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1) ACE ULEIS L2 hourly Z=1-30 flux data maxmize
Resource ID:spase://VSPO/NumericalData/ACE/ULEIS/PT3600S
Start:1998-02-19 00:00:00 Observatory:ACE Cadence:3600 seconds
Stop:2016-09-14 08:00:05 Instrument:Ultra-Low Energy Isotope Spectrometer (ULEIS) Resource:NumericalData
ACE ULEIS L2 1-hr, 1-d, 27-d Z=1-30 flux data at ASC

2) 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.

3) 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.

4) AIM/SOFIE daily plots, parameters vs.alt. & long., etc. (L3 Summary data) maxmize
Resource ID:spase://VSPO/DisplayData/AIM/SOFIE/PT90M
Start:2007-05-28 00:00:00 Observatory:AIM Cadence:90 minutes
Stop:2016-09-14 07:59:49 Instrument:AIM Solar Occultation For Ice Experiment Resource:NumericalData
This SOFIE (Solar Occultation for Ice Experiment) data set contains color-coded pairs of daily plots of several physical parameters vs altitude and longitude. Parameters include temperature, mixing ratios for H2O, O3 and CH4, and ice mass. Members of each pair are for the northern and southern hemispheres. The interface also supports plotting of lower level data.

5) AIM/SOFIE mixing ratios, extinction profiles, etc. (L2 data) maxmize
Resource ID:spase://VSPO/NumericalData/AIM/SOFIE/PT90M
Start:2007-05-28 00:00:00 Observatory:AIM Cadence:90 minutes
Stop:2016-09-14 08:00:04 Instrument:AIM Solar Occultation For Ice Experiment Resource:NumericalData
The daily netCDF files at GATS, Inc., hold level 2 SOFIE (Solar Occultation for Ice Experiment) data. These include primary absorber mixing ratios (CO2, CH4, NO,H2O, O3), 10 aerosol extinction profiles, uncertainity profiles for mixing ratios and extinctions, 83 km measurement lat./long., Temperatures, Pressures, Time, [0.150 km sampling, 150km to 3.0km, 30 profiles/day]. Vertical resolutions are 1km for gases and for polar mesospheric clouds, and .LT.3.5 km for temperatures and pressures.

6) AMPTE/IRM Plasma Data from the University of Iowa maxmize
Resource ID:spase://VSPO/NumericalData/AMPTE_IRM/PWS/PT1M
Start:1984-05-13 00:00:00 Observatory:AMPTE/IRM Cadence:1 minute
Stop:1985-07-18 00:00:00 Instrument:AMPTE/IRM Plasma Wave Spectrometer Resource:NumericalData
This set of AMPTE IRM data came from the University of Iowa single-channel digitized waveform file. Each file (table) contains plasa waves measured in the frequency range from quasi-dc to 5 MHz and occurring in an integral one minute interval. Each record (row) contains a 10 millisecond waveform series.

7) Aeros-A Neutral Gas Densities maxmize
Resource ID:spase://VSPO/NumericalData/Aeros-A/NATE/PT256S
Start:1972-12-26 00:00:00 Observatory:Aeros-A Cadence:256 seconds
Stop:1973-08-09 23:59:59 Instrument:The Neutral Atmosphere Temperature Experiment (NATE) Resource:NumericalData
This data set contains the neutral densities measured by the Neutral Density and Temperature Probe (PI: N. Spencer) during the AEROS-A satellite mission. The data are in ASCII format and cover the time period from 12/26/1972 to 8/9/1973. The four different files provided in this data set contain the data for He, O2, N2, and Ar, respectively. Each data record provides date, time, density, density error, altitude, latitude and longitude, and local solar time.

8) Akebono SMS summary plots of ion count rates maxmize
Resource ID:spase://VSPO/DisplayData/Akebono/SMS/PT8S
Start:1989-04-01 00:00:00 Observatory:Akebono Cadence:8 seconds
Stop:1997-12-23 00:00:00 Instrument:Suprathermal Mass Spectrometer(SMS) Resource:NumericalData
These data consist of plots of color-coded ion count rates vs. spin phase angle and time, for thermal H+, He++, He+ and O+ ions and for suprathermal H+ and O+ ions. Each plot covers some or all of one ~3.5 hour orbit. Digital binary data and a data reading program are also accessible.

