Magnetogram and soft X-ray comparisons of XBP and ER

Details Magnetogram and soft X-ray comparisons of XBP and ER Magnetogram and soft X-ray comparisons of XBP and ER

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nascp2442..365g&link_type=abstract

In NASA. Goddard Space Flight Center Coronal and Prominence Plasmas p 365-367 (SEE N87-20871 13-92)

Physics

2

Data Correlation, Magnetic Flux, Solar Corona, Solar Cycles, Solar Granulation, Magnetic Signatures, Polarity, X Rays

Scientific paper

The potential importance of the smallest emerging flux regions on the sun was discussed in numerous publications. The association between the objects seen in ground-based data, such as high resolution magnetrons or H alpha and soft X-ray data has produced results which are often contradictory. In the hope of resolving the present impasse, as much simultaneous soft X-ray and magnetogram data as possible were assembled in order to clarify the situation. It was found that separation of magnetic features into chance encounters and emerging flux makes some difference in overlapp with X-ray bright points (XBPs), although the effect is not overwhelming. The difference in solar cycle dependence between XBP and ephemeral regions is not explainable in terms of the results.

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