Van Allen Probe A Energetic Particle, Composition, and Thermal Plasma Suite (ECT) Helium Oxygen Proton Electron, HOPE, Mass Spectrometer Pitch Angle resolved Science Data. Electron Fluxes, 15 eV to 50 keV, and Ion Fluxes, 1 eV to 50 keV, as measured in alternate Spin Cadence, Level 3, Release #4 (L3), 11.35 s Data

https://doi.org/10.48322/17p9-rf75

2022-08-18 12:34:56.789

Van Allen Probe A, Energetic Particle, Composition, and Thermal Plasma Suite, ECT, Helium Oxygen Proton Electron, HOPE, Mass Spectrometer Pitch Angle resolved Science Data. Electron Fluxes from about 15 eV to 50 keV and Ion Fluxes from about 1 eV to 50 keV as measured in alternate Spin Cadence.

H.O. Funsten, R. Skoug, R. Friedel. Distribute freely, please acknowledge the original Principal Investigator. Please contact the Principal Investigator before any publication or Presentation of Data.

spase://VSPO/NumericalData/RBSP/A/ECT/HOPE/L3/PitchAngle/Release03/PT11.35S

spase://VSPO/NumericalData/RBSP/A/ECT/HOPE/L3/PitchAngle/Release03/PT60S

spase://VSPO/NumericalData/RBSP/A/ECT/HOPE/SCI-L3/PT60S

spase://VSPO/NumericalData/RBSP/A/ECT/HOPE/L3/PitchAngle/Release04/PT11.35S

Online

Open

CDF

None

H.O. Funsten, R. Skoug, R. Friedel. Distribute freely, please acknowledge the original Principal Investigator. Please contact the Principal Investigator before any publication or Presentation of Data. Please acknowledge the Data Providers and CDAWeb when using these Data.

Online

Open

CSV

H.O. Funsten, R. Skoug, R. Friedel. Distribute freely, please acknowledge the original Principal Investigator. Please contact the Principal Investigator before any publication or Presentation of Data. Please acknowledge the Data Providers and CDAWeb when using these Data.

PT11.35S

Electron Energy Range, Delta

Time Series defined by using: EPOCH_ELE

ENERGY_Ele_DELTA

Electron Energy Range, Delta

PT11.35S

eV

1.602176565e-19>J

0.0

60000.0

-1.0e+31

Ion Energy Range, Delta

Time Series defined by using: EPOCH_ION

ENERGY_Ion_DELTA

Ion Energy Range, Delta

PT11.35S

eV

1.602176565e-19>J

0.0

60000.0

-1.0e+31

Epoch Time, Electrons

Epoch_Ele

Epoch Time, Time Base for Electron Measurements

PT11.35S

01-Jan-2010 00:00:00.000

31-Dec-2029 23:59:59.999

31-Dec-9999 23:59:59.999

Epoch Time Delta, Electrons

Time Series defined by using: EPOCH_ELE

Epoch_Ele_DELTA

Epoch Time Delta, Half Electron Sample Time

Half of the HOPE Electron Sample Frame Time

PT11.35S

ms

1.0e-3>s

0.0

20000.0

-1.0e+31

Epoch Time, Ions

Epoch_Ion

Epoch Time, Time Base for Ion Measurements

PT11.35S

01-Jan-2010 00:00:00.000

31-Dec-2029 23:59:59.999

31-Dec-9999 23:59:59.999

Epoch Time Delta, Ions

Time Series defined by using: EPOCH_ION

Epoch_Ion_DELTA

Epoch Time Delta, Half Ion Sample Time

Half of the HOPE Ion Sample Frame Time

PT11.35S

ms

1.0e-3>s

0.0

20000.0

-1.0e+31

Pitch Angle

PITCH_ANGLE

Pitch Angle, from 0° to 180°

PT11.35S

°

0.0174532925>rad

0.0

180.0

-1.0e+31

Pitch Angle

PITCH_ANGLE_EXT

Pitch Angle, from 0° to 180°

PT11.35S

°

0.0174532925>rad

0.0

180.0

-1.0e+31

HOPE Electron Energy

Time Series defined by using: EPOCH_ELE

HOPE_ENERGY_Ele

HOPE Electron Energy

Note that the HOPE Instrument normally measures 72 Energy Steps. Before September 2013, adjacent Channels were combined for Downlink. The combined Values were then expanded on the Ground to recover the 72 Channels.

PT11.35S

eV

1.602176565e-19>J

1.0

100000.0

-1.0e+31

HOPE Ion Energy

Time Series defined by using: EPOCH_ION

HOPE_ENERGY_Ion

HOPE Ion Energy

Note that the HOPE Instrument normally measures 72 Energy Steps. Before September 2013, adjacent Channels were combined for Downlink. The combined Values were then expanded on the Ground to recover the 72 Channels.

PT11.35S

eV

1.602176565e-19>J

0.1

100000.0

-1.0e+31

Electron Differential Flux Intensity, Omnidirectional

Time Series defined by using: EPOCH_ELE

FEDO

Electron Differential Flux Intensity, Omnidirectional, Energies from ~15 eV to ~50 keV

Flux integrated, piecewise constant, over 11 Pitch Angles and 20 Gyro Angles as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and over 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

0.0

1.0e+16

-1.0e+31

Electron Differential Flux Intensity, Omnidirectional, Time Series Stack Plots

Time Series defined by using: EPOCH_ELE

FEDO_T

Electron Differential Flux Intensity, Omnidirectional, Time Series Stack Plots, Energies from ~15 eV to ~50 keV, with Perigee Mode excluded

Flux integrated, piecewise constant, over 11 Pitch Angles and 20 Gyro Angles as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and over 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions. This parameter is virtual. It is calculated by calling the function APPLY_ESA_QFLAG with the following input parameters: FEDO, Mode_Ele.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

0.0

1.0e+16

-1.0e+31

Electron Differential Flux Intensity, Unidirectional, Energy-Angle Plasmagrams

Time Series defined by using: EPOCH_ELE

FEDU

Electron Differential Flux Intensity, Unidirectional, Energy-Angle Plasmagrams, Energies from ~15 eV to ~50 keV. Column 1 Labels from PITCH_ANGLE: [ 4.50000, 18.0000, 36.0000, 54.0000, 72.0000, 90.0000, 108.000, 126.000, 144.000, 162.000, 175.500]

Electron Flux as a Function of 11 Pitch Angles, as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

-1.0e+31

Electron Differential Flux Intensity, Unidirectional, Spectrograms by Energy at Sample Pitch Angles

