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  • 1
    Electronic Resource
    Electronic Resource
    Shift measurements of H"α and H"β lines in arc plasmas
    Amsterdam : Elsevier
    Journal of Quantitative Spectroscopy and Radiative Transfer 36 (1986), S. 233-237 
    Details
    ISSN: 0022-4073
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Physics
    Type of Medium: Electronic Resource
    URL: http://linkinghub.elsevier.com/retrieve/pii/0022-4073(86)90070-1
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  • 2
    Electronic Resource
    Electronic Resource
    Asymmetry of the peaks of the H"β spectral line
    Amsterdam : Elsevier
    Journal of Quantitative Spectroscopy and Radiative Transfer 39 (1988), S. 347-351 
    Details
    ISSN: 0022-4073
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Physics
    Type of Medium: Electronic Resource
    URL: http://linkinghub.elsevier.com/retrieve/pii/0022-4073(88)90099-4
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  • 3
    Electronic Resource
    Electronic Resource
    Shift of the peaks of the H"β spectral line
    Amsterdam : Elsevier
    Journal of Quantitative Spectroscopy and Radiative Transfer 42 (1989), S. 571-573 
    Details
    ISSN: 0022-4073
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Physics
    Type of Medium: Electronic Resource
    URL: http://linkinghub.elsevier.com/retrieve/pii/0022-4073(89)90049-6
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  • 4
    Electronic Resource
    Electronic Resource
    A universal interpretation of the generation of geomagnetic storms using features of the solar corona
    Amsterdam : Elsevier
    Planetary and Space Science 17 (1969), S. 1039-1044 
    Details
    ISSN: 0032-0633
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Geosciences , Physics
    Type of Medium: Electronic Resource
    URL: http://linkinghub.elsevier.com/retrieve/pii/0032-0633(69)90108-1
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  • 5
    Electronic Resource
    Electronic Resource
    New Method of Forecasting Geomagnetic Activity using Features of the Solar Corona (1968)
    [s.l.] : Nature Publishing Group
    Nature 220 (1968), S. 250-251 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] From the point of view of geomagnetic effects, coronal streams and the minimum type corona are significant. The coronal stream above the centre of the solar disk is followed by a geomagnetic disturbance either with a sudden commencement, provided the stream was formed in the central region, or with ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/220250b0
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  • 6
    Electronic Resource
    Electronic Resource
    The intensity of the main phase of geomagnetic storms in relation to the parameters of the solar wind (1976)
    Springer
    Studia geophysica et geodaetica 20 (1976), S. 408-410 
    Details
    ISSN: 1573-1626
    Source: Springer Online Journal Archives 1860-2000
    Topics: Architecture, Civil Engineering, Surveying , Geosciences , Physics
    Notes: Summary On the basis of investigating 10 storms (1965–1967) good correlation was found between the density of the solar wind energy (ε2=1/2mNv2) and the intensity of the main phase of the geomagnetic storms, expressed in terms of the maximum decrease of the horizontal intensity (ΔB=ΔH/cosφ). The relation between ε2, or Nv2, and δB could then be used to determine the quantities β and ε0 (β is the factor expressing the increase in energy density in the magnetosphere, ε0 is the energy density of the particles in a quiet magnetosphere). A comparison with the directly observed distribution of the energy density of the particles in the magnetosphere indicates that the computed value of ε0 seems to be realistic. The magnitude of the factor β will have to be checked again.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF01617655
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  • 7
    Electronic Resource
    Electronic Resource
    Effect of the ns component of the interplanetary magnetic field on geomagnetic storms (1977)
    Springer
    Studia geophysica et geodaetica 21 (1977), S. 360-365 
    Details
    ISSN: 1573-1626
    Source: Springer Online Journal Archives 1860-2000
    Topics: Architecture, Civil Engineering, Surveying , Geosciences , Physics
    Notes: Summary The individual storm-time variations of the geomagnetic field were compared with the variations of the Bz-component of the interplanetary magnetic field over 24 and 48-hour intervals of storm time. Good correlation between Bz and Dst was observed in about one half of the 166 cases analysed (1965–72), the time lag of the manifestations of the interplanetary field at the Earth's surface having been taken into account. The effect of the Bz-field is reflected to a considerably larger extent in intense storms (Dst ≦ −80 nT). Good correlation was observed in 80% of the total number of 35 intense storms. Preliminary investigations have shown that Dst-variations, constructed from Bz-data using the relations derived herein, are quite close to the observed, particularly as regards the main phase (3 examples are given).
