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9-9.6 Sun Vocab

Terms

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Photosphere
region in the solar atmosphere from which most of the visible light escapes into space
Magnetic Dynamo (Babcock's theory)
explains phenomena of the solar cycle as a result of periodic winding and unwinding of the sun's magnetic field
Sunspot Minimum
the time during the solar cycle when the number of sunspots is minimum
Limb darkening
the phenomenon whereby the sun is darker near its limb than near the center of its disk
Sunspot Maximum
the time during the solar cycle when the number of sunspots is greatest
Filaments
dark curve seen above the sun's photosphere that is the top view of a solar prominence
Plage
bright spot on the sun believed to be associated with an emerging magnetic field
Differential Rotation
rotation of a nonrigid object in wich parts at different latitudes or different radial distances move at different speeds
Prominences
frame like protrusion seen near the limb of the sun and extending into the solar corona
Heliosphere
bubble in space containing the sun and planets created by the solar wind
Corona
sun's most outer atmosphere
Solar Cycle
22 year cycle during which the sun's magnetic field reverses its polarity twice
Supergranule
large convective cell in the sun's chromosphere containing man granule
Sunspots
temporary cool region in the solar photosphere created by protruding magnetic fields
Solar Flare
violent eruption on the sun's surface
Granule
lightly colored convection features about 1000 kilometers in diameter seen constantly in the solar photosphere
Maunder minimum
with a period of cold in europe so extreme that it was called the little ice age
Coronal Holes
dark region of the sun's inner corona as seen at X-ray wavelengths
Plasma
hot ionized gas
Chromosphere
ayer in the solar atmosphere between the photosphere and the corona
Tranisition Zone
region between the sun's chromosphere and corona where the temperature skyrockets to about 1 million K
Coronal Mass Ejections
large volumes of high energy gas release from the SUn' corona
Spicule
narrow jet of rising gas in the solar chromosphere
Solar Wind
outward flow of particles from the sun

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