stop:2005-05-18 23:59:59 Instrument:Far Ultraviolet Imager (FUV) Resource:DisplayData
This data set consists of images of thermospheric O/N2 column density ratios at 2-min resolution during times of strong geomagnetic storms (Dst.LT.-80nT) of 2000-2005. The ratios are generated from dayside airglow observations of the IMAGE Far Ultraviolet (FUV) Spectrographic Imager (SI). The SI has a peak response at the OI 135.6 nm oxygen emission line and a bandpass of 131.0 to 140.0 nm which includes the LBH band from N2 molecules. For each O/N2 plot, there is a plot of the SI image from which the O/N2 plot was generated, and there is an IDL saveset of the content of the O/N2 maps. The Information URL of this descriptor identifies detailed discussions of the derivations of O/N2 rations from the SI images.

23) IMAGE FUV SI plots of O/N2 Ratios maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/FUV/SI/O_N2_Ratios
Start:2000-05-24 00:00:00 Observatory:IMAGE Cadence:2 minutes
Stop:2005-05-18 23:59:59 Instrument:Far Ultraviolet Imager (FUV) Resource:DisplayData
This data set consists of images of thermospheric O/N2 column density ratios at 2-min resolution during times of strong geomagnetic storms (Dst.LT.-80nT) of 2000-2005. The ratios are generated from dayside airglow observations of the IMAGE Far Ultraviolet (FUV) Spectrographic Imager (SI). The SI has a peak response at the OI 135.6 nm oxygen emission line and a bandpass of 131.0 to 140.0 nm which includes the LBH band from N2 molecules. For each O/N2 plot, there is a plot of the SI image from which the O/N2 plot was generated, and there is an IDL saveset of the content of the O/N2 maps. The Information URL of this descriptor identifies detailed discussions of the derivations of O/N2 rations from the SI images.

24) IMAGE FUV SIE Auroral Images, Key Parameters maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/FUV/SIE/PT124S
Start:2000-04-25 00:00:00 Observatory:IMAGE Cadence:
Stop:2005-12-18 00:00:00 Instrument:Far Ultraviolet Imager (FUV) Resource:DisplayData
Electron Auroral Images at 1356A, Key Parameters, IMAGE Far UltraViolet (FUV) Spectrographic Imaging camera Electrons (SIE)

25) IMAGE FUV SIP Auroral Images, Key Parameters maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/FUV/SIP/PT124S
Start:2000-04-25 00:00:00 Observatory:IMAGE Cadence:
Stop:2005-12-18 00:00:00 Instrument:Far Ultraviolet Imager (FUV) Resource:DisplayData
Proton Auroral Images at 1218A, Key Parameters, IMAGE Far UltraViolet (FUV) Spectrographic Imaging camera Protons (SIP)

26) IMAGE FUV WIC Auroral Images, Key Parameters maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/FUV/WIC/PT124S
Start:2000-04-25 00:00:00 Observatory:IMAGE Cadence:
Stop:2016-09-14 07:59:48 Instrument:Far Ultraviolet Imager (FUV) Resource:DisplayData
Auroral Images, Key Parameters, IMAGE Far UltraViolet (FUV) Wide-band Imaging Camera (WIC)

27) IMAGE FUV/WIC Auroral Images maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/FUV/WIC/PT6M
Start:2000-05-19 00:00:00 Observatory:IMAGE Cadence:6 minutes
Stop:2000-12-18 00:00:00 Instrument:Far Ultraviolet Imager (FUV) Resource:DisplayData
Auroral Images in GIF format from the Wideband Imaging Camera (WIC) of the Far Ultraviolet (FUV) experiment on IMAGE, at UCB

28) IMAGE HENA Images, Key Parameters maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/HENA/124S
Start:2000-04-21 00:00:00 Observatory:IMAGE Cadence:
Stop:2005-12-18 00:00:00 Instrument:High-Energy Neutral Atom Imager (HENA) Resource:DisplayData
IMAGE High Energy Neutral Atom (HENA) images for several energy channels <10 to 60 keV, key parameters,

29) IMAGE LENA Low Images, Key Parameters maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/LENA/PT124S
Start:2000-05-24 00:00:00 Observatory:IMAGE Cadence:
Stop:2005-12-18 23:59:59 Instrument:Low-Energy Neutral Atom Imager (LENA) Resource:DisplayData
This set of images from IMAGE Low-Energy Neutral Atom (LENA) contains key parameters for several energy channels from 20 to 200 keV.

