sunspots - ορισμός. Τι είναι το sunspots
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Τι (ποιος) είναι sunspots - ορισμός

TEMPORARY PHENOMENA ON THE PHOTOSPHERE OF THE SUN THAT APPEAR VISIBLY AS DARK SPOTS COMPARED TO SURROUNDING REGION
Sun/Sunspot; Sunspots; Sun spots; Sun spot; Sun Spots; Penumbra (Sun); Sunspot theory; Sunpot region; Sunspot group; Solar pore; Light bridge
  • Solar Observatory - Debrecen, Hungary
  • The emergence and evolution of a sunspot group over a period of two weeks
  • The full solar disk over the course of 13 days during the rise of [[solar cycle 24]]
  • access-date=5 January 2022}}</ref> Solar pores are also visible to the left of the penumbra.
  • alt=Photo of six-story building with fenced balcony containing large telescope

sunspots         
1. Notional cause of an odd error. "Why did the program suddenly turn the screen blue?" "Sunspots, I guess." 2. Also the cause of bit rot - from the myth that sunspots will increase cosmic rays, which can flip single bits in memory. See also phase of the moon. [Jargon File]
Sunspots (economics)         
ECONOMIC THEORY
Sunspot equilibrium; Sunspot (economics); Extrinsic random variable
In economics, the term sunspots (or sometimes "a sunspot") refers to an extrinsic random variable, that is, a random variable that does not affect economic fundamentals (such as endowments, preferences, or technology). Sunspots can also refer to the related concept of extrinsic uncertainty, that is, economic uncertainty that does not come from variation in economic fundamentals.
sunspot         
(sunspots)
Sunspots are dark cool patches that appear on the surface of the sun and last for about a week.
N-COUNT

Βικιπαίδεια

Sunspot

Sunspots are phenomena on the Sun's photosphere that appear as temporary spots that are darker than the surrounding areas. They are regions of reduced surface temperature caused by concentrations of magnetic flux that inhibit convection. Sunspots appear within active regions, usually in pairs of opposite magnetic polarity. Their number varies according to the approximately 11-year solar cycle.

Individual sunspots or groups of sunspots may last anywhere from a few days to a few months, but eventually decay. Sunspots expand and contract as they move across the surface of the Sun, with diameters ranging from 16 km (10 mi) to 160,000 km (100,000 mi). Larger sunspots can be visible from Earth without the aid of a telescope. They may travel at relative speeds, or proper motions, of a few hundred meters per second when they first emerge.

Indicating intense magnetic activity, sunspots accompany other active region phenomena such as coronal loops, prominences, and reconnection events. Most solar flares and coronal mass ejections originate in these magnetically active regions around visible sunspot groupings. Similar phenomena indirectly observed on stars other than the Sun are commonly called starspots, and both light and dark spots have been measured.

Παραδείγματα από το σώμα κειμένου για sunspots
1. For decades, scientists have tracked the solar cycle and appearance of sunspots, but they have been unable to accurately predict the intensity or timing of solar storms, which increase as the number of sunspots increases.
2. Who Would Have Thought?Sunspots and Creative Inspirations '4;· "Correlations for Number of Sunspots, Unemployment Rate, and Suicide Mortality in Japan" by Akiko Otsu, et al., Perceptual and Motor Skills, Vol. 102.
3. At periods of highest activity, called a solar maximum, sunspots appear.
4. Amplified response: Prediction errors are like sunspots, amplifying the response to an inflationary shock.
5. Every 11 years or so, the sun goes through an active period, with lots of sunspots.