9) Akebono SMS digital binary ion count rates maxmize
Resource ID:spase://VSPO/NumericalData/Akebono/SMS/PT8S
Start:1989-02-26 00:00:00 Observatory:Akebono Cadence:8 seconds
Stop:2002-12-23 00:00:00 Instrument:Suprathermal Mass Spectrometer(SMS) Resource:NumericalData
These count rate data reside in the DARTS/Akebono binary Science DataBase (SDB). They consist of count rates at 8-sec spacecraft spin resolution, separately for thermal and suprathermal H+, He+ and O+ ions. Detailed information and a data-read program are found at http://darts.isas.jaxa.jp/akbn/readme/readme.sms.txt.

10) Apollo 12 Solar Wind Measurements at the Lunar Surface 1-HR Data maxmize
Resource ID:spase://VSPO/NumericalData/Apollo12-LM/SWS/PT1HR
Start:1969-11-19 19:30:00 Observatory:Apollo 12 Lunar Module/ALSEP Cadence:60 minutes
Stop:1976-03-25 08:30:00 Instrument:Solar Wind Spectrometer Resource:NumericalData
This data set contains hourly averaged plasma parameters from the Apollo 12 Solar Wind Spectrometer. Four sets of hourly averaged parameters are computed, using as input data -- (1) all fine-time scale parameters (FTSP), (2) all FTSP computed from spectra with small rms error on curve fitting and thermal speeds less than one-half the bulk velocity, (3) all FTSP computed from spectra that satisfy the requirements of criterion 2 as well as having only one flow angle that can be directly measured, and (4) all FTSP computed from spectra that satisfy the requirements of criterion 2 as well as having both flow angles directly measureable. Contained in each of the 4 sets of averages are the proton density, alpha-to-proton ratio, bulk speed, angle of flow, number of spectra, and rms deviations of each average.

11) Apollo 12 Solar Wind Measurements at the Lunar Surface 28-s Data maxmize
Resource ID:spase://VSPO/NumericalData/Apollo12-LM/SWS/PT28S
Start:1969-11-19 18:42:13 Observatory:Apollo 12 Lunar Module/ALSEP Cadence:28 seconds
Stop:1976-03-25 08:35:57 Instrument:Solar Wind Spectrometer Resource:NumericalData
This data set contains the highest time resolution plasma data available (28 sec per spectrum) from the solar wind experiment onboard Apollo 12. Contained in each record are: time, proton density, alpha-to-proton ratio, bulk speed, angle of flow, most probable thermal speed, and various housekeeping and fit parameters relating to the reliability of the calculated plasma parameters. During the local lunar night there is no solar wind signal so there are data gaps of about 15 days each lunation.

12) Apollo 15 Solar Wind Measurements at the Lunar Surface 1-HR Data maxmize
Resource ID:spase://VSPO/NumericalData/Apollo15-LM/SWS/PT1HR
Start:1971-07-31 19:30:00 Observatory:Apollo 15 Lunar Module/ALSEP Cadence:60 minutes
Stop:1972-06-30 17:30:00 Instrument:Solar Wind Spectrometer Resource:NumericalData
This data set contains hourly averaged plasma parameters from the Apollo 15 Solar Wind Spectrometer. Four sets of hourly averaged parameters are computed, using as input data -- (1) all fine-time scale parameters (FTSP), (2) all FTSP computed from spectra with small rms error on curve fitting and thermal speeds less than one-half the bulk velocity, (3) all FTSP computed from spectra that satisfy the requirements of criterion 2 as well as having only one flow angle that can be directly measured, and (4) all FTSP computed from spectra that satisfy the requirements of criterion 2 as well as having both flow angles directly measureable. Contained in each of the 4 sets of averages are the proton density, alpha-to-proton ratio, bulk speed, angle of flow, number of spectra, and rms deviations of each average.

