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1) AE-E MSIS Neutral Density Data maxmize
Resource ID:spase://VSPO/NumericalData/AE-E/BIMS_OSS/PT256S
Start:1977-07-01 00:00:00 Observatory:AE-E Cadence:256 seconds
Stop:1981-06-09 23:59:59 Instrument:Bennett Ion-Mass Spectrometer (BIMS) Resource:NumericalData
This set of neutral density data was deduced from the mass spectrometer measurements on the Atmosphere Explorer E's Bennett Ion-Mass Spectrometer and Open-Source Neutral Mass Spectrometer. The density numbers (in cm-3) for hydrogen, nitrogen and molecular oxygen were provided by A. Hedin (GSFC, Code 914, now retired). They are related to A. Hedin's atmospheric modelling work (Mass Spectrometer and Incoherent Scatter atmospheric model - MSIS). In addition to density, the record includes also orbital parameters.

2) AE-E Extreme UltraViolet (EUV) Spectrometer Flux maxmize
Resource ID:spase://VSPO/NumericalData/AE-E/EUVS/PT256S
Start:1977-07-01 00:00:00 Observatory:AE-E Cadence:256 seconds
Stop:1981-06-09 23:59:59 Instrument:The Extreme Ultraviolet Spectrometer (EUVS) Resource:NumericalData
The EUV flux data came from the Extreme UltraViolet Spectrometer on the Atmosphere Explorer E. The data for 15 wavelength groups are normalized to the reference spectrum SC21REFW.DAT (located in directory REF_SPEC). GET_EUVS.FOR is a program to read the EUV data file (written by Dean Pesnell). The EUVS instrument is described in an article by Hinteregger in Radio Science, Volume 8, Number 4, 349-360, 1973. For more references please consult the file REF_LIST in the AEDOC directory. In addition to the solar EUV measurements, the EUVS also provided an opportunity to study the optical depth (absorption) of the thermosphere. Details of this analysis are described in: L.M. Chaikin and K. Fukui, Absorption Data Analysis for EUVS Experiment on the Satellites AE-C, D, and E, Air Force Geophysics Laboratory, Report AFGL-TR-79-0191, Hanscom AFB, Massachusetts, August 1979.

3) 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.

4) Pioneer 11 Ultraviolet Photometer Daily Cruise Data maxmize
Resource ID:spase://VSPO/NumericalData/Pioneer11/UVP/PT1D
Start:1973-01-01 00:00:00 Observatory:Pioneer 11 Cadence:1 day
Stop:1993-01-01 00:00:00 Instrument:Ultraviolet Photometer Resource:NumericalData
This Pioneer 11 UV photometer data set contains daily averages of the spin-averaged short and long wavelength channels from April 6, 1973 onward. These data are used to study the interaction of the solar wind with the interstellar medium by measurements of spatial and temporal variations of the intensity of backscattered solar Lyman alpha emission at 1216 A and of the solar Helium line at 584 A.

5) STPSat-1 SHIMMER OH Data maxmize
Resource ID:spase://VSPO/NumericalData/STPSat1/SHIMMER/OH/PT1D
Start:2007-04-05 00:00:00 Observatory:STPSat-1 Cadence:24 hours
Stop:2009-09-24 00:00:00 Instrument:STPSat-1Spatial Heterodyne Imager for Mesospheric Radicals (SHIMMER) Resource:NumericalData
This dataset contains daily averaged mesospheric hydroxyl (OH) radiance profiles of solar resonance fluorescence measured near 309 nm by the Spatial Heterodyne Imager for MEsospheric Radicals (SHIMMER) onboard STPSat-1. OH data were obtained by imaging the limb every 20 s between 58N and 58S. These radiance profiles were inverted to retrieve daily averaged mesospheric OH densities between 60 and 90 km in 2 km increments. A total of 1816 OH profiles are available, 881 from the ascending (A) portion of the orbit and 935 from the descending (D) portion of the orbit. Because the satellite is moving eastward at latitudes between 50N and 58N, the profiles from the A portion are about 3 hours earlier in local solar time than the D portion in this latitude band. The OH number density profile data are stored in directories for the tropics ("0_to_15N") and for the mid-latitudes ("50N_to_58N"). See SHIMMER Data Manual for a list of missing days. They are available in ASCII format in 5 columns: altitude, OH densities, uncertainty in the OH densities (1 ?), OH radiances (uninverted intensities along the line of sight), and uncertainty in the OH radiances. In addition, there are "showstat" summary plots, in postscript files, with relevant viewing conditions for each of the six data periods (either tropics or mid-latitudes for each of the three years). Each of the figures has 6 panels that include a) Number of spectra obtained on each day, b) Solar zenith angle (SZA), c) Solar scattering angle (SSA), d) Latitude of the limb tangent point, e) Local solar time (LST) at the tangent point, and f) Altitude range of the limb observation (nominally 35-100 km, on occasion as high as 65-130 km).

