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 .

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.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 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 .