Measuring the Pecular Velocity of the System Without Going Beyond It

Svishch Vladimir

doi:doi:10.11648/j.optics.20221101.12

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Measuring the Pecular Velocity of the System Without Going Beyond It

Svishch Vladimir

Published in Optics (Volume 12, Issue 1)

Received: 26 July 2023 Accepted: 18 August 2023 Published: 31 August 2023

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Abstract

The proposed scheme for measuring the pecular velocity of the observer with respect to the relic radiation without leaving the observer's reference system is investigated. The stellar aberration phenomenon of the ground source using anisotropic matter is used to measure the velocity. A comparative analysis of relic radiation, stellar radiation, and ground-based sources has been carried out in order to use them for velocity measurements based on the stellar aberration of these sources. The principle of constancy of the velocity of light irrespective of the speed of the source and the observation device allows us to conclude that it is possible to use the radiation of terrestrial sources to measure the speed of the observer relative to the fossil emission, taking into account the difference of their wave fronts. The stellar aberration of the terrestrial source allows us to measure the velocity of the observer relative to the fossil radiation without leaving the observer's reference system. The use of an anisotropic medium eliminates the need to change the structure of the device in the measurement process. The expressions of the observer's velocity with respect to the relic radiation without leaving the observer's frame of reference are obtained depending on the parameters of the anisotropic medium used.

Published in	Optics (Volume 12, Issue 1)
DOI	10.11648/j.optics.20221101.12
Page(s)	1-4
Creative Commons	This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.
Copyright	Copyright © The Author(s), 2024. Published by Science Publishing Group

Keywords

Ground Source, Relic Radiation, Pecular Velocity, Light Aberration, Wavefront Curvature, Optical Crystal Axis, Refractive Index

References

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[16]	Svishch V. M. About the Informative Parameters of Michelson Interferometers with the Division of Amplitude and the Wave Front. East European Journal of Physics. – 2018. – No. 3 -Vol. 5 - P. 24-31
[17]	Svishch V. M. Aberration of Light from a Terrestrial Source, Optics. Vol. 7, No. 2, 2018, pp 74-79 (DOI: 1011648/j. optics. 20180702.13
[18]	Svishch V. M. Light aberration in optical anisotropic single-axis (uniaxial) medium. East European Journal of Physics. – 2017. – No. 3 Vol. 4 – P. 71-77
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[20]	Lorentz G. A. The theory of Electrons. – Leipzig. 1916.
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Vladimir, S. (2023). Measuring the Pecular Velocity of the System Without Going Beyond It. Optics, 12(1), 1-4. https://doi.org/10.11648/j.optics.20221101.12

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ACS Style

Vladimir, S. Measuring the Pecular Velocity of the System Without Going Beyond It. Optics. 2023, 12(1), 1-4. doi: 10.11648/j.optics.20221101.12

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AMA Style

Vladimir S. Measuring the Pecular Velocity of the System Without Going Beyond It. Optics. 2023;12(1):1-4. doi: 10.11648/j.optics.20221101.12

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@article{10.11648/j.optics.20221101.12,
  author = {Svishch Vladimir},
  title = {Measuring the Pecular Velocity of the System Without Going Beyond It},
  journal = {Optics},
  volume = {12},
  number = {1},
  pages = {1-4},
  doi = {10.11648/j.optics.20221101.12},
  url = {https://doi.org/10.11648/j.optics.20221101.12},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.optics.20221101.12},
  abstract = {The proposed scheme for measuring the pecular velocity of the observer with respect to the relic radiation without leaving the observer's reference system is investigated. The stellar aberration phenomenon of the ground source using anisotropic matter is used to measure the velocity. A comparative analysis of relic radiation, stellar radiation, and ground-based sources has been carried out in order to use them for velocity measurements based on the stellar aberration of these sources. The principle of constancy of the velocity of light irrespective of the speed of the source and the observation device allows us to conclude that it is possible to use the radiation of terrestrial sources to measure the speed of the observer relative to the fossil emission, taking into account the difference of their wave fronts. The stellar aberration of the terrestrial source allows us to measure the velocity of the observer relative to the fossil radiation without leaving the observer's reference system. The use of an anisotropic medium eliminates the need to change the structure of the device in the measurement process. The expressions of the observer's velocity with respect to the relic radiation without leaving the observer's frame of reference are obtained depending on the parameters of the anisotropic medium used.},
 year = {2023}
}