30) IMAGE MENA Images, Key Parameters maxmize
Resource ID:spase://VSPO/DisplayData/IMAGE/MENA/PT124S
Start:2000-04-04 00:00:00 Observatory:IMAGE Cadence:
Stop:2005-12-18 23:59:59 Instrument:Medium-Energy Neutral Atom Imager (MENA) Resource:DisplayData
This set of images and movies from IMAGE Medium-Energy Neutral Atom (MENA) contains key parameters for several energy channels from 1 to 70 keV.

31) IRIS Calibrated Images and Spectra Data maxmize
Resource ID:spase://VSPO/NumericalData/IRIS/IRIS/PT1S
Start:2013-09-15 00:00:01 Observatory:Interface Region Imaging Spectrograph (IRIS) Cadence:1 second
Stop:2016-09-14 07:59:51 Instrument:Interface Region Imaging Spectrograph (IRIS) Resource:NumericalData
This data set contains calibrated level-2 images and spectra data from the Interface Region Imaging Spectrograph (IRIS). UV images from IRIS telesccope record observations of features as small as 240 km (150 miles) on the sun every five to ten seconds at specific temperatures, ranging from 5,000 K and 65,000 K (and up to 10 million K during solar flares). This range is tailored to observe material traveling on the surface of the sun, called the photosphere, and in the lowermost layers of the atmosphere, called the chromosphere and transition region. Spectra are obtained every one to two seconds along a slit (1/3 arcsec wide) of solar material at temperatures from 5,000 K to 10 million K, providing information on exactly how much light is visible from any specific wavelength. This corresponds to how much material is present at specific velociites, temperatures and densities. The level-2 data is corrected for dark current, flat-field, and geometric deformation, scaled to the same plate-scale, and packaged into timeseries of slitjaw images and spectral raster scans. The calibration is preliminary and will improve in the coming months.

32) 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

33) 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

34) 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

35) 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

36) 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

37) 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

38) 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

39) 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

40) 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)

41) 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).

42) Polar PIXIE Auroral X-ray Plots and Movies, CDAWeb maxmize
Resource ID:spase://VSPO/DisplayData/POLAR/PIXIE/CDAWEB
Start:1996-03-19 00:00:00 Observatory:POLAR Cadence:
Stop:2002-11-09 00:00:00 Instrument:Polar Ionospheric X-ray Imaging Experiment (PIXIE) Resource:DisplayData
Polar PIXIE Auroral X-Ray Plots and Movies, CDAWeb

43) Polar PIXIE Auroral X-ray Plots and Movies maxmize
Resource ID:spase://VSPO/DisplayData/POLAR/PIXIE/PT10M
Start:1996-03-19 00:00:00 Observatory:POLAR Cadence:10 minutes
Stop:2002-11-09 00:00:00 Instrument:Polar Ionospheric X-ray Imaging Experiment (PIXIE) Resource:DisplayData
Polar PIXIE Auroral X-Ray Plots and Movies

44) Polar PIXIE Level 1 Data Archive maxmize
Resource ID:spase://VSPO/NumericalData/POLAR/PIXIE/PT60.00S
Start:1996-03-15 00:00:00 Observatory:POLAR Cadence:60.00 seconds
Stop:2003-12-29 00:00:00 Instrument:Polar Ionospheric X-ray Imaging Experiment (PIXIE) Resource:NumericalData
Polar PIXIE Level 1 Auroral X-ray Data Archive in CDF Format

45) Polar Ultraviolet Imager H0 High-Resolution Images maxmize
Resource ID:spase://VSPO/DisplayData/POLAR/UVI/H0
Start:1996-03-23 15:56:15 Observatory:POLAR Cadence:
Stop:2008-02-10 18:40:28 Instrument:Ultraviolet Imager (UVI) Resource:DisplayData
This data set contains detected and produced images of the ultraviolet light of the aurora, day and night. from the Polar UltraViolet Imager (UVI) experiment.

46) Polar Ultraviolet Imager H1 High-Resolution Images maxmize
Resource ID:spase://VSPO/DisplayData/POLAR/UVI/H1
Start:1998-04-29 11:52:00 Observatory:POLAR Cadence:
Stop:1998-05-09 20:20:00 Instrument:Ultraviolet Imager (UVI) Resource:DisplayData
This dataset contains high resolution MPEG canned images of aurora and airglow from the Polar Ultraviolet Imager (UVI).

