The investigation of auroral field-aligned current (FAC) sheets is crucial in the context of space weather research since they serve as main transmitters of energy and momentum across geospace domains. Different magnetosphere-ionosphere coupling modes are reflected by the FACs’ multiscale nature with spatial scales, i.e., latitudinal extensions, ranging from below 1 km to hundreds of kilometers. The multiscale property can be addressed conveniently using ESA’s three-spacecraft mission Swarm. According to common practice a linear correlation analysis is performed on lagged and band-pass filtered scalar FAC density estimates from two nearby spacecraft. We introduce the framework VALOR (Vectorial Association of Linearly Oriented Residua) wh...
©2016. The Authors. We present the first large-scale comparison of the spatial distribution of field...
Abstract Various ESA projects and several proposals to first Swarm DISC Call for Ideas (May 2016) s...
The ESA Swarm mission provides a qualitatively new level of observational geomagnetic data, \textbf{...
The orientation of field-aligned current sheets (FACs) can be inferred from dual-spacecraft correlat...
We investigate the statistical, dual‐spacecraft correlations of field‐aligned current (FAC) signatur...
The orientation of field-aligned current sheets (FACs) can be inferred from dual-spacecraft correlat...
Field-aligned currents (FACs) in the magnetosphere–ionosphere (M–I) system exhibit a range of spatia...
A pilot statistical study of field-aligned currents (FACs), using an automated FAC-finding technique...
Field-aligned currents (FACs) are a fundamental component of coupled solar wind-magnetosphere-ionosp...
Abstract In this study we performed a detailed analysis on the scale-size of field-aligned currents ...
In this paper we present analysis of current density when the Cluster spacecraft pass the nightside ...
By determining the location and size of the Region 1 (R1) and Region 2 (R2) large‐scale field‐aligne...
We present the first large-scale comparison of the spatial distribution of field-aligned currents as...
International audienceWe described the ground signatures of dynamic substorm features as observed by...
On the basis of field-aligned currents (FACs) and Hall currents derived from high-resolution magnet...
©2016. The Authors. We present the first large-scale comparison of the spatial distribution of field...
Abstract Various ESA projects and several proposals to first Swarm DISC Call for Ideas (May 2016) s...
The ESA Swarm mission provides a qualitatively new level of observational geomagnetic data, \textbf{...
The orientation of field-aligned current sheets (FACs) can be inferred from dual-spacecraft correlat...
We investigate the statistical, dual‐spacecraft correlations of field‐aligned current (FAC) signatur...
The orientation of field-aligned current sheets (FACs) can be inferred from dual-spacecraft correlat...
Field-aligned currents (FACs) in the magnetosphere–ionosphere (M–I) system exhibit a range of spatia...
A pilot statistical study of field-aligned currents (FACs), using an automated FAC-finding technique...
Field-aligned currents (FACs) are a fundamental component of coupled solar wind-magnetosphere-ionosp...
Abstract In this study we performed a detailed analysis on the scale-size of field-aligned currents ...
In this paper we present analysis of current density when the Cluster spacecraft pass the nightside ...
By determining the location and size of the Region 1 (R1) and Region 2 (R2) large‐scale field‐aligne...
We present the first large-scale comparison of the spatial distribution of field-aligned currents as...
International audienceWe described the ground signatures of dynamic substorm features as observed by...
On the basis of field-aligned currents (FACs) and Hall currents derived from high-resolution magnet...
©2016. The Authors. We present the first large-scale comparison of the spatial distribution of field...
Abstract Various ESA projects and several proposals to first Swarm DISC Call for Ideas (May 2016) s...
The ESA Swarm mission provides a qualitatively new level of observational geomagnetic data, \textbf{...