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Differential from can to core

There is actually another complication. It has been determined that not only is the absolute value of the core temperature important, but the differential from can to core is critical too. So if we increase the differential beyond the designed-in 5°C, the life can deteriorate severely, even if the can itself is held at a much lower temperature. But the designed-in differential of 5°C occurs ONLY when we pass the maximum specified ripple current (no temperature multipliers applied), irrespective of the ambient. Which means that as a matter of fact we cannot use any temperature multipliers at all. So, if the capacitor is rated to pass 1A at 105°C, then even at an ambient of, say, 65 °C, we are allowed to pass only 1A, not 2.23A. [Pg.104]

The first term with the positive exponent causes the life to increase above Lq, while the second term exerts the opposite effect. We can also see that a temperature differential from case to core in excess of the designed value is considered more harmful than a normal temperature differential (i.e., one that is caused by staying within the current rating). Chemicon models this excess temperature rise rather conservatively as causing a halving of life every 5°C increase, rather than the usual 10°C. [Pg.107]

This says that if we pass 1.73A at 85°C, or 1A at 105°C, the core temperature will be 115°C in either case. In fact, for most 105°C rated capacitors, we will have roughly a 5°C differential from ambient to the outer can and then another 5°C from the can to its innards (i.e., the core), giving us a total of 10°C from ambient to core. [Pg.103]

As a general rule, it is often easier to injection mold very thick parts using amorphous resins. This is not because of fill, but because of differential shrinkage. With semicrystalline materials in thick cross-sections, the rate of crystallization and the total amount of crystallization can vary significantly from skin to core. As a result, the total amount of mold shrinkage can vary through the part. This can lead to distortions (warping and/ or sink marks). [Pg.193]

To infer accumulation rate history from an ice core, one needs to measure the thickness of annual layers (either directly if annual layers are resolvable, or by differentiating the depth-age scale determined by other means) and then correct for the thinning of these layers caused by the ice flow (the vertical strain Fig. 18-4). Estimates of vertical strain can be very uncertain for the deep part of an ice core. But vertical strain will not change rapidly with depth. Thus, if annual layers are resolvable one can learn relative accumulation rate changes across climate transitions with great confidence. [Pg.478]

If the measured ripple current is confirmed to be within the rating, we can then take the case temperature measurement as the basis for applying the normal 10°C doubling rule, even if the heat is coming from adjacent sources. Again, that is only because the case to core temperature differential is actually within the capacitor s design expectations. [Pg.106]

Nevertheless, we can make some general statements about the geochemistry of differentiated planets. The planetesimals from which they accreted had compositions determined largely by element volatility. Once assembled into a planet and heated, the partitioning of elements into cores and mantles was governed by their siderophile or lithophile affinities. Further differentiation of mantles to form crusts was controlled by the compatible or incompatible behavior of elements. [Pg.507]

Magmatic iron meteorites are thought to be samples from the metal cores of differentiated asteroids (18) and as such are ideally suited for application of Hf-W chronometry. Iron meteorites contain virtually no Hf (i.e., HfrW 0), such that the timing of core formation in their parent bodies can be calculated from their alone. Tungsten isotope data are now available for a vast number... [Pg.215]

In Eq. (4.9) Ahs is the Helmholtz free energy of the hard core reference system with the optimized hard core diameter. The pressure the fiiU system can be found from Eq. (4.9) by differentiation with respect to volume. This [Hessure will be a function of the two Lennard-Jones parameters au and 8. [Pg.340]


See other pages where Differential from can to core is mentioned: [Pg.149]    [Pg.594]    [Pg.6]    [Pg.301]    [Pg.353]    [Pg.161]    [Pg.91]    [Pg.10]    [Pg.86]    [Pg.118]    [Pg.91]    [Pg.1150]    [Pg.170]    [Pg.433]    [Pg.10]    [Pg.180]    [Pg.5]    [Pg.177]    [Pg.302]    [Pg.391]    [Pg.150]    [Pg.225]    [Pg.491]    [Pg.522]    [Pg.171]    [Pg.476]    [Pg.199]    [Pg.504]    [Pg.437]    [Pg.450]    [Pg.365]   
See also in sourсe #XX -- [ Pg.89 ]

See also in sourсe #XX -- [ Pg.89 ]

See also in sourсe #XX -- [ Pg.89 ]




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