Erratum: An Assessment of Magnetic Conditions for Strong Coronal Heating in Solar Active Regions by Comparing Observed Loops with Computed Potential Field Lines

Details Erratum: An Assessment of Magnetic Conditions for Strong Coronal Heating in Solar Active Regions by Comparing Observed Loops with Computed Potential Field Lines Erratum: An Assessment of Magnetic Conditions for Strong Coronal Heating in Solar Active Regions by Comparing Observed Loops with Computed Potential Field Lines

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000apj...538..467f&link_type=abstract

The Astrophysical Journal, Volume 538, Issue 1, pp. 467-467.

Astronomy and Astrophysics

Astrophysics

Scientific paper

In the paper ``An Assessment of Magnetic Conditions for Strong Coronal Heating in Solar Active Regions by Comparing Observed Loops with Computed Potential Field Lines'' by D. A. Falconer, G. A. Gary, R. L. Moore, and J. G. Porter (ApJ, 528, 1004 [2000]), Figure 4 was rotated 180° and so did not match the figure caption. The correct orientation and figure caption is given here.

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