13) Apollo 15 Solar Wind Measurements at the Lunar Surface 28-s Data maxmize
Resource ID:spase://VSPO/NumericalData/Apollo15-LM/SWS/PT28S
Start:1971-07-31 19:38:38 Observatory:Apollo 15 Lunar Module/ALSEP Cadence:28 seconds
Stop:1972-06-30 18:14:35 Instrument:Solar Wind Spectrometer Resource:NumericalData
This data set contains the highest time resolution plasma data available (28 sec per spectrum) from the solar wind experiment onboard Apollo 15. Contained in each record are: time, proton density, alpha-to-proton ratio, bulk speed, angle of flow, most probable thermal speed, and various housekeeping and fit parameters relating to the reliability of the calculated plasma parameters. During the local lunar night there is no solar wind signal so there are data gaps of about 15 days each lunation.

14) 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.

15) 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.

16) DE 1 Energetic Ion Composition Spectrometer Validated Summary Data maxmize
Resource ID:spase://VSPO/NumericalData/DE1/EICS/PT96S
Start:1981-09-16 00:00:00 Observatory:Dynamics Explorer 1 Cadence:96 seconds
Stop:1991-02-18 00:00:00 Instrument:DE 1 Energetic Ion Composition Spectrometer Resource:NumericalData
This Validated Summary (VS) data set from the DE 1 Energetic Ion Composition Spectrometer (EICS) contains 96-second averaged fluxes (in units of 1/(cm^2-sec-sr-keV) ) for H+, O+, and He+ ions in 15 energy (~0.01 to ~20 keV) and 14 pitch angle bins. It also includes data uncertainties, data quality indicators, and spacecraft position. Data are in CDF format from CDAWeb.

17) DE 2 1s NACS Temperature and Composition maxmize
Resource ID:spase://VSPO/NumericalData/DE2/NACS/PT1S
Start:1981-08-08 00:00:00 Observatory:Dynamics Explorer 2 Cadence:1 second
Stop:1983-02-15 00:00:00 Instrument:Neutral Atmosphere Composition Spectrometer (NACS) Resource:NumericalData
This data set containss, at 1-sec resolution, the neutral temperature and the densities (and % error) of O, N2, He, N, and Ar from the Neutral Atmosphere Composition Spectrometer (NACS) flown on DE 2. Composition data are most reliable at altitudes less than 500 km. Data are available in ASCII from nssdcftp and in CDF format from CDAWeb (as well as CDAWeb plots and lists).

18) DE 2 2s WATS Wind Velocity, Density and Temperature maxmize
Resource ID:spase://VSPO/NumericalData/DE2/WATS/PT2S
Start:1981-08-08 00:00:00 Observatory:Dynamics Explorer 2 Cadence:2 seconds
Stop:1983-02-17 00:00:00 Instrument:Neutral Atmosphere Composition Spectrometer (NACS) Resource:NumericalData
This data set contains, at 2-sec resolution, the neutral wind horizontal velocity, temperature and density from the Wind and Temperature Spectrometer (WATS) flown on DE 2. Data are available in ASCII from nssdcftp and in CDF format from CDAWeb (as well as CDAWeb plots and lists).

19) DMSP SSJ/4 Particle Flux Spectral Plots maxmize
Resource ID:spase://VSPO/DisplayData/DMSP_5D-2/SSJ4/PLOTS
Start:1983-12-01 00:00:00 Observatory:DMSP_5D-2 Cadence:
Stop:2016-09-14 07:59:49 Instrument:SSJ/4 Special Sensor for Precipitating Particles, Version 4 Resource:DisplayData
DMSP SSJ/4 30 eV - 30 keV ion and electron spectral plots, multiple DMSP spacecraft

