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Swarm Data Processing and First Scientific Results

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Presentation on theme: "Swarm Data Processing and First Scientific Results"— Presentation transcript:

1 Swarm Data Processing and First Scientific Results
Nils Olsen and the Swarm SCARF Team Swarm Data Overview Magnetic Level 1b Data assessment SCARF: Level 2 Data Products and Processing Model of the Earth’s magnetic field including Swarm data Patrick Alken, Ciaran D Beggan, Stephan C. Buchert, Johnathan Burchill, Arnaud Chulliat, Eelco Doornbos, Joao Teixeira da Encarnacao, Ludwig Grunwaldt, Brian Hamilton, Rune Floberghagen, Eigil Friis-Christensen, Giuseppe Ottavianelli, Gauthier Hulot, Jose van den IJssel, David J. Knudsen, Alexey Kuvshinov, Jean-Michel Leger, Vincent Lesur, Hermann Luehr, Susan Macmillan, Stefan Maus, Ingo Michaelis, Max Noja, Nils Olsen, Poul Erik H Olsen, Jaeheung Park, Radek Peresty, Gernot Plank, Christoph Puethe, Jan Rauberg, Patricia Ritter, Martin Rother, Terence J Sabaka, Reyko Schachtschneider, Olivier Sirol, Claudia Stolle, Erwan Thebault, Alan W P Thomson, Lars Toeffner-Clausen, Jakub Velımsky, Pierre Vigneron, Pieter N Visser

2 Swarm Data Processing Hierarchy
L0 L1b Processor L1b L2 Processor L2 scientific users

3 Level-1b Data Products Magnetic Products Plasma Products
Ephemeris Products x = A, B or C  Type Descriptive Name MAGx_LR Low Rate magnetic data MAGx_HR High Rate magnetic data MAGx_CA Magnetic calibration data ASMxAUX Magnetic stray fields at ASM sensor VFMxAUX Magnetic stray fields at VFM sensor Type Descriptive Name EFIx_PL Plasma data LP_x_CA Langmuir probe calibration data TIIx_CA Thermal Ion Imager calibration data More on Swarm Level 1b Data Processing in Poster “ESA Swarm Mission - Level 1b Products” by Lars Tøffner-Clausen et al Type Descriptive Name GPSx_RO RINEX Observations GPSx_RN RINEX Navigation  data GPSxNAV Navigational Solution MODx_SC Medium-Precision Orbit Determination STRxATT Attitude ACCx_PR Non-gravitational Accelerations More on Plasma Products in Presentation “First results from the Swarm Electric Field Instruments” by David Knudsen et al

4 Magnetic Level-1b Data Product MAGx_LR
1 Hz magnetic field observations: time, position, F, BNEC and BVFM Element Contents Frame Units Timestamp Time of observation - CDF_EPOCH SyncStatus Time reference information Latitude Latitude of observation ITRF degree Longitude Longitude of observation Radius Radius of observation m F Magnetic field intensity nT dF_AOCS Magnetic stray field correction intensity related to attitude control magneto-torquers dF_other Magnetic stray field correction intensity of all other sources F_error Error estimate on magnetic field intensity B_VFM Magnetic field vector VFM B_NEC NEC dB_AOCS Magnetic stray field correction vector related to attitude control magneto-torquers dB_other Magnetic stray field correction vector of all other sources B_error Error estimates on magnetic field vector (B_VFM) q_NEC_CRF Rotation from NEC frame to STR Common Reference Frame (CRF), quaternion NEC  CRF Att_error Error estimate on attitude information degree/103 Flags_F Flags characterizing the magnetic field intensity Flags_B Flags characterizing the magnetic field vector measurement B_VFM and B_NEC Flags_q Flags characterizing the attitude information Flags_Platform Flags characterizing the spacecraft platform information ASM_Freq_Dev ASM reference frequency calibration data deviation – for ASM stability assessment Hz½

5 Swarm-A 1 sec Level1b Data MAGA_LR
2 December 2013 Quiet day (Kp  0+)

6 Swarm-A 1 sec Level1b Data MAGA_LR
2 December 2013 Quiet day (Kp  0+) CHAOS-4 model subtracted

7 Swarm-A and Swarm-B 1 sec Level1b Data MAGA_LR
2 December 2013 Quiet day (Kp  0+) CHAOS-4 model subtracted Difference Swarm A -Swarm B

8 Swarm Data Processing Hierarchy
L0 L1b Processor (Prototype Processor) L1b Processor (Operational Processor) L1b L2 Processor L2 scientific users

9 Level1b Data from Operational Processor
CHAOS-4 model subtracted Difference Swarm A -Swarm B

10 Level1b Data from Prototype Processor (non-validated data)
CHAOS-4 model subtracted Swarm-B data shifted by 15s since satellite flies 120 km behind Swarm-A (on that day) Difference Swarm A -Swarm B More on Swarm Scalar Field Measurements from ASM in Presentations by Gauthier Hulot and co-workers

