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The representation of magnetic fields by magnetic field lines is very useful in visualizing the strength and direction of the magnetic field. Each of the magnetic field lines forms a closed loop. The field lines emerge from the north pole (N), loop around to the south pole (S), and continue through the bar magnet back to the north pole.
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Related Experiment Video

Updated: Jun 6, 2026

Recording Ultra-Realistic Full-Color Analog Holograms for Use in a Moving Hologram Display
09:04

Recording Ultra-Realistic Full-Color Analog Holograms for Use in a Moving Hologram Display

Published on: January 14, 2020

Holographic stars.

E Simova, M Kavehrad

    Applied Optics
    |November 10, 2010
    PubMed
    Summary

    Holographic stars were fabricated using DuPont film and a laser. This method reduces required gratings and allows wavelength tuning by adjusting Bragg angles.

    Area of Science:

    • Optics and Photonics
    • Holography
    • Diffraction Gratings

    Background:

    • Holographic optical elements are crucial for various applications.
    • Fabricating complex holographic structures efficiently remains a challenge.

    Purpose of the Study:

    • To demonstrate holographic stars fabricated on DuPont HRF 600X010 film.
    • To explore a method reducing multiplexed gratings using Bragg degeneracy.
    • To show wavelength tunability of the holographic stars.

    Main Methods:

    • Fabrication of holographic stars using a He-Ne laser on DuPont holographic recording film HRF 600X010.
    • Utilizing plane waves and transmitted portions of input beams for output.
    • Employing multiple exposures based on the Bragg degeneracy effect.

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    Digital Inline Holographic Microscopy (DIHM) of Weakly-scattering Subjects

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    Last Updated: Jun 6, 2026

    Recording Ultra-Realistic Full-Color Analog Holograms for Use in a Moving Hologram Display
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    Published on: January 14, 2020

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    Digital Inline Holographic Microscopy (DIHM) of Weakly-scattering Subjects

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  • Arranging replay beams in a three-dimensional configuration.
  • Main Results:

    • Successful demonstration of holographic stars operating in the volume diffraction regime.
    • Significant reduction in the number of required multiplexed gratings.
    • Demonstrated wavelength tunability by readjusting Bragg angles.

    Conclusions:

    • The demonstrated holographic stars offer an efficient method for optical beam manipulation.
    • The use of Bragg degeneracy simplifies the fabrication of complex holographic structures.
    • The tunable nature of these stars enhances their versatility for different wavelength applications.