From 9ad3bb39ce1f0dd66b13ad1e67193e857e454226 Mon Sep 17 00:00:00 2001 From: Elena.Budnik Date: Fri, 29 Mar 2019 12:46:41 +0100 Subject: [PATCH] EPD + USYSS corr --- NumericalData/AMDA/Galileo/EPD/gll-epd-amalele.xml | 266 ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ NumericalData/AMDA/Galileo/EPD/gll-epd-callele.xml | 270 ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ NumericalData/AMDA/Galileo/EPD/gll-epd-ert.xml | 4 ++++ NumericalData/AMDA/Galileo/EPD/gll-epd-euroele.xml | 274 ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ NumericalData/AMDA/Galileo/EPD/gll-epd-ganyele.xml | 271 +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ NumericalData/AMDA/Galileo/EPD/gll-epd-ioele.xml | 269 +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ NumericalData/AMDA/Galileo/EPD/gll-epd-rt.xml | 4 ++++ NumericalData/AMDA/Galileo/EPD/gll-epd-survele.xml | 279 +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ NumericalData/AMDA/ULYSSES/Ephemeris/ulys-orb-all.xml | 8 ++++---- NumericalData/AMDA/ULYSSES/Ephemeris/ulys-orb-jup.xml | 2 +- Person/Quentin.Nenon.xml | 12 ++++++++++++ 11 files changed, 1654 insertions(+), 5 deletions(-) create mode 100644 NumericalData/AMDA/Galileo/EPD/gll-epd-amalele.xml create mode 100644 NumericalData/AMDA/Galileo/EPD/gll-epd-callele.xml create mode 100644 NumericalData/AMDA/Galileo/EPD/gll-epd-euroele.xml create mode 100644 NumericalData/AMDA/Galileo/EPD/gll-epd-ganyele.xml create mode 100644 NumericalData/AMDA/Galileo/EPD/gll-epd-ioele.xml create mode 100644 NumericalData/AMDA/Galileo/EPD/gll-epd-survele.xml create mode 100644 Person/Quentin.Nenon.xml diff --git a/NumericalData/AMDA/Galileo/EPD/gll-epd-amalele.xml b/NumericalData/AMDA/Galileo/EPD/gll-epd-amalele.xml new file mode 100644 index 0000000..8db751a --- /dev/null +++ b/NumericalData/AMDA/Galileo/EPD/gll-epd-amalele.xml @@ -0,0 +1,266 @@ + + + 2.2.6 + + spase://CDPP/NumericalData/AMDA/Galileo/EPD/gll-epd-amalele + + flyby amalthea + flyby amalthea : electrons + 2011-09-26T12:32:02Z + + Energetic electron count rates and fluxes measured by the EPD instrument + onboard Galileo in the Record acquisition mode. In this mode, the count rates are + accumulated during around 1.25 second. The full opening angle of the EPD telescopes + are relatively narrow, between 15° and 18°, and the acquisition period is very short compared + to the rotational spin period of Galileo. Counts and fluxes obtained with the Record + acquisition mode can therefore be considered as directional flux measurements. + The local and equatorial pitch angles that are given are for the particles observed by the + center of the telescope viewing cones. The motor that rotates the EPD telescopes around an + axis perpendicular to the spin axis of Galileo can have eight different step positions, + from 0 to 7. + +Data are extracted from the text file named 'galileo_epd_calibrated_low_res_v18.txt' +produced and provided by JHU/APL and publicly available at +http://sd-www.jhuapl.edu/Galileo_EPD/latest_calibrated_data/. +It is highly recommended to read the 'readme_v19.docx' document also available at the previous +link before using this dataset. It is also recommended to contact Peter Kollmann (JHU/APL), +as some measurement channels are highly contaminated or saturated. All unreliable measurements +are set to NaN. Energies, species and charge states observed by each measurement channel are +discussed in detail in