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  • LUNAR AND PLANETARY EXPLORATION  (2)
  • 23; Counting; DEPTH, water; Dermocystidium sp.; Fungi; Labyrinthula sp.; Labyrinthuloides sp.; North Sea; Number of species; Salinity; Sample code/label; Schizochytrium aggregatum; Schizochytrium sp.; Temperature, water; Thraustochytrium aggregatum; Thraustochytrium aureum; Thraustochytrium multirudimentale; Thraustochytrium pachydermum; Thraustochytrium sp.; Ulkenia minuta; Ulkenia visurgensis; VH_06_76_479-1; VH0676; Victor Hensen; Water sample; WS  (1)
  • GEOPHYSICS  (1)
  • 1980-1984  (4)
  • 1980  (4)
Collection
Keywords
Publisher
Years
  • 1980-1984  (4)
Year
  • 1
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    Unknown
    Abundance of fungi in deep water samples of site VH_06_76_479-1 of the North Sea (Table 15) (1980)
    PANGAEA
    Details
    Publication Date: 2023-07-09
    Keywords: 23; Counting; DEPTH, water; Dermocystidium sp.; Fungi; Labyrinthula sp.; Labyrinthuloides sp.; North Sea; Number of species; Salinity; Sample code/label; Schizochytrium aggregatum; Schizochytrium sp.; Temperature, water; Thraustochytrium aggregatum; Thraustochytrium aureum; Thraustochytrium multirudimentale; Thraustochytrium pachydermum; Thraustochytrium sp.; Ulkenia minuta; Ulkenia visurgensis; VH_06_76_479-1; VH0676; Victor Hensen; Water sample; WS
    Type: Dataset
    Format: text/tab-separated-values, 96 data points
    Location Call Number Expected Availability
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    DATA PANGAEA
  • 2
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    Unknown
    The morphology of metallic ions in the upper atmosphere (1980)
    In:  Other Sources
    Details
    Publication Date: 2019-06-28
    Description: Analysis of metallic ion data from a day-night pair of rockets, OGO 6, and the elliptic phases of AE-C and AE-D shows the presence of Fe(+) ions at altitudes above 400 km only at low magnetic latitudes. The detection probability of this ion decreases with altitude, with a maximum over the Atlantic and a minimum over India; the rocket data indicate ions in the E region during the day and on the bottom of the F layer at night. Mg(+) and Fe(+) are the dominant ions below 250 km at all latitudes, but Al(+), Na(+), Si(+), and Ca(+) are also detectable; a correlation was found between solar activity and metallic ion detection probability at low latitudes and high altitudes at night
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research; 85; Dec. 1
    Format: text
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    NASA TECHNICAL REPORTS
  • 3
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    Unknown
    Mariner 10 observations of hydrogen Lyman alpha emission from the Venus exosphere - Evidence of complex structure (1980)
    In:  Other Sources
    Details
    Publication Date: 2019-06-27
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Planetary and Space Science; 28; July 198
    Format: text
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    NASA TECHNICAL REPORTS
  • 4
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    Unknown
    A model of the SO2 atmosphere and ionosphere of Io (1980)
    In:  Other Sources
    Details
    Publication Date: 2019-06-27
    Description: The calculations of thermal structure for an SO2 atmosphere of Io lead to exospheric temperatures in 800-1200 K range. The Pioneer 10 electron density profiles can be fit with an SO2 surface density of 1.2 x 10 to the 11th per cu cm at 5:30 pm local time and exosphere temperature of 1030 K. Low energy electrons provide the major ionization source but the solar UV absorption dominates the heating of the atmosphere due to the long wavelength absorption threshold of SO2 and large absorption cross sections.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Geophysical Research Letters; 7; Jan. 198
    Format: text
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    NASA TECHNICAL REPORTS
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