Question

question
drag the tiles to the correct boxes to complete the pairs.
match each solar dynamic activity with its characteristic.
tiles
solar flares solar prominences cmes solar wind
pairs
dense features of hot ionized gases ejected
into the chromosphere and the corona
visible as a sudden, rapid, intense variation
in the brightness of the sun
formed by a continuous flow of plasma of
charged particles
an enormous burst of solar wind threaded
with magnetic fields released from the sun
into space

Explanation:

• Solar prominences are dense features of hot ionized gases ejected into the chromosphere and the corona.
• Solar flares are visible as a sudden, rapid, intense variation in the brightness of the Sun.
• Solar wind is formed by a continuous flow of plasma of charged particles.
• Coronal mass ejections (CMEs) are an enormous burst of solar wind threaded with magnetic fields released from the Sun into space.

Answer:

dense features of hot ionized gases ejected into the chromosphere and the corona $
ightarrow$ solar prominences

visible as a sudden, rapid, intense variation in the brightness of the Sun $
ightarrow$ solar flares

formed by a continuous flow of plasma of charged particles $
ightarrow$ solar wind

An enormous burst of solar wind threaded with magnetic fields released from the Sun into space $
ightarrow$ CMEs