20) DMSP SSJ/4 Particle Flux ASCII Files maxmize
Resource ID:spase://VSPO/NumericalData/DMSP_5D-2/SSJ4/PT1.0S
Start:1983-12-01 00:00:00 Observatory:DMSP_5D-2 Cadence:1.0 seconds
Stop:2016-09-14 07:59:52 Instrument:SSJ/4 Special Sensor for Precipitating Particles, Version 4 Resource:NumericalData
DMSP SSJ/4 30 eV - 30 keV ion and electron ASCII files, multiple DMSP spacecraft. Boundary crossing identifications also given

21) Explorer 32 ion mass spectrometer data maxmize
Resource ID:spase://VSPO/NumericalData/Explorer32/IMS/PT210S
Start:1966-06-10 00:00:00 Observatory:Explorer 32 Cadence:210 seconds
Stop:1967-01-17 00:00:00 Instrument:Ion Mass Spectrometer Resource:NumericalData
Explorer 32 (AE-B) ion mass spectrometer, densities of H+, He+, N+, O+,

22) FAST TMS Key Parameters maxmize
Resource ID:spase://VSPO/NumericalData/FAST/TMS/KP/PT5S
Start:1996-10-01 00:00:00 Observatory:FAST Cadence:5 seconds
Stop:2009-04-30 10:22:16 Instrument:Time of Flight Energy Angle Mass Spectrograph Resource:NumericalData
The data set provides the 5-second (spin-averaged) FAST survey data from the Time of flight Energy Angle Mass Spectrograph (TEAMS) in CDF format. The data set includes H+, O+, and He+ differential energy fluxes. Pitch-angle-averaged fluxes are provided for 48 energies (1eV-12keV). Energy-averaged fluxes are provided for 16 pitch angles (0-360 deg) for the energy range 0.01-1keV and >1keV. Each angle segment contains 2 (4) samples at each energy in the 32 (64) sweep/spin mode. The full angular range is covered in half a spin but the actual time resolution of the survey data product depends upon the telemetry mode. In the highest TM rate modes H+ and O+ survey data read out every half spin. In lowest TM rate mode these data are accumulated for 4 spins. The minimum accumulation time included in the CDF is 1 spin, so if the actual accumulation time is a half spin, two data points are averaged. Otherwise, the full resolution is included. In every mode He+ and He++ are accumulated twice as long as H+ and O+. To force the H+, O+, and He+ to have an equal number of data points when H+ and O+ have twice the time resolution, each He+ data point is written twice consecutively in the file. Orbit parameters are also included in this data set.

23) ISEE 3 Electron Moments Noramlized Hourly Averages maxmize
Resource ID:spase://VSPO/NumericalData/ISEE3/SWIC/Normalized/PT1H
Start:1978-08-16 00:00:00 Observatory:ISEE 3 Cadence:1 hour
Stop:1982-10-16 00:00:00 Instrument:Solar Wind Ion Composition, 300-600 km/s 840 eV/Q to 11.7 keV/Q; M/Q = 1.5 to 5.6 Resource:NumericalData
This data set contains ISEE 3 electron moments in the solar wind, normalized and in 1-hour resolution, from the LANL Solar Wind Plasma experiment. The data are electron-based and have been corrected and normalized to existing ion data. Each logical record contains the date (YYMMDD), the universal time (HRMIN), the spacecraft position in GSE coordinates in earth radii, the electron density (1/cm**3) normalized to the ion data, for dates 780816 - 821016, the bulk speed (km/s), and the electron temperature (K). Although the bulk parameters given are reliable, standard errors associated with them are higher for electrons than for ions. A few "bad" points remain on the tape. Densities less than .01/cm**3 and velocities less than 100 km/s should be considered erroneous. Each file contains data for a whole year.