Time Series defined by using: EPOCH_ELE

FEDU_byE_atA

Electron Differential Flux Intensity, Unidirectional, Spectrograms by Energy at Sample Pitch Angles, Energies from ~15 eV to ~50 keV, Perigee Mode excluded. * Column 1 Labels from PITCH_ANGLE: ["FEDU_Flux_4.5degPA","FEDU_Flux_18degPA","FEDU_Flux_36degPA","FEDU_Flux_54degPA","FEDU_Flux_72degPA","FEDU_Flux_90degPA","FEDU_Flux_108degPA","FEDU_Flux_126degPA","FEDU_Flux_144degPA","FEDU_Flux_162degPA","FEDU_Flux_175.5degPA"]. * Column 2 Labels from HOPE_ENERGY_ELE: ["FEDU_Flux_E01/~15eV","FEDU_Flux_E02/~17eV","FEDU_Flux_E03/~19eV","FEDU_Flux_E04/~21eV","FEDU_Flux_E05/~24eV","FEDU_Flux_E06/~27eV","FEDU_Flux_E07/~30eV","FEDU_Flux_E08/~33eV","FEDU_Flux_E09/~37eV","FEDU_Flux_E10/~42eV","FEDU_Flux_E11/~47eV","FEDU_Flux_E12/~53eV","FEDU_Flux_E13/~59eV","FEDU_Flux_E14/~67eV","FEDU_Flux_E15/~75eV","FEDU_Flux_E16/~84eV","FEDU_Flux_E17/~94eV","FEDU_Flux_E18/~106eV","FEDU_Flux_E19/~118eV","FEDU_Flux_E20/~133eV","FEDU_Flux_E21/~149eV","FEDU_Flux_E22/~167eV","FEDU_Flux_E23/~187eV","FEDU_Flux_E24/~210eV","FEDU_Flux_E25/~236eV","FEDU_Flux_E26/~260eV","FEDU_Flux_E27/~300eV","FEDU_Flux_E28/~330eV","FEDU_Flux_E29/~370eV","FEDU_Flux_E30/~420eV","FEDU_Flux_E31/~470eV","FEDU_Flux_E32/~530eV","FEDU_Flux_E33/~590eV","FEDU_Flux_E34/~660eV","FEDU_Flux_E35/~740eV","FEDU_Flux_E36/~830eV","FEDU_Flux_E37/~930eV","FEDU_Flux_E38/~1050eV","FEDU_Flux_E39/~1170eV","FEDU_Flux_E40/~1320eV","FEDU_Flux_E41/~1480eV","FEDU_Flux_E42/~1660eV","FEDU_Flux_E43/~1860eV","FEDU_Flux_E44/~2080eV","FEDU_Flux_E45/~2340eV","FEDU_Flux_E46/~2600eV","FEDU_Flux_E47/~3000eV","FEDU_Flux_E48/~3300eV","FEDU_Flux_E49/~3700eV","FEDU_Flux_E50/~4100eV","FEDU_Flux_E51/~4700eV","FEDU_Flux_E52/~5200eV","FEDU_Flux_E53/~5900eV","FEDU_Flux_E54/~6600eV","FEDU_Flux_E55/~7400eV","FEDU_Flux_E56/~8300eV","FEDU_Flux_E57/~9300eV","FEDU_Flux_E58/~10400eV","FEDU_Flux_E59/~11700eV","FEDU_Flux_E60/~13100eV","FEDU_Flux_E61/~14700eV","FEDU_Flux_E62/~16400eV","FEDU_Flux_E63/~18400eV","FEDU_Flux_E64/~20700eV","FEDU_Flux_E65/~23200eV","FEDU_Flux_E66/~26000eV","FEDU_Flux_E67/~30000eV","FEDU_Flux_E68/~33000eV","FEDU_Flux_E69/~37000eV","FEDU_Flux_E70/~41000eV","FEDU_Flux_E71/~46000eV","FEDU_Flux_E72/~52000eV"].

Electron Flux as a Function of 11 Pitch Angles, as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions. This parameter is virtual. It is calculated by calling the function APPLY_ESA_QFLAG with the following input parameters: FEDU, Mode_Ele.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

-1.0e+31

Electron Differential Flux Intensity, Unidirectional, Spectrograms by Pitch Angle at Sample Energies

Time Series defined by using: EPOCH_ELE

FEDU_byA_atE

Electron Differential Flux Intensity, Unidirectional, Spectrograms by Pitch Angle at Sample Energies, Energies from ~15 eV to ~50 keV, Perigee Mode excluded. * Column 1 Labels from PITCH_ANGLE: ["FEDU_Flux_4.5degPA","FEDU_Flux_18degPA","FEDU_Flux_36degPA","FEDU_Flux_54degPA","FEDU_Flux_72degPA","FEDU_Flux_90degPA","FEDU_Flux_108degPA","FEDU_Flux_126degPA","FEDU_Flux_144degPA","FEDU_Flux_162degPA","FEDU_Flux_175.5degPA"]. * Column 2 Labels from HOPE_ENERGY_ELE: ["FEDU_Flux_E01/~15eV","FEDU_Flux_E02/~17eV","FEDU_Flux_E03/~19eV","FEDU_Flux_E04/~21eV","FEDU_Flux_E05/~24eV","FEDU_Flux_E06/~27eV","FEDU_Flux_E07/~30eV","FEDU_Flux_E08/~33eV","FEDU_Flux_E09/~37eV","FEDU_Flux_E10/~42eV","FEDU_Flux_E11/~47eV","FEDU_Flux_E12/~53eV","FEDU_Flux_E13/~59eV","FEDU_Flux_E14/~67eV","FEDU_Flux_E15/~75eV","FEDU_Flux_E16/~84eV","FEDU_Flux_E17/~94eV","FEDU_Flux_E18/~106eV","FEDU_Flux_E19/~118eV","FEDU_Flux_E20/~133eV","FEDU_Flux_E21/~149eV","FEDU_Flux_E22/~167eV","FEDU_Flux_E23/~187eV","FEDU_Flux_E24/~210eV","FEDU_Flux_E25/~236eV","FEDU_Flux_E26/~260eV","FEDU_Flux_E27/~300eV","FEDU_Flux_E28/~330eV","FEDU_Flux_E29/~370eV","FEDU_Flux_E30/~420eV","FEDU_Flux_E31/~470eV","FEDU_Flux_E32/~530eV","FEDU_Flux_E33/~590eV","FEDU_Flux_E34/~660eV","FEDU_Flux_E35/~740eV","FEDU_Flux_E36/~830eV","FEDU_Flux_E37/~930eV","FEDU_Flux_E38/~1050eV","FEDU_Flux_E39/~1170eV","FEDU_Flux_E40/~1320eV","FEDU_Flux_E41/~1480eV","FEDU_Flux_E42/~1660eV","FEDU_Flux_E43/~1860eV","FEDU_Flux_E44/~2080eV","FEDU_Flux_E45/~2340eV","FEDU_Flux_E46/~2600eV","FEDU_Flux_E47/~3000eV","FEDU_Flux_E48/~3300eV","FEDU_Flux_E49/~3700eV","FEDU_Flux_E50/~4100eV","FEDU_Flux_E51/~4700eV","FEDU_Flux_E52/~5200eV","FEDU_Flux_E53/~5900eV","FEDU_Flux_E54/~6600eV","FEDU_Flux_E55/~7400eV","FEDU_Flux_E56/~8300eV","FEDU_Flux_E57/~9300eV","FEDU_Flux_E58/~10400eV","FEDU_Flux_E59/~11700eV","FEDU_Flux_E60/~13100eV","FEDU_Flux_E61/~14700eV","FEDU_Flux_E62/~16400eV","FEDU_Flux_E63/~18400eV","FEDU_Flux_E64/~20700eV","FEDU_Flux_E65/~23200eV","FEDU_Flux_E66/~26000eV","FEDU_Flux_E67/~30000eV","FEDU_Flux_E68/~33000eV","FEDU_Flux_E69/~37000eV","FEDU_Flux_E70/~41000eV","FEDU_Flux_E71/~46000eV","FEDU_Flux_E72/~52000eV"].

