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  • SPACE RADIATION  (38)
  • 25.70.Np  (1)
  • 3-D Reconstruction  (1)
  • 1
    Electronic Resource
    Electronic Resource
    Springer
    The European physical journal 348 (1994), S. 105-109 
    ISSN: 1434-601X
    Keywords: 25.70.Np
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We report the first measurement of the total charge-loss cross section σtot=σem+σnuc and partial cross sections (for ΔZ=1, 2, ..., 9) of 11.4 A GeV197Au nuclei in various targets. The large Coulomb barrier for Au reduces the electromagnetic contribution σem in a Pb target to only 18% of σnuc, compared with ∼ 70% for 14.5 A GeV28Si and 120% for 200 A GeV32S. With σem taken to be ∝Z T 1.8 , σnuc can be fitted with σnuc=α(A P 1/3 +A T 1/3 −b)2, with b=0.83 and α=59 mb, essentially the same as found at energies of 1 to 2 A GeV. Electromagnetic partial cross sections for ΔZ=1 exceed ∼ 40 mb in the Pb, Sn, Cu, and Fe targets and are substantial for larger values ofΔZ in the heavier targets.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    Cell & tissue research 204 (1979), S. 343-354 
    ISSN: 1432-0878
    Keywords: Hypothalamo-pituitary afferents ; Vasopressin ; Somatostatin ; 3-D Reconstruction
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Medicine
    Notes: Summary A three-dimensional reconstruction of the rat's hypothalamo-neurohypophysial system, depicting the neurons that project to the neurointermediate lobe of the pituitary, has been made by using retrograde transport of horseradish peroxidase injected into the neuro-intermediate lobe and by using immunocytochemistry with antisera to vasopressin and somatostatin. The overall picture illustrates the neurons situated in the walls of a pair of ill-defined cone-shaped tunnels, the apices pointing anteriorly. Among the neuronal aggregates in the tunnel wall two, the paraventricular and forniceal nuclei, appear similar in shape but clearly separated by a gap of at least 150 μm. Many of the vasopressin-positive neurons lie in the same nuclear aggregates with two notable exceptions: the suprachiasmatic nucleus contains many vasopressin-positive cells but does not project to the pituitary, and the forniceal aggregate, which does project to the pituitary, contains no vasopressin-positive cells. Somatostatin-positive cells are situated close to the third ventricle, and their size is intermediate between parvocellular and magnocellular. Cell counts show only half the cells in the system lying in the supraoptic and paraventricular nuclei, the rest being in “accessory nuclei”.
    Type of Medium: Electronic Resource
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  • 3
    Publication Date: 2005-11-30
    Description: During the Apollo 16 mission, a solar flare produced an enormous amount of low-energy nuclei, many orders of magnitude greater than the level inferred from studies of tracks in the window of the Apollo 12 spacecraft during a time when the sun was quiet. The differential energy spectrum of nuclei with Z less than or equal to 6 falls by seven orders of magnitude over the interval from 0.1 to 20 MeV/nucleon, then remains almost flat up to approximately 100 MeV/nucleon. The two parts correspond to contributions from the sun and from galactic cosmic rays. Any maximum in the spectrum occurs below the lowest energy studied.
    Keywords: SPACE RADIATION
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 8 p
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  • 4
    Publication Date: 2005-11-30
    Description: Investigations on the Fe-group nuclei track density vs depth in lunar rocks and Surveyor 3 TV camera filter glass were critically examined considering more factors than previously. The analysis gives a firmer basis to the observation of the preferential leakage of low energy Fe nuclei from the accelerating region of the sun. The track density gradients in lunar rock 12022 and filter glass are used to determine the lunar erosion rate of 3 angstroms/yr. Track gradients are less steep than predicted from energy spectrum observed in the Surveyor glass, perhaps due to sputtering. High densities of etchable tracks were found at all depths down to 60 cm in fines from Apollo cores and also in thin sections of the Pesjanoe, Pantar, and Fayetteville gas-rich meteorites. It is felt unlikely that suprathermal heavy ions were responsible for the high track densities.
    Keywords: SPACE RADIATION
    Type: NASA, Washington Analysis of Surveyor 3 Mater. and Phot. Returned by Apollo 12; p 221-226
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  • 5
    Publication Date: 2005-11-30
    Description: A silica glass window from Apollo 12 CM and a piece of flint glass from the Surveyor 3 camera filter were examined for Fe nuclei tracks. A large difference between observed and predicted track densitites was found. At low rigidity (or energy), the solar particle Fe/He ratio is much higher than the photospheric abundance ratio, but decreases with increasing rigidity until it approaches the photospheric value at a rigidity of about 500 MV. It is felt that the low-energy Fe tracks are of solar origin. The implications that heavy nuclei can be preferentially emitted from a source of energetic particles are discussed. Other conclusions are the following: Rocks exposed on the lunar surface for 10 million yr would accumulate about 6 x 10 to the 12th power tracks/sq cm, and the rate of radiation-induced erosion is about 10 to the -9 cm/yr. The lunar soil should contain heavily irradiated small grains, some with track densities of about 10 to the 12th power/sq cm that have flaked from radiation-damaged rock surfaces and some that were irradiated while at the top of the soil layer.
    Keywords: SPACE RADIATION
    Type: NASA, Washington Analysis of Surveyor 3 Mater. and Phot. Returned by Apollo 12; p 217-220
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  • 6
    Publication Date: 2006-01-11
    Description: The populations of interplanetary particles were studied by examining the energy spectra in a cosmic ray detector placed in the shade, facing away from the sun. Suprathermal ions of solar origin, and low-energy galactic cosmic rays are discussed.
    Keywords: SPACE RADIATION
    Type: NASA. Johnson Space Center Apollo 17 Prelim. Sci. Rept.; 5 p
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  • 7
    Publication Date: 2011-08-16
    Description: Iron nuclei emission during 1967-1969 solar flares from spacecraft window and lunar camera lens etched tracks, discussing Fe/He ratio and lunar soil densities
    Keywords: SPACE RADIATION
    Type: ; IENCES (
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  • 8
    Publication Date: 2011-08-16
    Keywords: SPACE RADIATION
    Type: Nature Physical Science; 243; May 7
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  • 9
    Publication Date: 2019-06-28
    Description: The survival of the Galactic magnetic field almost certainly sets an astrophysical upper bound of approx. 10 to the minus 15th power cm(-2) sr(-1) s(-1) on the flux of monopoles. To improve significantly upon this Parker limit with direct, real time searches would require a detector area of approx. 10,000 square meters and a collection time of years. Several such searches are being contemplated. A novel alternative scheme using large mica crystals capable of recording and storing tracks of slow monopoles over a time scale of approx. 10 to the 9th power years was proposed.
    Keywords: SPACE RADIATION
    Type: HE-6.1-8 , 19th Intern. Cosmic Ray Conf - Vol. 8; p 242-245; NASA-CP-2376-VOL-8
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  • 10
    Publication Date: 2019-06-28
    Description: To take the next big step beyond High Energy Astronomy Observatory (HEAO-3) the Heavy Nuclei Collector (HNC), to be carried on an LDEF reflight, has the goals of greatly increased collecting power ( 30 actinides) and charge resolution sigma sub Z or = 0.25 E for Z up to approximately 100, which will provide abundances of all the charges 40 or Z or = 96 and permit sensitive searches for hypothetical particles such as monopoles, superheavy elements, and quark nuggets.
    Keywords: SPACE RADIATION
    Type: OG-4.4-8 , 19th Intern. Cosmic Ray Conf - Vol. 2; p 131-134; NASA-CP-2376-VOL-2
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