24) ISEE 3 Electron Moments maxmize
Resource ID:spase://VSPO/NumericalData/ISEE3/SWIC/PT168.00S
Start:1980-02-01 00:00:00 Observatory:ISEE 3 Cadence:168.00 seconds
Stop:1992-06-13 00:00:00 Instrument:Solar Wind Ion Composition, 300-600 km/s 840 eV/Q to 11.7 keV/Q; M/Q = 1.5 to 5.6 Resource:NumericalData
ISEE 3 solar wind electron moments - density, bulk flow speed, bulk flow azimuth, minimum total temperature (Tper), maximum total temperature (Tpar,) azimuth of the maximum temperature, heat flux, and the heat flux azimuth - at 168-sec resolution from geocentric and deep-space orbit phases

25) ISEE 3 Electron Moments hourly averages maxmize
Resource ID:spase://VSPO/NumericalData/ISEE3/SWIC/PT1H
Start:1982-02-01 00:00:00 Observatory:ISEE 3 Cadence:1 hour
Stop:1992-06-13 00:00:00 Instrument:Solar Wind Ion Composition, 300-600 km/s 840 eV/Q to 11.7 keV/Q; M/Q = 1.5 to 5.6 Resource:NumericalData
This data set was generated at NSSDC by making one-hour averages of the ISEE 3 Solar Wind Electron Moments in 168 second resolution. There were no time shifts used in creating these hourly averages. Each data file contains data for one year. Data coverage runs from 1982/02/01 through 1992/06/13. There is a data gap from 16 October 1982 to 23 December 1983, corresponding to the geotail phase of the mission. Data parameters (hourly averages) are: electron density, bulk flow speed, bulk flow azimuth, minimum total temperature (Tper), maximum total temperature (Tpar), azimuth of maximum temperature, heat flux, and the heat flux azimuth. There is no spacecraft position information in this data set. The normalized 1-hr data set, however, does include the spacecraft position. Hourly ephemeris data are available online for the time period from soon after launch through the end of the primary mission, i.e., from August 13, 1978 through February 7, 1987. See the data set "isee3_dp_ephem.asc" and its description "aareadme_isee3_dp_ephem" in the directory at ftp://nssdcftp.gsfc.nasa.gov/spacecraft_data/isee/isee3/traj/hourly_magnetospheric. There is also a trajectory data set with one point per day for the ICE phase of the mission: 1984 - 1997. Its documentation can be found at ftp://nssdcftp.gsfc.nasa.gov/spacecraft_data/isee/isee3/traj/daily/icetrjdy_fmt.txt and the data set itself is at ftp://nssdcftp.gsfc.nasa.gov/spacecraft_data/isee/isee3/traj/daily/icetrja.asc.

26) ISIS 2/IMS/Plasma Data maxmize
Resource ID:spase://VSPO/NumericalData/ISIS2/IMS/Plasma_Data
Start:1971-04-21 00:12:41 Observatory:ISIS 2 Cadence:
Stop:1972-12-31 23:20:43 Instrument:ISIS2 Ion Mass Spectrometer Resource:NumericalData
This set of plasma data came from the ISIS 2 (International Satellites for Ionospheric Studies) ion-mass spectrometer experiment. Ion densities of various ion species are available for the lower range (1-8 atomic mass units, H+, D+, He+, N++, O++) and the upper range (8-64 atomic mass units, O++, N+, O+, 18+, N2+, NO+, O2+). Also included in the data set are spacecraft position data, geomagnetic field intensity, F107 flux (daily solar radio flux), Kp indices, and Dst indices.

27) Interball Tail PROMICS H+ and O+ 2-min Key Parameters maxmize
Resource ID:spase://VSPO/NumericalData/Interball-1/PROMICS3/PT120S
Start:1995-08-22 00:00:00 Observatory:Interball-1 Cadence:120 seconds
Stop:1996-06-07 00:00:00 Instrument:Ion Composition 3D Spectrometer (PROMICS-3) Resource:NumericalData
Interball Tail H+ and O+ count rates from multiple sensors on PROMICS, 2-min key parameters

28) 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.

29) 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.

30) 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.

31) OGO 6 BIMS ion mass spectrometer data maxmize
Resource ID:spase://VSPO/NumericalData/OGO6/BIMS/PT40S
Start:1969-06-12 00:00:00 Observatory:OGO 6 Cadence:40 seconds
Stop:1970-12-31 00:00:00 Instrument:Ion Mass Spectrometer Resource:NumericalData
OGO 6 Bennett Ion Mass Spectrometer (BIMS), densities of H+, He+, N+, O+ N2+, O2+, NO+

32) 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.

