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Dataset results
7 results for “MS waves”
DATA for 3D PIC simulation of MS waves
<p>Data for the paper of Excitation of magnetosonic waves in the Earth's dipole magnetic field: 3D PIC simulation</p>
DATA for MS wave modulation
<p>DATA for the paper of Modulation of magnetosonic waves by background plasma density in a dipole magnetic field: 2-D PIC simulation</p>
Fitting parameters for "Concurrent Observation of High-frequency EMIC Waves and Low-harmonic Fast MS Waves within a Magnetic Dip in the Inner Magnetosphere"
<p>1. whamp_input_ionfit_*.mat</p> <p>The fitting parameters for the growth rate calculation of HFEMIC waves, which includes: </p> <div> <div>Bi-Maxwellian distribution parameters:</div> <div>PlasmaModel.B - magnetic field in nT</div> <div>PlasmaModel.Species.m - mass/mass_proton (0 means electron)</div> <div>PlasmaModel.Species.n - density in cm^-3</div> <div>PlasmaModel.Species.t - temperature in eV</div> <div>PlasmaModel.Species.a - anisotropy, Tperp/Tpara</div> <div> </div> </div> <p>2. shell_dist_*.mat</p> <p>The fitting parameters for the growth rate calculation of MS waves, which includes:</p> <div>Bi-Maxwellian distribution parameters:</div> <div>PlasmaModel.B - magnetic field in nT</div> <div>PlasmaModel.Species.m - mass/mass_proton (0 means electron)</div> <div>PlasmaModel.Species.n - density in cm^-3</div> <div>PlasmaModel.Species.t - temperature in eV</div> <div>PlasmaModel.Species.a - anisotropy, Tperp/Tpara</div> <div> </div> <div>Partial shell distribution parameters:</div> <div> <div>PlasmaModel.Shell.m - mass/mass_proton (0 means electron)</div> <div>PlasmaModel.Shell.ns - density in cm^-3</div> <div>PlasmaModel.Shell.sigma - the degree of pitch angle anisotropy</div> <div>PlasmaModel.Shell.Vs - the shell speed in m/s <div>PlasmaModel.Shell.theta_s - the thermal spread of the shell in m/s</div> </div> </div>
Study on electron stochastic motions in the MS wave field: Test particle simulations
<p>The data used to generate the figures in this study.</p>
RENU2 COrnell Wire BOom Yo-yo (COWBOY) Electric Field Very Low Frequency Waves, High Time Resolution (H0), 1 ms Data
Rocket Experiment for Neutral Upwelling 2, RENU2, COrnell Wire BOom Yo-yo, COWBOY, Very Low Frequency, VLF, Electric Field Measurements
Van Allen Probe B Electric Field and Waves Suite (EFW) Burst Mode 1 (512 Samples/sec) Electric and Magnetic Fields, Waveform, in Spacecraft Spin (UVW) Coordinates, Level 1 (L1), 1.95 ms Data
The EFW Burst Modes provide targeted Measurements over Brief Time Intervals of 3-D Electric Fields, 3-D Wave Magnetic Fields, and Spacecraft Potential. There are two EFW Burst Modes: BURST1 (B1), Medium-Rate 512 samples/s nominal and BURST2 (B2), Higher-Rate, 16384 samples/s nominal. The Burst 1 Mode Data 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 (SCM_U_B1, SCM_V_B1, SCM_W_B1 from the EMFISIS Search Coil Magnetometer). 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 again from the EMFISIS Search Coil Magnetometer) and Single-ended Potential Measurements (V1ac_B1 through V6ac_B2) with the exception that in the Default Mode the Single-ended Potential 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 Spacecraft 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 Type, 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 to trigger on large Amplitude Signals near 1 kHz. Sample Rates for B1 and B2 can and are changed depending on varying Science Goals.
Van Allen Probe A Electric Field and Waves Suite (EFW) Burst Mode 1 (512 Samples/sec) Electric and Magnetic Fields, Waveform, in Spacecraft Spin (UVW) Coordinates, Level 1 (L1), 1.95 ms Data
The EFW Burst Modes provide targeted Measurements over Brief Time Intervals of 3-D Electric Fields, 3-D Wave Magnetic Fields, and Spacecraft Potential. There are two EFW Burst Modes: BURST1 (B1), Medium-Rate 512 samples/s nominal and BURST2 (B2), Higher-Rate, 16384 samples/s nominal. The Burst 1 Mode Data 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 (SCM_U_B1, SCM_V_B1, SCM_W_B1 from the EMFISIS Search Coil Magnetometer). 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 again from the EMFISIS Search Coil Magnetometer) and Single-ended Potential Measurements (V1ac_B1 through V6ac_B2) with the exception that in the Default Mode the Single-ended Potential 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 Spacecraft 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 Type, 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 to trigger on large Amplitude Signals near 1 kHz. Sample Rates for B1 and B2 can and are changed depending on varying Science Goals.
ScienceDex guides
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