Relevant bibliographies by topics / Relativistic Aberration

Academic literature on the topic 'Relativistic Aberration'

Author: Grafiati
Published: 10 December 2022
Last updated: 28 January 2023

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Journal articles on the topic "Relativistic Aberration"

1

Beig, Robert, and J. Mark Heinzle. "Relativistic aberration for accelerating observers." American Journal of Physics 76, no. 7 (July 2008): 663–70. http://dx.doi.org/10.1119/1.2888542.

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2

Wolf, Kurt Bernardo. "Relativistic aberration of optical phase space." Journal of the Optical Society of America A 10, no. 9 (September 1, 1993): 1925. http://dx.doi.org/10.1364/josaa.10.001925.

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3

Alam, Md Shah, and Md Didar Chowdhury. "Relativistic aberration of Mixed number Lorentz Transformation." Journal of the National Science Foundation of Sri Lanka 34, no. 3 (September 24, 2006): 143. http://dx.doi.org/10.4038/jnsfsr.v34i3.3645.

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Atakishiyev, Natig M., Wolfgang Lassner, and Kurt Bernardo Wolf. "The relativistic coma aberration. I. Geometrical optics." Journal of Mathematical Physics 30, no. 11 (November 1989): 2457–62. http://dx.doi.org/10.1063/1.528524.

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5

Crosta, Mariateresa, and Alberto Vecchiato. "Proper stellar directions and astronomical aberration." Proceedings of the International Astronomical Union 5, S261 (April 2009): 130–34. http://dx.doi.org/10.1017/s1743921309990263.

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AbstractThe general relativistic definition of astrometric measurement needs an appropriate use of the concept of reference frame, which should then be linked to the conventions of the IAU Resolutions (Soffel et al., 2003), which fix the celestial coordinate system. A consistent definition of the astrometric observables in the context of General Relativity is also essential to find uniquely the stellar coordinates and proper motion, this being the main physical task of the inverse ray tracing problem. Aim of this work is to set the level of reciprocal consistency of two relativistic models, GREM and RAMOD (Gaia, ESA mission), in order to guarantee a physically correct definition of light direction to a star, an essential item for deducing the star coordinates and proper motion within the same level of measurement accuracy.
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6

Sfarti, Adrian. "QED-Based Derivation of the General Forms of the Relativistic Doppler Effect and of the Relativistic Aberration." European Journal of Applied Physics 4, no. 6 (December 9, 2022): 42–46. http://dx.doi.org/10.24018/ejphysics.2022.4.6.225.

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The current paper derives the most general form of the relativistic Doppler effect and of the relativistic aberration starting from base principles available in classical electrodynamics and from the Lorentz transforms of the energy-momentum. Unlike any other material before us, we derive the relativistic Doppler formula for the case of both source and receiver moving in arbitrary directions with respect to an inertial reference frame. Thus, our derivation employs three different reference frames: one commoving with the source, the second one commoving with the receiver and the third one, commoving with the observer. The general formula, once derived, allows us to tease out all the specific cases, like the one from the perspective of the receiver, the one expressing the transverse Doppler effect, and the general formula for the Doppler rotor effect. We close with the derivation of the general formula for relativistic light aberration.
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7

Mersov, G. A. "The relativistic effects in localization of gamma-burst sources." Symposium - International Astronomical Union 114 (1986): 215–22. http://dx.doi.org/10.1017/s0074180900148223.

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The paper discusses influence of relativistic effects in gamma-burst propagation and the time sync. It is shown that the phenomenon of gamma-source aberration, while using the localization algorithm based on the estimates of gamma-burst arrival time instants should be regarded as relativistic effect. Criterions are derived which determine whether it is necessary to account for the relativistic effects, depending on the localization accuracy.
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8

Kiss, L. "Electrostatic lens potentials with small relativistic spherical aberration." Review of Scientific Instruments 60, no. 5 (May 1989): 907–9. http://dx.doi.org/10.1063/1.1140342.

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9

Atakishiyev, Natig M., Wolfgang Lassner, and Kurt Bernardo Wolf. "The relativistic coma aberration. II. Helmholtz wave optics." Journal of Mathematical Physics 30, no. 11 (November 1989): 2463–68. http://dx.doi.org/10.1063/1.528525.

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10

Kovalevsky, J., F. Mignard, and M. Froeschlé. "Space astrometry prospects and limitations." Symposium - International Astronomical Union 114 (1986): 369–82. http://dx.doi.org/10.1017/s0074180900148399.

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Among the few parameters that describe the generalized space time metrics, astrometric techniques are essentially sensitive to the displacement of the apparent positions of celestial bodies. This includes the relativistic light deflection and aberration. The possibilities of small field and wide field astrometry in measuring these effects are described. The case of the second order aberration terms is considered with some detail from the theoretical point of view, both for stellar and planetary aberration. New results are presented in the latter case.A section is devoted to a description of the existing space astrometry projects among which Space Telescope and HIPPARCOS are approved but will not contribute significantly to relativistic studies. Several “second generation” projects exist that aim at 2 or 3 orders of magnitude improvement in precision. They would yield results on second order relativistic effects and may be used to determine masses of some single stars. However, the present state of engineering of space astrometric missions has permitted to identify several limitations of the present and future missions. They will not all be readily suppressed and one should be very careful in assessing now their potentialities. It seems however that interferometric techniques have more chance to reach the 10−4 and 10−5 arc second precision than the imaging methods.
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Book chapters on the topic "Relativistic Aberration"

1

"A relativistic aberration." In Physics to a Degree, 50–51. CRC Press, 2018. http://dx.doi.org/10.1201/9781315273839-36.

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2

"A relativistic aberration." In Physics to a Degree, 165–68. CRC Press, 2018. http://dx.doi.org/10.1201/9781315273839-36a.

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