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Forward modeling of the coronal response to reconnection in an X-ray bright point (1999)

Kankelborg, Charles ; Longcope, Dana

Springer

Solar physics 190 (1999), S. 59-77

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ISSN: 1573-093X

Source: Springer Online Journal Archives 1860-2000

Topics: Physics

Notes: Abstract We use MDI magnetic field observations and the theory of reconnection through a separator to constrain a numerical simulation of an X-ray bright point observed in EUV by TRACE. A gasdynamic model is employed to describe the corona and transition region in the bright point loop. Nonlocal effects such as opacity and ambipolar diffusion are important to the transition region; these effects are approximated locally by modification of the radiative loss and thermal conduction. A straightforward comparison of measured light curves versus those generated by the simulation shows that the reconnection model is unable to account for the observations.

Type of Medium: Electronic Resource

URL: http://dx.doi.org/10.1023/A:1005205807984

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