15: The Sun - A Garden-Variety Star Flashcards
an area on the Sun where magnetic fields are concentrated - where sunspots, prominences, flares, and CMEs all tend to occur
active region
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)
aurora
the part of the solar atmosphere that lies immediately above the photospheric layers
chromosphere
the outer (hot) atmosphere of the Sun
corona
a region in the Sun’s outer atmosphere that appears darker because there is less hot gas there
coronal hole
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
coronal mass ejection (CME)
the phenomenon that occurs when different parts of a rotating object rotate at different rates at different latitudes
differential rotation
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
granulation
a period during the seventeenth century when the number of sunspots seen throughout the solar cycle was unusually low
Maunder Minimum
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
photosphere
a bright region of the solar surface observed in the light of some spectral line
plage
a hot ionized gas, with atoms stripped of electrons
plasma
a large, bright, gaseous feature that appears above the surface of the Sun and extends into the corona
prominence
a sudden and temporary outburst of electromagnetic radiation from an extended region of the Sun’s surface
solar flare
a flow of hot, charged particles leaving the Sun
solar wind
large, dark features seen on the surface of the Sun caused by increased magnetic activity
sunspot
the semiregular 11-year period with which the frequency of sunspots fluctuates
sunspot cycle
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
transition region
the number of Earths that could fit the volume of the Sun
1.3 million Earths
region above the Sun’s core that slowly transports light from the core through radiation
radiative zone
outermost layer of solar interior that transports energy from radiative zone to the surface through convection cells
convection zone
NASA space mission sent to investigate the transition region and why its sharp increase in temperature occurs
Interface Region Imaging Spectrograph (IRIS)
inner, darker core of a sunspot
umbra
lighter region of a sunspot that surrounds the umbra
penumbra
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
sunspot maximum
splitting of spectral lines in the presence of a magnetic field - used to measure solar magnetic field
Zeeman effect
mechanism that converts kinetic energy into electricity - churning of plasma in Sun’s interior that generates its magnetic field
dynamo
field of research predicting the effects of solar storms on Earth
space weather