11 Swarm Level-2 Data Products

12 Swarm Level-2 Data Processing
Swarm SCARF (Satellite Constellation Application and Research Facility) Consortium of 6 European partners (DTU, GFZ, IPGP, ETH, DEOS, BGS) with support from NASA/GSFC, CIRES and CUP ESA funded activity for Development, Implementation and Operation of a distributed L2 Processing Facility Cat-1 chains with “scientists in the loop” (operated by SCARF) advanced geomagnetic models, mantle conductivity … Cat-2 chains with automatic processing (operated by ESRIN) products describing Earth environment, NRT capability Development phase: Oct 2010 – March 2014 Exploitation phase: 2014 – (at least 5 years)

13 Swarm Data Processing Hierarchy
L0 L1b Processor (Prototype Processor) L1b Processor (Operational Processor) L1b L2 Processor SCARF L2 Processing Facility L2 scientific users

14 Level-2 Data Products Cat-1: Complex algorithms to derive Level-2 products describing specific sources of the Earth’s magnetic field. Product derived by SCARF since scientific experience is required to derive these products.

15 Level-2 Data Products Cat-2: Algorithms leading to Level-2 products with minimum delay, e.g. for space weather applications. Near real-time capability. Provided in CDF. Algorithms designed by SCARF, data processed by PDGS More on Swarm Level 2 Data Processing in Poster “SCARF - The Swarm Satellite Constellation Application and Research Facility” by Nils Olsen et al More on Swarm Cat-2 Data Products in talk “The Swarm Level-2 Cat-2 Data Products” by Hermann Lühr et al and Poster ”Swarm Equatorial Electric Field Inversion” by Patrick Alken et al.

16 Field Modelling using Swarm data First Results based on non-validated data
Data spaning 26 Nov 2013 to 27 April 2014 Non-validated data from L1b Prototype Processor Geomagnetic quiet conditions (Kp < 2o, |dDst/dt| < 2 nT/hr) “Dark regions” (sun at least 10 degrees below horizon) Model Parameterization Spherical Harmonic Model up to degree n=40 (static) linear time dependence (up to n=8) External field “CHAOS-4 parameterization” (SM, GSM, RC-dependence) Co-estimation of Euler angles describing VFM-STR transformation in bins of 10 days for each of the 3 Swarm satellites (as for CHAOS-4)

17 Spatial Data Distribution
Swarm A, B and C satellites Geomagnetic quiet conditions (Kp < 2o, |dDst/dt| < 2 nT/hr) ”Dark regions” (sun at least 10o below horizon) Swarm scalar data Swarm vector data

18 Spatial Data Distribution
Swarm A, B and C satellites Geomagnetic quiet conditions (Kp < 2o, |dDst/dt| < 2 nT/hr) ”Dark regions” (sun at least 10o below horizon)

19 Spatial Data Distribution
Swarm A, B and C satellites Geomagnetic quiet conditions (Kp < 2o, |dDst/dt| < 2 nT/hr) ”Dark regions” (sun at least 10o below horizon) Swarm scalar data Swarm vector data CHAMP scalar data (propagated in time by 3.5 years using CHAOS-4)

20 Geomagnetic Spectrum

21 Difference in Br wrt CHAOS-4 Crustal Field (n=15-30)
Good agreement of Swarm_04c and CHAOS-4

22 Difference in Br wrt CHAOS-4 Core Field (n=1-14)
Extrapolation error of CHAOS-4 (latest vector data: Sept 2010, latest scalar data: Jul 2013)

23 Difference in Br wrt CHAOS-4plus Core Field (n=1-14)
CHAOS-4plus: Update of CHAOS-4, combining Ørsted, CHAMP, SAC-C and Swarm data

24 Model rms misfit Swarm-04c CHAOS-4plus Swarm-only model SW-A SW-B SW-C
4.82 nT 4.44 nT 4.49 nT Br 3.15 nT 2.16 nT 2.31 nT Bq 4.21 nT 3.51 nT 3.60 nT Bf 2.83 nT 2.70 nT 2.67 nT SW-A SW-B SW-C CHAMP Ørsted F 4.46 nT 4.37 nT 4.41 nT 4.84 nT 3.38 nT Br 1.97 nT 2.39 nT 2.58 nT 2.80 nT 4.45 nT Bq 3.08 nT 3.37 nT 3.39 nT 3.59 nT 5.36 nT Bf 2.85 nT 2.87 nT 2.83 nT 2.76 nT 5.06 nT CHAOS-4plus combined model Model coefficients available at CHAOS-4 homepage More on CHAOS-4plus in Poster “Towards CHAOS-5 - How can Swarm contribute?” by Christopher C. Finlay et al

25 Conclusions We are waiting for more Swarm data!
Very good Swarm magnetic data quality inter-satellite agreement in scalar intensity during quiet dark conditions is better than 5 ppm (0.2 nT) CHAOS-4plus: Magnetic field model spanning 16 years of data show excellent agreement of data from 6 different satellites (Ørsted, CHAMP, SAC-C and 3 x Swarm) First Level-2 products expected at end of 2014 … … and already very soon for the CAT-2 products We are waiting for more Swarm data!

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