2.4.1
spase://CNES/NumericalData/CDPP-AMDA/MMS/MMS3/FPI/mms3-fpi-desmoms
MMS3 - FPI - fast mode - DES : electrons
Dual Electron Spectrometers : fast mode
2024-10-04T05:34:35Z
FPI usually operates in Fast Survey (FS) Mode in the MMS Region Of Interest (ROI) for
the current Mission Phase. Data are taken at burst (30/150 ms for DES/DIS) resolution in this mode. Data are also made
available at survey (4.5 s) resolution. Per mission design, not all burst-resolution data are downlinked, but all sur vey data are downlinked. Planning around calibration activities, avoidance of Earth radiation belts, etc, when possible
, FPI usually operates in Slow Survey (SS) Mode (60 s resolution) outside of ROI. This moments product contains results
from integrating the standard moments of phase-space distributions formed from the indicated data type (DES/DIS burst,
FS or SS). For convenience, some additional parameters are included to augment those most commonly found in a moments
product of this sort, plus time-stamps and other annotation characterizing the state of the instrument system at the in
dicated time.
spase://SMWG/Person/James.L.Burch
PrincipalInvestigator
spase://CNES/Person/CDPP-AMDA/B.Giles
PrincipalInvestigator
MMS home page at GSFC
http://mms.gsfc.nasa.gov
FPI overview
http://www.nasa.gov/mission_pages/mms/spacecraft/instruments.html#fpi
mms3-fpi-fast
PartOf
fast mode
spase://SMWG/Repository/CDPP/AMDA
Online
Open
CDPP/AMDA HAPI Server
https://amda.irap.omp.eu/service/hapi
mms3-fpi-desmoms
Web Service to this product using the HAPI interface.
CSV
Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.
spase://SMWG/Repository/CDPP/AMDA
Online
Open
CDPP/AMDA Web application
https://amda.cdpp.eu
Access to Data via CDPP/AMDA Web application.
CSV
VOTable
CDF
PNG
Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.
LASP
spase://CNES/Instrument/CDPP-AMDA/MMS3/FPI
MagneticField
2015-05-06T00:00:01Z
2024-08-14T00:57:17Z
PT4.5S
density
mms3_des_ne
cm^-3
TimeSeries
Electron
Scalar
NumberDensity
density : err
mms3_des_ne_err
cm^-3
TimeSeries
Electron
Scalar
NumberDensity
v_gse
mms3_des_vgse
km/s
Cartesian
GSE
TimeSeries
3
vx
Component.I
1
mms3_des_vgse(0)
vy
Component.J
2
mms3_des_vgse(1)
vz
Component.K
3
mms3_des_vgse(2)
Electron
Scalar
NumberDensity
v_gse : err
mms3_des_v_err
km/s
TimeSeries
3
vx
Component.I
1
mms3_des_v_err(0)
vy
Component.J
2
mms3_des_v_err(1)
vz
Component.K
3
mms3_des_v_err(2)
Electron
Scalar
NumberDensity
t_para
mms3_des_tpara
eV
TimeSeries
Electron
Scalar
Temperature
t_perp
mms3_des_tperp
eV
TimeSeries
Electron
Scalar
Temperature
heatq_gse
mms3_des_heatq
phys.pressure
mW/m^2
Cartesian
GSE
TimeSeries
3
x
1
mms3_des_heatq(0)
y
2
mms3_des_heatq(1)
z
3
mms3_des_heatq(2)
Electron
Vector
HeatFlux
pressure_gse
mms3_des_press
phys.pressure
nPa
Cartesian
GSE
TimeSeries
9
xx
1
mms3_des_press(0)
xy
2
mms3_des_press(1)
xz
3
mms3_des_press(2)
yx
4
mms3_des_press(3)
yy
5
mms3_des_press(4)
yz
6
mms3_des_press(5)
zx
7
mms3_des_press(6)
zy
8
mms3_des_press(7)
zz
9
mms3_des_press(8)
Electron
Tensor
Pressure
elec eflux : omni
mms3_des_omni
keV/(cm^2-s-sr-keV)
Spectrogram
Electron
EnergyFlux
elec eflux : para
mms3_des_para
keV/(cm^2-s-sr-keV)
Spectrogram
Electron
EnergyFlux
elec eflux : anti
mms3_des_anti
keV/(cm^2-s-sr-keV)
Spectrogram
Electron
EnergyFlux
elec eflux : perp
mms3_des_perp
keV/(cm^2-s-sr-keV)
Spectrogram
Electron
EnergyFlux
pa dist : lowen
mms3_des_palow
Low energy bin: 0 eV - 200 eV.
Pitch-angle bin size: 6 deg. Note that pitch angles are calculated in the spacecraft frame;
i.e., not shifted by the bulk velocity
keV/(cm^2-s-sr-keV)
Spectrogram
Electron
EnergyFlux
pa dist : miden
mms3_des_pamid
Mid energy bin: 200 eV - 2 keV.
Pitch-angle bin size: 6 deg. Note that pitch angles are calculated in the spacecraft frame;
i.e., not shifted by the bulk velocity
keV/(cm^2-s-sr-keV)
Spectrogram
Electron
EnergyFlux
pa dist : highen
mms3_des_pahigh
High energy bin: 2 keV - 30 keV.
Pitch-angle bin size: 6 deg. Note that pitch angles are calculated in the spacecraft frame;
i.e., not shifted by the bulk velocity
keV/(cm^2-s-sr-keV)
Spectrogram
Electron
EnergyFlux