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1) Van Allen Probe B Coordinates maxmize
Resource ID:spase://ViRBO/NumericalData/BAR/1A/L2/EPHM/2/PT4S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:1 second
Stop:2016-09-14 07:56:57 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Coordinates

2) Van Allen Probe B Fast time resolution (50ms) Bremsstrahlung X-ray spectrum. maxmize
Resource ID:spase://ViRBO/NumericalData/BAR/1A/L2/FSPC//PT.05S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:1 second
Stop:2016-09-14 07:56:57 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fast time resolution (50ms) Bremsstrahlung X-ray spectrum.

3) Van Allen Probe B Fast time resolution (50ms) Bremsstrahlung X-ray spectrum. maxmize
Resource ID:spase://ViRBO/NumericalData/BAR/1A/L2/FSPC/2/PT.05S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:1 second
Stop:2016-09-14 07:56:57 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fast time resolution (50ms) Bremsstrahlung X-ray spectrum.

4) Van Allen Probe B MAG X, Y, and Z maxmize
Resource ID:spase://ViRBO/NumericalData/BAR/1A/L2/MAGN/2/PT.25S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:1 second
Stop:2016-09-14 07:56:57 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
MAG X, Y, and Z

5) Van Allen Probe B Rate counters for scintillator diagnostics. maxmize
Resource ID:spase://ViRBO/NumericalData/BAR/1A/L2/RCNT/2/PT4S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:1 second
Stop:2016-09-14 07:56:57 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Rate counters for scintillator diagnostics.

6) Van Allen Probe B Slow time resolution (32s) X-ray spectrum maxmize
Resource ID:spase://ViRBO/NumericalData/BAR/1A/L2/SSPC/2/PT.03125S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:1 second
Stop:2016-09-14 07:56:57 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Slow time resolution (32s) X-ray spectrum

7) Van Allen Probe A ECT HOPE Spin averaged Level 2 Science Data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/ECT/HOPE/SCI-L2/PT24S
Start:2012-10-26 00:00:02 Observatory:Radiation Belt Storm Probe Satellite Cadence:24 seconds
Stop:2016-09-14 07:59:50 Instrument:Energetic Particle, Composition and Thermal Plasma Suite (ECT) Resource:NumericalData
This data set contains electron fluxes and proton fluxes measured by the Helium Oxygen Proton Electron (HOPE), which is one of three instruments on the Energetic Particle, Composition and Thermal Plasma Suite (ECT). As a mass spectrometer instrument, HOPE uses an electrostatic top-hat analyzer and time-gated coincidence detectors to measure electrons, protons, and helium and oxygen ions with energies from less than or equal to 20 eV or spacecraft potential (whichever is greater) to greater than or equal to 45 keV while rejecting penetrating backgrounds. Spectral measurements for both ions and electrons are acquired over 1 eV to 50 keV in 36 log-spaced steps at an energy resolution ?EFWHM/E ~15%. The dominant ion species (H+, He+, and O+) of the magnetosphere are identified using foil-based time-of-flight mass (TOF) spectrometry with channel electron multiplier (CEM) detectors. Angular measurements are derived using five polar pixels in a plane perpendicular to the spacecraft spin axis, and up to 16 azimuthal bins are acquired for each polar pixel over time as the spacecraft spins. Electrons and protons are measured in alternate spin cadence of 5 per minute.

8) Van Allen Probe A ECT HOPE Spin resolved Level 3 Science Data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/ECT/HOPE/SCI-L3/PT20S
Start:2012-10-13 15:00:24 Observatory:Radiation Belt Storm Probe Satellite Cadence:20 seconds
Stop:2016-09-14 07:59:50 Instrument:Energetic Particle, Composition and Thermal Plasma Suite (ECT) Resource:NumericalData
This data set contains spin resolved data from the Van Allen Probe A ECT HOPE plasma spectrometer. Plasma moments from electrons >200 eV and ions >30 eV are measured at apogee in alternate spin cadence. Please check the Data Quality and Caveats page on the ECT home page and contact the ECT team for known data issues