33) SNOE UVS (Ultraviolet Spectrometer) geographic coordinates maxmize
Resource ID:spase://VSPO/NumericalData/SNOE/UVS/GEO/PT1S
Start:1998-03-11 00:00:00 Observatory:Student Nitric Oxide Explorer (SNOE) Cadence:1 second
Stop:2000-09-30 23:59:59 Instrument:Student Nitric Oxide Explorer (SNOE) Ultraviolet Spectrometer (UVS) Resource:NumericalData
This set of SNOE UVS (Ultraviolet Spectrometer) data contains nitric oxide volume density translated from the spacecraft look angle through the atmosphere at the limb of Earth. Density data are provided from 100 to 150 km altitudes in 10 km intervals at the recorded geographic latitude and longitude (5-degree bins). Any data outages of size one (i.e. all adjacent neighbors contain valid data) in the dataset are filled in using linear interpolation in the altitude direction.

34) SNOE Daily Averages of Nitric Oxide (NO) Density in Geographic Bins maxmize
Resource ID:spase://VSPO/NumericalData/SNOE/UVS/GEO/PT24H
Start:1998-03-11 00:00:00 Observatory:Student Nitric Oxide Explorer (SNOE) Cadence:24 hours
Stop:2000-09-30 00:00:00 Instrument:Student Nitric Oxide Explorer (SNOE) Ultraviolet Spectrometer (UVS) Resource:NumericalData
This level 4 data set from the Student Nitric Oxide Explorer (SNOE) ultraviolet spectrometer (UVS) contains daily averages of nitric oxide (NO) density for the altitudes range 96.6 to 150 km as deduced from the UVS count rates ([0, 1] gamma band; 237 nm). Averaging was done in geographic coordinates in a 38x18 array, using bins of 5 degree latitude and 3.3 km altitude.

35) SNOE Orbital Averages of Nitric Oxide (NO) Density in Geographic Bins maxmize
Resource ID:spase://VSPO/NumericalData/SNOE/UVS/GEO/PT96M
Start:1998-03-11 00:00:00 Observatory:Student Nitric Oxide Explorer (SNOE) Cadence:96 minutes
Stop:2000-09-30 00:00:00 Instrument:Student Nitric Oxide Explorer (SNOE) Ultraviolet Spectrometer (UVS) Resource:NumericalData
This level 3 data set from the Student Nitric Oxide Explorer (SNOE) ultraviolet spectrometer (UVS) contains orbital averages of nitric oxide (NO) density for the altitudes range 96.6 to 150 km as deduced from the UVS count rates ([0, 1] gamma band; 237 nm). Averaging was done in geographic coordinates in a 38x20 array, using bins of 5 degree geographic latitude, 3.3 km altitude, and 24 degrees in geographic longitude.

36) SNOE UVS (Ultraviolet Spectrometer) geomagnetic coordinates maxmize
Resource ID:spase://VSPO/NumericalData/SNOE/UVS/MAG/PT1S
Start:1998-03-11 00:00:00 Observatory:Student Nitric Oxide Explorer (SNOE) Cadence:1 second
Stop:2000-09-30 23:59:59 Instrument:Student Nitric Oxide Explorer (SNOE) Ultraviolet Spectrometer (UVS) Resource:NumericalData
This set of SNOE UVS (Ultraviolet Spectrometer) data contains nitric oxide volume density translated from the spacecraft look angle through the atmosphere at the limb of Earth. Density data are provided from 100 to 150 km altitudes in 10 km intervals at the recorded geomagnetic latitude and longitude (5-degree bins). Any data outages of size one (i.e. all adjacent neighbors contain valid data) in the dataset are filled in using linear interpolation in the altitude direction.

