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solar wind

Artist’s impression of China’s Tianwen-1 spacecraft en route to Mars.
Posted inEditors' Highlights

First Solar Wind Plasma Observations from the Tianwen-1 Mission

by Limei Yan 6 May 20227 September 2022

Solar wind plasma data captured by the Tianwen-1 probe while in transit to Mars represent an important step toward a new era of cooperative Martian space exploration.

Artist rendering of magnetic reconnection taking place in the Earth's magnetosphere
Posted inEditors' Vox

Hidden Atmospheric Particles Sculpt Near-Earth Space Environment

by S. Toledo, M. André, N. Aunai, C.R. Chappell, J. Dargent, S.A. Fuselier, A. Glocer, D.B. Graham, S. Haaland, M. Hesse, L.M. Kistler, B. Lavraud, W. Li, T. E. Moore, P. Tenfjord and S.K. Vines 22 September 202118 July 2023

Charged particles escape our atmosphere following Earth’s magnetic field and constitute a main source of matter that modulates Sun-Earth interactions.

Illustration showing the dayside magnetosphere and its surroundings
Posted inEditors' Vox

New Results Concerning Solar Wind Entry into the Magnetosphere

by D. G. Sibeck, Q. Zong, P. Escoubet, G. Le and H. Zhang 28 October 202018 July 2023

A new book describes recent results defining the many pathways and foreshock, bow shock, magnetosheath, and magnetopause phenomena connecting the solar wind to the dayside magnetosphere.

Posted inEditors' Highlights

Solar Properties Rival for Control of Mars’s Bow Shock

by Michael W. Liemohn 9 July 20194 May 2022

While most planetary bow shocks are controlled by the solar wind, at Mars the solar EUV flux is equally important.

Annotated graphic of a solar wind discontinuity
Posted inResearch Spotlights

Understanding the Turbulent Nature of the Solar Wind

by Mark Zastrow 13 June 20194 May 2022

Sometimes the conditions in the solar wind can change dramatically over short distances. Satellite observations of these features show that they’re more complex than previously thought.

Jack Gosling at the Laboratory for Atmospheric and Space Physics, Space Sciences Building, at the University of Colorado Boulder
Posted inNews

John T. “Jack” Gosling (1938–2018)

by D. N. Baker, B. Feldman, D. McComas, S. Schwartz and M. Thomsen 26 September 20184 May 2022

This prolific researcher helped us understand the interactions of the solar wind and coronal mass ejections with Earth’s magnetic field.

Researchers assess how space storms impact satellites in geosynchronous orbit
Posted inResearch Spotlights

How Space Storms Affect the Satellite Superhighway

by E. Underwood 30 April 201813 April 2022

A powerful numerical model reveals how space weather disturbs magnetic field at geosynchronous orbit.

Posted inEditors' Highlights

Evidence That Earth’s Forehead Controls the Wagging of its Tail

by Michael W. Liemohn 23 March 201818 July 2023

Yes, Earth has a tail, a magnetotail, and there is debate about how much Earth’s upper atmosphere plays a role in the controlling the dynamics of this region of space.

Posted inEditors' Highlights

Fast CMEs Continue to Decelerate in the Outer Heliosphere

by Y. Wang 12 February 201831 May 2022

Most fast coronal mass ejections will be decelerated into ambient solar wind quickly in the inner heliosphere, but some of them continue the deceleration with an even larger amplitude beyond 1 AU.

Posted inEditors' Highlights

Where the Solar Wind Meets Mars

by Michael W. Liemohn 12 January 201812 October 2022

A comprehensive look at how the solar wind is diverted around Mars, including the relative strength of the three biggest forces at work in this region.

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