Image Details

Choose export citation format:

THE FORMATION OF IRIS DIAGNOSTICS. VI. THE DIAGNOSTIC POTENTIAL OF THE C II LINES AT 133.5 nm IN THE SOLAR ATMOSPHERE

  • Authors: Bhavna Rathore, Mats Carlsson, Jorrit Leenaarts, and Bart De Pontieu

2015 The Astrophysical Journal 811 81.

  • Provider: AAS Journals

Caption: Figure 7.

PDF of formation height as a function of transition region height (defined to be the lowest height in a column where the temperature is greater than 30 kK) for the C II 133.4 nm line (left) and the C II 133.5 nm line (right). Each column in the panels is scaled to maximum contrast to increase visibility. The green contours encompass 50% and 90% of all points. The Pearson correlation coefficient is given in the upper left corner, the red line denotes y = x.

Other Images in This Article

Show More

Copyright and Terms & Conditions