9) Van Allen Probe A ECT HOPE Pitch angle resolved Level 3 Science Data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/ECT/HOPE/SCI-L3/PT60S
Start:2012-10-13 15:00:36 Observatory:Radiation Belt Storm Probe Satellite Cadence:60 seconds
Stop:2016-09-14 07:59:50 Instrument:Energetic Particle, Composition and Thermal Plasma Suite (ECT) Resource:NumericalData
This data set contains pitch angle resolved data from the Van Allen Probe A ECT HOPE plasma spectrometer. Electrons and ion species (H+, He+, and O+) are measured over 1 eV to 50 keV in 36 log-spaced steps in alternate spin cadence. Note that there are no correections performed on the data (e.g. background subtraction, velocity corrections, etc.) Please check the Data Quality and Caveats page on the ECT home page and contact the ECT team for known data issues.

10) Van Allen Probe A MagEIS Level 2 data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/ECT/MAGEIS/PT24S
Start:2012-09-15 00:00:01 Observatory:Radiation Belt Storm Probe Satellite Cadence:24 seconds
Stop:2016-09-14 07:59:50 Instrument:Energetic Particle, Composition and Thermal Plasma Suite (ECT) Resource:NumericalData
This data set contains electron and proton fluxes from the Magnetic Electron Ion Spectrometer (MagEIS), which is one of three instruments on the Energetic Particle, Composition and Thermal Plasma Suite (ECT). MagEIS uses magnetic focusing and pulse height analysis from a set of four magnetic spectrometers covering three distinct energy ranges: Low (20 keV-1 MeV), Medium (Med35 and Med75 units), and High (700 keV to 4 MeV). Two identical Medium energy units on each Van Allen Probe spacecraft point in different directions to increase pitch angle coverage. Electrons enter the MagEIS aperture and are bent by the magnetic field through 180 with energy-dependent diameters. Electrons are additionally energy-analyzed by an array of solid state detectors to ensure extremely clean differentiation between primary electron measurements and contaminating background radiation. In addition, the MagEIS High spectrometer contains a solid state telescope that measures protons from roughly 50 keV to 20 MeV, Helium ions from roughly 300 keV - 1.5 MeV and Oxygen ions from roughly 1-5 MeV. Electrons and protons are measured in alternate spacecraft spin resolution of 5 per minute.

11) Van Allen Probe A Relativistic Electron Proton Telescope, Level 2 Science Data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/ECT/REPT/SCI_L2/PT24S
Start:2012-09-01 11:38:18 Observatory:Radiation Belt Storm Probe Satellite Cadence:24 seconds
Stop:2016-09-14 07:59:50 Instrument:Energetic Particle, Composition and Thermal Plasma Suite (ECT) Resource:NumericalData
This data set contains electron fluxes and proton fluxes measured by the Relativistic Electron Proton Telescope (REPT), which is one of three instruments on the Energetic Particle, Composition and Thermal Plasma Suite (ECT). REPT points perpendicular to the spin axis of the spacecraft and measures high-energy electrons (2-20 MeV). It also measures magnetospheric and solar protons in the energy range of 20-120 MeV to capture most intense events. REPT was designed to measure the directional electron intensities (in the range 10-2?106 particles/cm2 s-sr-MeV) and energy spectra (?E/E ? 25 %) throughout the slot and outer radiation belt region. Electrons and protons are measured in alternate spin cadence of 5 per minute.

12) Van Allen Probe A Relativistic Electron Proton Telescope, Level 3 Science Data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/ECT/REPT/SCI_L3/PT24S
Start:2012-09-01 11:38:18 Observatory:Radiation Belt Storm Probe Satellite Cadence:24 seconds
Stop:2016-09-14 07:59:50 Instrument:Energetic Particle, Composition and Thermal Plasma Suite (ECT) Resource:NumericalData
This data set contains Level 3 pitch angle sorted electron and proton fluxes from the Relativistic Electron Proton Telescope (REPT), which is one of three instruments on the Energetic Particle, Composition and Thermal Plasma Suite (ECT) onboard Van Allen Probe A. REPT points perpendicular to the spin axis of the spacecraft and measures high-energy electrons (4-10 MeV). It also measures magnetospheric and solar protons in the energy range of 20-75 MeV to capture most intense events. Please check the Data Quality and Caveats page on the ECT home page and contact the ECT team for known data issues.