6) STPSat-1 SHIMMER PMC Data maxmize
Resource ID:spase://VSPO/NumericalData/STPSat1/SHIMMER/PMC/PT1D
Start:2007-04-05 00:00:00 Observatory:STPSat-1 Cadence:24 hours
Stop:2009-09-24 00:00:00 Instrument:STPSat-1Spatial Heterodyne Imager for Mesospheric Radicals (SHIMMER) Resource:NumericalData
This dataset contains Polar Mesospheric Clouds (PMCs) observed by the Spatial Heterodyne Imager for MEsospheric Radicals (SHIMMER) onboard the STPSat-1 satellite. The PMC (primarily a summertime phenomenon) data are derived from over a million limb images during its three-year mission, minus September through November for each year. Each file has a five-line header that includes: (1) Year and day of the year (DOY), (2) Total number of PMC detected on that day, (3) The number of PMC detected when using a phase function of the ice particles, (4) Hydroxyl (OH) radiances at 80 and 87 km, and (5) Labels of the output: Year, DOY, GMT, LAT, LON, LST, SSA, SZA, PMCRAW (1 for PMC detection and 0 for none), PMCMIE (detection above the applied threshold), BGRND (average Rayleigh scattered background signal in kR/nm), BRT (background corrected peak brightness in kR/nm), THRRAW (threshold used to identify a PMC), THRPHS (threshold used to detect PMC in kR/nm), PK (altitude of the peak emission in km), OH80 (OH solar resonance fluorescence radiance detected at 80 km in kR), OHE80 (uncertainty for the 80 km OH radiance in kR), OH87 (OH solar resonance fluorescence radiance detected at 87 km in kR), and OHE87 (uncertainty for the 87 km OH radiance in kR). In addition to the PMC data, there are PMC maps and summary figures for each year of operations. The first figure for each year is map_YYYY.ps, where YYY represents the year. This shows the geographic location of each detected PMC, without regard to when it was detected. Also indicated on the maps are the total number of images tested for a PMC as well as the total number of PMC detected for each year. The second figure (summary_YYYY.ps) shows a time series of some important results of the analysis: the number of SHIMMER images tested, a time series of PMC detections for the year, a time series of thresholded PMC detections, and a time series of PMC altitudes defined as the altitude of peak brightness.

7) TIMED GUVI Imaging Level 1C Disk maxmize
Resource ID:spase://VITMO/NumericalData/TIMED/GUVI/Imaging/Imaging_L1C_Disk
Start:2002-01-08 00:00:00 Observatory:TIMED Cadence:
Stop:2007-12-11 00:05:38 Instrument:Global Ultraviolet Imager (GUVI) Resource:NumericalData
This Level 1C data product measured over multiple scans on the disk contains data directly measure by the sensors such as photometer counts, uncertainties, light intensities and pointing information derived from the GUVI raw sensor data and the TIMED Satellite ephemeris data. The data are geolocated at a 150 km altitude, then gridded and binned to a 25 km X 25 km resolution GUVI-based coordinate system consisting of the along orbit position of the sensor and the angle of the scan from the nadir position. This gridding eliminates overlap from scan to scan due to the large instantaneous field-of-view of GUVI (about 12 degrees) and involves coaddition to place the values on a uniform instrument shared grid. The data is then determined whether its from day, night, aurora or twilight pixels.

8) TIMED GUVI Imaging Level 1B Disk images maxmize
Resource ID:spase://VITMO/DisplayData/TIMED/GUVI/Imaging/L1B_Disk
Start:2002-01-07 00:00:00 Observatory:TIMED Cadence:
Stop:2005-12-27 23:08:34 Instrument:Global Ultraviolet Imager (GUVI) Resource:DisplayData
GUVI Level 1B FUV airglow radiance images.

9) TIMED GUVI Imaging Level 1B Disk maxmize
Resource ID:spase://VITMO/NumericalData/TIMED/GUVI/Imaging/L1B_Disk
Start:2002-01-07 00:00:00 Observatory:TIMED Cadence:
Stop:2007-12-11 00:05:38 Instrument:Global Ultraviolet Imager (GUVI) Resource:NumericalData
Level 1B Disk data contains calibrated radiance data over multiple scans that are geolocated into a GUVI-based coordinate system on the disk.

10) TIMED GUVI Imaging Level 1B Limb maxmize
Resource ID:spase://VITMO/NumericalData/TIMED/GUVI/Imaging/L1B_Limb
Start:2002-01-08 00:00:00 Observatory:TIMED Cadence:
Stop:2007-12-11 00:05:38 Instrument:Global Ultraviolet Imager (GUVI) Resource:NumericalData
Level 1B Limb data contains calibrated radiance data geolocated into a GUVI-based coordinate system on the limb.

11) TIMED GUVI Level 1B Spectrograph maxmize
Resource ID:spase://VITMO/NumericalData/TIMED/GUVI/Imaging/L1B_Spectrograph
Start:2002-01-07 00:00:00 Observatory:TIMED Cadence:
Stop:2016-09-11 07:58:11 Instrument:Global Ultraviolet Imager (GUVI) Resource:NumericalData
Level 1B Spectrograph data contains calibrated and geolocated radiance data into a GUVI based coordinate system in Spectrograph mode.

