Journal of Geophysical Research: Solid Earth RESEARCH ARTICLE

Pdfs (histogram style) of absolute momentum fluxes obtained with balloon observations (dark gray), and offline tests with the BCGWD (black) and CGWD (light gray, see text) configuration

(Three plas- moid observations were discarded, since they had a complex morphology making it difficult to clearly define a scale size and magnetic field signature.) For the solar wind,

The different behavior of the two ion species is further shown by statistics of H + and O + flow also outside BBFs: For perpendicular earthward velocities of H + above about 100 km/s,

G/R ratio profile for 67P from 10 to 10 4 km for a line of sight crossing the projected cometocentric distance according to different levels of solar activity: for medium solar

The equatorial orbit of the Time History of Events and Macroscale Interactions during Substorms (THEMIS) spacecraft can explain to a large extent this occurrence rate differ- ence,

Here we revisit the kinematics of the EAR using significantly augmented data sets (Figure 2), including newly available episodic GPS data from Ethiopia and Tanzania, an

From Figure 4 (top to bottom) are shown respectively the total intensity as measured in the reference channel, the DoLP, the AoLP, the local magnetic field inclination, and

The power density can be used as a primary indicator of potential reconnection regions, but selected events must be reviewed separately to confirm any possible reconnection signatures