Author Topic: Particles Shot Out of The Sun Reveal Distinct Patterns, Scientists Find  (Read 48 times)

0 Members and 1 Guest are viewing this topic.

Offline Buster's Uncle

  • Geo's kind, I unwind, HE'S the
  • Planetary Overmind
  • *
  • Posts: 53545
  • €517
  • View Inventory
  • Send /Gift
  • Because there are times when people just need a cute puppy  Soft kitty, warm kitty, little ball of fur  A WONDERFUL concept, Unity - & a 1-way trip that cost 400 trillion & 40 yrs.  
  • AC2 is my instrument, my heart, as I play my song.
  • Planet tales writer Smilie Artist Custom Faction Modder AC2 Wiki contributor Downloads Contributor
    • View Profile
    • My Custom Factions
    • Awards
Particles Shot Out of The Sun Reveal Distinct Patterns, Scientists Find
Russell McLendon
ScienceAlert
Fri, September 12, 2025 at 6:00 PM EDT
3 min read



Study Traces High-Speed Electrons Back to 2 Types of Solar Eruptions


Our sun can seem deceptively peaceful from Earth, but only because we have the luxury of living 150 million kilometers away. Up close, it's a nuclear-fuelled carnival ride of terror, launching countless tiny particles at speed far into interplanetary space.

"The Sun is the most energetic particle accelerator in the Solar System," writes a team of researchers behind a study on the energetic particles that stream forth in solar flares and coronal mass ejections (CMEs).

According to the study's lead author Alexander Warmuth, each of those events delivers streams of particles with very distinct features hinting at a different birthplace and backstory.

"We see a clear split between 'impulsive' particle events, where these energetic electrons speed off the Sun's surface in bursts via solar flares, and 'gradual' ones associated with more extended CMEs," says Warmuth, a heliophysicist at the Leibniz Institute for Astrophysics Potsdam (AIP) in Germany.

The latter, more gradual events "release a broader swell of particles over longer periods of time and over broader angular ranges," Warmuth adds.



An illustration of Solar Orbiter measuring different types of solar energetic electrons. (ESA & NASA/Solar Orbiter/STIX & EPD)


Using data from the European Space Agency-led Solar Orbiter, which gets as close as 42 million kilometers to the Sun, Warmuth and his team measured those particles on location, focusing on a type known as solar energetic electrons (SEEs).

A dichotomy of SEEs was already well established, but Solar Orbiter provided a wealth of data from an unprecedented proximity that revealed new details about where exactly each type of SEE came from.

"We were only able to identify and understand these two groups by observing hundreds of events at different distances from the Sun with multiple instruments – something only Solar Orbiter can do," Warmuth says.

"By going so close to our star, we were able to measure the particles in a pristine state and could thus accurately determine the time and place where they started at the Sun," he adds.

The study is based on observations of more than 300 SEE events between 2020 and 2022, representing the most exhaustive such analysis so far.

"It's the first time we've clearly seen this connection between particles in space and their source events taking place at the Sun," says co-author Frederic Schuller, also of AIP.

"We measured the energetic electrons in situ – that is, Solar Orbiter actually flew through the electron streams – while simultaneously using more of the spacecraft's instruments to observe what was happening at the Sun."

The probe's eccentric orbit offered data on events at different distances from the Sun, yielding new insight about how these electrons behave on their travels. That includes a potential explanation for confusing lags between visual signs of solar flares and radio bursts, and the subsequent release of SEEs into space.



An immense M7-class solar flare captured by NASA's Solar Dynamics Observatory on 19 July 2012. (NASA/Royal Observatory Belgium/SIDC)


"It turns out this is related to how the electrons travel through space – it's not a lag in release, but a lag in detection," says co-author and heliophysicist Laura Rodríguez-García.

"The electrons encounter turbulence, get scattered in different directions, and so on, so we don't spot them immediately," she adds. "These effects build up as you move further from the Sun."

The probe was meant to produce insights like these, the authors note, and it should continue to illuminate solar secrets for years to come.

"Thanks to Solar Orbiter, we're getting to know our star better than ever," says Daniel Müller, ESA project scientist for Solar Orbiter.

That kind of familiarity is valuable for many reasons, including its potential for helping us protect spacecraft and their crews.

"Knowledge such as this from Solar Orbiter will help protect other spacecraft in the future, by letting us better understand the energetic particles from the Sun that threaten our astronauts and satellites," he says.

The study was published in Astronomy & Astrophysics.

https://www.yahoo.com/news/articles/particles-shot-sun-reveal-distinct-220057164.html

 

* User

Welcome, Guest. Please login or register.
Did you miss your activation email?


Login with username, password and session length

Select language:

* Community poll

SMAC v.4 SMAX v.2 (or previous versions)
-=-
24 (7%)
XP Compatibility patch
-=-
9 (2%)
Gog version for Windows
-=-
106 (33%)
Scient (unofficial) patch
-=-
40 (12%)
Kyrub's latest patch
-=-
14 (4%)
Yitzi's latest patch
-=-
89 (28%)
AC for Mac
-=-
3 (0%)
AC for Linux
-=-
5 (1%)
Gog version for Mac
-=-
10 (3%)
No patch
-=-
16 (5%)
Total Members Voted: 316
AC2 Wiki Logo
-click pic for wik-

* Random quote

Information, the first principle of warfare, must form the foundation of all your efforts. Know, of course, thine enemy. But in knowing him do not forget above all to know thyself. The commander who embraces this totality of battle shall win even with inferior force.
~Spartan Battle Manual

* Select your theme

*
Templates: 5: index (default), PortaMx/Mainindex (default), PortaMx/Frames (default), Display (default), GenericControls (default).
Sub templates: 8: init, html_above, body_above, portamx_above, main, portamx_below, body_below, html_below.
Language files: 4: index+Modifications.english (default), TopicRating/.english (default), PortaMx/PortaMx.english (default), OharaYTEmbed.english (default).
Style sheets: 0: .
Files included: 45 - 1228KB. (show)
Queries used: 36.

[Show Queries]