929 resultados para jet fuel hedging


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The monthly fuel tax report from Iowa Department of Transportation to the Iowa Department of Revenue and Finance.

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The monthly fuel tax report from Iowa Department of Transportation to the Iowa Department of Revenue and Finance.

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The monthly fuel tax report from Iowa Department of Transportation to the Iowa Department of Revenue and Finance.

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The monthly fuel tax report from Iowa Department of Transportation to the Iowa Department of Revenue and Finance.

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The monthly fuel tax report from Iowa Department of Transportation to the Iowa Department of Revenue and Finance.

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The monthly fuel tax report from Iowa Department of Transportation to the Iowa Department of Revenue and Finance.

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The monthly fuel tax report from Iowa Department of Transportation to the Iowa Department of Revenue and Finance.

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The monthly fuel tax report from Iowa Department of Transportation to the Iowa Department of Revenue and Finance.

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The monthly fuel tax report from Iowa Department of Transportation to the Iowa Department of Revenue and Finance.

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The Seventy-ninth General Assembly of the State of Iowa, 2001 Regular Session, passed Senate File 465 which was signed by the Governor on April 19, 2001. This act created the biodiesel fuel revolving fund to be used to purchase biodiesel fued for use in the Iowa Department of Transportation (DOT vehicles. This report details activity of the fund for fiscal year 2009.

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House File 2754 requires by February 1 of each year the Iowa Department of Transportation shall deliver a report to the governor and legislative services agency regarding flexible fuel vehicles registered in Iowa.

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Here we discuss two consecutive MERLIN observations of the X-ray binary LS I +61◦303. The first observation shows a double-sided jet extending up to about 200 AU on both sides of a central source. The jet shows a bent S-shaped struct ure similar to the one displayed by the well-known precessing jet of SS 433. The precession suggested in the first MERLIN image becomes evident in the second one, showing a one-sided bent jet significantly rotated with respect to the jet of the day before. We conclude that the derived precession of the relativistic (β=0.6) jet explains puzzling previous VLBI results. Moreover , the fact that the precession is fast could be the explanation of the never understood short term (days) variability of the associated gamma-ray source 2CG 135 + 01 / 3EG J0241 + 6103.

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We present Very Long Baseline Interferometry (VLBI) observations of the high mass X-ray binary LSI+61303, carried out with the European VLBI Network (EVN). Over the 11 hour observing run, performed 10 days after a radio outburst, the radio source showed a constant flux density, which allowed sensitive imaging of the emission distribution. The structure in the map shows a clear extension to the southeast. Comparing our data with previous VLBI observations we interpret the extension as a collimated radio jet as found in several other X-ray binaries. Assuming that the structure is the result of an expansion that started at the onset of the outburst, we derive an apparent expansion velocity of 0.003 c, which, in the context of Doppler boosting, corresponds to an intrinsic velocity of at least 0.4 c for an ejection close to the line of sight. From the apparent velocity in all available epochs we are able to establish variations in the ejection angle which imply a precessing accretion disk. Finally we point out that LSI+61303, like SS433 and Cygnus X-1, shows evidence for an emission region almost orthogonal to the relativistic jet.

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The monthly fuel tax report from Iowa Department of Transportation to the Iowa Department of Revenue and Finance.

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The monthly fuel tax report from Iowa Department of Transportation to the Iowa Department of Revenue and Finance.