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1212** _ SO THE GOAL BECOMES HOW TO MAKE IMAGES WITH SMALL ANGULAR RESOLUTIONS._ **
1313
14- It seems that in astronomy, there is a relationship between the image resolution $\theta$ and the wavelength
15- $\lambda$ giving by $$ \theta = 1.22 \frac{\lambda} {D} $$
14+ It seems that in astronomy, there is a relationship between the image resolution $\theta$ and the wavelength $\lambda$ giving by
15+
16+ $$ \theta = 1.22 \frac{\lambda} {D} $$
17+
1618- Where $D$ is the diameter of the telescope.
1719- to get better resolution (small $\theta$), we need:
1820 - Large lenses ($D$)
Original file line number Diff line number Diff line change 1111
1212** _ SO THE GOAL BECOMES HOW TO MAKE IMAGES WITH SMALL ANGULAR RESOLUTIONS._ **
1313
14- It seems that in astronomy, there is a relationship between the image resolution $\theta$ and the wavelength
14+ It seems that in astronomy, there is a relationship between the image resolution $\theta$ and the wavelength $\lambda$ giving by
1515
16- $\lambda$ giving by $$ \theta = 1.22 \frac{\lambda} {D} $$
16+ $$ \theta = 1.22 \frac{\lambda} {D} $$
1717
1818- Where $D$ is the diameter of the telescope.
1919- to get better resolution (small $\theta$), we need:
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