Results 181 to 190 of about 103,405 (350)
Energetic particles in the Jovian magnetosphere [PDF]
J. H. Trainor +4 more
openalex +1 more source
Abstract Utilizing 8 years of dayside Magnetospheric Multiscale (MMS) mission plasma region identifications, we present an automatically identified and manually verified data set of 2,594 bow shock crossings in MMS burst‐mode. For each bow shock crossing, we identify the bow shock ramp in each MMS probe using two automated methods and apply multi ...
Vicki Toy‐Edens +4 more
wiley +1 more source
Thermal and suprathermal plasma densities in the outer magnetosphere [PDF]
D. A. Gurnett, L. A. Frank
openalex +1 more source
Geoeffectivity of Solar Wind Heavy Ions
Abstract The influence of solar wind properties, such as the southward interplanetary magnetic field, on geomagnetic activity has been well established. However, the role of heavy ions (i.e., particles heavier than protons) in the solar wind on geomagnetic storms is not fully understood.
Chris Jia +6 more
wiley +1 more source
Abstract We present a study of ground‐based Pc5 ultra‐low frequency (ULF) wave response to over 400 interplanetary (IP) shocks and 18 foreshock transients. We investigated the local time dependence of magnetospheric Pc5 wave power generated by IP shocks and foreshock transients and whether this dependence is related to the impact angle of IP shocks and
Veera Lipsanen +8 more
wiley +1 more source
Nose whistler dispersion as a measure of magnetosphere electron temperature
H. Guthart
openalex +1 more source
Energetic protons in the Jovian magnetosphere [PDF]
F. B. McDonald +2 more
openalex +1 more source
Abstract Magnetic reconnection is inherently structured, with distinct spatial regions such as inflows, outflows, and separatrices playing key roles in energy conversion and particle transport. While in situ spacecraft measurements provide detailed local information, determining where a spacecraft lies within the global reconnection geometry remains a ...
Cara L. Waters +7 more
wiley +1 more source

