Flares are our solar system's largest explosive events. They are seen as bright areas on the sun and they can last ...
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Sep 13, 2017 · Intrinsic to the reconnection picture of a solar eruptive event, ... Narukage & Shibata (2006) found a further six limb inflow events in ...
Aug 5, 2021 · Could solar storms knock out the global internet? ... how these happen and it has been impossible to predict when these events will occur.
Jan 31, 2020 · The NSF's new, cutting-edge solar observatory shows us the Sun as ... solar flare erupted from the Sun's surface in 2012: an event that was ...
The evolution of magnetic reconnection during a solar flare. Magnetic reconnection is a physical process occurring in highly conducting plasmas in which ... When the inflow density is comparable to the outflow density, ...
The convection is achieved and maintained by setting the entropy of the inflow of material at the bottom of the simulation box and solving the equations of ...
Dec 15, 2011 · The spatial size of a flare depends on individual events; in the smallest event the height of a flaring loop is less than 104 km, whereas it ...
May 16, 2017 · These events span a range of guide fields of 0 to 10 times the reconnecting magnetic field and inflow region plasma beta of 0.1 to 6.6.
The flare occurred on the northeast limb, displaying a nice cusp-shaped soft X-ray loop and a plasmoid ejection typical for the long-duration events. The EUV ...
In part I of this review, we have described in detail the ubiquitous and multi-scale observations of these magnetic structures in the solar wind and their ...