FERMI-LAT-SCIENTIFIC PLOTS
3
Fermi-LAT localization of the high-energy emission (100 MeV–10 GeV) for the 2011 March 7 (left) and June 7 (right) flares. In each image, the Sun is displayed in heliographic coordinates, where the projection of the rotational axis of the Sun is along the Y-axis, the Z-axis is the line of sight (from the Sun to the observer) and the X-axis is the remaining orthogonal basis vector. The grid of constant heliographic latitude and longitude is yellow and lines of constant R.A. and Dec. (J2000) are white. The backgrounds are SDO/AIA images at 304 ̊A of the chromosphere and transition region around the Sun at the given epoch. The labels indicate the NOAA numbers of the active regions. The LAT localizations of the flares are shown by the green circles, solid and dashed lines at the 68% and 95% error radii
respectively.
3
Fermi-LAT localization of the high-energy emission (100 MeV–10 GeV) for the 2011 March 7 (left) and June 7 (right) flares. In each image, the Sun is displayed in heliographic coordinates, where the projection of the rotational axis of the Sun is along the Y-axis, the Z-axis is the line of sight (from the Sun to the observer) and the X-axis is the remaining orthogonal basis vector. The grid of constant heliographic latitude and longitude is yellow and lines of constant R.A. and Dec. (J2000) are white. The backgrounds are SDO/AIA images at 304 ̊A of the chromosphere and transition region around the Sun at the given epoch. The labels indicate the NOAA numbers of the active regions. The LAT localizations of the flares are shown by the green circles, solid and dashed lines at the 68% and 95% error radii
respectively.