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  • SPACE RADIATION  (4)
  • Instrumentation and Photography  (2)
  • Plant organs  (1)
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  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Plant and soil 75 (1983), S. 435-442 
    ISSN: 1573-5036
    Keywords: Amino acids ; Asparagine ; Dopa ; Fababean ; Plant organs ; Vicia faba L.
    Source: Springer Online Journal Archives 1860-2000
    Topics: Agriculture, Forestry, Horticulture, Fishery, Domestic Science, Nutrition
    Notes: Summary Nodulated fababeans growing in unfertilized soil were sampled at intervals during development and the plants divided into their constituent organs before extraction and determination of the separate free amino acid contents. At each developmental stage asparagine and 3,4-dihydroxyphenylalanine (Dopa) were the most abundant free amino acids in all organs except the seeds. Of the second-order constituents, there were respectively, modest amounts of serine and glutamine in the leaves, tyrosine in the pods and alanine in the young seeds. During plant development there were marked differences in both the amount and composition of the free amino acid fraction in some organs. The concentration of asparagine increased sharply during pod-fill in both stems and pods and it is suggested that this is the form in which much N is moved into the seeds for protein synthesis. Young seeds contained much free asparagine, glutamine and alanine but with time the two latter constituents were replaced by arginine. There was a rapid accumulation of Dopa in the fruits and leaves during early pod-fill but the amount decreased as the plants aged and the Dopa content of the mature seeds were extremely low.
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 2011-08-24
    Description: The Northern Hemisphere data from the 19.2 GHz full sky survey are analyzed to place limits on the magnitude of Gaussian fluctuations in the cosmic microwave background implied by a variety of correlation functions. Included among the models tested are the monochromatic and Gaussian-shaped families, and those with power law spectra for n from -2 to 1. We place an upper bound on the quadrupole anisotropy of DeltaT/T less than 3.2 x 10 exp -5 rms, and an upper bound on scale-invariant (n = 1) fluctuations of a2 less than 4.5 x 10 exp -5 (95 percent confidence level). There is significant contamination of these data from Galactic emission, and improvement of our modeling of the Galaxy could yield a significant reduction of these upper bounds.
    Keywords: SPACE RADIATION
    Type: In: After the first three minutes; Proceedings of the 1st Astrophysics Workshop, Univ. of Maryland, College Park, Oct. 15-17, 1990 (A93-23605 07-90); p. 107-112.
    Format: text
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  • 3
    Publication Date: 2019-07-18
    Description: TopHat is a balloon-borne instrument designed to operate on the top of a balloon. From this location, the experiment could efficiently observe using a clean beam with extremely low sidelobes. The experiment was designed to scan a large portion of the sky directly above it and to map the anisotropy of the Cosmic Microwave Background (CMBR) and thermal emission from galactic dust. The instrument used a one meter class telescope with a five band single pixel radiometer spanning the frequency range from 150-600 GHz. The radiometer used bolometric detectors operating at approx. 250 mK. Here, we will report on the flight of the TopHat experiment over Antarctica in January, 2001 and describe the scientific goals, the operation, and in-flight performance.
    Keywords: Instrumentation and Photography
    Type: SPIE Meeting; Aug 22, 2002 - Aug 28, 2002; Waikoloa, HI; United States
    Format: text
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  • 4
    Publication Date: 2019-07-18
    Description: The SPEED camera is being developed to study the spectral energy distributions of high redshift galaxies using the Heinrich Hertz Telescope (HHT) in Arizona. SPEED requires a small cryogenic detector array of 2x2 pixels with each pixel having four frequency bands in the 150-350 GHz range. Here we describe the development of the detector array of these high efficiency FSBs. The FSB design provides the multi-pixel multi-spectral band capability required for SPEED in a compact stackable array. The SPEED bolometers will use proximity effect superconducting transition edge sensors as their temperature-sensing element allowing for higher levels of multiplexing in future applications.
    Keywords: Instrumentation and Photography
    Type: 10th International workshop on Low Temperature Detectors; Jul 07, 2003 - Jul 11, 2003; Genoa,; Italy
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  • 5
    Publication Date: 2019-08-28
    Description: We report preliminary results from two balloon flights of a millimeter-wave telescope designed to measure anisotropy in the cosmic microwave background (CMB) on angular scales from 0.3 to 3 degrees. The receiver used in the first flight, in November 1989, was a dichroic, He-3-cooled bolometric photometer with passbands centered at 3, 6, 9, and 12/cm. The second flight, in July 1990, employed improved bolometric detectors. The 3/cm band was removed in order to increase the efficiency of the remaining bands. Preliminary analysis of the data gives a factor of 3 improvement in sensitivity over the first flight in the 6/cm band. Future plans include a new receiver to provide an additional factor of 5 improvement in sensitivity and a new balloon-borne telescope which is optimized for low-background bolometric detectors at millimeter wavelengths.
    Keywords: SPACE RADIATION
    Type: In: After the first three minutes; Proceedings of the 1st Astrophysics Workshop, Univ. of Maryland, College Park, Oct. 15-17, 1990 (A93-23605 07-90); p. 123-128.
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  • 6
    Publication Date: 2019-08-28
    Description: The Northern Hemisphere data from the 19.2 GHz full sky survey are analyzed to place limits on the magnitude of Gaussian fluctuations in the cosmic microwave background implied by a variety of correlation functions. Included among the models tested are the monochromatic and Gaussian-shaped families, and those with power-law spectra for n values between -2 and 1. An upper bound is placed on the quadrupole anisotropy of Delta T/T less than 3.2 x 10 exp -5 rms, and an upper bound on scale-invariant (n = 1) fluctuations of a2 less than 4.5 x 10 exp -5 (95 percent confidence level). There is significant contamination of these data from Galactic emission, and improvement of the modeling of the Galaxy could yield a significant reduction of these upper bounds.
    Keywords: SPACE RADIATION
    Type: Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X); 391; 2, Ju; L49-L52
    Format: text
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  • 7
    Publication Date: 2019-08-27
    Description: The results of a search for anisotropy in the cosmic microwave background on angular scales near 1 deg are presented. Observations were simultaneously performed in bands centered at frequencies of 6, 9, and 12 per cm with a multifrequency bolometric receiver mounted on a balloon-borne telescope. The statistical sensitivity of the data is the highest reported to date at this angular scale, which is of critical importance for understanding the formation of structure in the universe. Signals in excess of random were observed in the data. The experiment, data analysis, and interpretation are described.
    Keywords: SPACE RADIATION
    Type: Astrophysical Journal, Part 1 (ISSN 0004-637X); 395; 2 Au
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