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  • Inductive grids  (1)
  • interstellar matter  (1)
  • 1
    Electronic Resource
    Electronic Resource
    Springer
    International journal of infrared and millimeter waves 6 (1985), S. 511-575 
    ISSN: 1572-9559
    Keywords: Filters ; Inductive grids ; Modal expansion methods
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We compare rigorous modal expansion methods with transmission-line models for the spectral properties of inductive grids. We compare the predictions of the former with measurements of grid transmittance, reflectance and phase angles as a function of wavelength. We show that the rigorous theory can accurately reproduce measured grid properties, both for normal and oblique incidence, and for both fundamental polarizations of incident radiation. We pay particular attention to the so-called “thickness dip”, an abrupt drop in transmittance which occurs for one polarization at off-normal incidence. We study the variation of $$\lambda _a$$ , the wavelength of the thickness dip, with grid parameters. We also study the variation of $$\lambda _m$$ , the wavelength of maximum transmittance, with grid parameters. We give four design rules which enable the optimization of grid parameters for use in multi-element filter stacks not relying on interference properties. We present a comprehensive set of curves showing the variation of spectral transmittance with grid aperture and thickness, for both fundamental polarizations and for a range of angles of incidence.
    Type of Medium: Electronic Resource
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  • 2
    ISSN: 1572-9508
    Keywords: balloon-borne instrumentation ; infrared detection ; interstellar matter
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We present here the French balloon-borne experiment named AROME. This astronomical instrument is specifically designed for the detection of near infrared emission bands (λ=3–12μm) from extended sources of low surface brightness with an angular resolution of 0.5°. The rms sensitivity achieved is of the order of 10-8 Wm-2sr-1, in terms of the power radiated in the 3.3μm band. We recall that this program led to the first detection of the 3.3μm feature in the spectrum of the diffuse galactic emission. The scientific results were presented and interpreted in Paper I, Giard et al., 1989. Future work will include both the observation of fainter objects at 3.3μm and the detection of other emission bands at 6.2 and 11.3μm.
    Type of Medium: Electronic Resource
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