Abstract SeparationandQuantificationofIonosphericConvectionSources:2.TheDipoleTiltAngleInfluenceonReverseConvectionCellsDuringNorthwardIMF

In a mean field approach, we may express the effective magnetic field as a superposition of the external magnetic field and a so-called exchange field that handles the

To better investigate if the magnetic field geometry could be responsible for a possible mode conversion process, we plot the distribution of the magnetic field inclinations

We see that when it is dark, the magnetic field perturbations are most commonly consistent with an equivalent current J eq = J ⟂,df ≈ −J ⟂,cf = −∇

In addition, an in situ package will measure the composition and speed of the solar wind and the strength and orientation of interplanetary magnetic field, measurements crucial

B) Average substorm MLT locations for 18 ◦ bins of IMF θ c for substorms identified from Polar data in the northern hemisphere. D) ∆MLT between the southern and northern

Here we extend an earlier study of the proton aurora in the cusp during northward interplanetary magnetic field (IMF) conditions [Frey et al., 2002] to southward IMF conditions..

of current systems exist in the magnetosphere, most notably the dayside magnetopause Chapman- Ferraro currents, high latitude “Region 1” field-aligned Birkeland currents, “Region

The main goal of this study is determine the magnetic field values of chromospheric spicules from high cadence, high spatial resolution data using the weak field approximation.. A