Kollmann et al. [2018, JGR]. + +* 2002-11-05T02:44:40 2002-11-05T06:35:08 + + + spase://SMWG/Person/Donald.J.Williams + PrincipalInvestigator + + + spase://CDPP/Person/Peter.Kollmann + DataProducer + + + spase://CDPP/Person/Quentin.Nenon + DataProducer + + + spase://CDPP/Person/Christopher.Paranicas + CoInvestigator + + + spase://CDPP/Person/Norbert.Krupp + CoInvestigator + + + gll-epd-record-el + PartOf + record mode : electron channels + + + + spase://SMWG/Repository/CDPP/AMDA + + http://amda.cdpp.eu + + NetCDF + + JHU/APL + spase://CDPP/Instrument/AMDA/Galileo/EPD + EnergeticParticles + + + 1996-11-04T13:14:51Z + 2001-05-25T11:44:00Z + + PT1S + PT2S + + Jupiter + Electron channels : + * B1 : ≥ 36.2 MeV + * DC0 : ≥ 14 MeV + * DC1 : ≥ 30 MeV + * DC2 : ≥ 1.8 MeV + * DC3 : ≥ 10.8 MeV + * E[0-3] : 15 - 93 keV + * F[0-3] : 93 - 884 keV + + + L-shell + gll_epd_l_amel + + + + TimeSeries + + + Other + + + + local pitch angle + gll_epd_paloc_amel + + degree + + TimeSeries + + + Other + + + + motor position + gll_epd_motor_amel + + + + TimeSeries + + + Other + + + + e- : E[0-3] : cnts + gll_epd_am_ecnts + + s**-1 + + Spectrogram + + + 4 + + + Electron + CountRate + + + + e- : E[0-3] : flux + gll_epd_am_eflux + + cm**-2.s**-1.sr**-1.keV**-1 + + Spectrogram + + + 4 + + + Electron + NumberFlux + + + + e- : F[0-3] : cnts + gll_epd_am_fcnts + + s**-1 + + Spectrogram + + + 4 + + + Electron + CountRate + + + + + e- : B1 : cnts + gll_epd_amel_bcnts + + s**-1 + + TimeSeries + + + Electron + CountRate + + + + + e- : DC[0-3] : cnts + gll_epd_am_dccnts + + s**-1 + + TimeSeries + + + 4 + + DC0 : > 14 MeV + 1 + gll_epd_am_dccnts(0) + + + DC1 : > 30 MeV + 2 + gll_epd_am_dccnts(1) + + + DC2 : > 1.8 MeV + 3 + gll_epd_am_dccnts(2) + + + DC3 : > 10.8 MeV + 3 + gll_epd_am_dccnts(3) + + + + Electron + CountRate + + + + + diff --git a/NumericalData/AMDA/Galileo/EPD/gll-epd-callele.xml b/NumericalData/AMDA/Galileo/EPD/gll-epd-callele.xml new file mode 100644 index 0000000..28cd1de --- /dev/null +++ b/NumericalData/AMDA/Galileo/EPD/gll-epd-callele.xml @@ -0,0 +1,270 @@ + + + 2.2.6 + + spase://CDPP/NumericalData/AMDA/Galileo/EPD/gll-epd-callele + + flybys callisto + flybys callisto : electrons + 2011-09-26T12:32:02Z + + Energetic electron count rates and fluxes measured by the EPD instrument + onboard Galileo in the Record acquisition mode. In this mode, the count rates are + accumulated during around 1.25 second. The full opening angle of the EPD telescopes + are relatively narrow, between 15° and 18°, and the acquisition period is very short compared + to the rotational spin period of Galileo. Counts and fluxes obtained with the Record + acquisition mode can therefore be considered as directional flux measurements. + The local and equatorial pitch angles that are given are for the particles observed by the + center of the telescope viewing cones. The motor that rotates the EPD telescopes around an + axis perpendicular to the spin axis of Galileo can have eight different step positions, + from 0 to 7. + +Data are extracted from the text file named 'galileo_epd_calibrated_low_res_v18.txt' +produced and provided by JHU/APL and publicly available at +http://sd-www.jhuapl.edu/Galileo_EPD/latest_calibrated_data/. +It is highly recommended to read the 'readme_v19.docx' document also available at the previous +link before using this dataset. It is also recommended to contact Peter Kollmann (JHU/APL), +as some measurement