diff --git a/NumericalData/AMDA/ACE/MFI/ace-imf-all.xml b/NumericalData/AMDA/ACE/MFI/ace-imf-all.xml index ad8b9ca..c382ffe 100644 --- a/NumericalData/AMDA/ACE/MFI/ace-imf-all.xml +++ b/NumericalData/AMDA/ACE/MFI/ace-imf-all.xml @@ -58,7 +58,7 @@ 1997-09-02T00:00:12Z - 2016-07-23T23:59:48Z + 2016-08-13T23:59:44Z PT16S diff --git a/NumericalData/AMDA/ACE/MFI/ace-mag-real.xml b/NumericalData/AMDA/ACE/MFI/ace-mag-real.xml index fc11a69..6e7971a 100644 --- a/NumericalData/AMDA/ACE/MFI/ace-mag-real.xml +++ b/NumericalData/AMDA/ACE/MFI/ace-mag-real.xml @@ -51,7 +51,7 @@ 2014-01-06T00:00:00Z - 2016-08-06T23:59:59Z + 2016-08-22T23:59:59Z PT60S diff --git a/NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml b/NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml index fd7c12d..d3dc6f9 100644 --- a/NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml +++ b/NumericalData/AMDA/ACE/SWEPAM/ace-swepam-real.xml @@ -44,7 +44,7 @@ 2014-01-06T00:00:00Z - 2016-08-06T23:59:59Z + 2016-08-22T23:59:59Z PT60S diff --git a/NumericalData/AMDA/ACE/SWEPAM/ace-swp-all.xml b/NumericalData/AMDA/ACE/SWEPAM/ace-swp-all.xml index 64877a3..6e5f63e 100644 --- a/NumericalData/AMDA/ACE/SWEPAM/ace-swp-all.xml +++ b/NumericalData/AMDA/ACE/SWEPAM/ace-swp-all.xml @@ -59,7 +59,7 @@ 2001-01-01T00:00:00Z - 2016-07-23T23:55:00Z + 2016-08-13T23:55:00Z PT5M diff --git a/NumericalData/AMDA/ACE/ephemeris/ace-orb-all.xml b/NumericalData/AMDA/ACE/ephemeris/ace-orb-all.xml index 7d57a00..1fd61de 100644 --- a/NumericalData/AMDA/ACE/ephemeris/ace-orb-all.xml +++ b/NumericalData/AMDA/ACE/ephemeris/ace-orb-all.xml @@ -33,7 +33,7 @@ 1997-08-26T00:00:00Z - 2016-10-09T23:47:00Z + 2016-10-24T23:47:00Z PT12M diff --git a/NumericalData/AMDA/MAVEN/Ephemeris/maven-orb-marsobs.xml b/NumericalData/AMDA/MAVEN/Ephemeris/maven-orb-marsobs.xml index 37f1018..74a8b96 100644 --- a/NumericalData/AMDA/MAVEN/Ephemeris/maven-orb-marsobs.xml +++ b/NumericalData/AMDA/MAVEN/Ephemeris/maven-orb-marsobs.xml @@ -42,7 +42,7 @@ 2014-06-01T00:00:00Z - 2016-05-17T19:47:00Z + 2016-08-16T19:37:00Z PT1M diff --git a/NumericalData/AMDA/MAVEN/MAG/mav-mag-pds.xml b/NumericalData/AMDA/MAVEN/MAG/mav-mag-pds.xml index 07bf8b0..2e9775a 100644 --- a/NumericalData/AMDA/MAVEN/MAG/mav-mag-pds.xml +++ b/NumericalData/AMDA/MAVEN/MAG/mav-mag-pds.xml @@ -44,7 +44,7 @@ 2014-10-10T00:00:00Z - 2016-02-15T00:00:02Z + 2016-05-09T00:00:01Z PT0.031S diff --git a/NumericalData/AMDA/MEX/ELS/mex-els-all.xml b/NumericalData/AMDA/MEX/ELS/mex-els-all.xml index 0c58fee..45b6099 100644 --- a/NumericalData/AMDA/MEX/ELS/mex-els-all.xml +++ b/NumericalData/AMDA/MEX/ELS/mex-els-all.xml @@ -41,7 +41,7 @@ Institute of Space Physics, PI, and the European Space Agency 2003-06-23T18:42:48Z - 2016-06-06T05:29:07Z + 2016-08-13T21:35:21Z PT4S diff --git a/NumericalData/AMDA/MEX/ephemeris/mex-orb-all.xml b/NumericalData/AMDA/MEX/ephemeris/mex-orb-all.xml