... ionospheric electric field deduced from the SuperDARN data is 34. then coupled with these results to estimate the electric field in the 35[r] ...

8

... left) **and** diamond state (DS, ...micron-size, **and** are explained by the Van den Berg (VdB) model ...of **magnetic** walls **and** vortices in the simulated states is very close to the predictions of VdB ...

8

... gun **and** a FEI Titan fitted in with a Schottky ...300kV **and** are fitted with a Gatan Imaging Filter for zero loss filtering [28] **and** thickness mapping ...resolution **magnetic** field-free imaging ...

23

... dipolarization, **and** the one observed at ~04:10 UT the 2 nd ...degrees **and** latitude of ~56-60 degrees in System III coordinate, using a **flux** equivalence mapping model [Vogt et ...The **auroral** ...

28

... other **and** thus in principle two degenerate ground states exist, which we named after the direction of magnetization of the bot- tom **and** top NCs, ...+) **and** (+, −) ...location **and** even the ...

6

... domains **and** domain walls with a topology different from that for flat elements[ 1 , 2 ...scarce **and** so far no material has given rise to well- defined **magnetic** ...domains **and** domain walls in ...

8

... interplanetary **magnetic** field (IMF) is most significant. **Magnetic** field lines are added to the tail lobes before under- going reconnection in the equatorial plane of the magnetotail **and** then ...

16

... polar **auroral** region have been recently reported in different studies **and** related to tail ...HST **auroral** intensifications in the dawn **auroral** sector, propagating at 330 % rigid corotation from ...

47

... altitude **magnetic** ﬁeld lines connecting to the main aurora (Northern **and** Southern ...together **and** depict a nonlinear trend —a factor of 10 increase in characteristic energy produces roughly ~100 ...

14

... **and** afternoon sectors during orbit ...broader **and** brighter during orbit 7 **and** characterized by two bright spots whose shape **and** relative intensity vary over the 7 consecutive ...longitude ...

10

... the **closure** rate from ~20 to 114 kV in the following ...the **closure** voltage of Figure 3 prior to the arrival of the shock results partly from a smearing of rapidly varying signals by our algorithms ...

12

... fast **and** good results compared to finite elements method ...angular **and** axial coordinate by means of the image ...problem **and** calculation ...open-circuit **magnetic** **flux** density in an ...

9

... A detailed explanation of tokamak physics, including an overview of existing experimental facilities, can be found in [18]. An overview of current challenges in Tokamak Plasma control as well as an introduction ...

7

... harmonics **and** the discretization ...harmonics **and** 1 894 053 points in the volume considered for a total computation time of nine ...smooth **and** the error is below 2% on each ...

8

... , **and** Jiang et al. 2014b ). The model’s behavior relative to emergence **and** model characteris- tics are fairly well understood (see, ...poleward **flux** strips (“surges”), require a delicate balance ...

19

... Saturn's secondary auroral ring Denis Grodent Aikaterini Radioti Bertrand Bonfond Jean-Claude Gérard Jacques Gustin Wayne Pryor.. ……...[r] ...

19

... the **magnetic** **flux** is perturbed by a non-conducting dispersed phase in liquid metal flow is an open ...variable **magnetic** **flux** density ~ B, the Lorentz force in mo- mentum conservation equation ...

9

... FIG. 4. FFT spectral density of fluctuations of jjDVjj 2 vs the modulating pul- sation x M for a ¼ 6:9% **and** U ¼ 0.001 m/s at 6283 rad/s (data from [ 21 ]). FIG. 5. / 0 vs x at U ¼ 0:001 ms 1 for a ¼ 0% ( 䊊, 䊉), ...

8

... 3.2. Field line deformation from the magnetosphere to the ionosphere Another possible interpretation of the UV **auroral** spirals, indirectly related to magne- 200 tospheric plasma vortices, is field line deformation ...

25

... of **auroral** electrons with atmospheric H atoms **and** H 2 molecules, following acceleration along **magnetic** field lines, give rise to excitation of these primary ...H **and** H 2 almost immediately ...

1