Results 41 to 50 of about 585,007 (286)
Evolution of the interplanetary magnetic field [PDF]
, 1994 Remote observations of magnetic field topologies in the solar corona and in situ observations of the solar wind and interplanetary magnetic field (IMF) in interplanetary space are used to examine the temporal evolution of the spatial distribution of open and closed field regions emanating from the Sun.
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32. Interplanetary magnetic field [PDF]
Symposium - International Astronomical Union, 1958 The magnetic field outside the sun (interplanetary magnetic field) is certainly far from a dipole field. A model of it has recently been suggested (Tellus,8, 1, 1956). This model is in agreement with cosmic ray and magnetic storm data and reconcilable with the coronal ray structure. Some possibilities to check the model are discussed.
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Revised time-of-flight calculations for high-latitude geomagnetic pulsations using a realistic magnetospheric magnetic field model [PDF]
, 2005 We present a simple time-of-flight analysis of Alfvén pulsations standing on closed terrestrial magnetic field lines. The technique employed in this study in order to calculate the characteristic period of such oscillations builds upon earlier time-of ...
Waters, C. L. +2 more
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Acceleration of an interplanetary shock through the magnetosheath: a global hybrid simulation
Frontiers in Astronomy and Space SciencesAccording to most observations and simulations, interplanetary shocks slow down when they propagate through the magnetosheath. In this article, we present results from a self-consistent global hybrid PIC simulation of an interplanetary shock which, by ...
C. Moissard +4 more
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Magnetic clouds seen at different locations in the heliosphere [PDF]
Annales Geophysicae, 2008 We analyze two magnetic clouds (MCs) observed in different points of the heliosphere. The main aim of the present study is to provide a link between the different aspects of this phenomenon, starting with information on the origins of the MCs at the ...
L. Rodriguez +13 more
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Forecasting intense geomagnetic activity using interplanetary magnetic field data [PDF]
Annales Geophysicae, 2008 Southward interplanetary magnetic fields are considered traces of geoeffectiveness since they are a main agent of magnetic reconnection of solar wind and magnetosphere.
E. Saiz, C. Cid, Y. Cerrato
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A model of interplanetary and coronal magnetic fields [PDF]
Solar Physics, 1969 Green function solution to Maxwell equations for interplanetary and coronal magnetic fields above photosphere, considering field at source ...
Kenneth H. Schatten +2 more
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Mercury’s Bow Shock and Magnetopause Variations According to MESSENGER Data
UniverseUsing data from the MESSENGER spacecraft magnetometer that describes the magnetopause and the bow shock crossing points of the Mercury’s magnetosphere, we have calculated the parameters of the paraboloids of revolution approximating the obtained points ...
Dmitry Nevsky +2 more
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Propagation Characteristics of Two Coronal Mass Ejections From the Sun Far into Interplanetary Space [PDF]
, 2017 Propagation of coronal mass ejections (CMEs) from the Sun far into interplanetary space is not well understood due to limited observations. In this study we examine the propagation characteristics of two geo-effective CMEs, which occurred on 2005 May 6 and 13, respectively. Significant heliospheric consequences associated with the two CMEs are observed,
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Evolution of Coronal and Interplanetary Magnetic Fields [PDF]
Symposium - International Astronomical Union, 1980 Numerous studies have provided the detailed information necessary for a substantive synthesis of the empirical relation between the magnetic field of the sun and the structure of the interplanetary field. We will point out the latest techniques and studies of the global solar magnetic field and its relation to the interplanetary field. The potential to
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