Swarm IPF Level 1B Data dated 16. and 17. July 2005 as agreed at L2PS CDR

Analysis of EFI Data by DTU

By: Claudia Stolle

Some variables of the test data set SW_TEST_EFIA_PL_1B_20050716T000000_20050716T235959_0001_MDR_EFI_PL.cdf have been plotted.
Descriptions of the plots are based on experiences with CHAMP or refer to literature.
Completeness of review is not guaranteed.




Plot1: For a complete 2Hz record, the vectors should contain 24*60*60*2=172800 records. The vectors is 172792 records long. The plot shows that there are regularly missing records, means regular gaps:

EFI_1-1.png



Plot2+3: Electron Densities are within the expected range. Highest values are expected around the equator (Equatorial Ionisation Anomaly). Plot2 and Plot3 shows that there are kind of anomalies near the equator, but there is also a kind of anomaly at 60 degree North. This is not physical. Please note also the random spikes. Plot3 is simply a plotting of the electron density vector over the corresponding latitude vector in the file.

EFI_1-2.png
EFI_1-3.png




Plot4+5: Electron Temperature has natural magnitudes between 500 and 3000K during quiet times. The magnitudes in the file do not exceed 0.5K expect during regular spikes where values reach 4.5K.

EFI_1-4.png
EFI_1-5.png



Ion Temperature is zero throughout (not plotted).


Plot6: The Electric Field changes largely with UT in the testdata set. This seems unreasonable, since Swarm should be in similar local times during one day.

EFI_1-6.png




Plot7: Electric field: The distribution is ok (low at equator, high at high latitudes), but the magnitudes are probably too high. The literature suggest up to +/-100 mV/m at polar latitudes, also accounting for some activity.
Refs:
Kelley, M.C., The Earth's Ionosphere: Plasma Physics and Electrodynamics, 2nd edition, Elsevier, London, 2009.
Prölss, G.W., Physics of the Earth's Space Environment - An Introduction, Springer, 2004.


EFI_1-7.png




Plot8:
Ion Velocities is also lower at low than at high latitudes, which seems reasonable. Despite of that, it seems to be quite randomly distributed. The magnitudes in polar regions are similar to what found in the literature (up to 2000m/s). Low latitudes should show below 100m/s (eastward), and below 500 m/s (vertical). This significant difference in magnitude is not visible in the plots.
Refs:
Kelley, M.C., The Earth's Ionosphere: Plasma Physics and Electrodynamics, 2nd edition, Elsevier, London, 2009.
Lin, C. H., A. D. Richmond, J. Y. Liu, H. C. Yeh, L. J. Paxton, G. Lu, H. F. Tsai, and S.-Y. Su (2005), Large-scale variations of the low-latitude ionosphere during the October/November 2003 superstorm: Observational results, J. Geophys. Res., 110, A09S28, doi:10.1029/2004JA010900.
Foster, J. C., et al. (2005), Multiradar observations of the polar tongue of ionization, J. Geophys. Res., 110, A09S31, doi:10.1029/2004JA010928.


EFI_1-8.png




Same plots but for 2011-07-17:

EFI_2-1.png

EFI_2-2.png

EFI_2-3.png

EFI_2-4.png

EFI_2-5.png

EFI_2-6.png

EFI_2-7.png

EFI_2-8.png