Abstract This paper describes the results of studying the helium component of the solar-wind ion-flux measurement by the BMSW instrument on the Spektr-R satellite with a time resolution of 3 s. In contrast to most previous works that presented values averaged over large (hourly average or daily average) intervals, we have shown that the relative helium-ion abundance in the solar wind experiences considerable (by a few percent and even 10%) variations on such short intervals as 10 seconds or even several seconds.


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    Title :

    Observation of fast variations of the helium-ion abundance in the solar wind



    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource



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