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF01613268
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  • 8
    Electronic Resource
    Electronic Resource
    Important flare events in variations of the auroral electrojet index (1977)
    Springer
    Studia geophysica et geodaetica 21 (1977), S. 410-414 
    Details
    ISSN: 1573-1626
    Source: Springer Online Journal Archives 1860-2000
    Topics: Architecture, Civil Engineering, Surveying , Geosciences , Physics
    Notes: Summary The effects of solar proton flares and enhanced solar activity, indicated by intensive radio bursts in the decimetre range, on the Auroral Electrojet (AE) Index at the time these events occurred, are investigated. A significant increase in the level of the AE index was observed after the occurrence of these events.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF01613276
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  • 9
    Electronic Resource
    Electronic Resource
    Analysis of quantitative relations between magnetic storms and interplanetary parameters (1983)
    Springer
    Studia geophysica et geodaetica 27 (1983), S. 257-272 
    Details
    ISSN: 1573-1626
    Source: Springer Online Journal Archives 1860-2000
    Topics: Architecture, Civil Engineering, Surveying , Geosciences , Physics
    Notes: Резюме Получены колuчесmвенные сооmношенuя u uзучены корреляцuонные связu меж¶rt;у мaксuмaльным nонuженuем орuзонmaльноŭ сосmaвляющеŭ еомa нumно о nоля(Dst-min.) в лaвноŭ фaзе мa нumных бурь u межnлaнеmнымu naрaмеmрaмu Еу (у-сосmaвляюшaя межnлaнеmно о элекmрuческо о nоля) u ε ( = vВ 2 sin 4 (1/2 Θ) l 0 2 ). В aнaлuзе рaссмоmрено l-чaсовое зanaз¶rt;ывaнuе nо временu Dst nо оmношенuю Еу u ε. Корреляцuя Dst-min. с эmuмu naрaмеmрaмu хорошaя. Резульmamы, nолученные nрu ¶rt;еmaльном aнaлuзе колuчесmвенных хaрaкmерuсmuк связеŭ, усmaновленных нa основaнuu нaзвaнных naрaмеmров, срaвнuвaюmся с mочкu зренuя фuзuческоŭ uнmерnреmaцuu. Большaя обобщенносmя nрuсущa сооmношенuям, включaющuм ε. Щылa maкже оnре¶rt;еленa корреляцuя меж¶rt;у Dst u межnлaнеmнымu naрaмеmрaмu ¶rt;ля оm¶rt;ельных 48-чaсовых uнmервaлов бурь, nрuчем хорошaя корреляцuя nроявляеmся ¶rt;ля 50% бурь Сооmношенuя, nолученные нa основaнuu uзолuровaнных знaченuŭ Dst-min. u Dst — вaрuaцuŭ, чuсленно срaвнuвaюmся. Для эmuх ¶rt;вух вaрuaнmов со лaсuе резульmamов вырaзumельнее ¶rt;ля naрaмеmрa ε, чем ¶rt;ля Еу.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF01592795
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  • 10
    Electronic Resource
    Electronic Resource
    Supply of energy to the magnetosphere during the main phase of magnetic storms (1984)
    Springer
    Studia geophysica et geodaetica 28 (1984), S. 82-89 
    Details
    ISSN: 1573-1626
    Source: Springer Online Journal Archives 1860-2000
    Topics: Architecture, Civil Engineering, Surveying , Geosciences , Physics
    Notes: Резюме Анaлuз uсхо¶rt;um uз сооmношенuя меж¶rt;у общеŭ кuнеmuческоŭ энергuеŭ чaсmuц, зaхвaченных мaгнumосфероŭ, u nонuженuем нanряженносmuгеомaгнumного nоля в mеченuе буры, a maкже uз nре¶rt;nоложенuя, чmо возрaсmaнuе энергuu в мaгнumосфере в mеченuе бурu( глaвноŭ фaзы) nроnорцuонaльно nереносuмоŭ uз межnлaнеmного nросmрaнсmвa в мaгнumосферу мощносmu, вырaжaемоŭ через naрaмеmры Еу uлu ε. Из срaвненuя mеореmuческuх сооmношенuŭ u нa основaнuu ¶rt;aнных aнaлuзa выбрaнных бурь ¶rt;aеmся оценкa оmносumельноŭ велuчuныгеомеmрuческuх naрaмеmров ¶rt;aнного nроцессa u фaкmорa, оnре¶rt;еляющего рaсхо¶rt; энергuu nрu мaксuмaльноŭ ¶rt;еnрессuuгеомaгнumного nоля в mеченuе бурu. Полученные сооmношенuя меж¶rt;у nрuросmом энергuu, вырaженным сооmвеmсmвующuмu межnлaнеmнымu naрaмеmрaмu Еу, ε ¶rt;ля оm¶rt;ельных бурь u мaксuмaльным nонuженuем нanряженносmuгеомaгнumного nоля, обнaружuвaюm высокую сmеnень корреляцuu, особенно в случaе с учеmом naрaмеmрa ε.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF01587112
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