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czas-i-pomiary: Equation of time

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The equation of time can be approximated by a sum of two sine waves: Δ t e y = − 7.
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The equation of time describes the discrepancy between two kinds of solar time. The two times that differ are the apparent solar time, which directly tracks the diurnal motion of the Sun, and mean solar time, which tracks a theoretical mean Sun with uniform motion along the celestial equator. Apparent solar time can be obtained by measurement of the current position (hour angle) of the Sun, as indicated (with limited accuracy) by a sundial. Mean solar time, for the same place, would be the time indicated by a steady clock set so that over the year its differences from apparent solar time would have a mean of zero. The equation of time is the east or west component of the analemma, a curve representing the angular offset of the Sun from its mean position on the celestial sphere as viewed from Earth. The equation of time values for each day of the year, compiled by astronomical observatories, were widely listed in almanacs and ephemerides. The equation of time can be approximated by a sum of two sine waves: Δ t e y = − 7.659 sin ⁡ ( D ) + 9.863 sin ⁡ ( 2 D + 3.5932 ) {\displaystyle \Delta t_{ey}=-7.659\sin(D)+9.863\sin \left(2D+3.5932\right)} [minutes] where: D = 6.240 040 77 + 0.01…
Kategoria: czas-i-pomiary
Rodzina: uklad-sloneczny
Jakość źródła: 65/100
Próby weryfikacji: 3
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Wikipedia ENPOTWIERDZAniezależne

Evidence: 45 • authority: 72

The equation of time describes the discrepancy between two kinds of solar time. The two times that differ are the apparent solar time, which directly tracks the diurnal motion of the Sun, and mean solar time, which tracks a theoretical mean Sun with uniform motion along the celestial equator. Apparent solar time can be obtained by measurement of the current position (hour angle) of the Sun, as indicated (with limited accuracy) by a sundial. Mean solar time, for the same place, would be the time indicated by a steady clock set so that over the year its differences from apparent solar time would have a mean of zero. The equation of time is the east or west component of the analemma, a curve r…

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OpenAlex / Punjab University Journal of Mathematicspomocniczeniezależne

Evidence: 41 • authority: 90

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Elsevier BVpomocniczeniezależne

Evidence: 41 • authority: 88

Spectral stability and slow–fast structure of traveling waves in a regularized sine–Gordon equation. We investigate the dynamics and spectral stability of traveling kink and antikink solutions in a dissipative sine--Gordon equation with two distinct fourth--order regularization mechanisms: a mixed space--time (inertial) term and a purely spatial (elliptic) term. The model includes damping, bias forcing, and higher--order dissipative effects, and is motivated by refined descriptions of fluxon dynamics in long Josephson junctions. Using a collective--coordinate reduction, we derive a Melnikov--type condition for speed selection, yielding explicit predictions for asymptotic propagation speeds,…

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Wikipedia ENpomocnicze

Evidence: 41 • authority: 72

In mathematics, a differential equation is an equation that relates one or more unknown functions and their derivatives. In applications, the functions generally represent physical quantities, the derivatives represent their rates of change, and the differential equation defines a relationship between the two. Such relations are common in mathematical models and scientific laws; therefore, differential equations play a prominent role in many disciplines including engineering, physics, economics, and biology. The study of differential equations consists mainly of the study of their solutions (the set of functions that satisfy each equation), and of the properties of their solutions. Only the…

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