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Astronomy II

Astronomy

QuestionAnswer
solar activity and the earth an 11-year cycle
sunspots the most obious sign of solar activity
umbra a very dark central region ( from the Latin word for "shadow")
penumbra surrounds umbra, which is not dark.
magnetic lines of force (magnetic field lines) directions mapping out the direction of the force between magnetic poles; the packing of the lines shows the strength of the force.
Zeeman effect the scientific process by which the splitting is made
differential rotation different latitudes on the Sun rotate at different angular speeds
the strongest magnetic fields in the sun occur where? sunspots
the parts of the corona above sunspots are hotter and denser than the normal corona.
Sunspots were discovered by whom ? Galileo, Fabricus and Christopher Scheiner, adn Thomas Harriot.
sunspot cycle the variation (individual cycles can be as short as 8 years or as long as 12 years.
butterfly diagram as a solar cycle advances year by year, sunspots appear closer to the equator.
solar flares tremendous eruptions that eject particles and emit radiation from all parts of the spectrum into space.
aurora borealis "the northern lights"
aurora australis "the southern lights"
plages bright areas surround the entire sunspot region.
prominences filaments on the limb of the sun, often in beautiful shapes.
active regions the regions around sunspots that show many kinds of solar activity.
Maunder minimum the sunspot cycle that may not have been operating for that 70 yr period
solar wind phenomenon the expansion that causes the comet tails always to poing away from the Sun
the solar constant amount of energy per second hitting each square meter of the Earth as its average distance from the Sun if the Earth had no atmosphere. 99% of solar energy ranges from 2760 A to 49,000 A (nearly 5 microns) and 99.9% is between 217 A and 10.94 microns.
Are there always sunspots on the Sun? No, at solar minimum there may be weeks without sunspots.
Are ther red spots on the edge of the Sun flares? No, often they are prominences, which are cooler than flares.
solar wind flows how? from coronal holes.
Created by: Msmlb_93
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