On the character of cosmic ray variations at f>2x10-5 Hz [PDF]
We examine the time series of cosmic ray (CR) intensity recorded by two neutron monitors (NMs) at medium latitudes for scaling properties on time scales shorter than the diurnal variation.
K. Kudela +3 more
doaj
Hybrid Simulations of the Cusp and Dayside Magnetosheath Dynamics Under Quasi-Radial Interplanetary Magnetic Fields. [PDF]
Ng J +4 more
europepmc +1 more source
THE EFFECT OF TURBULENCE INTERMITTENCE ON THE EMISSION OF SOLAR ENERGETIC PARTICLES BY CORONAL AND INTERPLANETARY SHOCKS [PDF]
L. G. Kocharov, T. Laitinen, Rami Vainio
openalex +1 more source
Small-scale interplanetary magnetic flux ropes (SMFRs) are similar to ICMEs in magnetic structure, but are smaller and do not exhibit coronal mass ejection plasma signatures.
Hameedullah Farooki +9 more
doaj +1 more source
In space plasmas, the rarity of collisions leads to complex structures in the velocity space where a turbulent cascade of the velocity distribution function (VDF) fluctuations is thought to occur.
A. Larosa +13 more
doaj +1 more source
FEATURES OF LONG PERIOD VARIATIONS OF GALACTIC COSMIC RAY INTENSITY IN RELATIONS WITH THE TURBULENCE OF THE INTERPLANETARY MAGNETIC FIELD in 1968 - 2014 [PDF]
M. V. Alania
openalex +1 more source
Unveiling the Global Characteristics of Turbulence in the Venusian Space Environment
Turbulence plays a crucial role in energy transfer from large to small scales in solar wind‐Venus interaction. Observations have identified magnetic field fluctuations and turbulence in the Venusian space environment. However, due to limited observations
Tong Dang +8 more
doaj +1 more source
Turbulence Properties of Interplanetary Coronal Mass Ejections in the Inner Heliosphere: Dependence on Proton Beta and Flux Rope Structure [PDF]
Simon Good +5 more
openalex +1 more source
Analysis of Turbulence Energy Transfer at an Interplanetary Shock Observed by MMS
Nawin Ngampoopun +3 more
openalex +1 more source

