magnetic reconnection tagged posts

For around half a century, scientists have been puzzled by the odd spectral lines produced by solar flares. Now we may have some answers.
Anew study looking at solar flares may have solved a 50-year-old mystery about our host star, finding that solar flares may be far hotter than we realized.

Solar flares are a common event on the Sun’s surface. They can be seen regularly throughout the year, and particularly during the solar maximum phase of the Sun’s cycle.

“A solar flare is an intense burst of radiation coming from the release of magnetic energy associated with sunspots. Flares are our solar system’s largest explosive events. They are seen as bright areas on the Sun and they can last from minutes to hours,” NASA explains...

New research from the University of St Andrews has proposed that particles in solar flares are 6.5 times hotter than previously thought. The research provides an unexpected solution to a 50-year-old mystery about our nearest star.

Solar flares are sudden and huge releases of energy in the sun’s outer atmosphere that heat parts of it to greater than 10 million degrees. These dramatic events greatly increase the solar X-rays and radiation reaching Earth and are hazardous to spacecraft and astronauts, as well as affecting our planet’s upper atmosphere.

The research, published in The Astrophysical Journal Letters, looks at evidence of how flares heat solar plasma to greater than 10 million degrees. This solar plasma is made up of ions and electrons...

Release of magnetic energy near the sun’s surface enables the solar wind to reach gravity-defying speeds. In a paper published June 7, 2023 in the journal Nature, a team of researchers used data from NASA’s Parker Solar Probe to explain how the solar wind is capable of surpassing speeds of 1 million miles per hour. They discovered that the energy released from the magnetic field near the sun’s surface is powerful enough to drive the fast solar wind, which is made up of ionized particles — called plasma — that flow outward from the sun.

James Drake, a Distinguished University Professor in the University of Maryland’s Department of Physics and Institute for Physical Science and Technology (IPST), co-led this research alongside firs...

NASA’s Parker Solar Probe (PSP) has flown close enough to the sun to detect the fine structure of the solar wind close to where it is generated at the sun’s surface, revealing details that are lost as the wind exits the corona as a uniform blast of charged particles.

It’s like seeing jets of water emanating from a showerhead through the blast of water hitting you in the face.

In a paper to be published in the journal Nature, a team of scientists led by Stuart D...