13) Van Allen Probe A EFW Burst 1 waveform data in UVW coordinates E, MSC and V maxmize
Resource ID:spase://VWO/NumericalData/RBSP/A/EFW/L1_B1/PT0.002S
Start:2012-09-05 14:36:16 Observatory:Radiation Belt Storm Probe Satellite Cadence:0.00195 seconds
Stop:2016-09-14 08:00:14 Instrument:Electric Field and Waves Suite (EFW) Resource:NumericalData
The EFW burst modes provide targeted measurements over brief time intervals of 3-d electric fields, 3-d wave magnetic fields (from the EMFISIS magnetic search coil sensors), and spacecraft potential. BURST1(B1): Medium-Rate (512 samples/s nominal) BURST2(B2): Higher-rate (16384 samples/s nominal) The burst 1 mode includes three components of the electric field (E12_B1, E34_B1, E56_B1), six components of the spacecraft?sensor potential (V1_B1 through V6_B1), and three components of the AC magnetic field from the EMFISIS search coil magnetometer (SCM_U_B1, SCM_V_B1, SCM_W_B1). The burst 2 mode data returns a similar complement of electric field (E_12ac_B2, E34ac_B2, E56ac_B2), search coil (SCM_B2, SCM_2B2, and SCM_B2) and single ended measurements (V1ac_B1 through V6ac_B2) with the exception that in the default mode the single ended and electric field signals are AC coupled with a higher gain. All quantities are in ?uvw? coordinates where ?u? and ?v? are the sensor coordinates rotating with the spacecraft and ?w? points along the spin axis. Burst waveform CDF files are available. The three data types available are the electric field ?E?, the searchcoil magnetic field ?MSC?, and antenna potential ?V?. The suffix on each of these is either ?B1? or ?B2?. B1, or burst 1 is the human-in-the-loop burst, meaning that both collection and playback (for arbitrary lengths of time) are requested on the ground. B2, or burst 2 is automatically telemetered as short bursts based on an onboard triggering algorithm, typically set so trigger on large amplitude signals near 1 kHz. Sample rates for B1 and B2 can and are changed depending on varying science goals.

14) Van Allen Probe A EFW Burst 2 waveform data in UVW coordinates E, MSC and V maxmize
Resource ID:spase://VWO/NumericalData/RBSP/A/EFW/L1_B2/PT0.00006S
Start:2012-09-05 14:36:16 Observatory:Radiation Belt Storm Probe Satellite Cadence:0.000061 seconds
Stop:2016-09-14 08:00:15 Instrument:Electric Field and Waves Suite (EFW) Resource:NumericalData
The EFW burst modes provide targeted measurements over brief time intervals of 3-d electric fields, 3-d wave magnetic fields (from the EMFISIS magnetic search coil sensors), and spacecraft potential. BURST1(B1): Medium-Rate (512 samples/s nominal) BURST2(B2): Higher-rate (16384 samples/s nominal) The burst 1 mode includes three components of the electric field (E12_B1, E34_B1, E56_B1), six components of the spacecraft?sensor potential (V1_B1 through V6_B1), and three components of the AC magnetic field from the EMFISIS search coil magnetometer (SCM_U_B1, SCM_V_B1, SCM_W_B1). The burst 2 mode data returns a similar complement of electric field (E_12ac_B2, E34ac_B2, E56ac_B2), search coil (SCM_B2, SCM_2B2, and SCM_B2) and single ended measurements (V1ac_B1 through V6ac_B2) with the exception that in the default mode the single ended and electric field signals are AC coupled with a higher gain. All quantities are in ?uvw? coordinates where ?u? and ?v? are the sensor coordinates rotating with the spacecraft and ?w? points along the spin axis. Burst waveform CDF files are available. The three data types available are the electric field ?E?, the searchcoil magnetic field ?MSC?, and antenna potential ?V?. The suffix on each of these is either ?B1? or ?B2?. B1, or burst 1 is the human-in-the-loop burst, meaning that both collection and playback (for arbitrary lengths of time) are requested on the ground. B2, or burst 2 is automatically telemetered as short bursts based on an onboard triggering algorithm, typically set so trigger on large amplitude signals near 1 kHz. Sample rates for B1 and B2 can and are changed depending on varying science goals.

