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Related Concept Videos

Potential Due to a Magnetized Object01:24

Potential Due to a Magnetized Object

Magnetic dipoles in magnetic materials are aligned when placed under an external magnetic field. For paramagnets and ferromagnets, dipole alignment occurs in the direction of the magnetic field. However, the dipoles align opposite to the field in the case of diamagnets. This state of magnetic polarization due to the external field is called magnetization. Magnetization is defined as the dipole moment per unit volume. It plays a similar role to polarization in electrostatics.
The vector...
Magnetic Field of a Solenoid01:18

Magnetic Field of a Solenoid

A solenoid is a conducting wire coated with an insulating material, wound tightly in the form of a helical coil. The magnetic field due to a solenoid is the vector sum of the magnetic fields due to its individual turns. Therefore, for an ideal solenoid, the magnetic field within the solenoid is directly proportional to the number of turns per unit length and the current. Conversely, the magnetic field outside the solenoid is zero.
Consider a solenoid with 100 turns wrapped around a cylinder of...
Diamagnetism01:26

Diamagnetism

Materials consisting of paired electrons have zero net magnetic moments. However, when these materials are placed under an external magnetic field, the moments opposite to the field are induced. Such materials are called diamagnets. Diamagnetism is the response of the diamagnets when placed in an external magnetic field.
Diamagnetism was discovered by Anton Brugmans in 1778 when he observed that bismuth gets repelled by magnetic fields, thus theorizing that diamagnets get repelled by magnets.
Magnetic Vector Potential01:15

Magnetic Vector Potential

In electrostatics, the electric field can be written as the negative gradient of the potential. In magnetostatics, the zero divergence of the magnetic field ensures that the magnetic field can be expressed as the curl of a vector potential. This potential is known as the magnetic vector potential.
Consider an ideal solenoid with n turns per unit length and radius R. If I is the current through the solenoid, the magnetic field inside the solenoid is expressed as the product of vacuum...
Magnetic Flux01:18

Magnetic Flux

The magnetic flux measures the number of magnetic field lines passing through a given surface area. The SI unit for magnetic flux is the weber (Wb). Magnetic flux is a scalar quantity. It depends on three factors: the strength of the magnetic field B, the area through which the field lines pass, and the relative orientation of the field with the surface area.
Suppose a surface is divided into elements of area dA. For each element, the component of the magnetic field that is normal to the...
Magnetic Declination01:19

Magnetic Declination

Magnetic declination is the angle between true north, which aligns with the Earth's rotational axis, and magnetic north, which follows the direction of the Earth's magnetic field. This discrepancy exists because the magnetic poles do not coincide with the geographic poles. The value of magnetic declination depends on the observer's location on Earth and is subject to changes over time due to the dynamic nature of the Earth's magnetic field.The declination is called eastern when magnetic north...

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Related Experiment Video

Updated: Jun 16, 2026

Demonstration of Spin-Multiplexed and Direction-Multiplexed All-Dielectric Visible Metaholograms
08:48

Demonstration of Spin-Multiplexed and Direction-Multiplexed All-Dielectric Visible Metaholograms

Published on: September 25, 2020

Solar magnetograph employing integrated diode arrays.

W C Livingston, J Harvey, C Slaughter

    Applied Optics
    |February 16, 2010
    PubMed
    Summary

    This study details a solar magnetograph using diode arrays, detecting faint photospheric magnetic fields. The detector shows promise for low-light astronomical observations.

    Area of Science:

    • Solar Physics and Astrophysics
    • Instrumentation and Detector Technology

    Background:

    • Solar magnetographs are crucial for studying the Sun's magnetic field.
    • Accurate detection of weak photospheric magnetic fields requires sensitive instruments.

    Purpose of the Study:

    • To describe a novel solar magnetograph system.
    • To evaluate the performance of integrated diode arrays as detectors for solar magnetic field measurements.
    • To assess the detector's suitability for low-light level sensing.

    Main Methods:

    • Utilized a solar magnetograph coupled with a 1.5-m telescope.
    • Employed a pair of self-scanning 512-element integrated diode arrays as detectors.
    • Characterized photometric properties including Modulation Transfer Function (MTF), dark current, readout completeness, and noise.

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    Published on: October 27, 2017

    Optimized Setup and Protocol for Magnetic Domain Imaging with In Situ Hysteresis Measurement
    09:43

    Optimized Setup and Protocol for Magnetic Domain Imaging with In Situ Hysteresis Measurement

    Published on: November 7, 2017

    Related Experiment Videos

    Last Updated: Jun 16, 2026

    Demonstration of Spin-Multiplexed and Direction-Multiplexed All-Dielectric Visible Metaholograms
    08:48

    Demonstration of Spin-Multiplexed and Direction-Multiplexed All-Dielectric Visible Metaholograms

    Published on: September 25, 2020

    Indoor Experimental Assessment of the Efficiency and Irradiance Spot of the Achromatic Doublet on Glass (ADG) Fresnel Lens for Concentrating Photovoltaics
    09:00

    Indoor Experimental Assessment of the Efficiency and Irradiance Spot of the Achromatic Doublet on Glass (ADG) Fresnel Lens for Concentrating Photovoltaics

    Published on: October 27, 2017

    Optimized Setup and Protocol for Magnetic Domain Imaging with In Situ Hysteresis Measurement
    09:43

    Optimized Setup and Protocol for Magnetic Domain Imaging with In Situ Hysteresis Measurement

    Published on: November 7, 2017

    Main Results:

    • Detected photospheric flux as low as 5x10^16 maxwells (DeltaI/I = 3x10^-4 at 0.8688 microm).
    • Measured detector noise equivalent to 950 electrons at the input with an integrating preamplifier.
    • Demonstrated low noise and cooling characteristics when operated near liquid nitrogen temperature.

    Conclusions:

    • The described solar magnetograph effectively detects weak photospheric magnetic fields.
    • The integrated diode array detector exhibits excellent performance at low light levels.
    • The detector shows significant potential for future low-light astronomical sensing applications.