Angular magnification is the ratio of the signed viewing angle with an optical instrument to the signed viewing angle in a stated reference arrangement. Measure both as apparent directions from the eye, positive toward the same side of the optical axis; then an inverted view has negative . If only positive angular sizes are compared, the result is and carries no orientation information. [ref]
https://openstax.org/books/college-physics-2e/pages/26-5-telescopes. Urone and Hinrichs, College Physics 2e, §26.5: Telescope angular magnification and inversion
.For the upright virtual image of a converging thin lens, let the eye be at and take the unaided reference to be the same small object at a distance from the eye. Within the small-angle approximation,Specify : keeping the object in its original position means , whereas the customary magnifier rating uses a near-point reference, often . A reference distance is a convention, not a claim that every eye has that near point. [ref]
https://openstax.org/books/university-physics-volume-3/pages/2-7-the-simple-magnifier. Ling, Sanny and Moebs, University Physics Volume 3, §2.7: Angle ratio and viewing distances
.For the virtual image diagram, , and . With , , whereas keeping the object at gives . Thus neither viewing comparison gives the transverse magnification four. A person may also be unable to focus on the unaided object at the shorter reference distance.
At , each outgoing bundle is parallel with slope ; its apparent viewing direction has angle . Consequently remains finite even though is undefined at a finite image plane. Equivalently, in the limit , the factors and both grow without bound but their ratio tends to . For and , the relaxed-view prediction is . [ref]
https://openstax.org/books/university-physics-volume-3/pages/2-7-the-simple-magnifier. Ling, Sanny and Moebs, §2.7: Image at infinity
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