Electron Flux as a Function of 11 Pitch Angles, as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions. This parameter is virtual. It is calculated by calling the function APPLY_ESA_QFLAG with the following input parameters: FEDU, Mode_Ele.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

-1.0e+31

Proton Differential Flux Intensity, Omnidirectional, Spectrograms

Time Series defined by using: EPOCH_ION

FPDO

Proton Differential Flux Intensity, Omnidirectional, Spectrograms, Energies from ~1 eV to ~50 keV

Flux integrated, piecewise constant, over 11 Pitch Angles and 20 Gyro Angles as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and over 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

0.0

1.0e+16

-1.0e+31

Proton Differential Flux Intensity, Omnidirectional, Time Series Stack Plots

Time Series defined by using: EPOCH_ION

FPDO_T

Proton Differential Flux Intensity, Omnidirectional, Time Series Stack Plots, Energies from ~15 eV to ~50 keV, Perigee Mode excluded

Flux integrated, piecewise constant, over 11 Pitch Angles and 20 Gyro Angles as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and over 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions. This parameter is virtual. It is calculated by calling the function APPLY_ESA_QFLAG with the following input parameters: FPDO, Mode_Ion.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

0.0

1.0e+16

-1.0e+31

Proton Differential Flux Intensity, Unidirectional, Energy-Angle Plasmagrams

Time Series defined by using: EPOCH_ION

FPDU

Proton Differential Flux Intensity, Unidirectional, Energy-Angle Plasmagrams, Energies from ~1 eV to ~50 keV. Column 1 Labels from PITCH_ANGLE: [ 4.50000, 18.0000, 36.0000, 54.0000, 72.0000, 90.0000, 108.000, 126.000, 144.000, 162.000, 175.500]

Proton Flux as a Function of 11 Pitch Angles, as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

-1.0e+31

Proton Differential Flux Intensity, Unidirectional, Spectrograms by Energy at Sample Pitch Angles

Time Series defined by using: EPOCH_ION

FPDU_byE_atA

Proton Differential Flux Intensity, Unidirectional, Spectrograms by Energy at Sample Pitch Angles, Energies from ~1 eV to ~50 keV, Perigee Mode excluded. * Column 1 Labels from PITCH_ANGLE: ["FPDU_Flux_4.5degPA","FPDU_Flux_18degPA","FPDU_Flux_36degPA","FPDU_Flux_54degPA","FPDU_Flux_72degPA","FPDU_Flux_90degPA","FPDU_Flux_108degPA","FPDU_Flux_126degPA","FPDU_Flux_144degPA","FPDU_Flux_162degPA","FPDU_Flux_175.5degPA"]. * Column 2 Labels from HOPE_ENERGY_ION: ["FPDU_Flux_E01/~1.00eV","FPDU_Flux_E02/~1.20eV","FPDU_Flux_E03/~1.34eV","FPDU_Flux_E04/~1.55eV","FPDU_Flux_E05/~1.83eV","FPDU_Flux_E06/~2.18eV","FPDU_Flux_E07/~2.5eV","FPDU_Flux_E08/~3.0eV","FPDU_Flux_E09/~3.4eV","FPDU_Flux_E10/~3.9eV","FPDU_Flux_E11/~4.6eV","FPDU_Flux_E12/~5.3eV","FPDU_Flux_E13/~6.3eV","FPDU_Flux_E14/~7.3eV","FPDU_Flux_E15/~8.5eV","FPDU_Flux_E16/~9.9eV","FPDU_Flux_E17/~11.5eV","FPDU_Flux_E18/~13.4eV","FPDU_Flux_E19/~15.7eV","FPDU_Flux_E20/~18.3eV","FPDU_Flux_E21/~21.2eV","FPDU_Flux_E22/~24.8eV","FPDU_Flux_E23/~29eV","FPDU_Flux_E24/~34eV","FPDU_Flux_E25/~39eV","FPDU_Flux_E26/~46eV","FPDU_Flux_E27/~53eV","FPDU_Flux_E28/~62eV","FPDU_Flux_E29/~72eV","FPDU_Flux_E30/~84eV","FPDU_Flux_E31/~98eV","FPDU_Flux_E32/~114eV","FPDU_Flux_E33/~133eV","FPDU_Flux_E34/~155eV","FPDU_Flux_E35/~181eV","FPDU_Flux_E36/~211eV","FPDU_Flux_E37/~246eV","FPDU_Flux_E38/~286eV","FPDU_Flux_E39/~330eV","FPDU_Flux_E40/~390eV","FPDU_Flux_E41/~450eV","FPDU_Flux_E42/~530eV","FPDU_Flux_E43/~610eV","FPDU_Flux_E44/~720eV","FPDU_Flux_E45/~830eV","FPDU_Flux_E46/~970eV","FPDU_Flux_E47/~1130eV","FPDU_Flux_E48/~1320eV","FPDU_Flux_E49/~1540eV","FPDU_Flux_E50/~1790eV","FPDU_Flux_E51/~2090eV","FPDU_Flux_E52/~2400eV","FPDU_Flux_E53/~2800eV","FPDU_Flux_E54/~3300eV","FPDU_Flux_E55/~3800eV","FPDU_Flux_E56/~4500eV","FPDU_Flux_E57/~5200eV","FPDU_Flux_E58/~6100eV","FPDU_Flux_E59/~7100eV","FPDU_Flux_E60/~8300eV","FPDU_Flux_E61/~9600eV","FPDU_Flux_E62/~11200eV","FPDU_Flux_E63/~13100eV","FPDU_Flux_E64/~15200eV","FPDU_Flux_E65/~17800eV","FPDU_Flux_E66/~20700eV","FPDU_Flux_E67/~24000eV","FPDU_Flux_E68/~28000eV","FPDU_Flux_E69/~33000eV","FPDU_Flux_E70/~38000eV","FPDU_Flux_E71/~44000eV","FPDU_Flux_E72/~52000eV"].

Proton Flux as a Function of 11 Pitch Angles, as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions. This parameter is virtual. It is calculated by calling the function ALTERNATE_VIEW with the following input parameters: FPDU.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

-1.0e+31

Proton Differential Flux Intensity, Unidirectional, Spectrograms by Pitch Angle at Sample Energies

Time Series defined by using: EPOCH_ION

FPDU_byA_atE

Proton Differential Flux Intensity, Unidirectional, Spectrograms by Pitch Angle at Sample Energies, Energies from ~1 eV to ~50 keV, Perigee Mode excluded. * Column 1 Labels from PITCH_ANGLE: ["FPDU_Flux_4.5degPA","FPDU_Flux_18degPA","FPDU_Flux_36degPA","FPDU_Flux_54degPA","FPDU_Flux_72degPA","FPDU_Flux_90degPA","FPDU_Flux_108degPA","FPDU_Flux_126degPA","FPDU_Flux_144degPA","FPDU_Flux_162degPA","FPDU_Flux_175.5degPA"]. * Column 2 Labels from HOPE_ENERGY_ION: ["FPDU_Flux_E01/~1.00eV","FPDU_Flux_E02/~1.20eV","FPDU_Flux_E03/~1.34eV","FPDU_Flux_E04/~1.55eV","FPDU_Flux_E05/~1.83eV","FPDU_Flux_E06/~2.18eV","FPDU_Flux_E07/~2.5eV","FPDU_Flux_E08/~3.0eV","FPDU_Flux_E09/~3.4eV","FPDU_Flux_E10/~3.9eV","FPDU_Flux_E11/~4.6eV","FPDU_Flux_E12/~5.3eV","FPDU_Flux_E13/~6.3eV","FPDU_Flux_E14/~7.3eV","FPDU_Flux_E15/~8.5eV","FPDU_Flux_E16/~9.9eV","FPDU_Flux_E17/~11.5eV","FPDU_Flux_E18/~13.4eV","FPDU_Flux_E19/~15.7eV","FPDU_Flux_E20/~18.3eV","FPDU_Flux_E21/~21.2eV","FPDU_Flux_E22/~24.8eV","FPDU_Flux_E23/~29eV","FPDU_Flux_E24/~34eV","FPDU_Flux_E25/~39eV","FPDU_Flux_E26/~46eV","FPDU_Flux_E27/~53eV","FPDU_Flux_E28/~62eV","FPDU_Flux_E29/~72eV","FPDU_Flux_E30/~84eV","FPDU_Flux_E31/~98eV","FPDU_Flux_E32/~114eV","FPDU_Flux_E33/~133eV","FPDU_Flux_E34/~155eV","FPDU_Flux_E35/~181eV","FPDU_Flux_E36/~211eV","FPDU_Flux_E37/~246eV","FPDU_Flux_E38/~286eV","FPDU_Flux_E39/~330eV","FPDU_Flux_E40/~390eV","FPDU_Flux_E41/~450eV","FPDU_Flux_E42/~530eV","FPDU_Flux_E43/~610eV","FPDU_Flux_E44/~720eV","FPDU_Flux_E45/~830eV","FPDU_Flux_E46/~970eV","FPDU_Flux_E47/~1130eV","FPDU_Flux_E48/~1320eV","FPDU_Flux_E49/~1540eV","FPDU_Flux_E50/~1790eV","FPDU_Flux_E51/~2090eV","FPDU_Flux_E52/~2400eV","FPDU_Flux_E53/~2800eV","FPDU_Flux_E54/~3300eV","FPDU_Flux_E55/~3800eV","FPDU_Flux_E56/~4500eV","FPDU_Flux_E57/~5200eV","FPDU_Flux_E58/~6100eV","FPDU_Flux_E59/~7100eV","FPDU_Flux_E60/~8300eV","FPDU_Flux_E61/~9600eV","FPDU_Flux_E62/~11200eV","FPDU_Flux_E63/~13100eV","FPDU_Flux_E64/~15200eV","FPDU_Flux_E65/~17800eV","FPDU_Flux_E66/~20700eV","FPDU_Flux_E67/~24000eV","FPDU_Flux_E68/~28000eV","FPDU_Flux_E69/~33000eV","FPDU_Flux_E70/~38000eV","FPDU_Flux_E71/~44000eV","FPDU_Flux_E72/~52000eV"].

