MMS Satellite Number 1 Dual Electron Spectrometer Burst-resolution instrument distributions

MMS1 FPI/DES burst data begin-time; derived from burst packet time.

[CDAWeb List/Download/Create ONLY] MMS1 FPI/DES burst sky-map instrument distribution

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.

MMS1 FPI/DES burst sky-map instrument distribution - 10.9 eV (E1/even)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst1_even(*,*,1)

MMS1 FPI/DES burst sky-map instrument distribution - 12.4 eV (E1/odd)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst1_odd(*,*,1)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst1_evenodd_movie(*,*,1)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst1_even_movie(*,*,1)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst1_odd_movie(*,*,1)

MMS1 FPI/DES burst sky-map instrument distribution - 37.9 eV (E6/even)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst6_even(*,*,6)

MMS1 FPI/DES burst sky-map instrument distribution - 42.9 eV (E6/odd)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst6_odd(*,*,6)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst6_evenodd_movie(*,*,6)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst6_even_movie(*,*,6)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst6_odd_movie(*,*,6)

MMS1 FPI/DES burst sky-map instrument distribution - 80.0 eV (E9/even)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst9_even(*,*,9)

MMS1 FPI/DES burst sky-map instrument distribution - 90.6 eV (E9/odd)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst9_odd(*,*,9)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst9_evenodd_movie(*,*,9)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst9_even_movie(*,*,9)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst9_odd_movie(*,*,9)

MMS1 FPI/DES burst sky-map instrument distribution - 169 eV (E12/even)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst12_even(*,*,12)

MMS1 FPI/DES burst sky-map instrument distribution - 191 eV (E12/odd)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst12_odd(*,*,12)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst12_evenodd_movie(*,*,12)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst12_even_movie(*,*,12)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst12_odd_movie(*,*,12)

MMS1 FPI/DES burst sky-map instrument distribution - 277 eV (E14/even)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst14_even(*,*,14)

MMS1 FPI/DES burst sky-map instrument distribution - 314 eV (E14/odd)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst14_odd(*,*,14)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst14_evenodd_movie(*,*,14)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst14_even_movie(*,*,14)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst14_odd_movie(*,*,14)

MMS1 FPI/DES burst sky-map instrument distribution - 456 eV (E16/even)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst16_even(*,*,16)

MMS1 FPI/DES burst sky-map instrument distribution - 517 eV (E16/odd)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst16_odd(*,*,16)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst16_evenodd_movie(*,*,16)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst16_even_movie(*,*,16)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst16_odd_movie(*,*,16)

MMS1 FPI/DES burst sky-map instrument distribution - 750 eV (E18/even)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst18_even(*,*,18)

MMS1 FPI/DES burst sky-map instrument distribution - 850 eV (E18/odd)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst18_odd(*,*,18)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst18_evenodd_movie(*,*,18)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst18_even_movie(*,*,18)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst18_odd_movie(*,*,18)

MMS1 FPI/DES burst sky-map instrument distribution - 1230 eV (E20/even)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst20_even(*,*,20)

MMS1 FPI/DES burst sky-map instrument distribution - 1400 eV (E20/odd)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst20_odd(*,*,20)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst20_evenodd_movie(*,*,20)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst20_even_movie(*,*,20)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst20_odd_movie(*,*,20)

MMS1 FPI/DES burst sky-map instrument distribution - 2600 eV (E23/even)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst23_even(*,*,23)

MMS1 FPI/DES burst sky-map instrument distribution - 2950 eV (E23/odd)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst23_odd(*,*,23)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst23_evenodd_movie(*,*,23)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst23_even_movie(*,*,23)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst23_odd_movie(*,*,23)

MMS1 FPI/DES burst sky-map instrument distribution - 5490 eV (E26/even)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst26_even(*,*,26)

MMS1 FPI/DES burst sky-map instrument distribution - 6210 eV (E26/odd)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst26_odd(*,*,26)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst26_evenodd_movie(*,*,26)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst26_even_movie(*,*,26)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst26_odd_movie(*,*,26)

MMS1 FPI/DES burst sky-map instrument distribution - 24400 eV (E32/even)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst32_even(*,*,32)

MMS1 FPI/DES burst sky-map instrument distribution - 27600 eV (E32/odd)

plasmagram>THUMBSIZE>60>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst32_odd(*,*,32)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst32_evenodd_movie(*,*,32)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst32_even_movie(*,*,32)

plasma_movie>xsz=2,ysz=4> x=mms1_des_phi_brst, y=mms1_des_theta_brst, z=mms1_des_dist_brst32_odd_movie(*,*,32)

[List/Create only in CDAWeb] 1-sigma error: MMS1 FPI/DES burst sky-map instrument distribution

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. Offsets reflect 128 steps over the 30 msec sweep period. See FPI docs for details.

MMS1 FPI/DES vector of data-quality indicators at burst-start time

Value of zero signifies no quality errors. For non-zero values: Bit-0 = manually flagged interval, Bit-1 = overcounting/saturation effects likely present in skymap

---> MMS1 FPI/DES compression lossless/lossy indicator at survey-start time

FPI/DES alternates between two tables, designated "even" (0) and "odd" (1).

---> MMS1 FPI/DES Del-Phi (obs spin-phase) count at burst-start time

Nominally, spin-phase counts range over [0000, 5759] cnts.  Each count represents 1/16 deg of observatory spin-phase.  Zero spin-phase count indicates obs +X-axis aligned with Sun.

---> MMS1 FPI/DES Del-Phi (obs spin-phase) angle at burst-start time

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.

Records P-value used to de-spin this burst sky-map on board.  See FPI docs for details.

Azimuth bin: sector index=00 looks "after" (spin-phase) Sun, ..., sector index=31 looks "before" Sun dir.

Azimuth bin: "sector00" looks after Sun, ..., "sector31" looks before Sun dir.

Head field-of-view: pixel index=00 looks to zenith, ..., pixel index=15 looks to nadir.

Head field-of-view: "pixel00" looks to zenith, ..., "pixel15" 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.

Note that the deltas are provided to indicate that FPI is reporting the energy bin centers. These do not necessarily reflect the energy bandwidth that is sampled by FPI at a given energy step.


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