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  • Solar Physics  (2)
  • Agroinfection  (1)
  • 2020-2023
  • 1995-1999  (3)
  • 1970-1974
  • 1995  (3)
  • 1
    ISSN: 1617-4623
    Keywords: Ds1 excision ; Maize Streak Virus ; Zea mays plants ; Agroinfection
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology
    Notes: Abstract A reverse genetic system for studying excision of the transposable elementDs1 in maize plants has been established previously. In this system, theDs1 element, as part of the genome of maize streak virus (MSV), is introduced into maize plants via agroinfection. In the presence of theAc element, excision ofDs1 from the MSV genome results in the appearance of viral symptoms on the maize plants. Here, we used this system to study DNA sequences requiredin cis for excision ofDs1. TheDs1 element contains theAc transposase binding motif AAACGG in only one of its subterminal regions (defined here as the 5′ subterminal region). We showed that mutation of these motifs abolished completely the excision capacity ofDs1. This is the first direct demonstration that the transposase binding motifs are essential for excision. Mutagenesis with oligonucleotide insertions in the other (3′) subterminal region resulted in elements with either a reduced or an increased excision efficiency, indicating that this subterminal region also has an important function.
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 2011-08-24
    Description: Coronal holes are the sources of the solar wind and, according to recent YOKOH observations, may undergo rapid changes which are associated with manifestations of explosive solar activity. Rapid changes in a hole's structure will produce rapid changes in the characteristics of the wind emerging from it and, in the particular c se of a sudden increase in wind velocity, this may lead to the formation of an interplanetary shock. We discuss the characteristics of shocks formed in such a way and compare them with interplanetary observations.
    Keywords: Solar Physics
    Type: International Solar Wind 8 Conference; 99; NASA-CR-199940
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  • 3
    Publication Date: 2011-08-24
    Description: Utilizing an iterative scheme, a self-consistent axisymmetric MHD model for the solar wind has been developed. We use this model to evaluate the properties of the solar wind issuing from the open polar coronal hole regions of the Sun, during solar minimum. We explore the variation of solar wind parameters across the extent of the hole and we investigate how these variations are affected by the geometry of the hole and the strength of the field at the coronal base.
    Keywords: Solar Physics
    Type: ; 65
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