From 03a67bdb8bb2ddd27900addc022cddd2fcfe634c Mon Sep 17 00:00:00 2001 From: Elena.Budnik Date: Thu, 22 Aug 2019 16:26:46 +0200 Subject: [PATCH] FIPS MESS ESPEC --- NumericalData/AMDA/MESSENGER/FIPS/mess-fips-espec.xml | 75 +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ NumericalData/AMDA/MESSENGER/FIPS/mess-fips-nobs.xml | 5 +++-- NumericalData/AMDA/MESSENGER/FIPS/mess-fips-ntp.xml | 33 ++++++++++++++++++++++++++++----- 3 files changed, 106 insertions(+), 7 deletions(-) create mode 100644 NumericalData/AMDA/MESSENGER/FIPS/mess-fips-espec.xml diff --git a/NumericalData/AMDA/MESSENGER/FIPS/mess-fips-espec.xml b/NumericalData/AMDA/MESSENGER/FIPS/mess-fips-espec.xml new file mode 100644 index 0000000..bd273b9 --- /dev/null +++ b/NumericalData/AMDA/MESSENGER/FIPS/mess-fips-espec.xml @@ -0,0 +1,75 @@ + + + 2.2.6 + + spase://CDPP/NumericalData/AMDA/MESSENGER/FIPS/mess-fips-espec + + espec + energy spectra + 2017-01-16T14:08:29Z + FIPS Energy Spectra (FIPS_ESPEC) contains differential energy flux at + each of the 64 E/q values (0.046 - 13.3 keV/e) for selected major + ion species during selected time periods. + + spase://CDPP/Person/George.Ho + DataProducer + + + + spase://CDPP/Repository/AMDA + Online + Open + + http://amda.cdpp.eu + + NetCDF + + PDS + Calibrated + MESS-E_V_H_SW-EPPS-3-FIPS-DDR-V2.0/FIPS_NOBS + spase://CDPP/Instrument/AMDA/MESSENGER/FIPS + IonComposition + + + 2008-08-20T16:03:35Z + 2015-04-30T15:08:18Z + + PT60S + + Mercury + Quality flag : + * 0 = Good + * 1 = Bad + + + eflux h+ + mes_fips_spec_h + + (keV/e)^-1 sec^-1 cm^-2 sr^-1 + + + eflux he2+ + mes_fips_spec_he2 + + (keV/e)^-1 sec^-1 cm^-2 sr^-1 + + + eflux he + mes_fips_spec_he + + (keV/e)^-1 sec^-1 cm^-2 sr^-1 + + + eflux na+ + mes_fips_spec_na + + (keV/e)^-1 sec^-1 cm^-2 sr^-1 + + + eflux o+ + mes_fips_spec_o + + (keV/e)^-1 sec^-1 cm^-2 sr^-1 + + + diff --git a/NumericalData/AMDA/MESSENGER/FIPS/mess-fips-nobs.xml b/NumericalData/AMDA/MESSENGER/FIPS/mess-fips-nobs.xml index 4e1c5c5..57863fd 100644 --- a/NumericalData/AMDA/MESSENGER/FIPS/mess-fips-nobs.xml +++ b/NumericalData/AMDA/MESSENGER/FIPS/mess-fips-nobs.xml @@ -4,9 +4,10 @@ spase://CDPP/NumericalData/AMDA/MESSENGER/FIPS/mess-fips-nobs - ion observed densities + nobs + ion observed densities 2017-01-16T14:08:29Z - This data set contains FIPS observed densities for selected ion species. + This data set contains FIPS observed densities ( FIPS_NOBS ) for selected ion species. spase://CDPP/Person/George.Ho DataProducer diff --git a/NumericalData/AMDA/MESSENGER/FIPS/mess-fips-ntp.xml b/NumericalData/AMDA/MESSENGER/FIPS/mess-fips-ntp.xml index 7a7aa8d..9e9c772 100644 --- a/NumericalData/AMDA/MESSENGER/FIPS/mess-fips-ntp.xml +++ b/NumericalData/AMDA/MESSENGER/FIPS/mess-fips-ntp.xml @@ -4,12 +4,21 @@ spase://CDPP/NumericalData/AMDA/MESSENGER/FIPS/mess-fips-ntp - ion moments + ntp + ion moments 2017-01-16T14:08:29Z - This data set contains FIPS ion number densities and temperatures, + This data set contains FIPS ( FIPS_NTP) ion number densities and temperatures, as well as the pressure calculated from their product. Quantities are calculated after sufficient time accumulation -to allow meaningful interpretation +to allow meaningful interpretation. + +In this version of the dataset, many of these products are provided + in regions determined by hand-picked or modeled bow shock and + magnetopause boundaries. Boundary picking was done by the MAG team at + a level of accuracy sufficient for the relatively low time resolution + FIPS data (10s - 60s). Where these were not available, the model given + by Slavin et al. [Science, 2010] is used. + spase://CDPP/Person/George.Ho DataProducer @@ -34,10 +43,24 @@ to allow meaningful interpretation 2008-08-20T16:03:35Z 2015-04-30T15:08:18Z - PT60S + PT7S + PT67S Mercury - Quality flag : + + The recovered density, temperature and pressure (NTP) product is + particularly sensitive to the region of Mercury's space environment in + which the data was taken. The reasons for this, based on validity of + required assumptions, are described in detail in the DDR SIS. This + data is provided within the magnetosphere, where the assumptions are + likely to hold for averages of 1 minute or more. It is also + provided in the magnetosheath within a 45 degree cone angle of the X_MSO + axis. The validity of the assumptions is much more variable here, + though they will often hold. USERS ARE STRONGLY CAUTIONED to read the + NTP section of the DDR SIS follow the recommendations for using these + quantities. + + Quality flag : * 0 = Good * non-0 = Bad (Non-zero flag values TBD) -- libgit2 0.21.2