Proton Flux as a Function of 11 Pitch Angles, as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions. This parameter is virtual. It is calculated by calling the function APPLY_ESA_QFLAG with the following input parameters: FPDU, Mode_Ion.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

-1.0e+31

Oxygen Differential Flux Intensity, Omnidirectional, Spectrograms

Time Series defined by using: EPOCH_ION

FODO

Oxygen Differential Flux Intensity, Omnidirectional, Spectrograms, Energies from ~1 eV to ~50 keV

Flux integrated, piecewise constant, over 11 Pitch Angles and 20 Gyro Angles as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and over 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

0.0

1.0e+16

-1.0e+31

Oxygen Differential Flux Intensity, Omnidirectional, Time Series Stack Plots

Time Series defined by using: EPOCH_ION

FODO_T

Oxygen Differential Flux Intensity, Omnidirectional, Time Series Stack Plots, Energies from ~1 eV to ~50 keV, with Perigee Mode excluded

Flux integrated, piecewise constant, over 11 Pitch Angles and 20 Gyro Angles as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and over 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions. This parameter is virtual. It is calculated by calling the function APPLY_ESA_QFLAG with the following input parameters: FODO, Mode_Ion.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

0.0

1.0e+16

-1.0e+31

Oxygen Differential Flux Intensity, Unidirectional, Energy-Angle Plasmagrams

Time Series defined by using: EPOCH_ION

FODU

Oxygen Differential Flux Intensity, Unidirectional, Energy-Angle Plasmagrams, Energies from ~1 eV to ~50 keV. Column 1 Labels from PITCH_ANGLE: [ 4.50000, 18.0000, 36.0000, 54.0000, 72.0000, 90.0000, 108.000, 126.000, 144.000, 162.000, 175.500]

Oxygen Flux as a Function of 11 Pitch Angles, as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

-1.0e+31

Oxygen Differential Flux Intensity, Unidirectional, Spectrograms by Energy at Sample Pitch Angles

Time Series defined by using: EPOCH_ION

FODU_byE_atA

Oxygen Differential Flux Intensity, Unidirectional, Spectrograms by Energy at Sample Pitch Angles, Energies from ~1 eV to ~50 keV, Perigee Mode excluded. * Column 1 Labels from PITCH_ANGLE: ["FODU_Flux_4.5degPA","FODU_Flux_18degPA","FODU_Flux_36degPA","FODU_Flux_54degPA","FODU_Flux_72degPA","FODU_Flux_90degPA","FODU_Flux_108degPA","FODU_Flux_126degPA","FODU_Flux_144degPA","FODU_Flux_162degPA","FODU_Flux_175.5degPA"]. * Column 2 Labels from HOPE_ENERGY_ION: ["FODU_Flux_E01/~1.00eV","FODU_Flux_E02/~1.20eV","FODU_Flux_E03/~1.34eV","FODU_Flux_E04/~1.55eV","FODU_Flux_E05/~1.83eV","FODU_Flux_E06/~2.18eV","FODU_Flux_E07/~2.5eV","FODU_Flux_E08/~3.0eV","FODU_Flux_E09/~3.4eV","FODU_Flux_E10/~3.9eV","FODU_Flux_E11/~4.6eV","FODU_Flux_E12/~5.3eV","FODU_Flux_E13/~6.3eV","FODU_Flux_E14/~7.3eV","FODU_Flux_E15/~8.5eV","FODU_Flux_E16/~9.9eV","FODU_Flux_E17/~11.5eV","FODU_Flux_E18/~13.4eV","FODU_Flux_E19/~15.7eV","FODU_Flux_E20/~18.3eV","FODU_Flux_E21/~21.2eV","FODU_Flux_E22/~24.8eV","FODU_Flux_E23/~29eV","FODU_Flux_E24/~34eV","FODU_Flux_E25/~39eV","FODU_Flux_E26/~46eV","FODU_Flux_E27/~53eV","FODU_Flux_E28/~62eV","FODU_Flux_E29/~72eV","FODU_Flux_E30/~84eV","FODU_Flux_E31/~98eV","FODU_Flux_E32/~114eV","FODU_Flux_E33/~133eV","FODU_Flux_E34/~155eV","FODU_Flux_E35/~181eV","FODU_Flux_E36/~211eV","FODU_Flux_E37/~246eV","FODU_Flux_E38/~286eV","FODU_Flux_E39/~330eV","FODU_Flux_E40/~390eV","FODU_Flux_E41/~450eV","FODU_Flux_E42/~530eV","FODU_Flux_E43/~610eV","FODU_Flux_E44/~720eV","FODU_Flux_E45/~830eV","FODU_Flux_E46/~970eV","FODU_Flux_E47/~1130eV","FODU_Flux_E48/~1320eV","FODU_Flux_E49/~1540eV","FODU_Flux_E50/~1790eV","FODU_Flux_E51/~2090eV","FODU_Flux_E52/~2400eV","FODU_Flux_E53/~2800eV","FODU_Flux_E54/~3300eV","FODU_Flux_E55/~3800eV","FODU_Flux_E56/~4500eV","FODU_Flux_E57/~5200eV","FODU_Flux_E58/~6100eV","FODU_Flux_E59/~7100eV","FODU_Flux_E60/~8300eV","FODU_Flux_E61/~9600eV","FODU_Flux_E62/~11200eV","FODU_Flux_E63/~13100eV","FODU_Flux_E64/~15200eV","FODU_Flux_E65/~17800eV","FODU_Flux_E66/~20700eV","FODU_Flux_E67/~24000eV","FODU_Flux_E68/~28000eV","FODU_Flux_E69/~33000eV","FODU_Flux_E70/~38000eV","FODU_Flux_E71/~44000eV","FODU_Flux_E72/~52000eV"].

