The Compression of the Heliospheric Magnetic Structure by Interplanetary Shocks: Is the Structure at 1AU a Manifestation of Solar-Wind Turbulence or Is It Fossil Structure From the Sun? [PDF]
Frontiers in Astronomy and Space Sciences, 2020 As a test of the action of MHD turbulence in the solar wind, the compression of the heliospheric magnetic structure at 1AU by 109 interplanetary shocks is examined.
Joseph E. Borovsky
openalex +2 more sources
Turbulence properties of interplanetary coronal mass ejection flux ropes at 1 au [PDF]
Monthly notices of the Royal Astronomical SocietyInterplanetary coronal mass ejection (ICME) is a massive, coherent magnetic structure emitting from the Sun in interplanetary space and plays an essential role in space weather processes.
Zubair Shaikh
openalex +2 more sources
The effects of expansion and turbulence on the interplanetary evolution of a magnetic cloud
Astronomy & AstrophysicsCoronal mass ejections (CMEs) represent the most extreme solar products, showing complex and dynamic structures when detected in situ. They are often preceded by a shock and carry a magnetic cloud organised as a flux rope, surrounded and permeated by turbulent fluctuations, and whose radial size expands during propagation.
Sangalli, Mattia +3 more
openaire +3 more sources
The connection of the interplanetary magnetic field turbulence and rigidity spectrum of Forbush decrease of the galactic cosmic ray intensity [PDF]
, 2015 We analyze the temporal changes in the rigidity spectrum of Forbush decrease (Fd) of the galactic cosmic ray (GCR) intensity observed in November 2004.
Anna Wawrzynczak, M. V. Alania
openalex +2 more sources
GENESIS OF INTERPLANETARY INTERMITTENT TURBULENCE: A CASE STUDY OF ROPE–ROPE MAGNETIC RECONNECTION [PDF]
, 2016 Abraham C.‐L. Chian +7 more
openalex +2 more sources
Non-Gaussianity and cross-scale coupling in interplanetary magnetic field turbulence during a rope–rope magnetic reconnection event [PDF]
, 2018 . In a recent paper ( Chian et al. , 2016 ) it was shown that magnetic reconnection at the interface region between two magnetic flux ropes is responsible for the genesis of interplanetary intermittent turbulence.
Rodrigo A. Miranda +3 more
openalex +2 more sources
The Turbulence Magnetic Helicity Signature in the Interplanetary Medium: A Blackman–Tukey and Morlet Wavelet Analysis [PDF]
, 2018 Bernard J. Vasquez +2 more
openalex +2 more sources
FEATURES OF LONG PERIOD VARIATIONS OF GALACTIC COSMIC RAY INTENSITY IN RELATIONS WITH THE TURBULENCE OF THE INTERPLANETARY MAGNETIC FIELD in 1968 - 2014 [PDF]
, 2016 Data of super neutron monitors, Bx, By, Bz components of the interplanetary magnetic field (IMF) a have been used to study a relation of the long-period variations of the galactic cosmic ray (GCR) intensity with IMF turbulence for the period of 1968-2014.
M. V. Alania
openalex +2 more sources
The Astrophysical Journal, 2023 Understanding the magnetic connections from the Sun to interplanetary space is crucial for linking in situ particle observations with the solar source regions of the particles.
T. Laitinen +3 more
doaj +1 more source
Shock waves propagation in the turbulent interplanetary plasma [PDF]
Advances in Space Research, 1996 AbstractEffect of turbulence on interplanetary shock waves propagation is considered. It is shown that background turbulence results in the additional shock wave deceleration which may be comparable with the deceleration due to plasma sweeping. The turbulent deceleration is connected with the energy losses due to the strong turbulence amplification ...
I. V. Chashei, V. I. Shishov
openaire +4 more sources