There is a reason some mass chase solar eclipses around the humans : this is unquestionably not a phenomenon where if you ’ve seen one , you ’ve go through them all . alternatively , each solar eclipse is different , and the April 8 North American total solar eclipse will likely come with a few supererogatory feature , including an abundance of red , pink , and possibly white pennant and closed circuit .

The upcoming solar eclipse will belonger than mostand will hap when several major planet , andmaybe even a comet , are in the sky , tot up to the show at totality . However , perhaps the most classifiable feature film of this eclipse is that it is happening so near to solar maximum , when the chances of flares and coronal mass ejections ( CMEs ) are highest .

Solar storm are knockout to forebode , sure as shooting more than a calendar week in advance , so we do n’t yet recognise if there will be activity while the Sun is blocked by the Moon , offer us a chance to see its corona . However , we know that , statistically , the fortune are much higher now than during the last total solar eclipse in the US in 2017 , when solar activity was on the decline from a peak much small than this one .

Solar prominences seen during the last total eclipse of the last millennium, as seen from France.

Red prominences from Chile during the 2019 total eclipse. The prominences can only be seen during eclipses or using hydrogen alpha filters, which hide the red color.Image credit: ESA/CESAR

Solar maximum is a product of the 22 - class cycle of the Sun ’s magnetized field , during which two peak occur around 11 years apart . decent now , that magnetic field of operations is tangled , producingsunspots , flares , and the CMEs that causeauroras .

Even when solar activity is at a lower limit , prominence can be get word around the edge of the Sun , either using atomic number 1 alpha filters or when the Moon parry most of the Sun ’s light source . This clip , however , they should be much longer and more abundant , looking like streamers point away from the Sun , often appearing red and pinkish . If a flare time itself well , you may see it lift off the Sun . CMEs are rarer , but can be visible for much longer ; if any come about before the eclipse , they could still be seen .

The 2023 solar eclipse that tinge the coast of Australia included afine display of bulge . The Sun was less active at that point than it is today , and the occultation was also a great raft shorter .

A solar prominence in 2010 compared to the size of the Earth

A solar prominence in 2010 compared to the size of the Earth.Image credit: NASA Solar Dynamics Observatory

Prominences are unremarkably longer than the diam of the Earth , and some have been as long as the width of the Sun . Most often one end is tethered to the Sun , make a streamer gist , but sometimes occurs as an arch , often with both endsanchored to sunspot region .

Although there is some uncertainty about their causes , swelling are composed of hydrogen and helium like the Sun itself , and are hold up against sombreness by magnetic bailiwick . Rarer coronal loops can resemble an arched excrescence in shape , but are much hot .

Prominences emit light in the red part of the spectrum as a result of thehydrogen alpha passage . However , fuse with white light from ordinary thermal emissions , it can give rise a pink effect .

The diamond ring seen during the 2017 eclipse from Oregan State Fair Grounds

The diamond ring seen during the 2017 eclipse from Oregon State Fair Grounds.Image credit: Dominic Hart/NASA

All of these are separate from the steady occultation phenomena of theDiamond Ring effect , triggered by a lean slither of unblocked Sun , andBaily ’s Beads , visible when valleys between lunar mountains reserve pockets of sunlight to pelt through .