Oxygen Flux as a Function of 11 Pitch Angles, as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions. This parameter is virtual. It is calculated by calling the function ALTERNATE_VIEW with the following input parameters: FODU.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

-1.0e+31

Oxygen Differential Flux Intensity, Unidirectional, Spectrograms by Pitch Angle at Sample Energies

Time Series defined by using: EPOCH_ION

FODU_byA_atE

Oxygen Differential Flux Intensity, Unidirectional, Spectrograms by Pitch Angle at Sample Energies, Energies from ~1 eV to ~50 keV, Perigee Mode excluded. * Column 1 Labels from PITCH_ANGLE: ["FODU_Flux_4.5degPA","FODU_Flux_18degPA","FODU_Flux_36degPA","FODU_Flux_54degPA","FODU_Flux_72degPA","FODU_Flux_90degPA","FODU_Flux_108degPA","FODU_Flux_126degPA","FODU_Flux_144degPA","FODU_Flux_162degPA","FODU_Flux_175.5degPA"]. * Column 2 Labels from HOPE_ENERGY_ION: ["FODU_Flux_E01/~1.00eV","FODU_Flux_E02/~1.20eV","FODU_Flux_E03/~1.34eV","FODU_Flux_E04/~1.55eV","FODU_Flux_E05/~1.83eV","FODU_Flux_E06/~2.18eV","FODU_Flux_E07/~2.5eV","FODU_Flux_E08/~3.0eV","FODU_Flux_E09/~3.4eV","FODU_Flux_E10/~3.9eV","FODU_Flux_E11/~4.6eV","FODU_Flux_E12/~5.3eV","FODU_Flux_E13/~6.3eV","FODU_Flux_E14/~7.3eV","FODU_Flux_E15/~8.5eV","FODU_Flux_E16/~9.9eV","FODU_Flux_E17/~11.5eV","FODU_Flux_E18/~13.4eV","FODU_Flux_E19/~15.7eV","FODU_Flux_E20/~18.3eV","FODU_Flux_E21/~21.2eV","FODU_Flux_E22/~24.8eV","FODU_Flux_E23/~29eV","FODU_Flux_E24/~34eV","FODU_Flux_E25/~39eV","FODU_Flux_E26/~46eV","FODU_Flux_E27/~53eV","FODU_Flux_E28/~62eV","FODU_Flux_E29/~72eV","FODU_Flux_E30/~84eV","FODU_Flux_E31/~98eV","FODU_Flux_E32/~114eV","FODU_Flux_E33/~133eV","FODU_Flux_E34/~155eV","FODU_Flux_E35/~181eV","FODU_Flux_E36/~211eV","FODU_Flux_E37/~246eV","FODU_Flux_E38/~286eV","FODU_Flux_E39/~330eV","FODU_Flux_E40/~390eV","FODU_Flux_E41/~450eV","FODU_Flux_E42/~530eV","FODU_Flux_E43/~610eV","FODU_Flux_E44/~720eV","FODU_Flux_E45/~830eV","FODU_Flux_E46/~970eV","FODU_Flux_E47/~1130eV","FODU_Flux_E48/~1320eV","FODU_Flux_E49/~1540eV","FODU_Flux_E50/~1790eV","FODU_Flux_E51/~2090eV","FODU_Flux_E52/~2400eV","FODU_Flux_E53/~2800eV","FODU_Flux_E54/~3300eV","FODU_Flux_E55/~3800eV","FODU_Flux_E56/~4500eV","FODU_Flux_E57/~5200eV","FODU_Flux_E58/~6100eV","FODU_Flux_E59/~7100eV","FODU_Flux_E60/~8300eV","FODU_Flux_E61/~9600eV","FODU_Flux_E62/~11200eV","FODU_Flux_E63/~13100eV","FODU_Flux_E64/~15200eV","FODU_Flux_E65/~17800eV","FODU_Flux_E66/~20700eV","FODU_Flux_E67/~24000eV","FODU_Flux_E68/~28000eV","FODU_Flux_E69/~33000eV","FODU_Flux_E70/~38000eV","FODU_Flux_E71/~44000eV","FODU_Flux_E72/~52000eV"].

Oxygen Flux as a Function of 11 Pitch Angles, as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions. This parameter is virtual. It is calculated by calling the function APPLY_ESA_QFLAG with the following input parameters: FODU, Mode_Ion.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

-1.0e+31

Helium Differential Flux Intensity, Omnidirectional, Spectrograms

Time Series defined by using: EPOCH_ION

FHEDO

Helium Differential Flux Intensity, Omnidirectional, Spectrograms, Energies from ~1 eV to ~50 keV

Flux integrated, piecewise constant, over 11 Pitch Angles and 20 Gyro Angles as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and over 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

0.0

1.0e+16

-1.0e+31

Helium Differential Flux Intensity, Omnidirectional, Time Series Stack Plots

Time Series defined by using: EPOCH_ION

FHEDO_T

Helium Differential Flux Intensity, Omnidirectional, Time Series Stack Plots, Energies from ~1 eV to ~50 keV, Perigee Mode excluded

Flux integrated, piecewise constant, over 11 Pitch Angles and 20 Gyro Angles as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and over 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions. This parameter is virtual. It is calculated by calling the function APPLY_ESA_QFLAG with the following input parameters: FHEDO, Mode_Ion.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

0.0

1.0e+16

-1.0e+31

Helium Differential Flux Intensity, Unidirectional, Energy-Angle Plasmagrams

Time Series defined by using: EPOCH_ION

FHEDU

Helium Differential Flux Intensity, Unidirectional, Energy-Angle Plasmagrams, Energies from ~1 eV to ~50 keV. Column 1 Labels from PITCH_ANGLE: [ 4.50000, 18.0000, 36.0000, 54.0000, 72.0000, 90.0000, 108.000, 126.000, 144.000, 162.000, 175.500]

Helium Flux as a Function of 11 Pitch Angles, as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

-1.0e+31

Helium Differential Flux Intensity, Unidirectional, Spectrograms by Energy at Sample Pitch Angles

Time Series defined by using: EPOCH_ION

FHEDU_byE_atA

Helium Differential Flux Intensity, Unidirectional, Spectrograms by Energy at Sample Pitch Angles, Energies from ~1 eV to ~50 keV, Perigee Mode excluded. * Column 1 Labels from PITCH_ANGLE: ["FHEDU_Flux_4.5degPA","FHEDU_Flux_18degPA","FHEDU_Flux_36degPA","FHEDU_Flux_54degPA","FHEDU_Flux_72degPA","FHEDU_Flux_90degPA","FHEDU_Flux_108degPA","FHEDU_Flux_126degPA","FHEDU_Flux_144degPA","FHEDU_Flux_162degPA","FHEDU_Flux_175.5degPA"]. * Column 2 Labels from HOPE_ENERGY_ION: ["FHEDU_Flux_E01/~1.00eV","FHEDU_Flux_E02/~1.20eV","FHEDU_Flux_E03/~1.34eV","FHEDU_Flux_E04/~1.55eV","FHEDU_Flux_E05/~1.83eV","FHEDU_Flux_E06/~2.18eV","FHEDU_Flux_E07/~2.5eV","FHEDU_Flux_E08/~3.0eV","FHEDU_Flux_E09/~3.4eV","FHEDU_Flux_E10/~3.9eV","FHEDU_Flux_E11/~4.6eV","FHEDU_Flux_E12/~5.3eV","FHEDU_Flux_E13/~6.3eV","FHEDU_Flux_E14/~7.3eV","FHEDU_Flux_E15/~8.5eV","FHEDU_Flux_E16/~9.9eV","FHEDU_Flux_E17/~11.5eV","FHEDU_Flux_E18/~13.4eV","FHEDU_Flux_E19/~15.7eV","FHEDU_Flux_E20/~18.3eV","FHEDU_Flux_E21/~21.2eV","FHEDU_Flux_E22/~24.8eV","FHEDU_Flux_E23/~29eV","FHEDU_Flux_E24/~34eV","FHEDU_Flux_E25/~39eV","FHEDU_Flux_E26/~46eV","FHEDU_Flux_E27/~53eV","FHEDU_Flux_E28/~62eV","FHEDU_Flux_E29/~72eV","FHEDU_Flux_E30/~84eV","FHEDU_Flux_E31/~98eV","FHEDU_Flux_E32/~114eV","FHEDU_Flux_E33/~133eV","FHEDU_Flux_E34/~155eV","FHEDU_Flux_E35/~181eV","FHEDU_Flux_E36/~211eV","FHEDU_Flux_E37/~246eV","FHEDU_Flux_E38/~286eV","FHEDU_Flux_E39/~330eV","FHEDU_Flux_E40/~390eV","FHEDU_Flux_E41/~450eV","FHEDU_Flux_E42/~530eV","FHEDU_Flux_E43/~610eV","FHEDU_Flux_E44/~720eV","FHEDU_Flux_E45/~830eV","FHEDU_Flux_E46/~970eV","FHEDU_Flux_E47/~1130eV","FHEDU_Flux_E48/~1320eV","FHEDU_Flux_E49/~1540eV","FHEDU_Flux_E50/~1790eV","FHEDU_Flux_E51/~2090eV","FHEDU_Flux_E52/~2400eV","FHEDU_Flux_E53/~2800eV","FHEDU_Flux_E54/~3300eV","FHEDU_Flux_E55/~3800eV","FHEDU_Flux_E56/~4500eV","FHEDU_Flux_E57/~5200eV","FHEDU_Flux_E58/~6100eV","FHEDU_Flux_E59/~7100eV","FHEDU_Flux_E60/~8300eV","FHEDU_Flux_E61/~9600eV","FHEDU_Flux_E62/~11200eV","FHEDU_Flux_E63/~13100eV","FHEDU_Flux_E64/~15200eV","FHEDU_Flux_E65/~17800eV","FHEDU_Flux_E66/~20700eV","FHEDU_Flux_E67/~24000eV","FHEDU_Flux_E68/~28000eV","FHEDU_Flux_E69/~33000eV","FHEDU_Flux_E70/~38000eV","FHEDU_Flux_E71/~44000eV","FHEDU_Flux_E72/~52000eV"].

