FPI Datasets
Fast Plasma Investigation (FPI)
The Fast Plasma Investigation (FPI) includes four dual electron spectrometers (DES) and four dual ion spectrometers (DIS) per spacecraft. When the data from the two sets of four dual-spectrometers are combined, FPI is able to provide the velocity-space distribution of electrons from 10 eV to 30 keV and ions from 10 eV to 30 keV with a time resolution of 30 ms, and 150 ms, respectively (Pollock et al., 2014).>.
For questions about the technical details of FPI or its data products, contact the FPI Lead Co-I: Daniel Gershman, NASA GSFC
For questions about the technical details of FPI or its data products, contact the FPI Lead Co-I: Daniel Gershman, NASA GSFC
Version Release Notes
Users interested in FPI data are strongly encouraged to familiarize themselves with the Version Release Notes, the full extent of which are included in the following pdf:
FPI Version Release Notes.
Included in the Version Release Notes are Caveats, Known features, and Helpful information on how to use and interpret the data. Any questions regarding the data should be addressed to the FPI science team.
FPI Version Release Notes.
Included in the Version Release Notes are Caveats, Known features, and Helpful information on how to use and interpret the data. Any questions regarding the data should be addressed to the FPI science team.
MMS-4 FPI Anomaly
NOTICE TO ALL FPI DATA USERS
On 7 June 2018 12:43 UTC, the MMS Fast Plasma Investigation (FPI) suffered its first impactful flight anomaly since launching in March, 2015. The electron spectrometer pair at quadrant 1 on MMS4 experienced a failure that appears non-recoverable. The symptoms – repeatable after further contact, reset, and commanding of the instrument – were a sustained high current draw and the absence of counts from this spectrometer pair. The spectrometer pair has been turned off. On 15 July 2018 00:47 UTC, the MMS FPI suffered its second impactful flight anomaly. The electron spectrometer pair at quadrant 0 on MMS4 experienced a similar failure that appears to be non-recoverable and this unit was also turned off. These failures appear to be unrelated.
One half of the contiguous solid angle space in each electron plasma distribution on the MMS4 spacecraft is impacted. To mitigate the scientific impact, level 2 MMS4 DES fast survey and burst distribution (des-dist) files reflecting post-anomaly data will contain fill data for angle space affected by the sensor outages. Lower temporal resolution MMS4 DES fast survey moments (des-moms) files for post-anomaly data will also be released. The FPI ground system team is continuing to analyze options for potential release of MMS4 DES post-anomaly burst moments.
There remain a full complement of operational spectrometers on the other three MMS spacecraft. In addition, the FPI ion spectrometers and corresponding MMS4 FPI ion data is also unaffected.
Further inquiries may be directed to the FPI Lead Co-I, Barbara Giles, at barbara.giles@nasa.gov.
On 7 June 2018 12:43 UTC, the MMS Fast Plasma Investigation (FPI) suffered its first impactful flight anomaly since launching in March, 2015. The electron spectrometer pair at quadrant 1 on MMS4 experienced a failure that appears non-recoverable. The symptoms – repeatable after further contact, reset, and commanding of the instrument – were a sustained high current draw and the absence of counts from this spectrometer pair. The spectrometer pair has been turned off. On 15 July 2018 00:47 UTC, the MMS FPI suffered its second impactful flight anomaly. The electron spectrometer pair at quadrant 0 on MMS4 experienced a similar failure that appears to be non-recoverable and this unit was also turned off. These failures appear to be unrelated.
One half of the contiguous solid angle space in each electron plasma distribution on the MMS4 spacecraft is impacted. To mitigate the scientific impact, level 2 MMS4 DES fast survey and burst distribution (des-dist) files reflecting post-anomaly data will contain fill data for angle space affected by the sensor outages. Lower temporal resolution MMS4 DES fast survey moments (des-moms) files for post-anomaly data will also be released. The FPI ground system team is continuing to analyze options for potential release of MMS4 DES post-anomaly burst moments.
There remain a full complement of operational spectrometers on the other three MMS spacecraft. In addition, the FPI ion spectrometers and corresponding MMS4 FPI ion data is also unaffected.
