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  • 1
    Electronic Resource
    Electronic Resource
    Amsterdam : Elsevier
    Scientia Horticulturae 50 (1992), S. 127-136 
    ISSN: 0304-4238
    Keywords: DIF ; [abr] ADT; average daily temperature ; [abr] DIF; difference between DT and NT ; [abr] DT; day temperature ; [abr] HPS; high pressure sodium lamps ; [abr] LD; long day(s) ; [abr] LDP; long day plant ; [abr] NT; night temperature ; [abr] PPFD; photosynthetic photon flux density ; [abr] RH; relative air humidity ; [abr] SD; short day(s) ; [abr] SDP; short day plant ; keeping quality ; poinsettia ; stem elongation ; supplementary lighting ; temperature
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Agriculture, Forestry, Horticulture, Fishery, Domestic Science, Nutrition
    Type of Medium: Electronic Resource
    Location Call Number Expected Availability
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  • 2
    Electronic Resource
    Electronic Resource
    Amsterdam : Elsevier
    Scientia Horticulturae 50 (1992), S. 127-136 
    ISSN: 0304-4238
    Keywords: DIF ; [abr] ADT; average daily temperature ; [abr] DIF; difference between DT and NT ; [abr] DT; day temperature ; [abr] HPS; high pressure sodium lamps ; [abr] LD; long day(s) ; [abr] LDP; long day plant ; [abr] NT; night temperature ; [abr] PPFD; photosynthetic photon flux density ; [abr] RH; relative air humidity ; [abr] SD; short day(s) ; [abr] SDP; short day plant ; keeping quality ; poinsettia ; stem elongation ; supplementary lighting ; temperature
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Agriculture, Forestry, Horticulture, Fishery, Domestic Science, Nutrition
    Type of Medium: Electronic Resource
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 3
    Publication Date: 2019-07-18
    Description: The Stellar Imager (SI) is a "Vision" mission in the Sun-Earth Connection (SEC) Roadmap, conceived for the purpose of understanding the effects of stellar magnetic fields, the dynamos that generate them, and the internal structure and dynamics of the stars in which they exist. The ultimate goal is to achieve the best possible forecasting of solar/stellar magnetic activity and its impact on life in the Universe. The science goals of SI require an ultra-high angular resolution, at ultraviolet wavelengths, on the order of 100 micro-arcsec and thus baselines on the order of 0.5 km. These requirements call for a large, multi-spacecraft (less than 20) imaging interferometer, utilizing precision formation flying in a stable environment, such as in a Lissajous orbit around the Sun-Earth L2 point. SI's resolution will make it an invaluable resource for many other areas of astrophysics, including studies of AGN s, supernovae, cataclysmic variables, young stellar objects, QSO's, and stellar black holes. ongoing mission concept and technology development studies for SI. These studies are designed to refine the mission requirements for the science goals, define a Design Reference Mission, perform trade studies of selected major technical and architectural issues, improve the existing technology roadmap, and explore the details of deployment and operations, as well as the possible roles of astronauts and/or robots in construction and servicing of the facility.
    Keywords: Astrophysics
    Type: 204th Meeting fo the American Astronomical Society; May 30, 2004 - Jun 03, 2004; Denver, CO; United States
    Format: text
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  • 4
    Publication Date: 2019-07-13
    Description: The Stellar Imager (SI) is a Vision Mission in the Sun-Earth Connection (SEC) NASA Roadmap, conceived for the purpose of understanding the effects of stellar magnetic fields, the dynamos that generate them, and the internal structure and dynamics of the stars in which they exist. The ultimate goal is to achieve the best possible forecasting of solar/stellar activity and its impact on life in the Universe. The science goals of SI require an ultra-high angular resolution, a t ultraviolet wavelengths, on the order of 100 micro-arcsec and baselines on the order of 0.5 km. These requirements call for a large, multi-spacecraft (〉20) imaging interferometer, utilizing precision formation flying in a stable environment, such as in a Lissajous orbit around the Sun-Earth L2 point. In this paper, we present an update on the ongoing SI mission concept and technology development studies.
    Keywords: Astrophysics
    Type: 2nd International Symposium on Formation Flying Missions and Technologies; Sep 14, 2004 - Sep 16, 2004; Crystal City, VA; United States
    Format: application/pdf
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