"The Science of EST" ep.5: Cool solar ejections of the size of the Earth

Surges are solar ejections that can be as large as the Earth - or even bigger- and relatively cool (in solar standards), which makes them a very interesting topic to study. With the European Solar Telescope we will able to capture the elusive details of the physical processes that lead to surges.

Daniel Nóbrega Siverio, postdoc at Rosseland Centre for Solar Physics, UiO. Image: UiO

Surges are solar ejections with typical sizes of tens of thousands of kilometers. This implies they are as large as the Earth’s size or even bigger! They are composed of cool plasma; but for solar standards, cool means a few thousands degrees: way enough to melt steel! Moreover, surges are ubiquitous and usually appear in close relation to other eruptive phenomena that also perturb the atmosphere of our closest star. This makes surges a really interesting topic to study.

In spite of their huge size, a full understanding of those ejections implies observing the smallest scales in order to unravel them, so how can we achieve this if the Sun is at about 150 million kilometers from the Earth? The answer is the European Solar Telescope: the most ambitious next generation solar telescope. This 4-metre telescope will be the largest one in Europe and specializes in high spatial, spectral and temporal resolution, together with extremely high magnetic field sensitivity. Thanks to the capabilities of the EST, we will able to capture the elusive details of the physical processes that lead to surges, thus providing unprecedented quality data to analyze and compare with the state-of-the-art numerical simulations that are carried out in large supercomputing facilities. This will provide a unique joint perspective between observations and theory, helping us to solve the pieces of the solar atmosphere puzzle.

earth planet, solar surges
Temperature map of a numerical simulation showing a surge. Credits: Nóbrega-Siverio et al. (2018).

The image shows a temperature map of a numerical simulation. Moreover, it shows a surge, the cool elongated vertical structure that resembles a fang, located to the right of a dome-shaped structure composed of plasma that has emerged from the solar interior. We have added an image of the Earth to put into context the huge scale of this phenomenon (note that 1 Mm = 1000 km). 


The science of EST” is a series of short posts for social media where researchers talk in a plain language about a particular topic of their choice and how EST will improve our knowledge on that topic. The aim is to raise awareness among the general public about why solar physicists study the Sun, what the hot topics in today’s solar physics are, and how EST will leap forward our knowledge of the Sun. 

 

All the posts can be found in "The Science of EST" (ext. link).

By Daniel Nóbrega Siverio
Published Mar. 16, 2020 11:54 AM - Last modified Mar. 30, 2020 5:53 PM