15) Van Allen Probe A 32 sample/sec despun electric field in modified-GSE (MGSE) coordinates maxmize
Resource ID:spase://VWO/NumericalData/RBSP/A/EFW/L2_ESVY_DESPUN/PT0.031S
Start:2012-09-05 00:00:00 Observatory:Radiation Belt Storm Probe Satellite Cadence:0.031 seconds
Stop:2016-09-14 08:00:14 Instrument:Electric Field and Waves Suite (EFW) Resource:NumericalData
These high time resolution de-spun data are EFW measurements of the spin plane electric field at 32 samples/s. These data are presented in the MGSE system. Special care should be taken in its use. The EFW instrument can be sensitive to the low energy plasma environment and spacecraft effects in ways that other instruments are not. Users should read the "RBSP/EFW Data Required Reading" document for more details. In addition, mismatches between the responses of the different probes can introduce error signals. A preliminary check of the quality of this data may be carried out by comparing the rotated 32 sample/s electric field in the high time resolution CDF to the spin fit data found in the spin fit CDFs. In order to carry out this comparison the high time resolution data should be averaged down to the spin period to eliminate the higher frequency turbulence.

16) Van Allen Probe A EFW Filterbank Data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EFW/L2_FBK/PT0.125S
Start:2012-09-05 15:01:53 Observatory:Radiation Belt Storm Probe Satellite Cadence:
Stop:2016-09-14 07:59:50 Instrument:Electric Field and Waves Suite (EFW) Resource:NumericalData
This data set contains Level 2 filterbank data from the Electric Field and Waves Suite (EFW) onboard Van Allen Probe A. Average power and peak amplitudes from either 7 (default) or 13 logarithmically spaced band-pass filters are measured between 0.8 Hz and 6.5 kHz sampled at a cadence of 8 samples/s. Two sources may be input into the filter banks at any one time. The possible sources include:.E12DC,E34DC,E56DC,.E12AC,E34AC,E56AC,.SCMU,SCMV,SCMW.(V1DC+V2DC+V3DC+V4DC)/4. In the default mode, V12ac, the AC coupled measurement of the electric field from sensors 1 and 2 in the spin plane is input into the first filter bank and SCMw, the spin axis component of the search coil magnetic field, serves as input into the second filter bank. The broadband filters provide a continuous stream of survey mode measurements over the entire orbit providing information on rapid time variations and bursty wave activity over a broad frequency spectrum. These measurements are also used as an input to burst trigger algorithms. All these quantities, the nature of the on board signal processing, their filtering, time resolution and their respective coordinate systems are described in the EFW instrument paper (Wygant et al. 2013).

17) Van Allen Probe A Spectrogram Data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EFW/L2_SPEC/PT4S
Start:2012-09-05 14:36:01 Observatory:Radiation Belt Storm Probe Satellite Cadence:
Stop:2016-09-14 07:59:50 Instrument:Electric Field and Waves Suite (EFW) Resource:NumericalData
This data set contains Level 2 wave electric field and search coil wave magnetic fields spectral data from the Electric Field and Waves Suite (EFW) onboard Van Allen Probe A. Spectrograms between ~40 Hz and ~8 kHz are calculated on-board the EFW instrument every 4 seconds. These data include one component of the ac-coupled electric field from the rotating V12 sensors (V12ac). The electric field quantity is labeled EFW/L2. Also included are two components of the wave magnetic field from the University of Iowa EMFISIS sensors. The search coil quantities are labeled EFW/L2 spec64 smu. In the labels  “smu” and “smv”, the suffixes “u” and “v” refer to the u and v sensor coordinates rotating with the spacecraft. All these quantities, the nature of the on board signal processing, their filtering, time resolution and their respective coordinate systems are described in the EFW instrument paper (Wygant et al. 2013). When the spectral CDF is opened, many other possible quantities are listed which have no data in them. Possible sources include: E12dc, E34dc, E56dc, E12ac, E34ac, E56ac, E DC parallel, E DC perpendicular 1, E DC perpendicular 1, E AC parallel, E AC perpendicular 1, E AC perpendicular 2, V1+V2+V3+V4/4AC, SCMu, SCMv, SCMw, SCM parallel, SCM perpendicular 1 and SCM perpendicular 2. Those without data are “place holder quantities” which are used by other instrument modes not currently selected. Examples of the spectral data may be found in Principal Investigator's on-line survey data plots.  EMFISIS instrument wave data may be found on the University of Iowa website. This includes valuable spectral electric field data up to 400 kHz and magnetic field data up to about ~6 kHz.

