Drag each item to the correct location.(1 point)

Question

Put responses in the correct input to answer the question. Select a response, navigate to the desired input and insert the response. Responses can be selected and inserted using the space bar, enter key, left mouse button or touchpad. Responses can also be moved by dragging with a mouse.
solar flare
sunspot
coronal mass ejection

Answer 1

It looks like you need to categorize the following items: solar flare, sunspot, and coronal mass ejection. However, since I don't have a visual interface to drag and drop items, I can help you categorize them based on typical classifications in solar phenomena:

1. Solar Flare: Short-term bursts of radiation resulting from the release of magnetic energy associated with sunspots.

2. Sunspot: Temporary phenomena on the Sun's photosphere that appear as spots darker than the surrounding areas due to their lower temperature.

3. Coronal Mass Ejection (CME): A significant release of plasma and magnetic field from the solar corona, often associated with solar flares and sunspots.

Would you like information on how to categorize them, or do you need help with something else?

Answer 2

What characteristic is shared by sunspots, solar flares, and coronal mass ejections? Select the two correct responses.(1 point)
Responses

They are caused by outward fluctuations of the sun's magnetic field.
They are caused by outward fluctuations of the sun's magnetic field.

They appear as dark spots on the sun's surface.
They appear as dark spots on the sun's surface.

They appear as bright spots on the sun's surface.
They appear as bright spots on the sun's surface.

They tend to occur during active periods of the solar cycle.

Answer 3

The two correct responses that describe a shared characteristic of sunspots, solar flares, and coronal mass ejections are:

1. They are caused by outward fluctuations of the sun's magnetic field.
2. They tend to occur during active periods of the solar cycle.

These responses indicate the connection between magnetic activity on the Sun and the manifestation of these phenomena during times of higher solar activity.