urn:nasa:pds:p11-crt-cal:data-15min-sat:p11_sat_crt_15min_het_let_ii 1.0 1.25.0.0 Product_Observational 2012 Pioneer 11 CRT 15 minute electron flux data from the Saturn Encounter. This file contains data from the High Energy Telescope (HET) channels R5B, and the Engery Telescope II (LET-II) channels SR2E(9), SR2F(9), SR2G(9), and SR2H(9). The data cover 1979-08-31 to 1979-09-03. This is a space-delimited ASCII table with fixed width columns. The data consist of a time column followed by a flux and flux uncertainty for each of the data channels. This file includes the following channels: Channel 1 = (R5B / 1.000E+00) R5B = A2 Channel 2 = (SR2E(9) / 1.500E-02) SR2E(9) = ^S1.S2(5).^S2(A).^S3(9) Channel 3 = (SR2F(9) / 1.500E-02) SR2F(9) = ^S1.S2(6).^S2(A).^S3(9) Channel 4 = (SR2G(9) / 1.500E-02) SR2G(9) = ^S1.S2(7).^S2(A).^S3(9) Channel 5 = (SR2H(9) / 1.500E-02) SR2H(9) = ^S1.S2(8).^S2(A).^S3(9) Individual detectors in LET-II subsystem are identified by S1, S2, S3, and S2(A), the annular guard detector. Detector A is in HET subsystem. The subscript in parentheses of a detector identifier refers to the trigger threshold on that detector. Several detectors defining a flux channel are in coincidence unless the symbol '^' preceding the detector identifier indicating that detector is in anti-coincidence. Frank Bethune McDonald Institute for Physical Science and Technology University of Maryland https://ror.org/047s2c258 1 Lal Nand Goddard Space Flight Center https://ror.org/0171mag52 2 2026-04-30 1.0 This is the first product released as part of the PDS4 bundle. The data themselves are unchanged. 1979-08-31T00:00:00.000Z 1979-09-03T18:45:00.000Z Science Calibrated Particles Electrons Cosmic Ray Particles Ions Cosmic Ray Pioneer 11 Mission urn:nasa:pds:context:investigation:mission.pioneer_11 data_to_investigation Cosmic Ray Telescope (CRT) Instrument urn:nasa:pds:context:instrument:crt.p11 is_instrument Pioneer 11 Host urn:nasa:pds:context:instrument_host:spacecraft.p11 is_instrument_host Solar Wind Plasma Stream urn:nasa:pds:context:target:plasma_stream.solar_wind data_to_target Saturn Planet urn:nasa:pds:context:target:planet.saturn data_to_target Jupiter-Saturn Cruise Saturn Encounter 50 21 Electrons Flux Ions Flux Proton Heavy Alpha urn:nasa:pds:p11-crt-cal:document:15min-data-desc::1.0 data_to_document P11-S-CRT-4-SUMM-FLUX-15MIN-V1.0:P11_SAT_CRT_15MIN_HET_LET_II:P11_SAT_CRT_15MIN_HET_LET_II.TAB data_to_calibrated_source_product 10.17189/1519795 PDS Planetary Plasma Interactions Node This is the first version of this product converted to PDS4. The DOI provided references the PDS3 source data set. P11_SAT_CRT_15MIN_HET_LET_II.TAB 1970-01-01T00:00:00.000Z 47808 80e3b99a6e03a8ce631a85386c3f170b This data file is unmodified from the PDS3 version. 0 288 Carriage-Return Line-Feed 11 0 166 START TIME 1 1 ASCII_Date_Time_YMD 23 %23s Spacecraft event time (UT) at which the particle counting begins. Time is given in the format of `yyyy-mm-ddThh:mm:ss.sss'. R5B_FLUX 2 26 ASCII_Real 13 %13.6e 1/(cm**2*sec*sr) Flux measured in HET energy channel R5B (> 2.01 MeV electrons). The coincidence logic for this channel is A2. -1 1.000000E+07 -0.9999 R5B_FLUX_UNCERTAINTY 3 40 ASCII_Real 13 %13.6e 1/(cm**2*sec*sr) Flux uncertainty for channel R5B. -1 1.000000E+04 -0.9999 SR2E(9)_FLUX 4 54 ASCII_Real 13 %13.6e 1/(cm**2*sec*sr) Flux measured in LET-II energy channel SR2E(9) (0.16-2.0 MeV electrons). The coincidence logic for this channel is ^S1.S2(5).^S2(A).^S3(9). -1 1.000000E+07 -0.9999 SR2E(9)_FLUX_UNCERTAINTY 5 68 ASCII_Real 13 %13.6e 1/(cm**2*sec*sr) Flux uncertainty for channel SR2E(9). -1 1.000000E+04 -0.9999 SR2F(9)_FLUX 6 82 ASCII_Real 13 %13.6e 1/(cm**2*sec*sr) Flux measured in LET-II energy channel SR2F(9) (0.43-2.0 MeV electrons). The coincidence logic for this channel is ^S1.S2(6).^S2(A).^S3(9). -1 1.000000E+07 -0.9999 SR2F(9)_FLUX_UNCERTAINTY 7 96 ASCII_Real 13 %13.6e 1/(cm**2*sec*sr) Flux uncertainty for channel SR2F(9). -1 1.000000E+04 -0.9999 SR2G(9)_FLUX 8 110 ASCII_Real 13 %13.6e 1/(cm**2*sec*sr) Flux measured in LET-II energy channel SR2G(9) (0.8-2.0 MeV electrons). The coincidence logic for this channel is ^S1.S2(7).^S2(A).^S3(9). -1 1.000000E+07 -0.9999 SR2G(9)_FLUX_UNCERTAINTY 9 124 ASCII_Real 13 %13.6e 1/(cm**2*sec*sr) Flux uncertainty for channel SR2G(9). -1 1.000000E+04 -0.9999 SR2H(9)_FLUX 10 138 ASCII_Real 13 %13.6e 1/(cm**2*sec*sr) Flux measured in LET-II energy channel SR2H(9) (1.1-2.0 MeV electrons). The coincidence logic for this channel is ^S1.S2(8).^S2(A).^S3(9). -1 1.000000E+07 -0.9999 SR2H(9)_FLUX_UNCERTAINTY 11 152 ASCII_Real 13 %13.6e 1/(cm**2*sec*sr) Flux uncertainty for channel SR2H(9). -1 1.000000E+04 -0.9999