18) Van Allen Probe A Spin-fit Electric field in modified-GSE (MGSE) coord, density, and other products maxmize
Resource ID:spase://VWO/NumericalData/RBSP/A/EFW/L3/PT11S
Start:2012-09-18 00:00:06 Observatory:Radiation Belt Storm Probe Satellite Cadence:11 seconds
Stop:2016-09-14 08:00:15 Instrument:Electric Field and Waves Suite (EFW) Resource:NumericalData
This data set contains Level 3 wave electric field and search coil wave magnetic fields data from the Electric Field and Waves Suite (EFW) onboard Van Allen Probe A. The spin-fit electric field (spin period resolution) tends to be the most accurate electric field measurement. However, as always, due diligence by the user/scientists must be exercised in using these data. The spin-fit electric field is provided in both an inertial and co-rotating frame. The electric field is presented in a MGSE (modified GSE) coordinate system. We provide two components (Y MGSE and Z MGSE) of the electric field. Both components are in the spin plane of the spacecraft and are measured with the long 50 m booms. The X MGSE component is along the spin-axis. The spin-axis of the spacecraft is oriented within 37 degrees of the Earth sun line. So the Y GSE direction is most nearly aligned with the Y MGSE axis and the Z MGSE direction is most nearly aligned with Z GSE.

19) Van Allen Probe A Spinfit DC Electric Field estimates in M-GSE coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EFW/MGSE/PT11S
Start:2012-09-05 14:36:16 Observatory:Radiation Belt Storm Probe Satellite Cadence:11 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric Field and Waves Suite (EFW) Resource:NumericalData
This data set contains spinfit DC Electric Field estimates in M-GSE coordinates that are measured by the Electric Field and Waves Suite (EFW) onboard Van Allen Probe A. One 2D vector estimate of the E-field is computed at a cadence of once per spin period (typically 10.7 to 11.1 s) using the survey E-field data product - the potential difference between EFW sensors V1 and V2 (E12) sampled at a nominal rate of 32 samp/s with a resolution of 16 bits. The X-component of the E-field estimate, corresponding to the axial component in the spacecraft coordinate system, is set to zero in this data product. See the EFW-FAQ (http://rbsp.space.umn.edu/efw_faq.html) for a discussion of this convention for this data product. The VxB electric field in the spacecraft frame due to orbital motion of the spacecraft around the Earth as computed from the spacecraft orbital velocity and measured B-field in the spacraft frame has been subtracted from the measured electric field, and so the data product is in the quasi-inertial frame equivalent to GSE (i.e. it is NOT in the corotation frame of the Earth!). Each spin fit is time-tagged with the time corresponding to the middle of the spin of data that went into the spin fit algorithm; in other words, if a given spin covers the interval (t1, t2), then the spin fit E-field estimate associated with that spin is given the time tag 0.5*(t1 + t2). The root mean square residual between the data included in the fit and the resulting best-fit model, sigma, and the final number of points included in the spin fit, npts, are also provided at spin-period cadence. The nominal dynamic range of the E-field estimate is +/- 1 V/m in any component.

20) Van Allen Probe A High Resolution DC Electric Field in UVW Coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EFW/UVW
Start:2012-09-25 00:00:07 Observatory:Radiation Belt Storm Probe Satellite Cadence:
Stop:2016-09-14 07:59:50 Instrument:Electric Field and Waves Suite (EFW) Resource:NumericalData
This data set contains high-resolution DC Electric Field data in UVW coordinates as measured by the Electric Field and Waves Suite (EFW) onboard Van Allen Probe A. As a reference for spin axis vector in GSE, there was no spinning-frame offset removal.

