diff --git a/Instrument/CDPP-AMDA/MESSENGER/Models.xml b/Instrument/CDPP-AMDA/MESSENGER/Models.xml index 9dba692..d8f1584 100644 --- a/Instrument/CDPP-AMDA/MESSENGER/Models.xml +++ b/Instrument/CDPP-AMDA/MESSENGER/Models.xml @@ -6,11 +6,11 @@ Analytical Models KT17: Mercury magnetic field model 2017-02-04T15:37:46Z - ToDo + Dynamic model of Mercury's magnetospheric magnetic field parameterized by heliocentric distance and magnetic activity - - + spase://CNES/Person/CDPP-AMDA/Haje.Korth + PrincipalInvestigator + Platform diff --git a/Instrument/CDPP-AMDA/Mariner10/Models.xml b/Instrument/CDPP-AMDA/Mariner10/Models.xml new file mode 100644 index 0000000..69892e8 --- /dev/null +++ b/Instrument/CDPP-AMDA/Mariner10/Models.xml @@ -0,0 +1,19 @@ + + 2.4.1 + + spase://CNES/Instrument/CDPP-AMDA/Mariner10/Models + + Analytical Models + KT17: Mercury magnetic field model + 2017-02-04T15:37:46Z + Dynamic model of Mercury's magnetospheric magnetic field parameterized by heliocentric distance and magnetic activity + + spase://CNES/Person/CDPP-AMDA/Haje.Korth + PrincipalInvestigator + + + Platform + + spase://CNES/Observatory/CDPP-AMDA/Mariner10 + + \ No newline at end of file diff --git a/NumericalData/CDPP-AMDA/MESSENGER/Models/mes-kt17-model.xml b/NumericalData/CDPP-AMDA/MESSENGER/Models/mes-kt17-model.xml index a2fb3af..f56da0c 100644 --- a/NumericalData/CDPP-AMDA/MESSENGER/Models/mes-kt17-model.xml +++ b/NumericalData/CDPP-AMDA/MESSENGER/Models/mes-kt17-model.xml @@ -4,23 +4,39 @@ spase://CNES/NumericalData/CDPP-AMDA/MESSENGER/Models/mes-kt17-model - KT17 @PDS - KT17 @PDS + KT17 model + KT17 mercury magnetic field model 2023-02-20T01:01:36Z - Magnetic field along Mercury orbit is being real-time calculated. - - - - TBD + Magnetic field along Mercury orbit is being real-time calculated. + S/C, sampling time, distance of Mercury from the Sun (AU) and Anderson et al., 2013 disturbance index should be defined by user. + + KT17 magnetic field model (Korth et al., 2017) model is used in calculations. + + James, M. K. - KT17 (v1.0.0) - https://github.com/mattkjames7/KT17/releases/tag/v1.0.0 - spase://CNES/Person/CDPP-AMDA/Connerney + spase://CNES/Person/CDPP-AMDA/Haje.Korth PrincipalInvestigator - - + + + Korth, H., Johnson, C. L., Philpott, L., Tsyganenko, N. A., Anderson, B. J. (2017). A dynamic model of Mercury's magnetospheric magnetic field. Geophysical Research Letters, 44, 10,147– 10,154. + https://doi.org/10.1002/2017GL074699 + Model description + + + James, M. K. - KT17 (v1.0.0) + https://github.com/mattkjames7/KT17/releases/tag/v1.0.0 + Software + + + Anderson, B. J., Johnson, C. L., and Korth, H. (2013), A magnetic disturbance index for Mercury's magnetic field derived from MESSENGER Magnetometer data, Geochem. Geophys. Geosyst., 14, 3875– 3886 + https://doi.org/10.1002/ggge.20242 + Disturbance index description + + mes-orb-orb spase://SMWG/Repository/CDPP/AMDA @@ -63,73 +79,36 @@ Mercury - b_mso internal - b_kt17_internal - - - nT - - - 3 - - bx - Component.I - 1 - b_kt17_internal(0) - - - by - Component.J - 2 - b_kt17_internal(1) - - - bz - Component.K - 3 - b_kt17_internal(2) - - - - Magnetic - - - - |b| - b_kt17_internal_tot + b msm + b_kt17_model_60_0.427_50_mes_xyz_orbmso - nT - - Magnetic - - - - b_mso external - b_kt17_external - - - nT - 3 bx Component.I 1 - b_kt17_external(0) + b_kt17_model_60_0.427_50_mes_xyz_orbmso(0) + + by Component.J 2 - b_kt17_external(1) + b_kt17_model_60_0.427_50_mes_xyz_orbmso(1) + + bz Component.K 3 - b_kt17_external(2) + b_kt17_model_60_0.427_50_mes_xyz_orbmso(2) + + + @@ -138,73 +117,16 @@ |b| - b_kt17_external_tot - - - nT - - Magnetic - - - - b_mso all - b_kt17_all - - - nT - - - 3 - - bx - Component.I - 1 - b_kt17_all(0) - - - by - Component.J - 2 - b_kt17_all(1) - - - bz - Component.K - 3 - b_kt17_all(2) - - - - Magnetic - - - - |b| - b_kt17_all_tot - - - nT - - Magnetic - - - - distance mercury-sun - b_kt17_rhel - - - nT - - Magnetic - - - - disturbance index - b_kt17_actIdx - - + b_kt17_model_tot_60_0.427_50_mes_xyz_orbmso + Scalar magnitude of the magnetic field in nT + phys.magField nT + 1e-9>T + + TimeSeries + + Magnitude Magnetic diff --git a/NumericalData/CDPP-AMDA/MESSENGER/Models/mes-kt17-pds.xml b/NumericalData/CDPP-AMDA/MESSENGER/Models/mes-kt17-pds.xml new file mode 100644 index 0000000..8f77991 --- /dev/null +++ b/NumericalData/CDPP-AMDA/MESSENGER/Models/mes-kt17-pds.xml @@ -0,0 +1,212 @@ + + + 2.4.1 + + spase://CNES/NumericalData/CDPP-AMDA/MESSENGER/Models/mes-kt17-pds + + KT17@PDS + MESSENGER Magnetometer KT17 Model Residual data + 2023-02-20T01:01:36Z + MESSENGER Magnetometer KT17 Model Residual data and associated products obtained from NASA/PDS plasma node. + + The research for and preparation of this bundle was funded by NASA?s Planetary Data Archiving, Restoration, and Tools (PDART) program under grant NNX16AJ01G issued to Dr. Haje Korth (Principal Investigator) at the Johns Hopkins Applied Physics Laboratory. + + + spase://CNES/Person/CDPP-AMDA/Haje.Korth + PrincipalInvestigator + + + Korth, H., Johnson, C. L., Philpott, L., Tsyganenko, N. A., Anderson, B. J. (2017). A dynamic model of Mercury's magnetospheric magnetic field. Geophysical Research Letters, 44, 10,147– 10,154. + https://doi.org/10.1002/2017GL074699 + Model description + + + + spase://SMWG/Repository/CDPP/AMDA + Online + Open + + CDPP/AMDA HAPI Server + http://amda.irap.omp.eu/service/hapi + + Web Service to this product using the HAPI interface. + + CSV + Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse".. See the Rules of the road at http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers. + + + spase://SMWG/Repository/CDPP/AMDA + Online + Open + + CDPP/AMDA Web application + http://amda.cdpp.eu + Access to Data via CDPP/AMDA Web application. + + CSV + VOTable + CDF + PNG + Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse".. See the Rules of the road at http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers. + + PDS + mess-mag-kt17-model-residuals + spase://CNES/Instrument/CDPP-AMDA/MESSENGER/Models + MagneticField + + + 2016-06-01T00:00:00Z + 2021-05-05T23:49:59Z + + PT1M + + Mercury + + + b_mso internal + b_kt17_internal + + + nT + + + 