ESC 1000 Earth Science           Name:__________________

Chapter 23 Part K: Key Terms

Fill in the blanks with the word(s) that best fit the description:

 

1. ___________________ – A continuous spectrum with dark lines superimposed.

 

2. ___________________ – A bright display of ever-changing light caused by solar radiation interacting with the upper atmosphere in the region of the poles.

 

3. ___________________– The bright lines produced by an incandescent gas under pressure.

 

4. ___________________– The property of a lens whereby light of different colors is focused at different places.

 

5. ___________________ – The first layer of the solar atmosphere found directly above the photosphere.

 

6. ___________________– An uninterrupted band of light emitted by an incandescent solid, liquid, or gas under pressure.

 

7. ___________________ – The outer, tenuous layer of the solar atmosphere.

 

8. ___________________– The apparent change in wavelength of radiation caused by relative motions of the source and the observer.

 

9. ___________________– The transfer of energy (heat) through space by electromagnetic waves.

 

10. ___________________ – A short-focal-length lens used to enlarge the image in a telescope. The lens that is nearest the eye.

 

11. ___________________– The distance from the lens to the point where it focuses parallel rays of light.

 

12. ___________________– The point where a lens or mirror causes light rays to converge.

 

13. ___________________ – The fine structure visible on the solar surface caused by the convection cells below.

 

14. ___________________– A type of nuclear reaction which consists of several small nuclei reacting to form a larger nucleus. This is the source of the sun’s energy.

 

15. ___________________– The collecting lens of a refracting telescope.

 

16. ___________________ – A discrete amount (quantum) if electromagnetic energy

 

17. ___________________– The region of the Sun that radiates energy to space. The visible surface of the sun.

 

18. ___________________   A concentration of material above the solar surface that appears as a bright archlike structure

 

19. ___________________– A chain of thermonuclear reactions by which nuclei of hydrogen are built up into nuclei of helium.

 

20. ___________________– The force exerted by electromagnetic radiation from an object such as the Sun.

 

21. ___________________– Two or more radio telescopes that combine their signals to achieve the resolving power of a larger telescope

 

22. ___________________– A telescope designed to make observations in radio wavelengths.

 

23. ___________________– A telescope that concentrates light from distant objects by using a concave mirror.

 

24. ___________________– A telescope that employs a lens to bend and concentrate the light from distant objects.

 

25. ___________________– A sudden and tremendous eruption in the solar chromosphere.

 

26. ___________________– Subatomic particles ejected at high speed from the solar corona.

 

27. ___________________ – A instrument for directly viewing the spectrum of light source.

 

28. ___________________   The study of spectra

 

29. ___________________ – A narrow jet of rising material in the solar chromosphere.

 

30. ___________________ – A dark spot on the Sun, which is cool by contrast to the surrounding photosphere.

 

Chapter 23 Light, Astronomical Observations, and the Sun Word List:

Aurora

Bright-line (emission) spectrum

Chromatic Aberration

Chromosphere

Continuous spectrum

Corona

Dark-line spectrum

         (absorption)

Doppler effect

Electromagnetic radiation

Eyepiece

Focal length

Focus

Granules

Nuclear fusion

Objective lens

Photon

Photosphere

Prominence

Proton-proton chain

Radiation pressure

 

Radio interferometer

Radio telescope

Reflecting telescope

Refracting telescope

Solar flare

Solar wind

Spectroscope

Spectroscopy

Spicule

Sunspot