index 105ff1b..ed579cb 100644 --- a/NumericalData/AMDA/MEX/ephemeris/mex-orb-all.xml +++ b/NumericalData/AMDA/MEX/ephemeris/mex-orb-all.xml @@ -27,7 +27,7 @@ 2004-01-10T07:54:21Z - 2016-07-31T13:17:49Z + 2016-10-09T05:10:11Z PT60S diff --git a/NumericalData/AMDA/OMNI/omni-5min-all.xml b/NumericalData/AMDA/OMNI/omni-5min-all.xml index 48ab9e2..b7fd4f2 100644 --- a/NumericalData/AMDA/OMNI/omni-5min-all.xml +++ b/NumericalData/AMDA/OMNI/omni-5min-all.xml @@ -47,7 +47,7 @@ for creating the OMNI data set. 1981-01-01T00:00:00Z - 2016-07-13T23:55:00Z + 2016-07-31T23:55:00Z PT5M diff --git a/NumericalData/AMDA/OMNI/omni-hour-all.xml b/NumericalData/AMDA/OMNI/omni-hour-all.xml index 438455e..f4086d6 100644 --- a/NumericalData/AMDA/OMNI/omni-hour-all.xml +++ b/NumericalData/AMDA/OMNI/omni-hour-all.xml @@ -47,7 +47,7 @@ for creating the OMNI data set. 1970-01-01T00:00:00Z - 2016-07-15T14:00:00Z + 2016-08-04T14:00:00Z PT1H diff --git a/NumericalOutput/AMDA/CAIN/b_cain.xml b/NumericalOutput/AMDA/CAIN/b_cain.xml index 0cc0895..cb0f0af 100644 --- a/NumericalOutput/AMDA/CAIN/b_cain.xml +++ b/NumericalOutput/AMDA/CAIN/b_cain.xml @@ -4,19 +4,19 @@ spase://CDPP/NumericalOutput/AMDA/CAIN/b_cain - Cain B - 2014-07-08T16:49:29Z - TBD + Cain B along s/c orbit + 2016-08-23T00:00:00Z + Cain model martian crustal magnetic field along s/c orbit is being real-time calculated. + S/c and sampling time should be defined by user. + TBD - - TBD - PrincipalInvestigator + + spase://SMWG/Person/Elena.Budnik + TechnicalContact Rules of use, and caveats - - TBD - + TBD TBD @@ -31,9 +31,7 @@ Text.ASCII - - TBD - + TBD spase://CDPP/SimulationRun/AMDA/CAIN/CainRun MagneticField @@ -42,7 +40,7 @@ 1970-01-01T00:00:00Z 1970-01-01T00:00:00Z - + UserDefined Mars @@ -61,7 +59,7 @@ 3 bx - + Component.I bcain_mso(0) @@ -70,7 +68,7 @@ by - + Component.J bcain_mso(1) @@ -79,7 +77,7 @@ bz - + Component.K bcain_mso(2) @@ -88,6 +86,9 @@ NaN + + Magnetic + b tot @@ -98,6 +99,9 @@ nT NaN + + Magnetic + - + diff --git a/NumericalOutput/AMDA/TAO/Jupiter/tao-jupiter-omni.xml b/NumericalOutput/AMDA/TAO/Jupiter/tao-jupiter-omni.xml index 5db980b..9e5bcdb 100644 --- a/NumericalOutput/AMDA/TAO/Jupiter/tao-jupiter-omni.xml +++ b/NumericalOutput/AMDA/TAO/Jupiter/tao-jupiter-omni.xml @@ -4,8 +4,8 @@ spase://CDPP/NumericalOutput/AMDA/TAO/Jupiter/tao-jupiter-omni - Tao SW Jupiter - 2014-07-08T16:49:29Z + Tao SW Jupiter / OMNI input + 2016-08-22T00:00:00Z TBD TBD @@ -44,11 +44,11 @@ PT1H - Saturn + Jupiter TBD - spase://CDPP/NumericalData/AMDA/OMNI/omni-5min-all + spase://CDPP/NumericalData/AMDA/OMNI/omni-hour-all Proton Number Density jupiter_omni_n diff --git a/NumericalOutput/AMDA/TSYG96/b_t96.xml b/NumericalOutput/AMDA/TSYG96/b_t96.xml new file mode 100644 index 0000000..6e92341 --- /dev/null +++ b/NumericalOutput/AMDA/TSYG96/b_t96.xml @@ -0,0 +1,106 @@ + + + 2.2.6 + + spase://CDPP/NumericalOutput/AMDA/TSYG96/b_t96 + + T96 Bgsm along s/c orbit + 2016-08-23T00:00:00Z + . + + TBD + + spase://SMWG/Person/Elena.Budnik + TechnicalContact + + + Rules of use, and caveats + TBD + TBD + + + + spase://SMWG/Repository/CDPP/AMDA + Online + Open + + AMDA at CDPP + + http://amda.cdpp.eu + + + Text.ASCII + TBD + + spase://CDPP/SimulationRun/AMDA/TSYG96/Tsyg96Run + MagneticField + + + 1970-01-01T00:00:00Z + 1970-01-01T00:00:00Z + + UserDefined + + Mars + + TBD + + + + b gsm + b_t96gsm + + + TBD + + nT + + 3 + + bx + Component.I + + b_t96gsm(0) + + + + + + by + Component.J + + b_t96gsm(1) + + + + + + bz + Component.K + + b_t96gsm(2) + + + + + + NaN + + Magnetic + + + + b tot + b_t96tot + TBD + + TBD + + nT + NaN + + Magnetic + + + + diff --git a/SimulationModel/AMDA/Cain.xml b/SimulationModel/AMDA/Cain.xml index cbd4ef8..b2be4d6 100644 --- a/SimulationModel/AMDA/Cain.xml +++ b/SimulationModel/AMDA/Cain.xml @@ -5,7 +5,7 @@ spase://CDPP/SimulationModel/AMDA/Cain Cain Model - Cain Mars Crustal magnetic Field Model + Cain martian crustal magnetic field model 2014-07-08T14:48:29Z Spherical Harmonic @@ -15,7 +15,7 @@ Model_Magnetic_Field PartOf - Mars Crustal Magnetic Field Models + Magnetic Field Models Spherical Harmonic diff --git a/SimulationModel/AMDA/Michigan.xml b/SimulationModel/AMDA/Michigan.xml index 1ad5f8a..a18ba9d 100644 --- a/SimulationModel/AMDA/Michigan.xml +++ b/SimulationModel/AMDA/Michigan.xml @@ -14,7 +14,7 @@ SW_Propagation PartOf - Model SW Propagation + Solar Wind Propagation MHD diff --git a/SimulationModel/AMDA/Morschhauser.xml b/SimulationModel/AMDA/Morschhauser.xml index c89c972..e5e52ca 100644 --- a/SimulationModel/AMDA/Morschhauser.xml +++ b/SimulationModel/AMDA/Morschhauser.xml @@ -9,13 +9,13 @@ 2014-07-08T14:48:29Z Spherical Harmonic - TBD + Morschhauser PrincipalInvestigator Model_Magnetic_Field PartOf - Mars Crustal Magnetic Field Models + Magnetic Field Models Spherical Harmonic diff --git a/SimulationModel/AMDA/Tao.xml b/SimulationModel/AMDA/Tao.xml index 2717478..4a8d7bb 100644 --- a/SimulationModel/AMDA/Tao.xml +++ b/SimulationModel/AMDA/Tao.xml @@ -14,7 +14,7 @@ SW_Propagation PartOf - Model SW Propagation + Solar Wind Propagation MHD diff --git a/SimulationModel/AMDA/Tsyganenko96.xml b/SimulationModel/AMDA/Tsyganenko96.xml new file mode 100644 index 0000000..a5f77a1 --- /dev/null +++ b/SimulationModel/AMDA/Tsyganenko96.xml @@ -0,0 +1,23 @@ + + + 2.2.6 + + spase://CDPP/SimulationModel/AMDA/Tsyganenko96 + + T96 Model + T96 geomagnetic field model + 2014-07-08T14:48:29Z + + + TBD + PrincipalInvestigator + + + Model_Magnetic_Field + PartOf + Magnetic Field Models + + + + + diff --git a/SimulationRun/AMDA/CAIN/CainRun.xml b/SimulationRun/AMDA/CAIN/CainRun.xml index 33493fe..57395ab 100644 --- a/SimulationRun/AMDA/CAIN/CainRun.xml +++ b/SimulationRun/AMDA/CAIN/CainRun.xml @@ -5,12 +5,38 @@ spase://CDPP/SimulationRun/AMDA/CAIN/CainRun