ISSN:
1573-1626
Source:
Springer Online Journal Archives 1860-2000
Topics:
Architecture, Civil Engineering, Surveying
,
Geosciences
,
Physics
Description / Table of Contents:
Summary The structure of the interplanetary magnetic field (IMF) is investigated theoretically in a kinematic approximation under frozen-in conditions in the solar wind and non-stationary boundary conditions. As an example, a time-dependent model of the IMF, created in the case of a change of the general magnetic field of the Sun represented by the dipole term, is analyzed. Very simple assumptions as to the field of velocities in the solar wind are made. The results show the formation of zero IMF points of two types(O, X). Points of theO-type are formed and move radially in the equatorial plane. They are surrounded by magnetic clouds with loops of lines of force. Points of theX-type are formed and move radially above the poles.
Notes:
Резюме Теореmuческu uссле¶rt;овaнa сmрукmурa межnлaнеmно о мa нumно о nоля(ММП) в кuнемamuческом nрuблuженuu nрu условuu вмороженносmu в солнечном веmре u несmaцuонaрном рaнuчном условuu. В кaчесmве nрuмерa рaссмоmренa мо¶rt;ель ММП, вознuкaюще о nрu uзмененuu обще о мa нumно о nоля Солнцa, nре¶rt;сmaвленно о ¶rt;unольным членом, зaвuсящuм оm временu. Оmносumельно nоля скоросmеŭ в солнечном веmре с¶rt;елaны nросmеŭшuе nре¶rt;nоложенuя. Резульmamы nокaзывaюm обрaзовaнuе нулевых mочек ММП ¶rt;вух munов(O, X). ТочкuO-muna вознuкaюm u ¶rt;вuжуmся рa¶rt;uaльно в эквaроmuaльноŭ nлоскосmu. Онu окружены мa нumнымu облaкaмu с nеmлямu сuловых лuнuŭ. ТочкuX-muna вознuкaюm u ¶rt;вuжуmся рa¶rt;uaльно нa¶rt; nолюсaмu.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF01635606
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