3 + + bx + Component.I + 1 + b_kt17_internal(0) + + + by + Component.J + 2 + b_kt17_internal(1) + + + bz + Component.K + 3 + b_kt17_internal(2) + + + + Magnetic + + + + |b| internal + b_kt17_internal_tot + + + nT + + Magnetic + + + + b_mso external + b_kt17_external + + + nT + + + 3 + + bx + Component.I + 1 + b_kt17_external(0) + + + by + Component.J + 2 + b_kt17_external(1) + + + bz + Component.K + 3 + b_kt17_external(2) + + + + Magnetic + + + + |b| external + b_kt17_external_tot + + + nT + + Magnetic + + + + b_mso all + b_kt17_all + + + nT + + + 3 + + bx + Component.I + 1 + b_kt17_all(0) + + + by + Component.J + 2 + b_kt17_all(1) + + + bz + Component.K + 3 + b_kt17_all(2) + + + + Magnetic + + + + |b| all + b_kt17_all_tot + + + nT + + Magnetic + + + + distance mercury-sun + b_kt17_rhel + + + nT + + Magnetic + + + + disturbance index + b_kt17_actIdx + + + nT + + Magnetic + + + + diff --git a/NumericalData/CDPP-AMDA/Mariner10/Models/m10-kt17-model.xml b/NumericalData/CDPP-AMDA/Mariner10/Models/m10-kt17-model.xml new file mode 100644 index 0000000..99504e7 --- /dev/null +++ b/NumericalData/CDPP-AMDA/Mariner10/Models/m10-kt17-model.xml @@ -0,0 +1,134 @@ + + + 2.4.1 + + spase://CNES/NumericalData/CDPP-AMDA/Mariner10/Models/m10-kt17-model + + KT17 model + KT17 mercury magnetic field model + 2023-02-20T01:01:36Z + Magnetic field along Mercury orbit is being real-time calculated. + S/C, sampling time, distance of Mercury from the Sun (AU) and Anderson et al., 2013 disturbance index should be defined by user. + + KT17 magnetic field model (Korth et al., 2017) model is used in calculations. + + James, M. K. - KT17 (v1.0.0) - https://github.com/mattkjames7/KT17/releases/tag/v1.0.0 + + spase://CNES/Person/CDPP-AMDA/Haje.Korth + PrincipalInvestigator + + + spase://CNES/Person/CDPP-AMDA/M.K.James + TechnicalContact + + + Korth, H., Johnson, C. L., Philpott, L., Tsyganenko, N. A., Anderson, B. J. (2017). A dynamic model of Mercury's magnetospheric magnetic field. Geophysical Research Letters, 44, 10,147– 10,154. + https://doi.org/10.1002/2017GL074699 + Model description + + + James, M. K. - KT17 (v1.0.0) + https://github.com/mattkjames7/KT17/releases/tag/v1.0.0 + Software + + + Anderson, B. J., Johnson, C. L., and Korth, H. (2013), A magnetic disturbance index for Mercury's magnetic field derived from MESSENGER Magnetometer data, Geochem. Geophys. Geosyst., 14, 3875– 3886 + https://doi.org/10.1002/ggge.20242 + Disturbance index description + + m10-m1-orb + + + spase://SMWG/Repository/CDPP/AMDA + Online + Open + + CDPP/AMDA HAPI Server + http://amda.irap.omp.eu/service/hapi + + Web Service to this product using the HAPI interface. + + CSV + Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse".. See the Rules of the road at http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers. + + + spase://SMWG/Repository/CDPP/AMDA + Online + Open + + CDPP/AMDA Web application + http://amda.cdpp.eu + Access to Data via CDPP/AMDA Web application. + + CSV + VOTable + CDF + PNG + Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse".. See the Rules of the road at