An Ocean of Air: Why the Wind Blows and Other Mysteries of by Gabrielle Walker PDF

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By Gabrielle Walker

ISBN-10: 054753695X

ISBN-13: 9780547536958

We don’t simply stay within the air; we are living due to it. It’s the main staggering substance on the earth, chargeable for our meals, our climate, our water, and our skill to listen to. during this exuberant ebook, talented technology author Gabrielle Walker peels again the layers of our surroundings with the tales of the folk who exposed its secrets:

• A flamboyant Renaissance Italian discovers how heavy our air fairly is: The air filling Carnegie corridor, for instance, weighs seventy thousand kilos.
• A one-eyed barnstorming pilot reveals a suite of winds that consistently blow 5 miles above our heads.
• An impoverished American farmer figures out why hurricanes circulation in a circle by means of carving equations along with his pitchfork on a barn door.
• A well-meaning inventor approximately destroys the ozone layer.
• A reclusive mathematical genius predicts, thirty years prior to he’s proved correct, that the sky includes a layer of floating steel fed by means of the gleaming tails of taking pictures stars.

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Extra resources for An Ocean of Air: Why the Wind Blows and Other Mysteries of the Atmosphere

Example text

2 and 3. respectively. These results assure that the NESR of IMG will be within the specifications. except in the very short wavelength region. 4. 1 Data Processing IMG wi II generate the raw data of three interferograms simultaneously every 13 seconds. 05 x 10 5 points for the shorter wavelength channels. 57 x 10 5 points for the longer wavelength channel. 000 Figure 6 Blackbody spectrum taken by IMG Bread Board Model. means of a Fast Fourier Transform (FFT). It is important to carefully select the apodization function for a precise reproduction of the spectra.

41 parameters. RIS is an on-board corner reflector. and acts as a reflector for ground based laser radars. 2 Configuration of IMG Fig. 1 shows a block diagram of IMG. IMG is composed of a Michelson interferometer. a focusing mirror. a focal plane with detector assembly. a He-Ne laser for measuring the displacement of the scanning mirror. an Image Motion CompensatorCIMC) mirror to compensate for the satel I ite motion. an on-board blackbody for calibration. and a Stirling-cycle cooler which cools the detector assembly.

Cooler Scanning Mirror FocaIU---~z-l1 Plane Fixed IMC Motor xt y z Beam Splitter Figure 1 Block diagram of IMG. The interferometer is composed of 1 fixed mirror. mirror and light beam scanning a 45 degree incl ined beam spl itter. The diameter of is 10 cm. The diameters of the mirrors and beam 42 splitter are 12-15 cm . The beam splitter is made of KBr coated with Ge. Al I the mirrors are made of Al coated by Au . Fig . 2 shows a block diagram of the mirror scanning mechanism. The scanning mirror is supported by a magnetic bearings and scanned with the aid of a linear motor.

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An Ocean of Air: Why the Wind Blows and Other Mysteries of the Atmosphere by Gabrielle Walker

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