Results 41 to 50 of about 934,352 (223)
Observations of electromagnetic whistler precursors at supercritical interplanetary shocks
Paul Kellogg +2 more
exaly +2 more sources
Formation of a strong southward IMF near the solar maximum of cycle 23 [PDF]
We analyzed observations of the solar activities and the solar wind parameters associated with large geomagnetic storms near the maximum of solar cycle 23.
S. Watari, M. Vandas, T. Watanabe
doaj +1 more source
Sources of interplanetary shocks [PDF]
Abstract The sources of interplanetary shocks are reviewed from the standpoint of today's knowledge. Recent progress from both new and accumulated observations and models indicates that contributions from the two major sources of the shocks: CMEs and stream interactions, have distinctive radial, latitudinal and temporal dependencies.
openaire +1 more source
Evolution of the Suprathermal Proton Population at Interplanetary Shocks
We investigate the evolution of the suprathermal (ST) proton population as interplanetary shocks cross 1 au. The variability of the ST proton intensities and energy spectra upstream of the shocks is analyzed in terms of the shock parameters, upstream ...
D. Lario +6 more
semanticscholar +1 more source
Efficiency of particle acceleration at interplanetary shocks: Statistical study of STEREO observations [PDF]
Context. Among others, shocks are known to be accelerators of energetic charged particles. However, many questions regarding the acceleration efficiency and the required conditions are not fully understood. In particular, the acceleration of electrons by
N. Dresing +3 more
semanticscholar +1 more source
Acceleration of protons by interplanetary shocks [PDF]
Short duration proton energy increases observation by Explorer 34, considering interpretation as acceleration associated interplanetary ...
K. W. Ogilvie, J. F. Arens
openaire +1 more source
The occurrence of geomagnetically induced currents (GICs) poses serious threats to modern technological infrastructure. Large GICs result from sharp variations of the geomagnetic field (dB/dt) caused by changes of large‐scale magnetospheric and ...
D. Oliveira +12 more
semanticscholar +1 more source
What causes the variations of the peak intensity of CIR accelerated energetic ion fluxes? [PDF]
The variation of the peak intensity of energetic ions accelerated at CIR related shocks in the interplanetary medium as observed by instruments on board of ULYSSES during its pass towards the south polar region and from the north polar region back to ...
E. Keppler
doaj +1 more source
The interaction between interplanetary (IP) shocks and the solar wind has been studied in the past for the understanding of energy dissipation mechanisms within collisionless plasmas.
Byeongseon Park +7 more
doaj +1 more source
Interplanetary Signatures during the 1972 Early August Solar Storms
In 1972, early August, a series of interplanetary shocks were observed in the heliosphere from 0.8 to 2.2 au. These shocks were attributed to a series of brilliant flares and plasma clouds since at that time coronal mass ejections (CMEs) and their ...
Consuelo Cid +3 more
doaj +1 more source

