![]() |
Introduction to Solar Observing |
Course Overview | Course Syllabus | Course Schedule |
| Index of Course Sessions |
| Previous Page | The Sun: A Light of Many Colors: Index | Next Page |
Instruments for Spectral Studies
| An entrance slit in front of a light source allows light to filter through to a collimating lens, which forms the light into parallel rays. The rays are then refracted by the prism and focused by the camera lens. A ray of violet light is brought to focus; the ray is imaged as a line at the focal surface. Red light from the slit is also imaged but, because of its different refractive properties, it images at the other end of the focal surface. |
![]() Figure 22 One possible design for a spectrograph utilizing a prism. |
| The spectroscope design in Figure 23 below employs a slit in the barrier allows a narrow beam of light to pass. The beam passes through a prism and is split into its component colors. A lens then focuses the light into a sharp image that is either projected onto a screen, as shown here, or analyzed as it is passed through a detector. |
![]() Figure 23 Simple spectroscope using a prism. |
| Previous Page | The Sun: A Light of Many Colors: Index | Next Page |
| Page last updated 10/29/01 | Copyright © 2001 M.C.Gino |