37) SNOE Daily Averages of Nitric Oxide (NO) Density in Geomagnetic Bins maxmize
Resource ID:spase://VSPO/NumericalData/SNOE/UVS/MAG/PT24H
Start:1998-03-11 00:00:00 Observatory:Student Nitric Oxide Explorer (SNOE) Cadence:24 hours
Stop:2000-09-30 00:00:00 Instrument:Student Nitric Oxide Explorer (SNOE) Ultraviolet Spectrometer (UVS) Resource:NumericalData
This level 4 data set from the Student Nitric Oxide Explorer (SNOE) ultraviolet spectrometer (UVS) contains daily averages of nitric oxide (NO) density for the altitudes range 96.6 to 150 km as deduced from the UVS count rates ([0, 1] gamma band; 237 nm). Averaging was done in geomagnetic coordinates in a 38x18 array, using bins of 5 degree (geomagnetic) latitude and 3.3 km altitude.

38) SNOE Orbital Averages of Nitric Oxide (NO) Density in Geomagnetic Bins maxmize
Resource ID:spase://VSPO/NumericalData/SNOE/UVS/MAG/PT96M
Start:1998-03-11 00:00:00 Observatory:Student Nitric Oxide Explorer (SNOE) Cadence:96 minutes
Stop:2000-09-30 00:00:00 Instrument:Student Nitric Oxide Explorer (SNOE) Ultraviolet Spectrometer (UVS) Resource:NumericalData
This level 3 data set from the Student Nitric Oxide Explorer (SNOE) ultraviolet spectrometer (UVS) contains orbital averages of nitric oxide (NO) density for the altitudes range 96.6 to 150 km as deduced from the UVS count rates ([0, 1] gamma band; 237 nm). Averaging was done in geomagnetic coordinates in a 38x20 array, using bins of 5 degree geomagnetic latitude, 3.3 km altitude, and 24 degrees in longitude.

39) SOHO UVCS Data maxmize
Resource ID:spase://VSPO/NumericalData/SOHO/UVCS/PT9M
Start:1996-01-02 00:00:00 Observatory:SOHO Cadence:9 minutes
Stop:2016-09-14 07:59:51 Instrument:Ultraviolet Coronagraph Spectrometer (UVCS) Resource:NumericalData
SOHO/UVCS (Ultraviolet Coronagraph Spectrometer) Spectral Data Files from SDAC via VSO

40) SOLIS ISS Spectra maxmize
Resource ID:spase://VSPO/DisplayData/SOLIS/ISS/P1D
Start:2006-12-02 00:00:00 Observatory:SOLIS Cadence:1 day
Stop:2016-09-09 07:59:49 Instrument:The SOLIS Integrated Sunlight Spectrometer Resource:DisplayData
This data product from the Integrated SOLIS Spectrometer (ISS) consists of high spectral resolution, disk- integrated spectra across various spectral bands of interest. Many are for the Ca II K line. The data are available as both JPEG images for browsing and as FITS files for quantitative work.

41) SOLIS ISS Spectra, FITS maxmize
Resource ID:spase://VSPO/NumericalData/SOLIS/ISS/P1D
Start:2006-12-02 00:00:00 Observatory:SOLIS Cadence:1 day
Stop:2016-09-09 08:00:04 Instrument:The SOLIS Integrated Sunlight Spectrometer Resource:NumericalData
This data product from the Integrated SOLIS Spectrometer (ISS) consists of high spectral resolution, disk- integrated spectra across various spectral bands of interest. Many are for the Ca II K line. The data are available as both JPEG images for browsing and as FITS files for quantitative work.

42) SOLIS VSM Daily Images maxmize
Resource ID:spase://VSPO/DisplayData/SOLIS/VSM/P1D
Start:2003-08-21 00:00:00 Observatory:SOLIS Cadence:1 day
Stop:2016-09-09 07:59:49 Instrument:The SOLIS Vector Spectromagnetograph Resource:DisplayData
This data product consists of daily sets of four images created from SOLIS Vector Spectromagnetograph (VSM) data: (a) photospheric longitudinal magnetic field, based on FeI 630.15 and 630.25 nm lines; (b) photospheric vector magnetic field, based on FeI 630.15 and 630.25 nm lines; (c) chromospheric equivalent widths based on the HeI 1083.0 nm line; (d) lower chromosphere longitudinal magnetic field based on the CaII 854.2 nm lines. Some recent data are "quick look" while most data are based on Milne-Eddington inversions. The data are available as both JPEG images for browsing and as FITS files for quantitative work.