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TY  - JOUR
T1  - Measuring the Pecular Velocity of the System Without Going Beyond It
AU  - Svishch Vladimir
Y1  - 2023/08/31
PY  - 2023
N1  - https://doi.org/10.11648/j.optics.20221101.12
DO  - 10.11648/j.optics.20221101.12
T2  - Optics
JF  - Optics
JO  - Optics
SP  - 1
EP  - 4
PB  - Science Publishing Group
SN  - 2328-7810
UR  - https://doi.org/10.11648/j.optics.20221101.12
AB  - The proposed scheme for measuring the pecular velocity of the observer with respect to the relic radiation without leaving the observer's reference system is investigated. The stellar aberration phenomenon of the ground source using anisotropic matter is used to measure the velocity. A comparative analysis of relic radiation, stellar radiation, and ground-based sources has been carried out in order to use them for velocity measurements based on the stellar aberration of these sources. The principle of constancy of the velocity of light irrespective of the speed of the source and the observation device allows us to conclude that it is possible to use the radiation of terrestrial sources to measure the speed of the observer relative to the fossil emission, taking into account the difference of their wave fronts. The stellar aberration of the terrestrial source allows us to measure the velocity of the observer relative to the fossil radiation without leaving the observer's reference system. The use of an anisotropic medium eliminates the need to change the structure of the device in the measurement process. The expressions of the observer's velocity with respect to the relic radiation without leaving the observer's frame of reference are obtained depending on the parameters of the anisotropic medium used.
VL  - 12
IS  - 1
ER  -

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Author Information

Svishch Vladimir

Kharkov National University of Aerospace named after Nikolay Zhukovsky, Kharkov Aviation Institute, Kharkov, Ukraine

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APA Style

Vladimir, S. (2023). Measuring the Pecular Velocity of the System Without Going Beyond It. Optics, 12(1), 1-4. https://doi.org/10.11648/j.optics.20221101.12

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ACS Style

Vladimir, S. Measuring the Pecular Velocity of the System Without Going Beyond It. Optics. 2023, 12(1), 1-4. doi: 10.11648/j.optics.20221101.12

Copy | Download

AMA Style

Vladimir S. Measuring the Pecular Velocity of the System Without Going Beyond It. Optics. 2023;12(1):1-4. doi: 10.11648/j.optics.20221101.12

Copy | Download

@article{10.11648/j.optics.20221101.12,
  author = {Svishch Vladimir},
  title = {Measuring the Pecular Velocity of the System Without Going Beyond It},
  journal = {Optics},
  volume = {12},
  number = {1},
  pages = {1-4},
  doi = {10.11648/j.optics.20221101.12},
  url = {https://doi.org/10.11648/j.optics.20221101.12},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.optics.20221101.12},
  abstract = {The proposed scheme for measuring the pecular velocity of the observer with respect to the relic radiation without leaving the observer's reference system is investigated. The stellar aberration phenomenon of the ground source using anisotropic matter is used to measure the velocity. A comparative analysis of relic radiation, stellar radiation, and ground-based sources has been carried out in order to use them for velocity measurements based on the stellar aberration of these sources. The principle of constancy of the velocity of light irrespective of the speed of the source and the observation device allows us to conclude that it is possible to use the radiation of terrestrial sources to measure the speed of the observer relative to the fossil emission, taking into account the difference of their wave fronts. The stellar aberration of the terrestrial source allows us to measure the velocity of the observer relative to the fossil radiation without leaving the observer's reference system. The use of an anisotropic medium eliminates the need to change the structure of the device in the measurement process. The expressions of the observer's velocity with respect to the relic radiation without leaving the observer's frame of reference are obtained depending on the parameters of the anisotropic medium used.},
 year = {2023}
}

Copy | Download

TY  - JOUR
T1  - Measuring the Pecular Velocity of the System Without Going Beyond It
AU  - Svishch Vladimir
Y1  - 2023/08/31
PY  - 2023
N1  - https://doi.org/10.11648/j.optics.20221101.12
DO  - 10.11648/j.optics.20221101.12
T2  - Optics
JF  - Optics
JO  - Optics
SP  - 1
EP  - 4
PB  - Science Publishing Group
SN  - 2328-7810
UR  - https://doi.org/10.11648/j.optics.20221101.12
AB  - The proposed scheme for measuring the pecular velocity of the observer with respect to the relic radiation without leaving the observer's reference system is investigated. The stellar aberration phenomenon of the ground source using anisotropic matter is used to measure the velocity. A comparative analysis of relic radiation, stellar radiation, and ground-based sources has been carried out in order to use them for velocity measurements based on the stellar aberration of these sources. The principle of constancy of the velocity of light irrespective of the speed of the source and the observation device allows us to conclude that it is possible to use the radiation of terrestrial sources to measure the speed of the observer relative to the fossil emission, taking into account the difference of their wave fronts. The stellar aberration of the terrestrial source allows us to measure the velocity of the observer relative to the fossil radiation without leaving the observer's reference system. The use of an anisotropic medium eliminates the need to change the structure of the device in the measurement process. The expressions of the observer's velocity with respect to the relic radiation without leaving the observer's frame of reference are obtained depending on the parameters of the anisotropic medium used.
VL  - 12
IS  - 1
ER  -

Copy | Download