Ignition Disable

 
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An ignition interlock device is a mechanism that prevents a vehicle from starting when the breath alcohol concentration in a breath alcohol test meets or exceeds the startup set point. The ignition interlock device is used extensively as a part of licensing actions administered by the Kansas Division of Vehicles. General Motors (NYSE:GM) agrees to a $5.75M settlement with the state of California to resolve allegations it made false statements to investors about problems with its deadly ignition switches. Ignition Disable Wiring in the Ignition Disable on the tracking device can allow vehicle owners to remotely disable the vehicle’s ignition. Note – this will not disable the vehicle while it is driving! It does not incur an additional monthly charge and the relay that we sell to install it properly is just $15.00. The coil on a snowmobile is much like a capacitor. It has the ability to take 12 volts, raise the voltage much higher and store it until it is grounded. By grounding it, the field collapses and releases this energy through its secondary terminal. The amount of voltage rise is solely dependent on the amount of field. Police say the cold weather is playing a role in the rising number of thefts as more people are leaving their keys in the ignition unattended.

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Abstract: Sub-Chandrasekhar mass carbon-oxygen white dwarfs (CO WDs) with a surfacehelium (He) shell have been proposed as progenitors of Type Ia supernovae (SNeIa). If true, the resulting thermonuclear explosions should be able to accountfor at least some of the range of SNe Ia observables. To study this, we conducta parameter study based on 3D simulations of double detonations in CO WDs witha He shell, assuming different core and shell masses. An admixture of C to theshell and solar metallicity are included in the models. The hydrodynamicsimulations are carried out using the AREPO code. This allows us to follow theHe shell detonation with high numerical resolution, and improves thereliability of predicted nucleosynthetic shell detonation yields. The additionof C to the shell leads to a lower production of 56Ni while including solarmetallicity increases the production of IMEs. The production of higher masselements is further shifted to stable isotopes at solar metallicity. Moreover,we find different core detonation ignition mechanisms depending on the core andshell mass configuration. This has an influence on the ejecta structure. Wepresent the bolometric light curves predicted from our explosion simulationsusing the radiative transfer code ARTIS, and make comparisons with SNe Ia data.The bolometric light curves of our models show a range of brightnesses, able toaccount for sub-luminous to normal SNe Ia. We show the model bolometricwidth-luminosity relation compared to data for a range of viewing angles. Wefind that, on average, our brighter models lie within the observed data. Theejecta asymmetries produce a wide distribution of observables, which mightaccount for outliers in the data. However, the models overestimate the extentof this compared to data. We also find the bolometric decline rate over 40 daysappears systematically faster than data. (abridged)

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From: Sabrina Gronow [view email]
Ignition Disable[v1]Fri, 12 Feb 2021 19:00:26 UTC (1,437 KB)
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