A General Theory of Connectivity and Current Sheets in Coronal Magnetic Fields Anchored to Discrete Sources

نویسندگان

  • D. W. Longcope
  • I. Klapper
چکیده

A scheme is presented for mapping the connectivity of a potential magnetic field arising from an arbitrary distribution of discrete sources. The field lines interconnecting the sources are classified into Nd domains, defining the field’s connectivity. The number of domains is shown to depend on the number of sources and on the numbers of nulls and separators according to a simple relation. A class of nonpotential equilibria are then generated by minimizing magnetic energy subject to constraints on the flux of each domain. The resulting equilibria are current-free within each domain and contain singular currents along each of the field’s separators. Subject headings:MHD — Sun: corona — Sun: magnetic fields

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Two-current-sheet Reconnection Model of Interdependent Flare and Coronal Mass Ejection

Time-dependent resistive magnetohydrodynamic simulations are carried out to study a flux rope eruption caused by magnetic reconnection with implication in coexistent flare-CME (coronal mass ejection) events. An early result obtained in a recent analysis of double catastrophe of a flux rope system is used as the initial condition, in which an isolated flux rope coexists with two current sheets: ...

متن کامل

Quasi-Static Theory for Uniaxial Chiral Omega Media

The problem of unbounded uniaxial chiral omega media in the presence of both static electric and magnetic point charges is investigated. For this purpose scalar electric and magnetic potentials in these media are introduced. Using these potentials, the corresponding electric and magnetic fields are determined. The similar problem of static electric and magnetic current sources with the goal of ...

متن کامل

Spectral Lines for Polarization Measurements of the Coronal Magnetic Field. Iv. Stokes Signals in Current-carrying Fields

We present the first theoretical, forward calculations of the Stokes profiles of several magnetic dipole (‘‘M1’’) coronal emission lines produced in current-carrying magnetic structures. An idealized coronal model of Low, Fong, and Fan is used, which describes a spherically symmetric, hydrostatic background atmosphere, isothermal at a coronal temperature of 1:6 ; 10 K. Embedded is a global, axi...

متن کامل

Solar Magnetic Tracking. V. As the Features Turn

The corona is hot, but we don’t know why. One explanation is that random convective motions “shuffle” the photospheric footpoints of magnetic fields that thread the corona, thereby inducing electric currents (perhaps current sheets) in the coronal magnetic field, and dissipation of these currents then heats the coronal plasma. The exact process leading to current dissipation is unknown,

متن کامل

Yet Another Application of the Theory of ODE in the Theory of Vector Fields

In this paper we are supposed to define the θ−vector field on the n−surface S and then investigate about the existence and uniqueness of its integral curves by the Theory of Ordinary Differential Equations. Then thesubject is followed through some examples.

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2002