21) Van Allen Probe A DC-coupled EFW 1-second sensor potentials relative to spacecraft in volts maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EFW/VSVY/PT1S
Start:2012-09-05 14:36:00 Observatory:Radiation Belt Storm Probe Satellite Cadence:1 second
Stop:2016-09-14 07:59:50 Instrument:Electric Field and Waves Suite (EFW) Resource:NumericalData
This data set contains DC-coupled sensor potentials and negative of spacecraft potential relative to sensor floating potentials from the Electric Field and Waves Suite (EFW) onboard Van Allen Probe A. All six EFW sensor potentials are included. Also included are average potentials from opposing booms, i.e., (V1+V2)/2, (V3+V4)/2, and (V5+V6)/2, from autoscale and fixed scale (-15 to 5 V). These quantities are the negative of the spacecraft potential relative to the sensor floating potential, and have the contribution from the external electric field removed. Four spin-plane components of the electric field are measured at DC-12 Hz with 0.05 mV/m accuracy, and two spin-axis components, with ~3 mV/m accuracy. Spacecraft potentials cover cold plasma densities of 0.1 to ~100 cm-3 at 1-second cadence. The default sampling rate is 16 samp/s at 16-bit resolution, covering a +/- 225-V range. Further details on the EFW instrument in general or these data in particular can be found in the EFW Instrument paper, Wygant et al., 2013 (Space Science Reviews; submitted, 02/2013).

22) Van Allen Probe A Fluxgate Magnetometer high resolution data in GEI coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/GEI/PT0.015625S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:0.015625 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fluxgate magnetometer data - Craig Kletzing (University of Iowa)

23) Van Allen Probe A Fluxgate Magnetometer 1 second resolution data in GEI coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/GEI/PT1S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:1 second
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fluxgate magnetometer data - Craig Kletzing (University of Iowa)

24) Van Allen Probe A Fluxgate Magnetometer 4 second resolution data in GEI coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/GEI/PT4S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:4 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fluxgate magnetometer data - Craig Kletzing (University of Iowa)

25) Van Allen Probe A Fluxgate Magnetometer hight resolution data in GEO coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/GEO/PT0.015625S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:0.015625 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fluxgate magnetometer data - Craig Kletzing (University of Iowa)

26) Van Allen Probe A Fluxgate Magnetometer 1 second resolution data in GEO coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/GEO/PT1S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:1 second
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fluxgate magnetometer data - Craig Kletzing (University of Iowa)

27) Van Allen Probe A Fluxgate Magnetometer 4 second resolution data in GEO coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/GEO/PT4S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:4 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fluxgate magnetometer data - Craig Kletzing (University of Iowa)

28) Van Allen Probe A Fluxgate Magnetometer high resolution data in GSE coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/GSE/PT0.015625S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:0.015625 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fluxgate magnetometer data - Craig Kletzing (University of Iowa)

29) Van Allen Probe A Fluxgate Magnetometer 1 second resolution data in GSE coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/GSE/PT1S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:1 second
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fluxgate magnetometer data - Craig Kletzing (University of Iowa)

30) Van Allen Probe A Fluxgate Magnetometer 4 second resolution data in GSE coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/GSE/PT4S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:4 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fluxgate magnetometer data - Craig Kletzing (University of Iowa)

31) Van Allen Probe A Fluxgate Magnetometer high resolution data in GSM coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/GSM/PT0.015625S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:0.015625 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fluxgate magnetometer data - Craig Kletzing (University of Iowa)

32) Van Allen Probe A Fluxgate Magnetometer 1 second resolution data in GSM coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/GSM/PT1S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:1 second
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fluxgate magnetometer data - Craig Kletzing (University of Iowa)

33) Van Allen Probe A Fluxgate Magnetometer 4 second resolution data in GSM coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/GSM/PT4S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:4 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fluxgate magnetometer data - Craig Kletzing (University of Iowa)

34) Van Allen Probe A Single Axis AC Electric Field Spectra burst data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/HFR-SPECTRA-BURST/PT6S
Start:2012-09-01 21:25:35 Observatory:Radiation Belt Storm Probe Satellite Cadence:6 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Single Axis AC Electric Field Spectra ~5-10,000 Hz - Craig Kletzing (University of Iowa)

