{"id":432476,"date":"2026-05-19T23:05:00","date_gmt":"2026-05-19T13:05:00","guid":{"rendered":"https:\/\/science.nasa.gov\/get-involved\/citizen-science\/nasas-new-shock-detectives-project-invites-volunteers-to-help-study-solar-wind\/"},"modified":"2026-05-19T23:05:00","modified_gmt":"2026-05-19T13:05:00","slug":"nasas-new-shock-detectives-project-invites-volunteers-to-help-study-solar-wind","status":"publish","type":"post","link":"https:\/\/www.vibewire.com.au\/?p=432476","title":{"rendered":"NASA\u2019s New Shock Detectives Project Invites Volunteers to Help Study Solar Wind"},"content":{"rendered":"

The Sun sprays an extremely fast stream of charged particles called the solar wind. At approximately 56,000 miles (90,000 kilometers) in front of the Earth toward the Sun, the solar wind collides with the Earth\u2019s protective magnetic field, generating a long-lasting shock wave that stretches for hundreds of thousands of miles. Now, you can help scientists examine data about this \u201cbow shock<\/a>\u201d to better understand how the solar wind affects the Earth by joining a new research project: Shock Detectives.<\/p>\n

At this enormous shock wave boundary, the ever-changing magnetic field can either make the solar wind messy and dynamic (\u201cchaotic\u201d) or leave it smooth and stable (\u201cpeaceful\u201d).<\/p>\n

When \u201cchaotic\u201d plasma dominates, more energy can reach Earth\u2019s magnetosphere, possibly leading to disruptions in GPS signals, communications, and power grids. Scientists don\u2019t yet fully understand when the plasma changes between \u201cpeaceful\u201d and \u201cchaotic\u201d states or how those changes affect energy transfer to Earth.<\/p>\n

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