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Related Concept Videos

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

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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...
Atomic Emission Spectroscopy: Lab01:29

Atomic Emission Spectroscopy: Lab

AES is a powerful analytical technique, especially effective when used with plasma sources, producing abundant spectra in characteristic emission lines. The Inductively Coupled Plasma (ICP), in particular, yields superior quantitative analytical data due to its high stability, low noise, low background, and minimal interferences under optimal experimental conditions. However, newer air-operated microwave sources are emerging as promising alternatives that could be more cost-effective than...
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Rocket Propulsion in Empty Space - I

The driving force for the motion of any vehicle is friction, but in the case of rocket propulsion in space, the friction force is not present. The motion of a rocket changes its velocity (and hence its momentum) by ejecting burned fuel gases, thus causing it to accelerate in the direction opposite to the velocity of the ejected fuel. In this situation, the mass and velocity of the rocket constantly change along with the total mass of ejected gases. Due to conservation of momentum, the rocket's...
Light Acquisition02:16

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The motion of a rocket is governed by the conservation of momentum principle. A rocket's momentum changes by the same amount (with the opposite sign) as the ejected gases. As time goes by, the rocket's mass (which includes the mass of the remaining fuel) continuously decreases, and its velocity increases. Therefore, the principle of conservation of momentum is used to explain the dynamics of a rocket's motion. The ideal rocket equation gives the change in velocity that a rocket experiences by...

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Related Experiment Video

Updated: Jul 12, 2026

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

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Published on: February 12, 2013

Light flashes observed by astronauts on skylab 4.

L S Pinsky, W Z Osborne, R A Hoffman

    Science (New York, N.Y.)
    |May 30, 1975
    PubMed
    Summary

    Astronauts observed light flashes correlating with cosmic rays and the South Atlantic Anomaly (SAA). Findings suggest a potential new source of radiation in the SAA, possibly multiply charged nuclei.

    Area of Science:

    • Space physics
    • Astronomy
    • Cosmic ray physics

    Background:

    • Light flashes observed by astronauts can provide insights into space radiation.
    • The Skylab 4 mission offered a unique platform for dedicated astronomical observations.
    • The South Atlantic Anomaly (SAA) is a region of intense radiation in Earth's inner Van Allen belt.

    Purpose of the Study:

    • To analyze astronaut observations of light flashes during the Skylab 4 mission.
    • To investigate the correlation between light flash frequency and cosmic-ray flux.
    • To determine the relationship between light flashes and the South Atlantic Anomaly (SAA) radiation environment.

    Main Methods:

    • Dedicated light flash observing sessions conducted by a Skylab 4 crewman.
    • Analysis of observed flash frequency.

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  • Correlation analysis between flash frequency, cosmic-ray flux, and SAA radiation levels.
  • Calculations to model potential radiation sources.
  • Main Results:

    • A strong correlation was found between the frequency of observed light flashes and primary cosmic-ray flux.
    • An even stronger correlation was identified between flash frequency and the SAA region.
    • Calculations suggest that an all-proton inner belt cannot account for the observed SAA flash rates.

    Conclusions:

    • The observed light flashes are strongly linked to space radiation, particularly within the SAA.
    • The data indicate that the current models of the inner belt radiation may be incomplete.
    • A previously unobserved flux of multiply charged nuclei in the inner belt is suggested as a possible explanation for the SAA flash rate.