35) Van Allen Probe A Single Axis AC Electric Field Spectra merged data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/HFR-SPECTRA-MERGED/PT6S
Start:2012-09-01 00:00:02 Observatory:Radiation Belt Storm Probe Satellite Cadence:6 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Single Axis AC Electric Field Spectra ~5-10,000 Hz - Craig Kletzing (University of Iowa)

36) Van Allen Probe A Single Axis AC Electric Field Spectra data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/HFR-SPECTRA/PT6S
Start:2012-08-30 02:12:39 Observatory:Radiation Belt Storm Probe Satellite Cadence:6 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Single Axis AC Electric Field Spectra ~5-10,000 Hz - Craig Kletzing (University of Iowa)

37) Van Allen Probe A high frequency receiver waveform data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/HFR-WAVEFORM
Start:2012-09-01 21:03:07 Observatory:Radiation Belt Storm Probe Satellite Cadence:
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
High Frequency Receiver (HFR) Field Waveform Samples in V/m (Selectable between the U, V and W Axes) - Craig Kletzing (University of Iowa)

38) Van Allen Probe A Fluxgate Magnetometer high resolution data in SM coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/SM/PT0.015625S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:0.015625 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fluxgate magnetometer data - Craig Kletzing (University of Iowa)

39) Van Allen Probe A Fluxgate Magnetometer 1 second resolution data in SM coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/SM/PT1S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:1 second
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fluxgate magnetometer data - Craig Kletzing (University of Iowa)

40) Van Allen Probe A Fluxgate Magnetometer 4 second resolution data in SM coordinates maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/SM/PT4S
Start:2012-10-08 00:00:03 Observatory:Radiation Belt Storm Probe Satellite Cadence:4 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fluxgate magnetometer data - Craig Kletzing (University of Iowa)

41) Van Allen Probe A UVW Science Coordinates data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/UVW
Start:2012-09-08 00:00:05 Observatory:Radiation Belt Storm Probe Satellite Cadence:
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
Fluxgate magnetometer data - Craig Kletzing (University of Iowa)

42) Van Allen Probe A WFR Spectral Matrix diagonal merged data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/WFR-SPECTRAL-MATRIX-DIAGONAL-MERGED/PT6S
Start:2012-09-01 00:00:02 Observatory:Radiation Belt Storm Probe Satellite Cadence:6 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
WaveForm Receiver (WFR) Spectral Matrix ~5-10,000 Hz (Merged, Diagonal Elements Only) - Craig Kletzing (University of Iowa)

43) Van Allen Probe A WFR Spectral Matrix data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/WFR-SPECTRAL-MATRIX-DIAGONAL/PT6S
Start:2012-08-30 22:55:42 Observatory:Radiation Belt Storm Probe Satellite Cadence:6 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
WaveForm Receiver (WFR) Spectral Matrix ~5-10000 Hz (Diagonal Elements Only) - Craig Kletzing (University of Iowa)

44) Van Allen Probe A WFR waveform continuous burst data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/WFR-WAVEFORM-CONTINUOUS-BURST/PT6S
Start:2012-09-01 22:14:55 Observatory:Radiation Belt Storm Probe Satellite Cadence:6 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
WaveForm Receiver (WFR) Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV, BW) continuous burst waveforms @ 35 kS/sec - Craig Kletzing (University of Iowa)

45) Van Allen Probe A WFR waveform data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/EMFISIS/WFR-WAVEFORM/PT6S
Start:2012-08-30 23:00:36 Observatory:Radiation Belt Storm Probe Satellite Cadence:6 seconds
Stop:2016-09-14 07:59:50 Instrument:Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) Resource:NumericalData
WFR Three Axis Electric Field (EU, EV, EW) and Three Axis Magnetic field (BU, BV, BW) waveforms as 16384 samples @ 35 kS/sec - Craig Kletzing (University of Iowa)

46) Van Allen Probe A 1-min Position Data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/Ephemeris/PT12M
Start:2012-08-30 00:00:00 Observatory:Radiation Belt Storm Probe Satellite Cadence:12 minutes
Stop:2016-09-14 07:59:50 Instrument:RBSP A Positions Resource:NumericalData
RBSP A satellite position and magnetic field model information.

