Results 71 to 80 of about 2,118 (212)
The Sun is a variable active-dynamo star, emitting radiation in all wavelengths and solar-wind plasma to the interplanetary space. The Earth is immersed in this radiation and solar wind, showing various responses in geospace and atmosphere.
Kazuo Shiokawa, Katya Georgieva
doaj +1 more source
Investigating Potential Benefits of Future Sub‐L1 Missions With STEREO‐A
Abstract We present the first statistical study of geomagnetic storm forecasting using in situ data from the STEREO‐A spacecraft as a sub‐L1 monitor. Between November 2022 and June 2024, STEREO‐A crossed the Sun–Earth line, covering longitudinal and radial separations of ±15° $\pm 15{}^{\circ}$ from the Sun–Earth line and 0.01–0.06 au from Earth.
E. Weiler +6 more
wiley +1 more source
Regional and Seasonal Effects of Geomagnetic Storms on Terrestrial Weather
Abstract It has long been a mystery why small Total Solar Irradiation changes have significant effects on Earth's climate. Solar cycle correlation studies abound but cannot conclusively point to a viable physical mechanism. Here, I show that geomagnetic storms have a profound terrestrial weather impact.
J. Raeder
wiley +1 more source
The authors present a space-based array designed to localize and track the radio emission associated with coronal mass ejections (CMEs) from the Sun. Radio emission from CMEs is a direct tracer of the particle acceleration in the inner heliosphere and ...
Kasper, Justin C. +2 more
core +2 more sources
Voyager 2 observation of the multifractal spectrum in the heliosphere and the heliosheath [PDF]
We look in detail at the multifractal scaling of the fluctuations in the interplanetary magnetic field strength as measured onboard Voyager 2 in the entire heliosphere and even in the heliosheath.
W. M. Macek, A. Wawrzaszek
doaj +1 more source
The 3-D Sun and heliosphere at solar maximum [PDF]
Bob Forsyth and Andy Breen report from the RAS G Discussion Meeting at the Geological Society on 11 January 2002. Presentations came from both the solar and heliospheric communities, on the 3-D structure and dynamics of the solar corona and heliosphere and their inter-relation during the present maximum in the solar activity cycle.
Bob Forsyth, Andy Breen
openaire +1 more source
Soft X‐Ray Emission From Saturn's Magnetosheath II: Solar Wind Driving
Abstract Saturn's magnetosphere is dominated by Enceladus‐sourced neutrals, which spread throughout the system into the magnetosheath. The neutrals can charge exchange with highly charged solar wind ions, causing soft X‐ray emission (<2 ${< } 2$ keV) upon de‐excitation of the ion.
D. Naylor +4 more
wiley +1 more source
ICMEs in the inner heliosphere: origin, evolution and propagation effects
This report assesses the current status of research relating the origin at the Sun, the evolution through the inner heliosphere and the effects on the inner heliosphere of the interplanetary counterparts of coronal mass ejections (ICMEs).
Forsyth, R. +38 more
core +1 more source
First Imaging of Coronal Mass Ejections in the Heliosphere Viewed from Outside the Sun Earth Line [PDF]
peer reviewedWe show for the first time images of solar coronal mass ejections (CMEs) viewed using the Heliospheric Imager (HI) instrument aboard the NASA STEREO spacecraft. The HI instruments are wide-angle imaging systems designed to detect CMEs in the
Moses, Daniel J +47 more
core +1 more source
JD 7: The Sun and the Heliosphere as an Integrated System [PDF]
AbstractWe summarize here the oral contributions given at the Joint Discussion (JD) 7The Sun and the Heliosphere as an Integrated System, held on July 17, 2003, in Sydney, as part of IAU XXV and give a list of posters presented at the JD.
Poletto, Giannina, Suess, Steven T.
openaire +2 more sources