Helium Flux as a Function of 11 Pitch Angles, as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions. This parameter is virtual. It is calculated by calling the function ALTERNATE_VIEW with the following input parameters: FHEDU.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

-1.0e+31

Helium Differential Flux Intensity, Unidirectional, Spectrograms by Pitch Angle at Sample Energies

Time Series defined by using: EPOCH_ION

FHEDU_byA_atE

Helium Differential Flux Intensity, Unidirectional, Spectrograms by Pitch Angle at Sample Energies, Energies from ~1 eV to ~50 keV, Perigee Mode excluded. * Column 1 Labels from PITCH_ANGLE: ["FHEDU_Flux_4.5degPA","FHEDU_Flux_18degPA","FHEDU_Flux_36degPA","FHEDU_Flux_54degPA","FHEDU_Flux_72degPA","FHEDU_Flux_90degPA","FHEDU_Flux_108degPA","FHEDU_Flux_126degPA","FHEDU_Flux_144degPA","FHEDU_Flux_162degPA","FHEDU_Flux_175.5degPA"]. * Column 2 Labels from HOPE_ENERGY_ION: ["FHEDU_Flux_E01/~1.00eV","FHEDU_Flux_E02/~1.20eV","FHEDU_Flux_E03/~1.34eV","FHEDU_Flux_E04/~1.55eV","FHEDU_Flux_E05/~1.83eV","FHEDU_Flux_E06/~2.18eV","FHEDU_Flux_E07/~2.5eV","FHEDU_Flux_E08/~3.0eV","FHEDU_Flux_E09/~3.4eV","FHEDU_Flux_E10/~3.9eV","FHEDU_Flux_E11/~4.6eV","FHEDU_Flux_E12/~5.3eV","FHEDU_Flux_E13/~6.3eV","FHEDU_Flux_E14/~7.3eV","FHEDU_Flux_E15/~8.5eV","FHEDU_Flux_E16/~9.9eV","FHEDU_Flux_E17/~11.5eV","FHEDU_Flux_E18/~13.4eV","FHEDU_Flux_E19/~15.7eV","FHEDU_Flux_E20/~18.3eV","FHEDU_Flux_E21/~21.2eV","FHEDU_Flux_E22/~24.8eV","FHEDU_Flux_E23/~29eV","FHEDU_Flux_E24/~34eV","FHEDU_Flux_E25/~39eV","FHEDU_Flux_E26/~46eV","FHEDU_Flux_E27/~53eV","FHEDU_Flux_E28/~62eV","FHEDU_Flux_E29/~72eV","FHEDU_Flux_E30/~84eV","FHEDU_Flux_E31/~98eV","FHEDU_Flux_E32/~114eV","FHEDU_Flux_E33/~133eV","FHEDU_Flux_E34/~155eV","FHEDU_Flux_E35/~181eV","FHEDU_Flux_E36/~211eV","FHEDU_Flux_E37/~246eV","FHEDU_Flux_E38/~286eV","FHEDU_Flux_E39/~330eV","FHEDU_Flux_E40/~390eV","FHEDU_Flux_E41/~450eV","FHEDU_Flux_E42/~530eV","FHEDU_Flux_E43/~610eV","FHEDU_Flux_E44/~720eV","FHEDU_Flux_E45/~830eV","FHEDU_Flux_E46/~970eV","FHEDU_Flux_E47/~1130eV","FHEDU_Flux_E48/~1320eV","FHEDU_Flux_E49/~1540eV","FHEDU_Flux_E50/~1790eV","FHEDU_Flux_E51/~2090eV","FHEDU_Flux_E52/~2400eV","FHEDU_Flux_E53/~2800eV","FHEDU_Flux_E54/~3300eV","FHEDU_Flux_E55/~3800eV","FHEDU_Flux_E56/~4500eV","FHEDU_Flux_E57/~5200eV","FHEDU_Flux_E58/~6100eV","FHEDU_Flux_E59/~7100eV","FHEDU_Flux_E60/~8300eV","FHEDU_Flux_E61/~9600eV","FHEDU_Flux_E62/~11200eV","FHEDU_Flux_E63/~13100eV","FHEDU_Flux_E64/~15200eV","FHEDU_Flux_E65/~17800eV","FHEDU_Flux_E66/~20700eV","FHEDU_Flux_E67/~24000eV","FHEDU_Flux_E68/~28000eV","FHEDU_Flux_E69/~33000eV","FHEDU_Flux_E70/~38000eV","FHEDU_Flux_E71/~44000eV","FHEDU_Flux_E72/~52000eV"].

Helium Flux as a Function of 11 Pitch Angles, as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis, and 72 Energies. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions. This parameter is virtual. It is calculated by calling the function APPLY_ESA_QFLAG with the following input parameters: FHEDU, Mode_Ion.

PT11.35S

(cm^2 s sr keV)^-1

6.24161e-16>(m^2 s sr J)^-1

-1.0e+31

Data Quality Flag Type Descriptions, Electron Data

Time Series defined by using: EPOCH_ELE

Flags_Ele

Data Quality Flag Type Descriptions, Electron Data

Flags to indicate potential Issues with Electron Data. Each Element of this Array contains the Flag Status for a particular Concern. A Value of Zero of r a particular File Type indicates no unusual Concerns of that Type for that Time Sample. Increasing Flag Values indicate increasing Concern. See the FLAGS Variable for a Description of each Element.

PT11.35S

0

254

255

Data Quality Flag Type Descriptions, Ion Data

Time Series defined by using: EPOCH_ION

Flags_Ion

Data Quality Flag Type Descriptions, Ion Data

Flags to indicate potential Issues with Ion Data. Each Element of this Array contains the Flag Status for a particular Concern. A Value of Zero of r a particular File Type indicates no unusual Concerns of that Type for that Time Sample. Increasing Flag Values indicate increasing Concern. See the FLAGS Variable for a Description of each Element.

PT11.35S

0

254

255

Instrument Data Mode, Electron

Time Series defined by using: EPOCH_ELE

Mode_Ele

Instrument Data Mode, Electron

Indicates the Instrument Mode for the Data Collection. Each Instrument Mode has a different Set of Energy Channels. See the corresponding HOPE_ENERGY_Electron Record. 0=Apogee Mode: Normal Operation, 1=Perigee Mode: Minimum Energy Channel raised during the Pass through Perigee, 2=Burst Mode: Subset of Energies sampled at rapid Cadence.

