Jove
Visualize
Contact Us

Related Concept Videos

Adjusting a Traverse01:12

Adjusting a Traverse

In the site survey of a four-sided traverse, internal angles are essential to ensure geometric accuracy. The survey revealed that the sum of the measured internal angles was 359 degrees and 48 minutes, which is 12 minutes less than the expected 360 degrees. This discrepancy signals an error likely arising from measurement inaccuracies during the fieldwork.To rectify this error, the adjustment process involved distributing the 12-minute shortfall equally across the four internal angles. By...
Common Leveling Mistakes and Errors01:17

Common Leveling Mistakes and Errors

A survey team is tasked with determining the elevation difference between points Point A and Point B, separated by uneven terrain. They use a leveling instrument and a leveling rod.Common MistakesMisreading the Rod: During a backsight reading at Point A, the instrumentman observes the rod partially obscured by tall grass. Instead of reading 1.135 m, they mistakenly record 1.735 m due to the misalignment of the crosshair with the wrong graduation. This error adds 0.600 m to all subsequent...
NMR Spectrometers: Resolution and Error Correction01:14

NMR Spectrometers: Resolution and Error Correction

When magnetic nuclei in a sample achieve resonance and undergo relaxation, the signal detected in NMR is an approximately exponential free induction decay. Fourier transform of an exponential decay yields a Lorentzian peak in the frequency domain. Lorentzian peaks in an NMR spectrum are defined by their amplitude, full width at half maximum, and position, where the peak width is governed by the spin-spin relaxation time alone. In real experiments, however, the applied magnetic field is rendered...
Focusing of Light in the Eye01:16

Focusing of Light in the Eye

Light rays enter the eye through the cornea, a transparent dome-shaped tissue that is the eye's outermost layer. The cornea bends or refracts, light rays traveling to the pupil. The shape of the cornea determines how much of the light is bent and whether the image will be focused correctly on the retina at the back of the eye. Once the light has passed through both refraction layers, it converges into a single focal point onto a small area. This is where photoreceptors start transforming...
Influence of Earth's Curvature and Atmospheric Refraction on Leveling01:26

Influence of Earth's Curvature and Atmospheric Refraction on Leveling

During leveling, the Earth's curvature and atmospheric refraction introduce deviations in the line of sight from a true horizontal reference. When the line of sight is leveled, it remains perpendicular to the plumb line only at a single point. Beyond this, it deviates due to the Earth’s curvature, represented by the correction C. For a sight distance D, the deviation can be derived using the relationship:This relationship shows that the deviation increases quadratically with distance. Over a...

You might also read

Related Articles

Articles linked to this work by shared authors, journal, and citation graph.

Sort by
Same author

Endothelial cytochrome P450 -derived cholesterol limits angiogenesis.

Redox biology·2026
Same author

GM-CSF downregulates type I IFN responses in glioblastoma-associated monocytes.

Experimental & molecular medicine·2026
Same author

Enhanced IGFL1 translation in response to IL-1β is controlled by distinct 3'UTR elements.

PloS one·2026
Same author

Pupil aberration coefficients in plane-symmetric optical systems.

Journal of the Optical Society of America. A, Optics, image science, and vision·2026
Same author

Single-step alignment of a two-mirror telescope using sigma vectors in nodal aberration theory.

Applied optics·2026
Same author

Two-level optimizer for large-scale metasurfaces with strong near-field coupling.

Optics express·2026
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Related Experiment Video

Updated: Jun 12, 2026

Bringing the Visible Universe into Focus with Robo-AO
10:35

Bringing the Visible Universe into Focus with Robo-AO

Published on: February 12, 2013

Misalignment-induced nodal aberration fields in two-mirror astronomical telescopes.

Tobias Schmid1, Kevin P Thompson, Jannick P Rolland

  • 1CREOL, The College of Optics and Photonics, University of Central Florida, 4000 Central Florida Boulevard, Orlando, Florida 32816, USA. tschmid@creol.ucf.edu

Applied Optics
|June 3, 2010
PubMed
Summary

Misaligned two-mirror telescopes may still have significant aberrations even with on-axis correction. Proper alignment is crucial to avoid image degradation, especially for Ritchey-Chrétien designs, due to astigmatism with binodal field dependence.

More Related Videos

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
12:14

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry

Published on: August 12, 2013

Assembly, Tuning and Use of an Apertureless Near Field Infrared Microscope for Protein Imaging
12:27

Assembly, Tuning and Use of an Apertureless Near Field Infrared Microscope for Protein Imaging

Published on: November 25, 2009

Related Experiment Videos

Last Updated: Jun 12, 2026

Bringing the Visible Universe into Focus with Robo-AO
10:35

Bringing the Visible Universe into Focus with Robo-AO

Published on: February 12, 2013

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
12:14

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry

Published on: August 12, 2013

Assembly, Tuning and Use of an Apertureless Near Field Infrared Microscope for Protein Imaging
12:27

Assembly, Tuning and Use of an Apertureless Near Field Infrared Microscope for Protein Imaging

Published on: November 25, 2009

Area of Science:

  • Optics
  • Astronomy
  • Telescope Engineering

Background:

  • Nodal aberration theory offers a general framework for analyzing telescope performance.
  • Misalignments in optical systems can degrade image quality, particularly in complex designs.
  • Traditional methods for assessing telescope alignment may be insufficient.

Purpose of the Study:

  • To investigate the impact of misalignments on third-order aberrations in two-mirror telescopes.
  • To demonstrate the utility of nodal aberration theory for analyzing misaligned telescopes.
  • To highlight the inadequacy of on-axis correction as a sole criterion for telescope alignment.

Main Methods:

  • Application of nodal aberration theory to two-mirror telescope designs.
  • Analysis of field dependence of third-order aberration fields.
  • Simulation and theoretical evaluation of misalignment effects.

Main Results:

  • On-axis performance does not guarantee a fully aligned telescope.
  • Aligning Ritchey-Chrétien telescopes solely for zero on-axis coma leaves significant misalignments.
  • Astigmatism with binodal field dependence causes image degradation, particularly off-axis.

Conclusions:

  • Nodal aberration theory provides a comprehensive approach to understanding telescope aberrations.
  • Solely correcting for on-axis coma is insufficient for optimal alignment of two-mirror telescopes.
  • Careful alignment is essential to mitigate image quality issues caused by residual aberrations.