Solar orbiter reveals plasma jets as potential source of Solar Wind
The ESA/NASA Solar Orbiter has uncovered a series of brief material jets emerging from the sun's outer layer, each lasting 20 to 100 seconds and expelling plasma at 100 km/s. These jets hold the potential to be the elusive source of the solar wind.
The solar wind, a stream of charged particles, continuously escapes the sun and interacts with celestial bodies. Upon colliding with Earth's magnetic field, it produces auroras.
Understanding the solar wind's origin near the sun has been a longstanding challenge. However, the Solar Orbiter's advanced instruments have made significant progress. Data from the spacecraft's Extreme Ultraviolet Imager (EUI) reveals faint, transient features at the sun's south pole associated with small plasma jets.
Lakshmi Pradeep Chitta from the Max Planck Institute notes that EUI's high-resolution images were crucial for detecting these jets. Notably, the extreme ultraviolet channel of EUI's imagery captured million-degree solar plasma at a 17.4-nanometer wavelength.
Analysis confirms that these features indeed result from plasma expulsion from the solar atmosphere.
Previous knowledge linked a portion of the solar wind to magnetic structures called coronal holes, where the sun's magnetic field extends outward. Plasma travels along these "open" magnetic lines, forming the solar wind. The origin of this plasma ejection remained unclear.
Traditionally, the assumption was that due to the corona's heat, it would naturally expand, causing some plasma to escape along the magnetic field lines. However, the Solar Orbiter's focus on a coronal hole challenges this idea. The discovered individual jets suggest that the solar wind's production might be more intermittent than previously thought.
Andrei Zhukov from the
Read more on tech.hindustantimes.com