PT11.35S

0

2

255

Instrument Data Mode, Ion

Time Series defined by using: EPOCH_ION

Mode_Ion

Instrument Data Mode, Ion

Indicates the Instrument Mode for the Data Collection. Each Instrument Mode has a different Set of Energy Channels. See the corresponding HOPE_ENERGY_Electron Record. 0=Apogee Mode: Normal Operation, 1=Perigee Mode: Minimum Energy Channel raised during the Pass through Perigee, 2=Burst Mode: Subset of Energies sampled at rapid Cadence.

PT11.35S

0

1

255

HOPE Electron Differential Counts, Omnidirectional

Time Series defined by using: EPOCH_ELE

Counts_E_Omni

HOPE Electron Differential Counts, Omnidirectional

Counts summed over over 72 Energies and over 20 Gyro Angles and 11 Pitch Angles as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions.

PT11.35S

0.0

1.0e+16

-1.0e+31

HOPE Electron Differential Counts, Directional

Time Series defined by using: EPOCH_ELE

Counts_E

HOPE Electron Differential Counts, Directional, not for Plotting. Column 1 Labels from PITCH_ANGLE: [ 4.50000, 18.0000, 36.0000, 54.0000, 72.0000, 90.0000, 108.000, 126.000, 144.000, 162.000, 175.500]

Counts as a Function of 72 Energies and 11 Pitch Angles as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions. The Counts are summed over all Measurements in each Pitch Angle/Gyro Angle Bin.

PT11.35S

-1.0e+31

HOPE Proton Differential Counts, Omnidirectional

Time Series defined by using: EPOCH_ION

Counts_P_Omni

HOPE Proton Differential Counts, Omnidirectional

Counts summed over over 72 Energies and over 20 Gyro Angles and 11 Pitch Angles as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions.

PT11.35S

0.0

1.0e+16

-1.0e+31

HOPE Proton Differential Counts, Directional

Time Series defined by using: EPOCH_ION

Counts_P

HOPE Proton Differential Counts, Directional, not for Plotting. Column 1 Labels from PITCH_ANGLE: [ 4.50000, 18.0000, 36.0000, 54.0000, 72.0000, 90.0000, 108.000, 126.000, 144.000, 162.000, 175.500]

Counts as a Function of 72 Energies and 11 Pitch Angles as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions. The Counts are summed over all Measurements in each Pitch Angle/Gyro Angle Bin.

PT11.35S

-1.0e+31

HOPE Helium Differential Counts, Omnidirectional

Time Series defined by using: EPOCH_ION

Counts_He_Omni

HOPE Helium Differential Counts, Omnidirectional

Counts summed over over 72 Energies and over 20 Gyro Angles and 11 Pitch Angles as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions.

PT11.35S

0.0

1.0e+16

-1.0e+31

HOPE Helium Differential Counts, Directional

Time Series defined by using: EPOCH_ION

Counts_He

HOPE Helium Differential Counts, Directional, not for Plotting. Column 1 Labels from PITCH_ANGLE: [ 4.50000, 18.0000, 36.0000, 54.0000, 72.0000, 90.0000, 108.000, 126.000, 144.000, 162.000, 175.500]

Counts as a Function of 72 Energies and 11 Pitch Angles as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions. The Counts are summed over all Measurements in each Pitch Angle/Gyro Angle Bin.

PT11.35S

-1.0e+31

HOPE Oxygen Differential Counts, Omnidirectional

Time Series defined by using: EPOCH_ION

Counts_O_Omni

HOPE Oxygen Differential Counts, Omnidirectional

Counts summed over over 72 Energies and over 20 Gyro Angles and 11 Pitch Angles as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions.

PT11.35S

0.0

1.0e+16

-1.0e+31

HOPE Oxygen Differential Counts, Directional

Time Series defined by using: EPOCH_ION

Counts_O

HOPE Oxygen Differential Counts, Directional, not for Plotting. Column 1 Labels from PITCH_ANGLE: [ 4.50000, 18.0000, 36.0000, 54.0000, 72.0000, 90.0000, 108.000, 126.000, 144.000, 162.000, 175.500]

Counts as a Function of 72 Energies and 11 Pitch Angles as computed by using the Magnetic Field Direction crossed with the Spacecraft Spin Axis. Note that the Data have been expanded to the highest possible Resolution. Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions. The Counts are summed over all Measurements in each Pitch Angle/Gyro Angle Bin.

PT11.35S

-1.0e+31

Number of Samples in the Summation, Electron Differential Flux Intensity, Omnidirectional

Time Series defined by using: EPOCH_ELE

Ele_SAMPLES_Omni

Number of Samples in the Summation, Electron Differential Flux Intensity, Omnidirectional, not for Plotting

Number of Samples used in computing the Flux summed over Pitch Angle. Note that the Data have been expanded to the highest possible Resolution (16 Spin angles, 72 Energies). Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions.

PT11.35S

0

253

255

Number of Samples in the Summation, Electron Differential Flux Intensity, Unidirectional

Time Series defined by using: EPOCH_ELE

Ele_SAMPLES

Number of Samples in the Summation, Electron Differential Flux Intensity, Unidirectional, not for Plotting. Column 1 Labels from PITCH_ANGLE: [ 4.50000, 18.0000, 36.0000, 54.0000, 72.0000, 90.0000, 108.000, 126.000, 144.000, 162.000, 175.500]

Number of Samples used in computing the Flux summed over Pitch Angle. Note that the Data have been expanded to the highest possible Resolution (16 Spin angles, 72 Energies). Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions.

PT11.35S

255

Number of Samples in the Summation, Ion Differential Flux Intensity, Omnidirectional

Time Series defined by using: EPOCH_ION

Ion_SAMPLES_Omni

Number of Samples in the Summation, Ion Differential Flux Intensity, Omnidirectional, not for Plotting

Number of Samples used in computing the Flux summed over Pitch Angle. Note that the Data have been expanded to the highest possible Resolution (16 Spin angles, 72 Energies). Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions.

PT11.35S

0

253

255

Number of Samples in the Summation, Ion Differential Flux Intensity, Unidirectional

Time Series defined by using: EPOCH_ION

Ion_SAMPLES

Number of Samples in the Summation, Ion Differential Flux Intensity, Unidirectional, not for Plotting. Column 1 Labels from PITCH_ANGLE: [ 4.50000, 18.0000, 36.0000, 54.0000, 72.0000, 90.0000, 108.000, 126.000, 144.000, 162.000, 175.500]

Number of Samples used in computing the Flux summed over Pitch Angle. Note that the Data have been expanded to the highest possible Resolution (16 Spin angles, 72 Energies). Before September 2013, the transmitted Data were collapsed to 36 Energies and 4-8-16-8-4 Spin Angles in order to meet Telemetry Allocation Restrictions.

