SW_AEJxLPL_2F

Auroral electrojets line profile - Line current method (LC)

Thematic areas: Ionosphere/Magnetosphere, Space Weather

Applicable missions: Swarm

Applicable spacecraft: Swarm-A, Swarm-B, Swarm-C

Description

Characterization of the electrojet sheet current density as well as the total horizontal sheet and associated large-scale field-aligned current density along the Swarm orbit ionospheric footprints at auroral latitudes (by using LC method).

Data access

FAST processing

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File contents

Variable Units Description Dim Type
t Time of observation, UTC 1 CDF_EPOCH
Latitude deg Position in ITRF - Geocentric latitude 1 CDF_DOUBLE
Longitude deg Position in ITRF - Geocentric longitude 1 CDF_DOUBLE
Latitude_QD deg Quasi-dipole latitude 1 CDF_DOUBLE
Longitude_QD deg Quasi-dipole longitude 1 CDF_DOUBLE
MLT hour Magnetic Local Time (QD) 1 CDF_DOUBLE
J A/km North and East component of horizontal sheet current density vector in geocentric frame 2 CDF_DOUBLE
J_QD A/km East component of horizontal sheet current density in QD frame 1 CDF_DOUBLE
t_qual Time instants of quality information (RMS_misfit and Confidence), UTC 1 CDF_EPOCH
RMS_misfit nT Root Mean Square error misfit between observations and model values for the oval crossings3 1 CDF_DOUBLE
Confidence - Goodness of fit computed as 1 - (residual rms / signal rms) for the oval crossings3 1 CDF_DOUBLE

More details

Product identifier AEJxLPL_2F
Definition Latitude profiles of high-latitude ionospheric horizontal sheet current densities using the Line Current method
Input Data MAGx_LR_1B, Latest CHAOS model1 including, core, lithosphere, magnetosphere and secondary currents.
Input Time Span 24 h
Spatial representation One geographic and quasi-dipole latitude/longitude pair for each output value. Longi-tudes and latitudes of nearest magnetic-field measurement. Given at Swarm footprints (at 110 km altitude) according to the time representation of this product2. The footprints have been determined with radial mapping.
Time representation 1 deg latitude corresponding to ~ 15 s
Units A/km
Resolution Full resolution (Double precision)
Uncertainty c.f. Olsen, N, Geophys. Res. Lett., 23, 3635-3638 and Aakjaer, C. D. et al., doi:10.1186/s40623-016-0509-y
Quality indicator RMS characterizing the misfit between modelled and measured magnetic field by Swarm
Data volume ~250 kB
Data format CDF
Output time span 24 h2
Update rate Daily
Latency < 1 day
Notes 1 Version information of Input Data are available in the CDF global attributes.
2 Product always contain data from the start of the first oval crossing of the day until the end of the last oval crossing starting that day, i.e. may contain data from the next day if oval crossing occurs around midnight.
3 In Line Current method the equatorward boundary of oval crossing is always at +/- 50 QD latitude and the poleward boundary is at the most poleward point in QD latitude of the satellite trajectory.

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