http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers. + + IRAP + spase://CNES/Instrument/CDPP-AMDA/Mariner10/Models + MagneticField + + + 2016-06-01T00:00:00Z + 2021-05-05T23:49:59Z + + PT1M + + Mercury + + + b msm + b_kt17_model_60_0.427_50_m10_m1_xyz_mso + + nT + + 3 + + bx + Component.I + 1 + b_kt17_model_60_0.427_50_m10_m1_xyz_mso(0) + + + + + by + Component.J + 2 + b_kt17_model_60_0.427_50_m10_m1_xyz_mso(1) + + + + + bz + Component.K + 3 + b_kt17_model_60_0.427_50_m10_m1_xyz_mso(2) + + + + + + + Magnetic + + + + |b| + b_kt17_model_tot_60_0.427_50_m10_m1_xyz_mso + Scalar magnitude of the magnetic field in nT + phys.magField + nT + 1e-9>T + + TimeSeries + + + Magnitude + Magnetic + + + + diff --git a/NumericalOutput/CDPP-AMDA/JRM33/b_jrm33.xml b/NumericalOutput/CDPP-AMDA/JRM33/b_jrm33.xml index dbbe169..3ae7da5 100644 --- a/NumericalOutput/CDPP-AMDA/JRM33/b_jrm33.xml +++ b/NumericalOutput/CDPP-AMDA/JRM33/b_jrm33.xml @@ -118,7 +118,7 @@ |b| b_jrm33_con_tot Scalar magnitude of the magnetic field in nT - phys.magField + phys.magField nT 1e-9>T diff --git a/NumericalOutput/CDPP-AMDA/KT17/b_kt17.xml b/NumericalOutput/CDPP-AMDA/KT17/b_kt17.xml index 5dc36ed..c738578 100644 --- a/NumericalOutput/CDPP-AMDA/KT17/b_kt17.xml +++ b/NumericalOutput/CDPP-AMDA/KT17/b_kt17.xml @@ -6,22 +6,34 @@ KT17 along s/c orbit 2023-02-17T00:00:00Z - Magnetic field along s/c orbit is being real-time calculated. - S/C and sampling time should be defined by user. + Magnetic field along Mercury orbit is being real-time calculated. + S/C, sampling time, distance of Mercury from the Sun (AU) and Anderson et al., 2013 disturbance index should be defined by user. + + KT17 magnetic field model (Korth et al., 2017) model is used in calculations. - + James, M. K. - KT17 (v1.0.0) - https://github.com/mattkjames7/KT17/releases/tag/v1.0.0 - + spase://CNES/Person/CDPP-AMDA/M.K.James + TechnicalContact - Model description + Korth, H., Johnson, C. L., Philpott, L., Tsyganenko, N. A., Anderson, B. J. (2017). A dynamic model of Mercury's magnetospheric magnetic field. Geophysical Research Letters, 44, 10,147– 10,154. + https://doi.org/10.1002/2017GL074699 + Model description + + + James, M. K. - KT17 (v1.0.0) + https://github.com/mattkjames7/KT17/releases/tag/v1.0.0 + Software + + + Anderson, B. J., Johnson, C. L., and Korth, H. (2013), A magnetic disturbance index for Mercury's magnetic field derived from MESSENGER Magnetometer data, Geochem. Geophys. Geosyst., 14, 3875– 3886 https://doi.org/10.1002/ggge.20242 - + Disturbance index description @@ -59,7 +71,7 @@ MissionDependent - PTUserDefined + PT60S Mercury @@ -105,7 +117,7 @@ |b| b_kt17_model_tot Scalar magnitude of the magnetic field in nT - phys.magField + phys.magField nT 1e-9>T diff --git a/Person/CDPP-AMDA/Haje.Korth.xml b/Person/CDPP-AMDA/Haje.Korth.xml new file mode 100644 index 0000000..b1a02b4 --- /dev/null +++ b/Person/CDPP-AMDA/Haje.Korth.xml @@ -0,0 +1,10 @@ + + + 2.4.1 + + spase://CNES/Person/CDPP-AMDA/Haje.Korth + 2023-03-01T15:02:46Z + Dr. Haje Korth + Johns Hopkins Applied Physics Laboratory + + -- libgit2 0.21.2