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  • 1
    Publication Date: 1947
    Description: Untersuchungen zur Entwicklung der Obstbaumspinnmilbe, ihrer Eiablage und ihres sonstigen Verhaltens unter natürlichen Umweltbedingungen KATASTER-BESCHREIBUNG: Zusammenhänge zwischen Temperatur und Niederschlag und der Anzahl und dem zeitlichen Vorkommen der Generationen sowie des Schlüpfens der Larven. KATASTER-DETAIL: Delta Nied +, dann Zeit für Entwicklung der Milben +; Delta T +, dann Zeit von Eiablage bis Schlüpfen -; Delta T + ,Delta Sonn + und/oder Delta Relf +, dann Anzahl schlüpfender Larven +; Delta T - und/oder Delta Nied +, dann Zeit für Entwicklung der Larven und Nymphen +; Delta T - und/oder Delta Nied +, dann Mortalität(Larven und Nymphen)+; Delta T + und Delta Relf -, dann Anzahl gelegter Sommereier +; Delta T +, dann Zeit für Entwicklung der Sommereier -; Delta T -, dann Anzahl gelegter Wintereier -; T 〈= 8°C, dann keine Eiablage; Delta Wind +, dann Anzahl abgewehter Milben +; Delta T (Frühjahr und Sommer) + und Delta Relf (Frühjahr und Sommer) -, dann starker Befall
    Keywords: Bergisches Land und Labor ; 1943-1944, 1946 ; Niederschlag ; Pflanzenschädling ; Temperatur ; Witterung ; Obst
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  • 2
    Publication Date: 2019-07-18
    Description: The MARIE instrument aboard Mars Odyssey functions as a telescope for the detection of charged, energetic, nuclei. The directionality that leads to the telescope description is achieved by requiring coincident signals in two designated detectors in MARIE s silicon detector stack for the instrument to trigger. Because of this, MARIE is actually a bi directional telescope. Triggering particles can enter the detector stack by passing through the lightly shielded front of the instrument, but can also enter the back of the instrument by passing through the bulk of Odyssey. Because of this, understanding how to relate the signals recorded by MARIE to astrophysically important quantities such as particle fluxes or spectra exterior to the spacecraft clearly requires detailed modeling of the physical interactions that occur as the particles pass through the spacecraft and the instrument itself. In order to facilitate in the calibration of the MARIE data, we have begun a program to simulate the response of MARIE using the FLUKA [1] [2] Monte Carlo radiation transport code.
    Keywords: Instrumentation and Photography
    Type: Lunar and Planetary Science XXXIV; LPI-Contrib-1156
    Format: text
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