Scientific visualization · Physics · Catalog HVG8SDCD

Fast Magnetic Reconnection and the Hall Effect

NASA Scientific Visualization Studio — Tom Bridgman · 2022

Particle paths reveal how magnetic fields transfer their energy into motion.

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Exact rights statement: Public domain (United States)
Verification notes: NASA SVS work 4987 (2022), Fast Magnetic Reconnection and the Hall Effect. NASA SVS explicitly places its content in the public domain unless otherwise marked. Exact work page checked for copyright, licensed music, and third-party media exceptions; none identified for these raw visualizations. Media link targets an original raw visualization file, or its exact work page when a direct MP4 is not listed. Public-domain assessment is U.S.-based; preserve NASA credit and do not imply endorsement. Data/model collaborators in scientific credits do not constitute a separate media license.
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Scientific visualization · Physics · Catalog HVG8SDCD

Fast Magnetic Reconnection and the Hall Effect

NASA Scientific Visualization Studio — Tom Bridgman · 2022

Particle paths reveal how magnetic fields transfer their energy into motion.

Watch at the source

Open at the source ↗

External website. Its content and terms may change. Report a concern if the destination no longer matches this listing.

RIGHTS & PROVENANCE

U.S. public domain

Source documented

The record documents a United States public-domain basis. Rights can differ outside the United States.

View evidence and reuse notes

Exact rights statement: Public domain (United States)
Verification notes: NASA SVS work 4987 (2022), Fast Magnetic Reconnection and the Hall Effect. NASA SVS explicitly places its content in the public domain unless otherwise marked. Exact work page checked for copyright, licensed music, and third-party media exceptions; none identified for these raw visualizations. Media link targets an original raw visualization file, or its exact work page when a direct MP4 is not listed. Public-domain assessment is U.S.-based; preserve NASA credit and do not imply endorsement. Data/model collaborators in scientific credits do not constitute a separate media license.
Cover or thumbnail: NASA scientific visualization preview. Public domain under the source’s stated reuse terms; see the work credits.

Original source record ↗Source reuse policy ↗Cover or thumbnail source ↗Community & sharing principles

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Fast Magnetic Reconnection and the Hall Effect

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Solar Magnetic Field - from Solar Minimum to Solar Maximum

The Carruthers Geocorona Observatory at the Earth-Sun Lagrange Point 1

Magnetic Reconnection Throughout the Solar System

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Fast Magnetic Reconnection and the Hall Effect

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Solar Magnetic Field - from Solar Minimum to Solar Maximum

The Carruthers Geocorona Observatory at the Earth-Sun Lagrange Point 1

Magnetic Reconnection Throughout the Solar System

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