Zobrazeno 1 - 10
of 41
pro vyhledávání: '"Richard B. Holmes"'
Autor:
Richard B. Holmes
Publikováno v:
AIAA Journal. 60:5633-5644
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::636fd0dc6a7b074b6f769a479ac78d00
https://doi.org/10.2514/1.j061766
https://doi.org/10.2514/1.j061766
Publikováno v:
Unconventional Imaging and Adaptive Optics 2022.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7bf6255d464fe4f28ac3a023b104b4c6
https://doi.org/10.1117/12.2632776
https://doi.org/10.1117/12.2632776
Autor:
Richard B. Holmes
Publikováno v:
Journal of Modern Physics. 12:1483-1517
A modest extension of the Standard Model allows a family-specific, feeble form of SU(3) that causes rapid binding of neutrinos at neutrino decoupling. These bound neutrinos become nonrelativistic well before recombination. Neutrinos are bound when al
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::59973a08422f0fc7c23951dcb95e5797
https://doi.org/10.4236/jmp.2021.1211090
https://doi.org/10.4236/jmp.2021.1211090
Autor:
Richard B. Holmes
Publikováno v:
Journal of Modern Physics. 11:854-885
The objective of this research is to provide an explanation of galactic haloes using established particles and forces using recent theoretical developments. Light fermions, with masses on the order of 1 eV/c2, are not a leading candidate for dark mat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ce29e80270e15d3ab644d28e6eb5226b
https://doi.org/10.4236/jmp.2020.116053
https://doi.org/10.4236/jmp.2020.116053
Autor:
Richard B. Holmes
Publikováno v:
Journal of Modern Physics. 11:648-667
It is well-known that equilibrium density profiles of gases and fluids in gravitational potentials have an r−1 dependence, where r is the radius. This is found in both astronomical observations and detailed simulations in spherically-symmetric geom
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::190a1fa02fef42c2caf62887f117f45b
https://doi.org/10.4236/jmp.2020.115042
https://doi.org/10.4236/jmp.2020.115042
Publikováno v:
SPIE Proceedings.
Intensity interferometry utilizes measurements of the squared-magnitude of the Fourier transform of an object using relatively simple, phase-insensitive hardware, and therefore holds the promise of extremely high spatial resolution in astronomy and v
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dda26d63ee4b9ecf55a03a9278348e62
https://doi.org/10.1117/12.858438
https://doi.org/10.1117/12.858438
Publikováno v:
SPIE Proceedings.
The GEO Light Imaging National Testbed (GLINT) system will image objects in geo-synchronous and semi-synchronous orbits using a synthetic aperture technique known as Fourier Telescopy. The testbed will be located in the vicinity of Socorro, New Mexic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::98fb41895c2a6f91ee6bcc3c33a2bc42
https://doi.org/10.1117/12.405789
https://doi.org/10.1117/12.405789
Autor:
Richard B. Holmes, Timothy J. Brinkley
Publikováno v:
SPIE Proceedings.
Fourier Telescopy is an imaging method that can form images of very dim objects with angular resolution of a few nanoradians, attained by means of a synthetic aperture that overcomes the effects of intervening aberrations using mathematical algorithm
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c66237e5b8c8e8106ae660be2db8f2b8
https://doi.org/10.1117/12.364129
https://doi.org/10.1117/12.364129
Publikováno v:
SPIE Proceedings.
A technique for polychromatic image restoration is proposed in the context of high-resolution synthetic aperture imaging.Noise and aberrations from the atmosphere are included in the analysis. The technique is simulated and successful imagerestoratio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::09346e24539a12ab371637f1ffec0045
https://doi.org/10.1117/12.292749
https://doi.org/10.1117/12.292749
Autor:
Richard B. Holmes
Publikováno v:
SPIE Proceedings.
In astronomical imaging techniques, the relative level of the zero-frequency component of an image is usually unknown relative to all other components. This problem arises because the overall object brightness cannot easily be separated from backgrou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::49ea6c7426b38feb3ef0f963a13bec39
https://doi.org/10.1117/12.258220
https://doi.org/10.1117/12.258220