47) Van Allen Probe A RBSPICE High Energy Resolution Electron Rates converted Level-2 data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/RBSPICE/L2/ESRHELT
Start:2012-11-13 22:06:46 Observatory:Radiation Belt Storm Probe Satellite Cadence:
Stop:2016-09-14 07:59:50 Instrument:Radiation Belt Storm Probes Ion Composition Experiment (RBSPICE) Resource:NumericalData
This data set contains Van Allen Probe A RBSPICE (Radiation Belt Storm Probes Ion Composition Experiment) high-energy resolution electron rates that are measured at low-time resolution. Unidirectional Differential Electron Flux (FEDU) measured by 6 telescopes in 64 channels from ~0.02-1.0 MeV are available in physical units (counts/(s*sr*cm^2*MeV) by telescope in sector order (T0= ~110 PA, T3= ~all PAs, T5= FEDU background). Also available are percentage error of measurement, quality flag, current sector number where each spin is dividied into 36 sectors, duration of the accumulation, current spin number of the spacecraft, orbit number, dipole L using the SM reference frame, and position of the spacecraft in SM coordinates.

48) Van Allen Probe A RBSPICE Low Energy Resolution Electron Rates converted Level-2 data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/RBSPICE/L2/ESRLEHT
Start:2012-11-13 22:06:46 Observatory:Radiation Belt Storm Probe Satellite Cadence:
Stop:2016-09-14 07:59:50 Instrument:Radiation Belt Storm Probes Ion Composition Experiment (RBSPICE) Resource:NumericalData
This data set contains Van Allen Probe A RBSPICE (Radiation Belt Storm Probes Ion Composition Experiment) low-energy resolution electron rates that are measured at high-time resolution. Unidirectional Differential Electron Flux (FEDU) measured by 6 telescopes in 14 channels from ~0.02-1.0 MeV are available in physical units (counts/(s*sr*cm^2*MeV) by telescope in sector order (T0= ~110 PA, T3= ~all PAs, T5= FEDU background). Also available are percentage error of measurement, quality flag, current sector number where each spin is dividied into 36 sectors, duration of the accumulation, current spin number of the spacecraft, orbit number, dipole L using the SM reference frame, and position of the spacecraft in SM coordinates.

49) Van Allen Probe A RBSPICE High Energy Resolution Ion Species Rates converted Level-2 data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/RBSPICE/L2/ISRHELT
Start:2012-10-29 00:01:17 Observatory:Radiation Belt Storm Probe Satellite Cadence:
Stop:2016-09-14 07:59:50 Instrument:Radiation Belt Storm Probes Ion Composition Experiment (RBSPICE) Resource:NumericalData
This data set contains Van Allen Probe A RBSPICE (Radiation Belt Storm Probes Ion Composition Experiment) high-energy resolution ion rates that are measured at low-time resolution. Ion species measured by 6 telescopes in 64 channels from ~0.05-1.0 MeV are available in physical units (counts/(s*sr*cm^2*MeV) by telescope in sector order (T0= ~110 PA, T3= ~all PAs, T5= ~70 PA). Also available are percentage error of measurement, quality flag, current sector number where each spin is dividied into 36 sectors, duration of the accumulation, current spin number of the spacecraft, orbit number, dipole L value calculated using the SM reference frame, and position of the spacecraft in SM coordinates.

50) Van Allen Probe A RBSPICE TOF x Energy Hydrogen Rates converted Level-2 data maxmize
Resource ID:spase://VSPO/NumericalData/RBSP/A/RBSPICE/L2/TOFXEH
Start:2013-01-26 10:04:16 Observatory:Radiation Belt Storm Probe Satellite Cadence:
Stop:2016-09-14 07:59:50 Instrument:Radiation Belt Storm Probes Ion Composition Experiment (RBSPICE) Resource:NumericalData
This data set contains Van Allen Probe A RBSPICE (Radiation Belt Storm Probes Ion Composition Experiment) TOF x energy proton rates that are measured at high-energy and low-time resolution by 6 telescopes in 14 channels from ~0.02-1.0 MeV are available in physical units (counts/(s*sr*cm^2*MeV) by telescope in sector order. Also available are percentage error of measurement, quality flag, current sector number where each spin is dividied into 36 sectors, duration of the accumulation, current spin number of the spacecraft, orbit number, dipole L value using the SM reference frame, and position of the spacecraft in SM coordinates.

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