Further inquiries may be directed to the FPI Lead Co-I, Barbara Giles, at barbara.giles@nasa.gov.
FPI Data Variables
Click on the dataset name for information about the file content.
Note: Due to the number of variables in each file, not all are shown below.
Note: Due to the number of variables in each file, not all are shown below.
Level-2 Fast Survey Distributions | ||||
File Name Pattern: MMS[1,2,3,4]_FPI_FAST_L2_DES-DIST_YYYYMMDDHHMMSS_V2.1.0.cdf | ||||
File Name Pattern: MMS[1,2,3,4]_FPI_FAST_L2_DIS-DIST_YYYYMMDDHHMMSS_V2.1.0.cdf | ||||
Sensor | Data Mode | Variable Name | Units | Comments |
DES/DIS | Fast | EPOCH | ns | Survey data acquisition time; derived from packet time. |
DES/DIS | Fast/td> | MMS |
d | Az bin: sector ind=00 looks "after" (spin-phase) Sun, ..., sector ind=31 looks "before" Sun dir. Head field-of-view: pixel index=00 looks to zenith, ..., pixel index=15 looks to nadir. FPI operations nominally bin data from 64 energy filters into 32 pairwise energy bins, indexed 0-31. Nominally, bins are indexed in increasing energy order. See FPI docs for details. |
DES/DIS | Fast/td> | MMS |
[# / {(cm/s)3 * cc}] | Az bin: sector ind=00 looks "after" (spin-phase) Sun, ..., sector ind=31 looks "before" Sun dir. Head field-of-view: pixel index=00 looks to zenith, ..., pixel index=15 looks to nadir. FPI operations nominally bin data from 64 energy filters into 32 pairwise energy bins, indexed 0-31. Nominally, bins are indexed in increasing energy order. See FPI docs for details. |
DES/DIS | Fast | MMS |
degrees | Pixel zenith angles. |
DES/DIS | Fast | MMS |
eV | Geometric mean of parity 0 and parity 1 energies in the 64-step FPI energy table. |
DES/DIS | Fast | MMS |
degrees | Azimuth Angles |
Level-2 DES Burst Distributions. | ||||
File Name Pattern: MMS[1,2,3,4]_FPI_BRST_L2_DES-DIST_YYYYMMDDHHMMSS_V2.1.0.cdf | ||||
Sensor | Data Mode | Variable Name | Units | Comments |
DES | Burst | Epoch | ns | Survey data acquisition time; derived from packet time. |
DES | Burst | MMS |
degrees | MMS1 FPI/DES burst sky-map instrument azimuthal angles |
DES | Burst | MMS |
[# / {(cm/s)3 * cc}] | Az bin: sector ind=00 looks "after" (spin-phase) Sun, ..., sector ind=31 looks "before" Sun dir. Head field-of-view: pixel index=00 looks to zenith, ..., pixel index=15 looks to nadir. FPI operations nominally bin data from 64 energy filters into 32 pairwise energy bins, indexed 0-31. Nominally, bins are indexed in increasing energy order. See FPI docs for details. |
DES | Burst | MMS |
[# / {(cm/s)3 * cc}] | Az bin: sector ind=00 looks "after" (spin-phase) Sun, ..., sector ind=31 looks "before" Sun dir. Head field-of-view: pixel index=00 looks to zenith, ..., pixel index=15 looks to nadir. FPI operations nominally bin data from 64 energy filters into 32 pairwise energy bins, indexed 0-31. Nominally, bins are indexed in increasing energy order. See FPI docs for details. |
DES | Burst | MMS |
eV | Odd energies (parity 1) in the 64-step FPI energy table |
DES | Burst | MMS |
eV | Even energies (parity 0) in the 64-step FPI energy table |
Level-2 DIS Burst Distributions | ||||
File Name Pattern: MMS[1,2,3,4]_FPI_BRST_L2_DIS-DIST_YYYYMMDDHHMMSS_V2.1.0.cdf | ||||
Sensor | Data Mode | Variable Name | Units | Comments |
