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  • 1
    ISSN: 1432-0878
    Keywords: Corticotropin ; Opioid peptides ; Anterior pituitary ; Human fetus ; Electron microscopic immunocytochemistry
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Medicine
    Notes: Summary Cells immunoreactive with anti-α-(17–39) ACTH, β-(1–24) corticotropin, β-LPH, α- and β-EP were identified in the human fetal anterior pituitary at the ultrastructural level using the peroxidase-antiperoxidase complex method on ultrathin sections. Only one definite cell type was revealed by all these antisera. All granules of each individual immunostained cell reacted regardless of the antiserum used. The immunostained cells occurred in groups and were sometimes located in the wall of the follicle-like structures commonly observed in the fetal anterior pituitary. The cells revealed two main aspects: 1) The largest elements were rich in organelles, and their numerous secretory granules showed significant variations in size (250–500 nm in diameter), electron density of their content and stain-deposit intensity. The ergastoplasm, consisting of irregular tubules, was poorly developed. In the vicinity of the conspicuous Golgi apparatus, organelles related to the GERL complex were commonly observed. Multivesicular bodies were frequent. Some of these cells showed bundles of microfilaments (60 nm in thickness). 2) The smaller cells had an electron-lucent hyaloplasm with sparse organelles; they contained fewer granules and never showed microfilaments. The immunocytological results are consistent with the synthesis of a molecule similar to pro-opiocortin by this type of endocrine cell in human fetuses. Morphological evidence for the maturation process of this precursor and for the secretory activity of these cells and its possible regulation is presented and discussed.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    Cell & tissue research 181 (1977), S. 545-552 
    ISSN: 1432-0878
    Keywords: Somatotrophs ; Anterior pituitary ; Human fetus ; Electron microscopic immunocytochemistry
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Medicine
    Notes: Summary An immunocytochemical staining of ultrathin sections using the peroxidase-antiperoxidase complex was employed to localize the somatotrophs in the anterior pituitary of the human fetus. This technique allowed a specific identification of the somatotrophs and a detailed description of their ultrastructure which was well preserved by the fixation employed. They appeared as cells with a dense cytoplasmic matrix, lamellar rough endoplasmic reticulum, and prominent Golgi apparatus. Their secretory granules had a mean diameter of 300 nm.
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  • 3
    Publication Date: 2019-07-17
    Description: The Cloud Absorption Radiometer (CAR) was flown aboard the University of Washington Convair CV-580 research aircraft and took measurements on 23 flights between August 15 and September 16. On 12 of those flights, BRF (bidirectional reflection function) measurements were obtained over different natural surfaces and ecosystems in southern Africa. The BRF measurements were done to characterize surface anisotropy in support of SAFARI 2000 science objectives principally to validate products from NASA's EOS (Earth Observing System) satellites, and to parameterize and validate BRF models. In this paper we present results of BRFs taken over two EOS validation sites: Skukuza tower, South Africa (25.0 S, 31.5 E) and Mongu tower, Zambia (15.4 S, 23.3 E). The CAR is capable of measuring scattered light in fourteen spectral bands. The scan mirror, rotating at 100 rpm, directs the light into a Dall-Kirkham telescope where the beam is split into nine paths. Eight light beams pass through beam splitters, dichroics, and lenses to individual detectors (0.34-1.27 microns), and finally are registered by eight data channels. They are sampled simultaneously and continuously. The ninth beam passes through a spinning filter wheel to an InSb detector cooled by a Stirling cycle cooler. Signals registered by the ninth data channel are selected from among six spectral channels (1.55-2.30 microns). The filter wheel can either cycle through all six spectral bands at a prescribed interval (usually changing filter every fifth scan line), or lock onto any one of the six spectral bands and sample it continuously. To measure the BRF of the surface-atmosphere system, the University of Washington CV-580 had to bank at a comfortable roll angle of approximately 20 degrees and fly in a circle about 3 km in diameter above the surface for roughly two minutes. Replicated observations (multiple circular orbits) were acquired over selected surfaces so that average BRF smooth out small-scale surface and atmospheric inhomogeneities. At an altitude of 600 m above the targeted surface area and with a 1 degree IFOV, the pixel resolution is about 10 m at nadir and about 270 m at an 80 degree viewing angle from the CAR.
    Keywords: Geophysics
    Type: SAFARI 2000 First Data Workshop; Aug 28, 2000 - Aug 31, 2000; Siavonga; Zambia
    Format: text
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  • 4
    Publication Date: 2019-07-13
    Description: VIR-MS, Dawn's Visible and Infrared Mapping Spectrometer, obtained hyperspectral images of a wide part of Vesta's surface at a variety of spatial resolutions [1]. Vesta spectra are similar to those of the howardite-eucrite-diogenite (HED) meteorites. Moreover, they are characterized by the two iron-bearing pyroxene bands at 0.9 (band I) and 1.9 microns (band II). Vesta surface's is dominated by eucrite/howardite with some diogenitic regions situated in the southern hemisphere near the Rheasilvia basin [2]. The surface is heavily craterized and impacts can expose fresh material, thus generating the Bright Material Deposits (BMD) observed within and surrounding certain craters. BMD can be classified into six different types based on their morphological characteristics: Crater Wall/Scarp Material (CWM), Radial Material (RM), Slope Material (SM), Patchy Material (PM), Spot Material (SpM) and Diffuse Plains Material (DPM) [3]. The most widespread BMD are CWM, SM and RM. CWM, SM, RM originate from impacts. CWM is situated on the edge of the craters. Mass wasting from the crater walls and generates the SM, while RM is associated with the ejecta of the craters [4]. BMD are characterized by albedo greater than that of the vestan average, 0.38 [5]. Therefore the different types of deposits present distinct levels of reflectance respect to the Surrounding Regions (SR), in particular: the CWM and SM is approx.40% brighter, the RM is approx.30- 40% brighter; the SpM is about 20-25% brighter and the PM is about 20% brighter. Near the edge of the Rheasilvia basin it is possible to find some extremely bright areas ~80% brighter than the vestan average [6].
    Keywords: Geophysics
    Type: JSC-CN-28143 , Lunar and Planetary Science Conference; Mar 18, 2013 - Mar 22, 2013; The Woodlands, TX; United States
    Format: application/pdf
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