One line resonated through the space‑weather community this week: “Stealthy #solarstorms are back” wrote physicist Tamitha ...

The banana-size solar flares could lead to a better understanding of high-energy solar physics. When you purchase through links on our site, we may earn an affiliate commission. Here’s how it works.

The solar atmosphere is a turbulent and magnetized environment, with the release of magnetic energy readily manifesting as ...

Coronal loops, well-defined hot strands of plasma that arch out into the sun’s atmosphere, are iconic to the sun’s imagery. But many of the supposed coronal loops we see might not be there at all.

The highest-resolution images of a solar flare captured at the H-alpha wavelength (656.28 nm) ever captured may reshape how we understand the sun's magnetic architecture—and improve space weather ...

(MENAFN- IANS) New Delhi, Feb 18 (IANS) Astronomers from the Indian Institute of Astrophysics (IIA), an autonomous institute of the Department of Science and Technology, have accurately estimated the ...

We present the results of a detailed numerical simulation of the circumstellar environment around three exoplanet-hosting stars. A state-of-the-art global magnetohydrodynamic (MHD) model is considered ...

A solar researcher has spotted a hitherto-unreported feature of the Sun's atmosphere, giving us an insight into the star's magnetic structure. [partner id="wireduk ...

Many coronal loops -- ropey strands of plasma that scientists have long thought existed in the sun's atmosphere -- may actually be optical illusions, according to a new paper that challenges ...

A METHOD of determining the large scale structure of the coronal and interplanetary magnetic fields has recently been described 1. The model originated as an attempt to explain the observed large ...