channels are highly contaminated or saturated. All unreliable measurements +are set to NaN. Energies, species and charge states observed by each measurement channel are +discussed in detail in Kollmann et al. [2018, JGR]. + + * 1996-11-04T13:15:10 1996-11-04T14:00:12 + * 1997-06-25T13:25:50 1997-06-25T14:11:18 + * 1997-09-16T23:48:59 1997-09-17T00:49:38 + * 2001-05-25T11:09:41 2001-05-25T11:45:04 + + + + spase://SMWG/Person/Donald.J.Williams + PrincipalInvestigator + + + spase://CDPP/Person/Peter.Kollmann + DataProducer + + + spase://CDPP/Person/Quentin.Nenon + DataProducer + + + spase://CDPP/Person/Christopher.Paranicas + CoInvestigator + + + spase://CDPP/Person/Norbert.Krupp + CoInvestigator + + + gll-epd-record-el + PartOf + record mode : electron channels + + + + spase://SMWG/Repository/CDPP/AMDA + + http://amda.cdpp.eu + + NetCDF + + JHU/APL + spase://CDPP/Instrument/AMDA/Galileo/EPD + EnergeticParticles + + + 1996-11-04T13:14:51Z + 2001-05-25T11:44:00Z + + PT1S + PT2S + + Jupiter + Electron channels : + * B1 : ≥ 36.2 MeV + * DC0 : ≥ 14 MeV + * DC1 : ≥ 30 MeV + * DC2 : ≥ 1.8 MeV + * DC3 : ≥ 10.8 MeV + * E[0-3] : 15 - 93 keV + * F[0-3] : 93 - 884 keV + + + L-shell + gll_epd_l_cael + + + + TimeSeries + + + Other + + + + local pitch angle + gll_epd_paloc_cael + + degree + + TimeSeries + + + Other + + + + motor position + gll_epd_motor_cael + + + + TimeSeries + + + Other + + + + e- : E[0-3] : cnts + gll_epd_ca_ecnts + + s**-1 + + Spectrogram + + + 4 + + + Electron + CountRate + + + + e- : E[0-3] : flux + gll_epd_ca_eflux + + cm**-2.s**-1.sr**-1.keV**-1 + + Spectrogram + + + 4 + + + Electron + NumberFlux + + + + e- : F[0-3] : cnts + gll_epd_ca_fcnts + + s**-1 + + Spectrogram + + + 4 + + + Electron + CountRate + + + + e- : F[0-3] : flux + gll_epd_ca_fflux + + cm**-2.s**-1.sr**-1.keV**-1 + + Spectrogram + + + 4 + + + Electron + NumberFlux + + + + e- : B1 : cnts + gll_epd_cael_bcnts + + s**-1 + + TimeSeries + + + Electron + CountRate + + + + + e- : DC[0-3] : cnts + gll_epd_ca_dccnts + + s**-1 + + TimeSeries + + + 4 + + DC0 : > 14 MeV + 1 + gll_epd_ca_dccnts(0) + + + DC1 : > 30 MeV + 2 + gll_epd_ca_dccnts(1) + + + DC2 : > 1.8 MeV + 3 + gll_epd_ca_dccnts(2) + + + DC3 : > 10.8 MeV + 3 + gll_epd_ca_dccnts(3) + + + + Electron + CountRate + + + + + diff --git a/NumericalData/AMDA/Galileo/EPD/gll-epd-ert.xml b/NumericalData/AMDA/Galileo/EPD/gll-epd-ert.xml index c1bb52c..d40257a 100644 --- a/NumericalData/AMDA/Galileo/EPD/gll-epd-ert.xml +++ b/NumericalData/AMDA/Galileo/EPD/gll-epd-ert.xml @@ -39,6 +39,10 @@ spase://CDPP/Person/Peter.Kollmann DataProducer + + spase://CDPP/Person/Quentin.Nenon + DataProducer + spase://CDPP/Person/Christopher.Paranicas CoInvestigator diff --git a/NumericalData/AMDA/Galileo/EPD/gll-epd-euroele.xml b/NumericalData/AMDA/Galileo/EPD/gll-epd-euroele.xml new file mode 100644 index 0000000..1b67761 --- /dev/null +++ b/NumericalData/AMDA/Galileo/EPD/gll-epd-euroele.xml @@ -0,0 +1,274 @@ + + + 2.2.6 + + spase://CDPP/NumericalData/AMDA/Galileo/EPD/gll-epd-euroele + + flybys europa + flybys europa : electrons + 2011-09-26T12:32:02Z + + Energetic electron count rates and fluxes measured by the EPD instrument + onboard Galileo in the Record acquisition mode. In this mode, the count rates are + accumulated during around 1.25 second. The full opening angle of the EPD telescopes + are relatively narrow, between 15° and 18°, and the acquisition period is very short compared + to the rotational spin period of Galileo. Counts and fluxes obtained with the Record + acquisition mode can therefore be considered as directional flux measurements. + The local and equatorial pitch angles that are given are for the particles observed by the + center of the telescope viewing cones. The motor that rotates the EPD telescopes around an + axis perpendicular to the spin axis of Galileo can have eight different step positions, + from 0 to 7. + +Data are extracted from the text file named 'galileo_epd_calibrated_low_res_v18.txt' +produced and provided by JHU/APL and publicly available at +http://sd-www.jhuapl.edu/Galileo_EPD/latest_calibrated_data/. +It is highly recommended to read the 'readme_v19.docx' document also available at the previous +link before using this dataset. It is also recommended to contact Peter Kollmann (JHU/APL), +as some measurement channels are highly contaminated or saturated. All unreliable measurements +are set to NaN. Energies, species and charge states observed by each measurement channel are +discussed in detail in Kollmann et al. [2018, JGR]. + + * 1996-12-19T06:33:28 1996-12-9T07:24:15 + * 1997-11-06T20:09:34 1997-11-06T22:51:19 + * 1997-12-16T11:42:56 1997-12-16T12:28:25 + * 1998-03-29T13:05:38 1998-03-29T14:00:13 + * 1998-05-31T20:42:30 1998-05-31T21:43:10 + * 1998-09-26T03:30:04 1998-09-26T04:29:58 + * 1999-02-01T01:49:38 1999-02-01T02:39:08 + * 1999-11-25T16:00:12 1999-11-25T17:00:00 + * 2000-01-03T17:29:34 2000-01-03T18:30:14 + + + spase://SMWG/Person/Donald.J.Williams + PrincipalInvestigator + + + spase://CDPP/Person/Peter.Kollmann + DataProducer + + + spase://CDPP/Person/Quentin.Nenon + DataProducer + + + spase://CDPP/Person/Christopher.Paranicas + CoInvestigator + + + spase://CDPP/Person/Norbert.Krupp + CoInvestigator + + + gll-epd-record-el + PartOf + record mode : electron channels + + + + spase://SMWG/Repository/CDPP/AMDA + + http://amda.cdpp.eu + + NetCDF + + JHU/APL + spase://CDPP/Instrument/AMDA/Galileo/EPD + EnergeticParticles + + + 1996-11-04T13:14:51Z + 2001-05-25T11:44:00Z + + PT1S + PT2S + + Jupiter + Electron channels : + * B1 : ≥ 36.2 MeV + * DC0 : ≥ 14 MeV + * DC1 : ≥ 30 MeV + * DC2 : ≥ 1.8 MeV + * DC3 : ≥ 10.8 MeV + * E[0-3] : 15 - 93 keV + * F[0-3] : 93 - 884 keV + + + L-shell + gll_epd_l_euel + + + + TimeSeries + + + Other + + + + local pitch angle + gll_epd_paloc_euel + + degree + + TimeSeries + + + Other + + + + motor position + gll_epd_motor_euel + + + + TimeSeries + + + Other + + + + e- : E[0-3] : cnts + gll_epd_eu_ecnts + + s**-1 + + Spectrogram + + + 4 + + + Electron + CountRate + + + + e- : E[0-3] : flux + gll_epd_eu_eflux + + cm**-2.s**-1.sr**-1.keV**-1 + + Spectrogram + + + 4 + + + Electron + NumberFlux + + + + e- : F[0-3] : cnts + gll_epd_eu_fcnts + + s**-1 + + Spectrogram + + + 4 + + + Electron + CountRate + + + + e- : F[0-3] : flux + gll_epd_eu_fflux + + cm**-2.s**-1.sr**-1.keV**-1 + + Spectrogram + + + 4 + + + Electron + NumberFlux + + + + e- : B1 : cnts + gll_epd_euel_bcnts + + s**-1 + + TimeSeries + + + Electron + CountRate + + + + + e- : DC[0-3] : cnts + gll_epd_eu_dccnts + + s**-1 + + TimeSeries + + + 4 + + DC0 : > 14 MeV + 1 + gll_epd_eu_dccnts(0) + + + DC1 : > 30 MeV + 2 + gll_epd_eu_dccnts(1) + + + DC2 : > 1.8 MeV + 3 + gll_epd_eu_dccnts(2) + + + DC3 : > 10.8 MeV + 3 + gll_epd_eu_dccnts(3) + + + + Electron + CountRate + + + + + diff --git a/NumericalData/AMDA/Galileo/EPD/gll-epd-ganyele.xml