Titlebook: Observing Photons in Space; A Guide to Experimen Martin C. E. Huber,Anuschka Pauluhn,Alex Zehnder Book 2013Latest edition Springer Science+

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書目名稱Observing Photons in Space影響因子(影響力)




書目名稱Observing Photons in Space影響因子(影響力)學科排名




書目名稱Observing Photons in Space網絡公開度




書目名稱Observing Photons in Space網絡公開度學科排名




書目名稱Observing Photons in Space被引頻次




書目名稱Observing Photons in Space被引頻次學科排名




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書目名稱Observing Photons in Space年度引用學科排名




書目名稱Observing Photons in Space讀者反饋




書目名稱Observing Photons in Space讀者反饋學科排名

pineal-gland

Anonymous

,High-energy astrophysics — energies above 100 keV,mpact, energetic and violent objects in the Universe: neutron stars, stellar and supermassive black holes, supernovae including their remnants and cosmic rays interacting in the interstellar medium. An overview is given of the history of gamma-ray astronomy, the production mechanisms for gamma-rays and of the main results achieved.

Control-Group

ALLAY

Goniopolarimetric techniques for low-frequency radio astronomy in space,ing systems, goniopolarimetric (or “direction-finding”) techniques have been developed. These techniques are presented, and their limitations are discussed. An example from a recent study on auroral radio emissions at Saturn from Cassini/RPWS measurements illustrates the techniques.

NICHE

Imaging Michelson interferometers,aller angle sensitivity and its relative insensitivity to temperature. For these reasons SWFM filter systems were chosen as the imaging spectrometers for the Michelson Doppler Imager on . and for the Helioseismic and Magnetic Imager on the .. Theory and practice in space are described for SWFM filters.

Defraud

草率男

Normal- and grazing-incidence gratings and mountings used in space,In most spectrometers, the grating is the component chosen to give the necessary spectral resolution either to filter the wavelength band or to obtain the line profiles. An overview of the grating properties and mountings used in space instrumentation is given.

Gourmet

X-ray imaging with collimators, masks and grids,The basic principles of X-ray and gamma-ray imaging for astronomy with non-focusing optics are briefly reviewed. Specific topics include coded masks, and bigrid and multigrid collimators. The advantages and limitations of the various design options are discussed and illustrated with representative examples.

FLUSH

Narrow-band imaging by use of interferometers,The principles of operation of imaging spectrometers based on the use of Fabry–Perot and Fourier transform interferometers are described. The advantages and disadvantages of the two techniques are discussed, and some examples are given of their application in space-borne instruments for astronomy and Earth observation.