DIS | Burst | Epoch | ns | Survey data acquisition time; derived from packet time. |
DIS | Burst | MMS |
degrees | MMS FPI/DIS burst sky-map instrument azimuthal angles |
DIS | Burst | MMS |
[# / {(cm/s)3 * cc}] | Az bin: sector ind=00 looks "after" (spin-phase) Sun, ..., sector ind=31 looks "before" Sun dir. Head field-of-view: pixel index=00 looks to zenith, ..., pixel index=15 looks to nadir. FPI operations nominally bin data from 64 energy filters into 32 pairwise energy bins, indexed 0-31. Nominally, bins are indexed in increasing energy order. See FPI docs for details. |
DIS | Burst | MMS |
[# / {(cm/s)3 * cc}] | Az bin: sector ind=00 looks "after" (spin-phase) Sun, ..., sector ind=31 looks "before" Sun dir. Head field-of-view: pixel index=00 looks to zenith, ..., pixel index=15 looks to nadir. FPI operations nominally bin data from 64 energy filters into 32 pairwise energy bins, indexed 0-31. Nominally, bins are indexed in increasing energy order. See FPI docs for details. |
DIS | Burst | MMS |
eV | Odd energies (parity 1) in the 64-step FPI energy table |
DIS | Burst | MMS |
eV | Even energies (parity 0) in the 64-step FPI energy table |
Level-2 Moments | ||||
File Name Pattern: MMS[1,2,3,4]_FPI_FAST_L2_DES-MOMS_YYYYMMDDHHMMSS_V2.1.0.cdf | ||||
File Name Pattern: MMS[1,2,3,4]_FPI_FAST_L2_DIS-MOMS_YYYYMMDDHHMMSS_V2.1.0.cdf | ||||
File Name Pattern: MMS[1,2,3,4]_FPI_BRST_L2_DES-MOMS_YYYYMMDDHHMMSS_V2.1.0.cdf | ||||
File Name Pattern: MMS[1,2,3,4]_FPI_BRST_L2_DIS-MOMS_YYYYMMDDHHMMSS_V2.1.0.cdf | ||||
Sensor | Data Mode | Variable Name | Units | Comments |
DES/DIS | Fast/Burst | Epoch | ns | Survey data acquisition time; derived from packet time. |
DES/DIS | Fast/Burst | MMS |
degrees | Nominally, spin-phase angles range over [0, 360) deg. Each count represents 1/16 deg of observatory spin-phase. Zero spin-phase angle indicates obs +X-axis aligned with Sun. |
DES/DIS | Fast/Burst | MMS |
----- | low energy bin: 0 eV - 200 eV. pitch-angle bin size: 6 deg. |
DES/DIS | Fast/Burst | MMS |
----- | mid energy bin: 2000 eV - 2 keV. pitch-angle bin size: 6 deg. |
DES/DIS | Fast/Burst | MMS |
----- | high energy bin: 2 keV - 30 keV. pitch-angle bin size: 6 deg. |
DES/DIS | Fast/Burst | MMS |
----- | Counts, summed over DSC velocity-dirs closest to -[X,Y,Z]_DSC, by energy bin. |
DES/DIS | Fast/Burst | MMS |
cm^-3 | Number Density |
DES/DIS | Fast/Burst | MMS |
km/s | Bulk Speed |
DES/DIS | Fast/Burst | MMS |
km/s | Bulk velocity vector GSE [X,Y,Z] component. |
DES/DIS | Fast/Burst | MMS |
erg/cm^3 | Pressure tensor GSE [X,Y,Z][X,Y,Z] component |
DES/DIS | Fast/Burst | MMS |
eV | Temperature tensor GSE [X,Y,Z][X,Y,Z] component |
DES/DIS | Fast/Burst | MMS |
(erg/s)/cm^2 | Heat flux vector magnitude |
DES/DIS | Fast/Burst | MMS |
degrees | Pitch-angles angles used in pitch angle spectrograms (bent Pipe field) |
DES/DIS | Fast/Burst | MMS |
eV | Odd energies (parity 1) in the 64-step FPI energy table |
DES/DIS | Fast/Burst | MMS |
eV | Even energies (parity 0) in the 64-step FPI energy table |
DES/DIS | Fast/Burst | MMS |
eV | Parallel temperature |
DES/DIS | Fast/Burst | MMS |
eV | Perpendicular temperature |
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