b/NumericalData/AMDA/Galileo/EPD/gll-epd-ganyele.xml new file mode 100644 index 0000000..3b9d7fb --- /dev/null +++ b/NumericalData/AMDA/Galileo/EPD/gll-epd-ganyele.xml @@ -0,0 +1,271 @@ + + + 2.2.6 + + spase://CDPP/NumericalData/AMDA/Galileo/EPD/gll-epd-ganyele + + flybys ganymede + flybys ganymede : electrons + 2011-09-26T12:32:02Z + + Energetic electron count rates and fluxes measured by the EPD instrument + onboard Galileo in the Record acquisition mode. In this mode, the count rates are + accumulated during around 1.25 second. The full opening angle of the EPD telescopes + are relatively narrow, between 15° and 18°, and the acquisition period is very short compared + to the rotational spin period of Galileo. Counts and fluxes obtained with the Record + acquisition mode can therefore be considered as directional flux measurements. + The local and equatorial pitch angles that are given are for the particles observed by the + center of the telescope viewing cones. The motor that rotates the EPD telescopes around an + axis perpendicular to the spin axis of Galileo can have eight different step positions, + from 0 to 7. + +Data are extracted from the text file named 'galileo_epd_calibrated_low_res_v18.txt' +produced and provided by JHU/APL and publicly available at +http://sd-www.jhuapl.edu/Galileo_EPD/latest_calibrated_data/. +It is highly recommended to read the 'readme_v19.docx' document also available at the previous +link before using this dataset. It is also recommended to contact Peter Kollmann (JHU/APL), +as some measurement channels are highly contaminated or saturated. All unreliable measurements +are set to NaN. Energies, species and charge states observed by each measurement channel are +discussed in detail in Kollmann et al. [2018, JGR]. + + * 1996-09-06T18:32:45 1996-09-06T19:28:22 + * 1997-04-05T06:44:41 1997-04-05T07:40:18 + * 1997-05-07T15:36:54 1997-05-07T16:22:23 + * 1997-12-15T09:30:24 1997-12-15T10:30:00 + * 2000-05-20T09:40:04 2000-05-20T10:40:41 + * 2000-12-28T07:54:42 2000-12-28T08:55:20 + + + spase://SMWG/Person/Donald.J.Williams + PrincipalInvestigator + + + spase://CDPP/Person/Peter.Kollmann + DataProducer + + + spase://CDPP/Person/Quentin.Nenon + DataProducer + + + spase://CDPP/Person/Christopher.Paranicas + CoInvestigator + + + spase://CDPP/Person/Norbert.Krupp + CoInvestigator + + + gll-epd-record-el + PartOf + record mode : electron channels + + + + spase://SMWG/Repository/CDPP/AMDA + + http://amda.cdpp.eu + + NetCDF + + JHU/APL + spase://CDPP/Instrument/AMDA/Galileo/EPD + EnergeticParticles + + + 1996-11-04T13:14:51Z + 2001-05-25T11:44:00Z + + PT1S + PT2S + + Jupiter + Electron channels : + * B1 : ≥ 36.2 MeV + * DC0 : ≥ 14 MeV + * DC1 : ≥ 30 MeV + * DC2 : ≥ 1.8 MeV + * DC3 : ≥ 10.8 MeV + * E[0-3] : 15 - 93 keV + * F[0-3] : 93 - 884 keV + + + L-shell + gll_epd_l_gael + + + + TimeSeries + + + Other + + + + local pitch angle + gll_epd_paloc_gael + + degree + + TimeSeries + + + Other + + + + motor position + gll_epd_motor_gael + + + + TimeSeries + + + Other + + + + e- : E[0-3] : cnts + gll_epd_ga_ecnts + + s**-1 + + Spectrogram + + + 4 + + + Electron + CountRate + + + + e- : E[0-3] : flux + gll_epd_ga_eflux + + cm**-2.s**-1.sr**-1.keV**-1 + + Spectrogram + + + 4 + + + Electron + NumberFlux + + + + e- : F[0-3] : cnts + gll_epd_ga_fcnts + + s**-1 + + Spectrogram + + + 4 + + + Electron + CountRate + + + + e- : F[0-3] : flux + gll_epd_ga_fflux + + cm**-2.s**-1.sr**-1.keV**-1 + + Spectrogram + + + 4 + + + Electron + NumberFlux + + + + e- : B1 : cnts + gll_epd_gael_bcnts + + s**-1 + + TimeSeries + + + Electron + CountRate + + + + + e- : DC[0-3] : cnts + gll_epd_ga_dccnts + + s**-1 + + TimeSeries + + + 4 + + DC0 : > 14 MeV + 1 + gll_epd_ga_dccnts(0) + + + DC1 : > 30 MeV + 2 + gll_epd_ga_dccnts(1) + + + DC2 : > 1.8 MeV + 3 + gll_epd_ga_dccnts(2) + + + DC3 : > 10.8 MeV + 3 + gll_epd_ga_dccnts(3) + + + + Electron + CountRate + + + + + diff --git a/NumericalData/AMDA/Galileo/EPD/gll-epd-ioele.xml b/NumericalData/AMDA/Galileo/EPD/gll-epd-ioele.xml new file mode 100644 index 0000000..a76f9f9 --- /dev/null +++ b/NumericalData/AMDA/Galileo/EPD/gll-epd-ioele.xml @@ -0,0 +1,269 @@ + + + 2.2.6 + + spase://CDPP/NumericalData/AMDA/Galileo/EPD/gll-epd-ioele + + flybys io + flybys io : electrons + 2011-09-26T12:32:02Z + + Energetic electron count rates and fluxes measured by the EPD instrument + onboard Galileo in the Record acquisition mode. In this mode, the count rates are + accumulated during around 1.25 second. The full opening angle of the EPD telescopes + are relatively narrow, between 15° and 18°, and the acquisition period is very short compared + to the rotational spin period of Galileo. Counts and fluxes obtained with the Record + acquisition mode can therefore be considered as directional flux measurements. + The local and equatorial pitch angles that are given are for the particles observed by the + center of the telescope viewing cones. The motor that rotates the EPD telescopes around an + axis perpendicular to the spin axis of Galileo can have eight different step positions, + from 0 to 7. + +Data are extracted from the text file named 'galileo_epd_calibrated_low_res_v18.txt' +produced and provided by JHU/APL and publicly available at +http://sd-www.jhuapl.edu/Galileo_EPD/latest_calibrated_data/. +It is highly recommended to read the 'readme_v19.docx' document also available at the previous +link before using this dataset. It is also recommended to contact Peter Kollmann (JHU/APL), +as some measurement channels are highly contaminated or saturated. All unreliable measurements +are set to NaN. Energies, species and charge states observed by each measurement channel are +discussed in detail in Kollmann et al. [2018, JGR]. + +* 1995-12-07T15:21:02 1995-12-07T18:25:40 +* 1999-10-11T03:42:20 1999-10-11T06:41:52 +* 2000-02-22T13:04:50 2000-02-22T14:25:42 +* 2001-08-06T04:25:48 2001-08-06T05:29:08 + + + spase://SMWG/Person/Donald.J.Williams + PrincipalInvestigator + + + spase://CDPP/Person/Peter.Kollmann + DataProducer + + + spase://CDPP/Person/Quentin.Nenon + DataProducer + + + spase://CDPP/Person/Christopher.Paranicas + CoInvestigator + + + spase://CDPP/Person/Norbert.Krupp + CoInvestigator + + + gll-epd-record-el + PartOf + record mode : electron channels + + + + spase://SMWG/Repository/CDPP/AMDA + + http://amda.cdpp.eu + + NetCDF + + JHU/APL + spase://CDPP/Instrument/AMDA/Galileo/EPD + EnergeticParticles + + + 1996-11-04T13:14:51Z + 2001-05-25T11:44:00Z + + PT1S + PT2S + + Jupiter + Electron channels : + * B1 : ≥ 36.2 MeV + * DC0 : ≥ 14 MeV + * DC1 : ≥ 30 MeV + * DC2 : ≥ 1.8 MeV + * DC3 : ≥ 10.8 MeV + * E[0-3] : 15 - 93 keV + * F[0-3] : 93 - 884 keV + + + L-shell + gll_epd_l_ioel + + + + TimeSeries + + + Other + + + + local pitch angle + gll_epd_paloc_ioel + + degree + + TimeSeries + + + Other + + + + motor position + gll_epd_motor_ioel + + + + TimeSeries + + + Other + + + + e- : E[0-3] : cnts + gll_epd_io_ecnts + + s**-1 + + Spectrogram + + + 4 + + + Electron + CountRate + + + + + e- : F[0-3] : cnts + gll_epd_io_fcnts + + s**-1 + + Spectrogram + + + 4 + + + Electron + CountRate + + + + + e- : B1 : cnts + gll_epd_ioel_bcnts + + s**-1 + + TimeSeries + + + Electron + CountRate + + + + + e- : DC[0-3] : cnts + gll_epd_io_dccnts + + s**-1 + + TimeSeries + + + 4 + + DC0 : > 14 MeV + 1 + gll_epd_io_dccnts(0) + + + DC1 : > 30 MeV + 2 + gll_epd_io_dccnts(1) + + + DC2 : > 1.8 MeV + 3 + gll_epd_io_dccnts(2) + + + DC3 : > 10.8 MeV + 3 + gll_epd_io_dccnts(3) + + + + Electron + CountRate + + + + + diff --git a/NumericalData/AMDA/Galileo/EPD/gll-epd-rt.xml b/NumericalData/AMDA/Galileo/EPD/gll-epd-rt.xml index b0e21b3..dc3c254 100644 --- a/NumericalData/AMDA/Galileo/EPD/gll-epd-rt.xml +++ b/NumericalData/AMDA/Galileo/EPD/gll-epd-rt.xml @@ -39,6 +39,10 @@ spase://CDPP/Person/Peter.Kollmann DataProducer + + + spase://CDPP/Person/Quentin.Nenon + DataProducer spase://CDPP/Person/Christopher.Paranicas diff --git a/NumericalData/AMDA/Galileo/EPD/gll-epd-survele.xml b/NumericalData/AMDA/Galileo/EPD/gll-epd-survele.xml new file mode 100644 index 0000000..15c3f66 --- /dev/null +++ b/NumericalData/AMDA/Galileo/EPD/gll-epd-survele.xml @@ -0,0 +1,279 @@ + + + 2.2.6 + + spase://CDPP/NumericalData/AMDA/Galileo/EPD/gll-epd-survele + + survey + survey : electrons + 2011-09-26T12:32:02Z + + Energetic electron count rates and fluxes measured by the EPD instrument + onboard Galileo in the Record acquisition mode. In this mode, the count rates are + accumulated during around 1.25 second. The full opening angle of the EPD telescopes + are relatively narrow, between 15° and 18°, and the acquisition period is very short compared + to the rotational spin period of Galileo. Counts and fluxes obtained with the Record + acquisition mode can therefore be considered as directional flux measurements. + The local and equatorial pitch angles that are given are for the particles observed by the + center of the telescope viewing cones. The motor that rotates the EPD telescopes around an + axis perpendicular to the spin axis of Galileo can have eight different step positions, + from 0 to 7. + +Data are extracted from the text file named 'galileo_epd_calibrated_low_res_v18.txt' +produced and provided by JHU/APL and publicly available at +http://sd-www.jhuapl.edu/Galileo_EPD/latest_calibrated_data/. +It is highly recommended to read the 'readme_v19.docx' document also available at the previous +link before using this dataset. It is also recommended to contact Peter Kollmann (JHU/APL), +as some measurement channels are highly contaminated or saturated. All unreliable measurements +are set to NaN. Energies, species and charge states observed by each measurement channel are +discussed in detail in Kollmann et al. [2018, JGR]. + + * 1996-09-11T02:38:24 1996-09-11T03:18:50 + * 1997-03-30T18:49:45 1997-03-30T19:35:13 + * 1997-05-06T13:00:21 1997-05-06T15:09:46 + * 1997-06-28T13:50:33 1997-06-28T14:51:12 + * 1997-07-23T13:11:41 1997-07-23T13:57:11 + * 1997-08-07T11:06:40 1997-08-07T12:47:46 + * 1997-08-23T14:07:49 1997-08-23T16:09:09 + * 1997-09-18T22:34:48 1997-09-18T23:21:18 + * 1999-05-03T15:59:53 1999-05-03T18:01:12 + * 1999-07-01T23:52:38 1999-07-02T01:47:27 + * 1999-08-12T08:17:59 1999-08-12T13:06:56 + * 1999-09-14T14:36:17 1999-09-14T21:28:48 + * 2001-10-15T15:30:20 