47) Polar Ultraviolet Imager, Key Parameters maxmize
Resource ID:spase://VMO/NumericalData/POLAR/UVI/K0_CDF
Start:1996-03-23 15:56:15 Observatory:POLAR Cadence:
Stop:2008-02-10 18:40:28 Instrument:Ultraviolet Imager (UVI) Resource:NumericalData
The Ultraviolet Imager (UVI) is a small camera that detected and produced images of the ultraviolet light of the aurora, day and night. Key Parameter (KP) images are calculated at nominal 5-10 minute intervals at spacecraft altitudes above 6 Re. The UVI KP image is background subtracted and calibrated to radiance values (photon cm^-2 cm^-1). The data is a rectangular two-dimensional array (228 rows x 200 columns). Only a circular region of the rectangular array contains valid image data. The UVI KP Image Archive (http://tideuvira.nsstc.nasa.gov/uvi/kpgs-Data.htm) allows the user to look at all the KP Mosaics for a selected month. The gif or png plot files contain the up to 35 KP images taken with the LBHL filter. Reference images are also provided showing the location of the UVI field of view relative to continental outlines.

48) Polar VIS Images from CDAWeb maxmize
Resource ID:spase://VSPO/DisplayData/POLAR/VIS/EJ
Start:1996-06-17 00:00:00 Observatory:POLAR Cadence:
Stop:2000-07-16 00:00:00 Instrument:Visible Imaging System (VIS) Resource:DisplayData
Polar VIS Images from CDAWeb

49) Polar Visible Imaging System 24-sec Key Parameters maxmize
Resource ID:spase://VSPO/DisplayData/POLAR/VIS/PT240S
Start:1996-11-01 00:00:00 Observatory:POLAR Cadence:240 seconds
Stop:2008-04-28 00:00:00 Instrument:Visible Imaging System (VIS) Resource:DisplayData
This dataset contains the investigator-selected Key Parameters from the Polar Visible Imaging System (VIS). The VIS key parameter data set is a survey of auroral activity provided by a series of single images showing a significant area of the auroral zone at visible wavelengths. An auroral image of 256 x 256 pixels is produced approximately every 24 seconds dependent on the integration time and filter selected. Some coordinate information is included for viewer orientation. Coordinates are calculated for a grid of 18 x 18 points corresponding to one pixel out of every 15 x 15 pixel block. In addition, a rotation matrix and a table of distortion-correcting look direction unit vectors are provided for the purpose of calculating coordinates for every pixel. To facilitate viewing of the images, a mapping of pixel value to a recommended color table based on the characteristics of the selected filter is included with each image. A relative intensity scale is provided by the uncompressed count table of variable 27. Approximate intensity levels in kiloRayleighs are given in the intensity table of variable 28. The VIS site at http://eiger.physics.uiowa.edu/~vis/software contains information on the availability of more precisely calibrated intensities. The data set also contains various imager-related parameters, plus spacecraft position and velocity vectors, spin axis unit vector, and the sun position unit vector, all in GCI coordinates. Times are given in both the CDF-standard Epoch and the ISTP-standard Time_PB5.

50) Polar Visible Imaging System Earth Camera Key Parameters maxmize
Resource ID:spase://VSPO/DisplayData/POLAR/VIS/PT300S
Start:1996-11-01 00:00:00 Observatory:POLAR Cadence:300 seconds
Stop:2008-04-28 00:00:00 Instrument:Visible Imaging System (VIS) Resource:DisplayData
This dataset contains the investigator-selected Earth Camera Key Parameters from the Polar Visible Imaging System (VIS). It contains global images of the auroral oval at ultraviolet wavelengths. One or more Earth camera images of 256 x 256 pixels are produced every five minutes, depending on the commanded mode. Some coordinate information is included for viewer orientation. Coordinates are calculated for a grid of 18 x 18 points corresponding to one pixel out of every 15 x 15 pixel block. In addition, a rotation matrix and a table of distortion-correcting look direction unit vectors are provided for the purpose of calculating coordinates for every pixel. To facilitate viewing of the images, a mapping of pixel value to a recommended color table based on the characteristics of the selected filter is included with each image. A relative intensity scale is provided by the uncompressed count table of variable 27. Approximate intensity levels in kiloRayleighs are given in the intensity table of variable 28. The VIS site at http://eiger.physics.uiowa.edu/~vis/software contains information on the availability of more precisely calibrated intensities. The data set also contains various imager-related parameters, plus spacecraft position and velocity vectors, spin axis unit vector, and the sun position unit vector, all in GCI coordinates. Times are given in both the CDF-standard Epoch and the ISTP-standard Time_PB5.

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