distant source
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2022 ◽  
Author(s):  
Andrzej Kulowski

Abstract After introducing Leonardo da Vinci’s (LdV) predecessors in the field of light propagation research, his drawings on the topic of focussing light through a spherical mirror are analysed. The discovery of LdV is presented, according to which, at an infinitely distant source of rays, a small fragment of the canopy is enough to generate a focus, while the rest of the mirror forms caustics for which LdV did not indicate an application. An analytical description of the energy concentration in the focus and on the caustics is given, together with its reference to the geometric representation of the acoustic field in rooms. Using symmetry in the description of energy relations in acoustics and electromagnetism, the interference that occurs on the caustics produced by the acoustic and electromagnetic wave is discussed. It is explained why in the sound field in existing halls, instead of a whole caustic only its cusp is observed, which is perceived as a point-like sound focus. The size of the mirror aperture, shown graphically by LdV, is determined. How the development of receiving techniques increased the mirror aperture compared to the LdV estimate is also shown. The implementation of these improvements is presented via the example of the Arecibo and FAST radio telescopes.


2021 ◽  
Vol 12 (1) ◽  
Author(s):  
Tina Dura ◽  
Andra J. Garner ◽  
Robert Weiss ◽  
Robert E. Kopp ◽  
Simon E. Engelhart ◽  
...  

AbstractThe amplification of coastal hazards such as distant-source tsunamis under future relative sea-level rise (RSLR) is poorly constrained. In southern California, the Alaska-Aleutian subduction zone has been identified as an earthquake source region of particular concern for a worst-case scenario distant-source tsunami. Here, we explore how RSLR over the next century will influence future maximum nearshore tsunami heights (MNTH) at the Ports of Los Angeles and Long Beach. Earthquake and tsunami modeling combined with local probabilistic RSLR projections show the increased potential for more frequent, relatively low magnitude earthquakes to produce distant-source tsunamis that exceed historically observed MNTH. By 2100, under RSLR projections for a high-emissions representative concentration pathway (RCP8.5), the earthquake magnitude required to produce >1 m MNTH falls from ~Mw9.1 (required today) to Mw8.0, a magnitude that is ~6.7 times more frequent along the Alaska-Aleutian subduction zone.


2021 ◽  
Vol 2021 (2) ◽  
pp. 4383-4387
Author(s):  
ANTON PANDA ◽  
◽  
VOLODYMYR NAHORNYI ◽  
PETER PIGULEVSKY ◽  
IVETA PANDOVA ◽  
...  

The article presents the results of approbation the vibration forecasting methodology based on the synchronous measurement results of water level fluctuations in several observing wells. These fluctuations are caused by the shocks impact generated in a distant source of a maturing vibrations. The approbation demonstrated the reliable forecast possibility of earthquake time and its epicenter coordinates.


2021 ◽  
Vol 11 (1) ◽  
pp. 6-9
Author(s):  
Sankar Palchoudhury

All kinds of waves occur for the disturbances in the quiet gravitational field. Different waves powered differently and propagated in the gravitational field. A black hole is the higher GFI (Gravitational Field Intensity) area. The rays do not possess, coming from a distant source when pass by the black holes, adequate strength to disturb in the higher GFI area of the black holes. Naturally, the rays take on a curve path as the provision in a circular area depends on the radius (distance), keeping distance according to the lower GFI area around the black holes’ centre.


2020 ◽  
Vol 7 ◽  
Author(s):  
Moritz Wandres ◽  
Jérôme Aucan ◽  
Antonio Espejo ◽  
Naomi Jackson ◽  
Antoine De Ramon N’Yeurt ◽  
...  

Sedimentology ◽  
2020 ◽  
Vol 67 (3) ◽  
pp. 1249-1273 ◽  
Author(s):  
Seanpaul La Selle ◽  
Bruce M. Richmond ◽  
Bruce E. Jaffe ◽  
Alan R. Nelson ◽  
Frances R. Griswold ◽  
...  

2019 ◽  
Vol 67 (2) ◽  
pp. 320-335 ◽  
Author(s):  
Yimao Sun ◽  
K. C. Ho ◽  
Qun Wan
Keyword(s):  

2018 ◽  
Vol 14 (S342) ◽  
pp. 252-253
Author(s):  
Krisztina Perger ◽  
Sándor Frey ◽  
Krisztina É. Gabányi

AbstractWe constrained the jet proper motion of PMN J2134–0419 at z = 4.33 to μ = 0.035±0.023mas yr−1 using very long baseline interferometry (VLBI). This is the second most distant source where such a measurement could be made. Another distant blazar SDSS J1026+2542 (z = 5.27) shows jet component proper motions up to μ = 0.112 ± 0.031 mas yr−1. In both cases, the measured values are consistent with the expectations of current ΛCDM cosmological models.


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