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  • 1
    Electronic Resource
    Electronic Resource
    On the probability of occurrence of the type IIIb burst as a precursor (1974)
    Springer
    Solar physics 37 (1974), S. 225-233 
    Details
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract It is shown that a precursor type IIIb burst is really associated with a type III burst. The broad longitude distribution of occurrence of type IIIb bursts also suggests that these bursts are emitted at a large angle to the open magnetic field in the corona.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00157859
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    Paper (German National Licenses)
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  • 2
    Electronic Resource
    Electronic Resource
    Solar radio type III bursts and coronal density structures (1977)
    Springer
    Solar physics 52 (1977), S. 133-139 
    Details
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The comparison of solar radio type III bursts measured at 169 MHz with K corona observations leads to the conclusion that about 75% of the active regions over which type III bursts occur are associated with low density coronal structures. The comparison with X-ray maps of the solar disk shows that all these regions are located in low intensity regions. It is concluded that the idea generally accepted that the type III bursts are associated with dense coronal structures and travel in these structures is not at all proven for a large number of cases.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00935796
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    Paper (German National Licenses)
    Fulltext
  • 3
    Electronic Resource
    Electronic Resource
    The spectrum and position of solar noise storms at decameter wavelengths (1977)
    Springer
    Solar physics 55 (1977), S. 195-209 
    Details
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract Decametric storm radiation during the period July–August 1970 has been observed simultaneously with a high sensitivity spectrograph at Arecibo Observatory and with the log-periodic, swept-frequency array of the Clark Lake Radio Observatory. The observations complement each other; different types of fine structure emissions can be easily identified on the spectrograph records and their position can be determined from the swept-frequency recordings. We study the relative positions of the different emissions which have been observed during the storms. Four distinct sources appeared to be present. The continuum emission, the type I bursts and the flare-related type III's were all emitted at different locations. The storm type III bursts, type IIIb's and drift pairs overlapped in position, but appeared at different locations than the previously mentioned sources.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00150885
    Library Location Call Number Volume/Issue/Year Availability
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    Paper (German National Licenses)
    Fulltext
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