Cain Model - Mars Model Crustal magnetic Field alog s/c orbit - 2014-07-08T14:48:29Z - + Cain model of martian crustal magnetic field + 2016-08-22T00:00:00Z + [1] A potential function using spherical harmonics up to degree and order 90 was derived +from a selection of Mars Global Surveyor vector data. These included all three +components of those taken below 200 km altitude during the two aerobraking phases +(AB1 and AB2), the Science Phase Orbits (SPO), and the higher-altitude (367–435 km) +data taken on the nightside during the Mapping Phase Orbits (MPO). The merger of these +sets of data provided total global coverage. The technique used was a least squares +minimization developed for Earth field analysis whereby the relative weighting of each +data source was determined by the width of a Gaussian fit to the residual distribution about +the potential function. Also, data selection by area and area weight functions were used to +improve normalization. The residual misfit distributions for the vertical component for +different data sources are (nT) AB1, 6.5; AB2 (in shadow), 6.7; AB2 (sunlit), 10.3; SPO, +6.4; and MPO, 5.9. The horizontal component misfits are about the same for MPO and +AB2 in shadow, but for data taken in sunlight the scatter of horizontal component residuals +increases by 50% for AB1, a factor of two for SPO, and 30% for AB2. The energy density +spectrum evaluated at 3535 km radius (the mean altitude of the AB and SPO data) +decreased from a high of 0.2 J/km3 near n = 20 to an order of magnitude less at n = 90. +Most of the power in the spectrum lies between n = 15 and n = 40. The dipole moment +was only 8 Â 1016 A Á m2, which is likely close to the noise of the coefficients. This +spectrum is 40 times greater than that of Earth at the scale sizes represented by values of n +from 20 to 40. Comparisons with other published maps and models for Mars show general +agreement with the field representations at MPO altitudes, but disagreements up to several +INhundred nT in components calculated for areodetic altitudes below 200 km. + - + spase://CDPP/Person/Joseph.C.Cain PrincipalInvestigator + + + spase://SMWG/Person/Elena.Budnik + TechnicalContact @@ -23,10 +49,13 @@ MSO 3 - - + km + - Orbit + Orbit + + Ephemeris + diff --git a/SimulationRun/AMDA/TSYG96/Tsyg96Run.xml b/SimulationRun/AMDA/TSYG96/Tsyg96Run.xml new file mode 100644 index 0000000..ee2d867 --- /dev/null +++ b/SimulationRun/AMDA/TSYG96/Tsyg96Run.xml @@ -0,0 +1,40 @@ + + + 2.2.6 + + spase://CDPP/SimulationRun/AMDA/TSYG96/Tsyg96Run + + T96 Model + + 2016-08-22T00:00:00Z + + + + spase://CDPP/Person/Nikolai.Tsyganenko + PrincipalInvestigator + + + spase://SMWG/Person/Elena.Budnik + TechnicalContact + + + + spase://CDPP/SimulationModel/AMDA/Tsyganenko96 + + Earth + + + Cartesian + GSM + + 3 + km + + + Orbit + + Ephemeris + + + + -- libgit2 0.21.2