2001-10-15T23:23:40 + * 2002-11-04T21:48:26 2002-11-04T22:34:00 + + + spase://SMWG/Person/Donald.J.Williams + PrincipalInvestigator + + + spase://CDPP/Person/Peter.Kollmann + DataProducer + + + spase://CDPP/Person/Quentin.Nenon + DataProducer + + + spase://CDPP/Person/Christopher.Paranicas + CoInvestigator + + + spase://CDPP/Person/Norbert.Krupp + CoInvestigator + + + gll-epd-record-el + PartOf + record mode : electron channels + + + + spase://SMWG/Repository/CDPP/AMDA + + http://amda.cdpp.eu + + NetCDF + + JHU/APL + spase://CDPP/Instrument/AMDA/Galileo/EPD + EnergeticParticles + + + 1996-11-04T13:14:51Z + 2001-05-25T11:44:00Z + + PT1S + PT2S + + Jupiter + Electron channels : + * B1 : ≥ 36.2 MeV + * DC0 : ≥ 14 MeV + * DC1 : ≥ 30 MeV + * DC2 : ≥ 1.8 MeV + * DC3 : ≥ 10.8 MeV + * E[0-3] : 15 - 93 keV + * F[0-3] : 93 - 884 keV + + + L-shell + gll_epd_l_hrel + + + + TimeSeries + + + Other + + + + local pitch angle + gll_epd_paloc_hrel + + degree + + TimeSeries + + + Other + + + + motor position + gll_epd_motor_hrel + + + + TimeSeries + + + Other + + + + e- : E[0-3] : cnts + gll_epd_hr_ecnts + + s**-1 + + Spectrogram + + + 4 + + + Electron + CountRate + + + + e- : E[0-3] : flux + gll_epd_hr_eflux + + cm**-2.s**-1.sr**-1.keV**-1 + + Spectrogram + + + 4 + + + Electron + NumberFlux + + + + e- : F[0-3] : cnts + gll_epd_hr_fcnts + + s**-1 + + Spectrogram + + + 4 + + + Electron + CountRate + + + + + e- : B1 : cnts + gll_epd_hrel_bcnts + + s**-1 + + TimeSeries + + + Electron + CountRate + + + + + e- : DC[0-3] : cnts + gll_epd_hr_dccnts + + s**-1 + + TimeSeries + + + 4 + + DC0 : > 14 MeV + 1 + gll_epd_hr_dccnts(0) + + + DC1 : > 30 MeV + 2 + gll_epd_hr_dccnts(1) + + + DC2 : > 1.8 MeV + 3 + gll_epd_hr_dccnts(2) + + + DC3 : > 10.8 MeV + 3 + gll_epd_hr_dccnts(3) + + + + Electron + CountRate + + + + + diff --git a/NumericalData/AMDA/ULYSSES/Ephemeris/ulys-orb-all.xml b/NumericalData/AMDA/ULYSSES/Ephemeris/ulys-orb-all.xml index b4c173e..b5e2a88 100644 --- a/NumericalData/AMDA/ULYSSES/Ephemeris/ulys-orb-all.xml +++ b/NumericalData/AMDA/ULYSSES/Ephemeris/ulys-orb-all.xml @@ -5,7 +5,7 @@ spase://CDPP/NumericalData/AMDA/Ulysses/Ephemeris/ulys-orb-all orbit sun - 2015-10-13T14:31:00Z + 2010-10-22T16:46:44Z Ulysses spacecraft positions data product spase://SMWG/Person/Elena.Budnik @@ -64,7 +64,7 @@ distance ulys-sun - ulys_carr(0) + ulys_carr_r pos.heliocentric AU @@ -73,7 +73,7 @@ lon iau_sun - ulys_carr(1) + ulys_carr_lon pos.heliocentric deg @@ -82,7 +82,7 @@ lat iau_sun - ulys_carr(2) + ulys_carr_lat pos.heliocentric deg diff --git a/NumericalData/AMDA/ULYSSES/Ephemeris/ulys-orb-jup.xml b/NumericalData/AMDA/ULYSSES/Ephemeris/ulys-orb-jup.xml index 89a9c3c..c760fa2 100644 --- a/NumericalData/AMDA/ULYSSES/Ephemeris/ulys-orb-jup.xml +++ b/NumericalData/AMDA/ULYSSES/Ephemeris/ulys-orb-jup.xml @@ -5,7 +5,7 @@ spase://CDPP/NumericalData/AMDA/Ulysses/Ephemeris/ulys-orb-jup flyby jupiter - 2015-10-13T15:08:29Z + 2011-09-06T10:05:35Z Ulysses spacecraft positions data product spase://SMWG/Person/Elena.Budnik diff --git a/Person/Quentin.Nenon.xml b/Person/Quentin.Nenon.xml new file mode 100644 index 0000000..cf56c06 --- /dev/null +++ b/Person/Quentin.Nenon.xml @@ -0,0 +1,12 @@ + + + 2.2.2 + + spase://CDPP/Person/Quentin.Nenon + 2019-04-01T12:34:56.789 + Dr. Quentin Nenon + Space Science Laboratory, University of California at Berkeley +
7 Gauss Way, Berkeley CA 94720, USA
+ q.nenon@gmail.com + + -- libgit2 0.21.2