15: The Sun - A Garden-Variety Star Flashcards

1
Q

an area on the Sun where magnetic fields are concentrated - where sunspots, prominences, flares, and CMEs all tend to occur

A

active region

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2
Q

light radiated by atoms and ions in the ionosphere excited by charged particles from the Sun, mostly seen in the magnetic polar regions (northern and southern lights)

A

aurora

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3
Q

the part of the solar atmosphere that lies immediately above the photospheric layers

A

chromosphere

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4
Q

the outer (hot) atmosphere of the Sun

A

corona

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5
Q

a region in the Sun’s outer atmosphere that appears darker because there is less hot gas there

A

coronal hole

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6
Q

a solar flare in which immense quantities of coronal material (mainly protons and electrons) is ejected at high speeds (500–1000 kilometers per second) into interplanetary space

A

coronal mass ejection (CME)

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7
Q

the phenomenon that occurs when different parts of a rotating object rotate at different rates at different latitudes

A

differential rotation

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8
Q

the rice-grain-like structure of the solar photosphere - produced by upwelling currents of gas that are slightly hotter, and therefore brighter, than the surrounding regions, which are flowing downward into the Sun

A

granulation

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9
Q

a period during the seventeenth century when the number of sunspots seen throughout the solar cycle was unusually low

A

Maunder Minimum

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10
Q

the region of the solar (or stellar) atmosphere from which continuous radiation escapes into space - boundary where Sun becomes opaque and past which we cannot see

A

photosphere

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11
Q

a bright region of the solar surface observed in the light of some spectral line

A

plage

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12
Q

a hot ionized gas, with atoms stripped of electrons

A

plasma

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13
Q

a large, bright, gaseous feature that appears above the surface of the Sun and extends into the corona

A

prominence

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14
Q

a sudden and temporary outburst of electromagnetic radiation from an extended region of the Sun’s surface

A

solar flare

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15
Q

a flow of hot, charged particles leaving the Sun

A

solar wind

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16
Q

large, dark features seen on the surface of the Sun caused by increased magnetic activity

A

sunspot

17
Q

the semiregular 11-year period with which the frequency of sunspots fluctuates

A

sunspot cycle

18
Q

the region in the Sun’s atmosphere where the temperature rises very rapidly from the relatively low temperatures that characterize the chromosphere to the high temperatures of the corona

A

transition region

19
Q

the number of Earths that could fit the volume of the Sun

A

1.3 million Earths

20
Q

region above the Sun’s core that slowly transports light from the core through radiation

A

radiative zone

21
Q

outermost layer of solar interior that transports energy from radiative zone to the surface through convection cells

A

convection zone

22
Q

NASA space mission sent to investigate the transition region and why its sharp increase in temperature occurs

A

Interface Region Imaging Spectrograph (IRIS)

23
Q

inner, darker core of a sunspot

A

umbra

24
Q

lighter region of a sunspot that surrounds the umbra

A

penumbra

25
Q

period at which the number of observable sunspots is the greatest (occurs every 11 years on average) - more than 100 spots can be seen at once

A

sunspot maximum

26
Q

splitting of spectral lines in the presence of a magnetic field - used to measure solar magnetic field

A

Zeeman effect

27
Q

mechanism that converts kinetic energy into electricity - churning of plasma in Sun’s interior that generates its magnetic field

A

dynamo

28
Q

field of research predicting the effects of solar storms on Earth

A

space weather