PT11.35S

255

Model Spacecraft Magnetic Field Magnitude, Electrons

Time Series defined by using: EPOCH_ELE

B_Calc_Ele

Model Spacecraft Magnetic Field Magnitude, Electron Time Base

The Model Magnetic Field Data was interpolated from the 1 min Magnetic Field Ephemeris Time Resolution to match the Electron Measurement Time Base. Calculated by using the LANLGeoMag Software Library. Internal Magnetic Field Model: International Geomagnetic Reference Field, IGRF. External Magnetic Field Model: Olson-Pfitzer 1977 Quiet, OP77Q. Average Type: standard

PT11.35S

nT

1.0e-9>T

0.0

99999.0

-1.0e+31

Model Spacecraft Magnetic Field Magnitude, Ions

Time Series defined by using: EPOCH_ION

B_Calc_Ion

Model Spacecraft Magnetic Field Magnitude, Ion Time Base

The Model Magnetic Field Data was interpolated from the 1 min Magnetic Field Ephemeris Time Resolution to match the Ion Measurement Time Base. Calculated by using the LANLGeoMag Software Library. Internal Magnetic Field Model: International Geomagnetic Reference Field, IGRF. External Magnetic Field Model: Olson-Pfitzer 1977 Quiet, OP77Q. Average Type: standard

PT11.35S

nT

1.0e-9>T

0.0

99999.0

-1.0e+31

Model Magnetic Field Magnitude, Magnetic Equator, Electrons

Time Series defined by using: EPOCH_ELE

B_Eq_Ele

Model Magnetic Field Magnitude, Magnetic Equator, Electron Time Base

The Model Magnetic Field Data was interpolated from the 1 min Magnetic Field Ephemeris Time Resolution to match the Electron Measurement Time Base. Calculated by using the LANLGeoMag Software Library. Internal Magnetic Field Model: International Geomagnetic Reference Field, IGRF. External Magnetic Field Model: Olson-Pfitzer 1977 Quiet, OP77Q. Average Type: standard

PT11.35S

nT

1.0e-9>T

0.0

99999.0

-1.0e+31

Model Magnetic Field Magnitude, Magnetic Equator, Ions

Time Series defined by using: EPOCH_ION

B_Eq_Ion

Model Magnetic Field Magnitude, Magnetic Equator, Ion Time Base

The Model Magnetic Field Data was interpolated from the 1 min Magnetic Field Ephemeris Time Resolution to match the Ion Measurement Time Base. Calculated by using the LANLGeoMag Software Library. Internal Magnetic Field Model: International Geomagnetic Reference Field, IGRF. External Magnetic Field Model: Olson-Pfitzer 1977 Quiet, OP77Q. Average Type: standard

PT11.35S

nT

1.0e-9>T

0.0

99999.0

-1.0e+31

Electron Second Adiabatic Invariant, Bounce, Electrons

Time Series defined by using: EPOCH_ELE

I_Ele

Electron Second Adiabatic Invariant, Bounce, Electron Time Base

The Model Magnetic Field Data was interpolated from the 1 min Magnetic Field Ephemeris Time Resolution to match the Electron Measurement Time Base. Calculated by using the LANLGeoMag Software Library. Internal Magnetic Field Model: International Geomagnetic Reference Field, IGRF. External Magnetic Field Model: Olson-Pfitzer 1977 Quiet, OP77Q. Average Type: standard

PT11.35S

0.0

1000.0

-1.0e+31

Ion Second Adiabatic Invariant, Bounce, Ions

Time Series defined by using: EPOCH_ION

I_Ion

Ion Second Adiabatic Invariant, Bounce, Ion Time Base

The Model Magnetic Field Data was interpolated from the 1 min Magnetic Field Ephemeris Time Resolution to match the Ion Measurement Time Base. Calculated by using the LANLGeoMag Software Library. Internal Magnetic Field Model: International Geomagnetic Reference Field, IGRF. External Magnetic Field Model: Olson-Pfitzer 1977 Quiet, OP77Q. Average Type: standard

PT11.35S

0.0

1000.0

-1.0e+31

McIlwain L Shell Parameter, Electrons

Time Series defined by using: EPOCH_ELE

L_Ele

McIlwain L Shell Parameter, Electron Time Base

The Model Magnetic Field Data was interpolated from the 1 min Magnetic Field Ephemeris Time Resolution to match the Electron Measurement Time Base. Calculated by using the LANLGeoMag Software Library. Internal Magnetic Field Model: International Geomagnetic Reference Field, IGRF. External Magnetic Field Model: Olson-Pfitzer 1977 Quiet, OP77Q. Average Type: standard

PT11.35S

0.0

1000.0

-1.0e+31

McIlwain L Shell Parameter, Ions

Time Series defined by using: EPOCH_ION

L_Ion

McIlwain L Shell Parameter, Ion Time Base

The Model Magnetic Field Data was interpolated from the 1 min Magnetic Field Ephemeris Time Resolution to match the Ion Measurement Time Base. Calculated by using the LANLGeoMag Software Library. Internal Magnetic Field Model: International Geomagnetic Reference Field, IGRF. External Magnetic Field Model: Olson-Pfitzer 1977 Quiet, OP77Q. Average Type: standard

PT11.35S

0.0

1000.0

-1.0e+31

Roederer L* generalized L Shell Parameter, Electrons

Time Series defined by using: EPOCH_ELE

L_star_Ele

Roederer L* generalized L Shell Parameter, Electron Time Base

The Model Magnetic Field Data was interpolated from the 1 min Magnetic Field Ephemeris Time Resolution to match the Electron Measurement Time Base. Calculated by using the LANLGeoMag Software Library. Internal Magnetic Field Model: International Geomagnetic Reference Field, IGRF. External Magnetic Field Model: Olson-Pfitzer 1977 Quiet, OP77Q. Average Type: standard

PT11.35S

0.0

1000.0

-1.0e+31

Roederer L* generalized L Shell Parameter, Ions

Time Series defined by using: EPOCH_ION

L_star_Ion

Roederer L* generalized L Shell Parameter, Ion Time Base

The Model Magnetic Field Data was interpolated from the 1 min Magnetic Field Ephemeris Time Resolution to match the Ion Measurement Time Base. Calculated by using the LANLGeoMag Software Library. Internal Magnetic Field Model: International Geomagnetic Reference Field, IGRF. External Magnetic Field Model: Olson-Pfitzer 1977 Quiet, OP77Q. Average Type: standard

PT11.35S

0.0

1000.0

-1.0e+31

Spacecraft Position, Magnetic Local Time, Electrons

Time Series defined by using: EPOCH_ELE

MLT_Ele

Spacecraft Position, Magnetic Local Time, MLT, in Hours, Electron Time Base

The Model Magnetic Field Data was interpolated from the 1 min Magnetic Field Ephemeris Time Resolution to match the Electron Measurement Time Base. Calculated by using the LANLGeoMag Software Library. Internal Magnetic Field Model: International Geomagnetic Reference Field, IGRF. External Magnetic Field Model: Olson-Pfitzer 1977 Quiet, OP77Q. Average Type: standard

PT11.35S

h

3600>s

0.0

24.0

-1.0e+31

Spacecraft Position, Magnetic Local Time, Ions

Time Series defined by using: EPOCH_ION

MLT_Ion

Spacecraft Position, Magnetic Local Time, MLT, in Hours, Ion Time Base

The Model Magnetic Field Data was interpolated from the 1 min Magnetic Field Ephemeris Time Resolution to match the Ion Measurement Time Base. Calculated by using the LANLGeoMag Software Library. Internal Magnetic Field Model: International Geomagnetic Reference Field, IGRF. External Magnetic Field Model: Olson-Pfitzer 1977 Quiet, OP77Q. Average Type: standard

PT11.35S

h

3600>s

0.0

24.0

-1.0e+31

Spacecraft Position Vector, Geographic Cartesian Coordinates, Electrons

Time Series defined by using: EPOCH_ELE

Position_Ele

Spacecraft Position Vector, Geographic, GEO, Cartesian Coordinates, Electron Time Base

The Origin is the Center of Mass of the Earth. The X-Axis points to the Intersection of the Greenwich Meridian and Geographic Equator. The Z Axis points to the Geographic North Pole. The Y Axis completes the Right-Handed Cartesian Triad with Y = -X × Z.

PT11.35S

km

1.0e3>m

-63700.0

63700.0

-1.0e+31

Spacecraft Position Vector, Geographic Cartesian Coordinates, Ions

Time Series defined by using: EPOCH_ION

Position_Ion

Spacecraft Position Vector, Geographic, GEO, Cartesian Coordinates, Ion Time Base

The Origin is the Center of Mass of the Earth. The X-Axis points to the Intersection of the Greenwich Meridian and Geographic Equator. The Z Axis points to the Geographic North Pole. The Y Axis completes the Right-Handed Cartesian Triad with Y = -X × Z.

PT11.35S

km

1.0e3>m

-63700.0

63700.0

-1.0e+31