12) TIMED GUVI Level 1C FUV airglow radiance images. maxmize
Resource ID:spase://VITMO/DisplayData/TIMED/GUVI/Imaging/L1C_Disk
Start:2002-03-22 00:00:00 Observatory:TIMED Cadence:
Stop:2007-12-11 00:05:38 Instrument:Global Ultraviolet Imager (GUVI) Resource:DisplayData
Global maps of GUVI Level 1C FUV airglow radiances.

13) TIMED GUVI Nightside Cylindrical Composite Disk Images maxmize
Resource ID:spase://VITMO/DisplayData/TIMED/GUVI/Nightside_Cylindrical_Disk
Start:2002-01-14 00:00:00 Observatory:TIMED Cadence:
Stop:2007-12-11 00:00:00 Instrument:Global Ultraviolet Imager (GUVI) Resource:DisplayData
This composite image is produced from GUVI radiance data (Level 1C) where the SZA > 95 deg. (nightside) for a complete day mapped onto the globe. It is a composite of the O I 130.4 nm emission (blue), O I 135.6 nm (green), and LBH Short (140 - 150 nm) (red). White color indicates emission from particles in aurora (all colors), pink areas generally indicate particle precipitation (SAA) or solar glint, blue emissions indicate typical nighttime recombination emissions.

14) TIMED GUVI Strip Disk Composite Images maxmize
Resource ID:spase://VITMO/DisplayData/TIMED/GUVI/Nightside_Strip_Disk
Start:2002-01-14 00:00:00 Observatory:TIMED Cadence:
Stop:2007-12-11 00:00:00 Instrument:Global Ultraviolet Imager (GUVI) Resource:DisplayData
This composite image is produced from GUVI radiance data (Level 1C) plotted as a strip image for a complete day. It is a composite of the O I 130.4 nm emission (blue), O I 135.6 nm (green), and LBH Short (140 - 150 nm) (red). White color indicates emission from particles in aurora (all colors), pink areas generally indicate particle precipitation (SAA) or solar glint, blue emissions indicate typical nighttime recombination emissions, light grey typically indicates dayglow emission.

15) TIMED GUVI Strip Limb Composite Images maxmize
Resource ID:spase://VITMO/DisplayData/TIMED/GUVI/Nightside_Strip_Limb
Start:2002-01-14 00:00:00 Observatory:TIMED Cadence:
Stop:2007-12-11 00:00:00 Instrument:Global Ultraviolet Imager (GUVI) Resource:DisplayData
This composite image is produced from GUVI radiance data (Level 1C) plotted as a strip image for a complete day. It is a composite of the O I 130.4 nm emission (blue), O I 135.6 nm (green), and LBH Short (140 - 150 nm) (red). White typically indicates dayglow emission, green indicates nightside recombination emission, white streaks typically indicate stars in the instrument field-of-view.

16) TIMED SABER Level 1B maxmize
Resource ID:spase://VITMO/NumericalData/TIMED/SABER/L1B
Start:2002-01-25 00:00:00 Observatory:TIMED Cadence:
Stop:2016-08-15 07:58:11 Instrument:Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) Resource:NumericalData
Contains the SABER Level 1B calibrated radiance profiles converted to radiance units with instrument effects removed, geolocated and gridded to uniform angle spacing.

17) TIMED TIDI LOS maxmize
Resource ID:spase://VITMO/NumericalData/TIMED/TIDI/L1_LOS
Start:2002-01-25 00:00:00 Observatory:TIMED Cadence:
Stop:2016-09-11 07:58:11 Instrument:TIMED Doppler Interferometer (TIDI) Resource:NumericalData
Contains the TIDI Level 1B spectra corrected for instrumental effects and converted to Rayleighs/cm^-1, ancillary data and profiles of apparent LOS wind, temperature, and volume emission rates and their variances annotated with profile location and processing state.

18) TIMED TIDI Profiles maxmize
Resource ID:spase://VITMO/NumericalData/TIMED/TIDI/L2_Profiles
Start:2002-01-25 00:00:00 Observatory:TIMED Cadence:
Stop:2016-09-11 07:58:11 Instrument:TIMED Doppler Interferometer (TIDI) Resource:NumericalData
Contains the TIDI Level 2 inverted profiles of wind, temperature and volume emission rates annotated with profile location and processing status. Profiles are produced at the maximum temporal resolution of the instrument.

19) TIMED TIDI Vectors maxmize
Resource ID:spase://VITMO/NumericalData/TIMED/TIDI/L3_Vectors
Start:2002-01-25 00:00:00 Observatory:TIMED Cadence:
Stop:2016-09-11 07:58:11 Instrument:TIMED Doppler Interferometer (TIDI) Resource:NumericalData
Contains the TIDI Level 3 data mapped onto a fixed angle-along-the-track grid. The wind is decomposed into its zonal and meridional components. Each profile is annotated with ancillary data including profile position and processing status.

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