Scaling laws for the energy transfer in space plasma turbulence

R Marino, L Sorriso-Valvo - Physics Reports, 2023 - Elsevier
One characteristic trait of space plasmas is the multi-scale dynamics resulting from non-
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …

The advanced composition explorer

EC Stone, AM Frandsen, RA Mewaldt… - Space Science …, 1998 - Springer
Abstract The Advanced Composition Explorer was launched August 25, 1997 carrying six
high-resolution spectrometers that measure the elemental, isotopic, and ionic charge-state …

Solar wind spatial scales in and comparisons of hourly Wind and ACE plasma and magnetic field data

JH King, NE Papitashvili - Journal of Geophysical Research …, 2005 - Wiley Online Library
Hourly averaged interplanetary magnetic field (IMF) and plasma data from the Advanced
Composition Explorer (ACE) and Wind spacecraft, generated from 1 to 4 min resolution data …

Solar wind turbulence and the role of ion instabilities

O Alexandrova, CHK Chen, L Sorriso-Valvo… - Space Science …, 2013 - Springer
Solar wind is probably the best laboratory to study turbulence in astrophysical plasmas. In
addition to the presence of magnetic field, the differences with neutral fluid isotropic …

Global dayside ionospheric uplift and enhancement associated with interplanetary electric fields

B Tsurutani, A Mannucci, B Iijima… - Journal of …, 2004 - Wiley Online Library
The interplanetary shock/electric field event of 5–6 November 2001 is analyzed using ACE
interplanetary data. The consequential ionospheric effects are studied using GPS receiver …

Earth-affecting solar transients: a review of progresses in solar cycle 24

J Zhang, M Temmer, N Gopalswamy… - Progress in Earth and …, 2021 - Springer
This review article summarizes the advancement in the studies of Earth-affecting solar
transients in the last decade that encompasses most of solar cycle 24. It is a part of the effort …

Flux tube texture of the solar wind: Strands of the magnetic carpet at 1 AU?

JE Borovsky - Journal of Geophysical Research: Space …, 2008 - Wiley Online Library
It is argued here that the inner heliosphere is filled with a network of entangled magnetic flux
tubes and that the flux tubes are fossil structures that originate at the solar surface. 65,860 …

Direct evidence for magnetic reconnection in the solar wind near 1 AU

JT Gosling, RM Skoug, DJ McComas… - Journal of Geophysical …, 2005 - Wiley Online Library
We have obtained direct evidence for local magnetic reconnection in the solar wind using
solar wind plasma and magnetic field data obtained by the Advanced Composition Explorer …

Properties of interplanetary coronal mass ejections at one AU during 1995–2004

L Jian, CT Russell, JG Luhmann, RM Skoug - Solar Physics, 2006 - Springer
We present a comprehensive survey of 230 interplanetary CMEs (ICMEs) during 1995–2004
using Wind and ACE in situ observations near one AU, and examine the solar-cycle …

Properties of stream interactions at one AU during 1995–2004

L Jian, CT Russell, JG Luhmann, RM Skoug - Solar Physics, 2006 - Springer
A stream interaction region (SIR) forms when a fast solar stream overtakes a slow stream,
leading to structure that evolves as an SIR moves away from the Sun. Based on Wind (1995 …