43) SOLIS VSM Daily Images, FITS maxmize
Resource ID:spase://VSPO/NumericalData/SOLIS/VSM/P1D
Start:2003-08-21 00:00:00 Observatory:SOLIS Cadence:1 day
Stop:2016-09-09 08:00:04 Instrument:The SOLIS Vector Spectromagnetograph Resource:NumericalData
This data product consists of daily sets of four images created from SOLIS Vector Spectromagnetograph (VSM) data: (a) photospheric longitudinal magnetic field, based on FeI 630.15 and 630.25 nm lines; (b) photospheric vector magnetic field, based on FeI 630.15 and 630.25 nm lines; (c) chromospheric equivalent widths based on the HeI 1083.0 nm line; (d) lower chromosphere longitudinal magnetic field based on the CaII 854.2 nm lines. Some recent data are "quick look" while most data are based on Milne-Eddington inversions. The data are available as both JPEG images for browsing and as FITS files for quantitative work.

44) SOLIS VSM Synoptic Maps maxmize
Resource ID:spase://VSPO/DisplayData/SOLIS/VSM/P27D
Start:2003-01-28 00:00:00 Observatory:SOLIS Cadence:27 days
Stop:2016-08-15 07:59:49 Instrument:The SOLIS Vector Spectromagnetograph Resource:DisplayData
These maps show magnetic flux emanating from the photosphere as gray coding against the sun's full latitude and Carrington longitude ranges. The maps are available once per Carrington rotation and also, from a separate subdirectory, at "daily" (more typically, once every several days) resolution. For some intervals, the data are available as both jpegs for browsing and as gzipped FITS-formatted files for quantitative work.

45) SOLIS VSM Synoptic Maps, FITS maxmize
Resource ID:spase://VSPO/NumericalData/SOLIS/VSM/P27D
Start:2003-01-28 00:00:00 Observatory:SOLIS Cadence:27 days
Stop:2016-08-15 08:00:04 Instrument:The SOLIS Vector Spectromagnetograph Resource:NumericalData
These maps show magnetic flux emanating from the photosphere as gray coding against the sun's full latitude and Carrington longitude ranges. The maps are available once per Carrington rotation and also, from a separate subdirectory, at "daily" (more typically, once every several days) resolution. For some intervals, the data are available as both jpegs for browsing and as gzipped FITS-formatted files for quantitative work.

46) 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

47) Skylab UV Solar EUV Data in Original and FITS Format maxmize
Resource ID:spase://VSPO/NumericalData/Skylab/Spectroheliometer/RasterFITS/PT330S
Start:1973-05-28 00:00:00 Observatory:Skylab Cadence:330 seconds
Stop:1974-02-08 23:59:59 Instrument:Skylab UV Scanning Polychromator/Spectroheliometer Resource:NumericalData
This data set contains Skylab UV solar EUV data provided by the Principal Investigator. The data consist of both FITS data files and raw data files, contained in two subdirectories: /fits_data and /raw_data. The subdirectory /fits_data contains fits data files created in 2012 by copying from CDs (Compact Disks) which were in turn written by Mathieu Hirtzig at CfA in 2001 from SKYLAB-S055 data stored at the time on tape at CfA. These data are stored in 22 subdirectories (/fits_data/CD01 through /fits_data/CD22), each of which is a copy of one of the 22 CD's. Each of the subdirectories contains an identical sub-subdirectory named /README_S055, which contains a number of files some of which may be helpful in examining the data. It is recommended that those unfamiliar with the S055 experiment look at the file README_S055.txt for background, as well as other files in the README_S055 sub-subdirectory, some of which provide useful auxilliary information. The subdirectory /raw_data contains the raw data from which the fits data files were created. This is probably of limited use, but is included for archival purposes.

48) 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.

49) 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.

50) 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.

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