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Flame Photometry: Lab01:16

Flame Photometry: Lab

In a flame photometer, when a solution like potassium chloride is aspirated into the flame, the solvent evaporates, leaving behind dehydrated salt. This salt dissociates into free gaseous atoms in their ground state. Some of these atoms absorb energy from the flame, leading to their excitation. The excited atoms return to the ground state, emitting photons at characteristic wavelengths. Because only electronic transitions are involved, the resulting emission lines are very narrow. The intensity...
Flame Photometry: Overview01:02

Flame Photometry: Overview

Flame photometry, also known as flame emission spectrometry, is a technique used for the qualitative and quantitative analysis of elements present in a sample using a flame as the source of excitation energy. The concept of flame photometry was realized in the early 1860s by Kirchhoff and Bunsen, who discovered that specific elements emit characteristic radiation when excited in flames. The first instrument developed for this purpose was used to measure sodium (Na) in plant ash using a Bunsen...
X-ray Imaging01:24

X-ray Imaging

German physicist Wilhelm Röntgen (1845–1923) was experimenting with electrical current when he discovered that a mysterious and invisible "ray" would pass through his flesh but leave an outline of his bones on a screen coated with a metal compound. In 1895, Röntgen made the first durable record of the internal parts of a living human: an "X-ray" image (as it came to be called) of his wife’s hand. Scientists worldwide quickly began their own experiments with X-rays, and by 1900, X-ray was widely...
Light Acquisition02:16

Light Acquisition

In order to produce glucose, plants need to capture sufficient light energy. Many modern plants have evolved leaves specialized for light acquisition. Leaves can be only millimeters in width or tens of meters wide, depending on the environment. Due to competition for sunlight, evolution has driven the evolution of increasingly larger leaves and taller plants, to avoid shading by their neighbors with contaminant elaboration of root architecture and mechanisms to transport water and nutrients.
Phase Contrast and Differential Interference Contrast Microscopy01:26

Phase Contrast and Differential Interference Contrast Microscopy

Phase-Contrast Microscopes
In-phase-contrast microscopes, interference between light directly passing through a cell and light refracted by cellular components is used to create high-contrast, high-resolution images without staining. It is the oldest and simplest type of microscope that creates an image by altering the wavelengths of light rays passing through the specimen. Altered wavelength paths are created using an annular stop in the condenser. The annular stop produces a hollow cone of...
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...

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Related Experiment Video

Updated: Jun 16, 2026

Multimodal Volumetric Retinal Imaging by Oblique Scanning Laser Ophthalmoscopy (oSLO) and Optical Coherence Tomography (OCT)
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Multimodal Volumetric Retinal Imaging by Oblique Scanning Laser Ophthalmoscopy (oSLO) and Optical Coherence Tomography (OCT)

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White Light Coronagraph in OSO-7.

M J Koomen, C R Detwiler, G E Brueckner

    Applied Optics
    |February 6, 2010
    PubMed
    Summary
    This summary is machine-generated.

    The Orbiting Solar Observatory 7 (OSO-7) coronagraph captured daily images of the white light corona, revealing transient events and constant solar changes over 2.75 years.

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    Area of Science:

    • Solar physics
    • Coronagraphy
    • Space-based solar observation

    Background:

    • The study details a coronagraph designed for the Orbiting Solar Observatory 7 (OSO-7).
    • Previous solar observations lacked continuous, high-resolution data of the white light corona.

    Purpose of the Study:

    • To describe the design and operation of the OSO-7 coronagraph.
    • To present findings on the dynamic nature of the solar corona.

    Main Methods:

    • Utilized a small, externally occulted Lyot-type coronagraph on OSO-7.
    • Employed an SEC vidicon detector and a dedicated data system.
    • Integrated the instrument into the spacecraft for orbital operation.

    Main Results:

    • Acquired daily images of the white light corona from 2.8 to 10 solar radii for 2.75 years.
    • Recorded the first observations of white light coronal transient events.
    • Demonstrated the continuously evolving nature of the solar corona.

    Conclusions:

    • The OSO-7 coronagraph provided unprecedented long-term data on coronal dynamics.
    • Coronal transient events are a significant feature of solar activity.
    • The solar corona is a highly dynamic and variable environment.