1987 Coronal Synoptic Maps

With CME Lat/Long Overlay

In the following list, "CR" represent Carrington Rotation. The number(s) following "CR" indicates the rotation designation(s). Finally, the height [units of solar radii] at which the synoptic map is created is provided.

Please choose a synoptic map of interest below:

6-Rotation Maps [No CME overlay]

[ CR 1787-1793 2.0 Rsun ] [ CR 1787-1793 2.8 Rsun ] [ CR 1787-1793 3.4 Rsun ]
[ CR 1791-1797 2.0 Rsun ] [ CR 1791-1797 2.8 Rsun ] [ CR 1791-1797 3.4 Rsun ]

4-Rotation Maps [No CME overlay]

[ CR 1787-1790 2.0 Rsun ] [ CR 1787-1790 2.8 Rsun ] [ CR 1787-1790 3.4 Rsun ]

3-Rotation Maps [No CME overlay]

[ CR 1787-1789 2.0 Rsun ] [ CR 1787-1789 2.8 Rsun ] [ CR 1787-1789 3.4 Rsun ]
[ CR 1790-1792 2.0 Rsun ] [ CR 1790-1792 2.8 Rsun ] [ CR 1790-1792 3.4 Rsun ]
[ CR 1793-1795 2.0 Rsun ] [ CR 1793-1795 2.8 Rsun ] [ CR 1793-1795 3.4 Rsun ]
[ CR 1796-1798 2.0 Rsun ] [ CR 1796-1798 2.8 Rsun ] [ CR 1796-1798 3.4 Rsun ]

1-Rotation Maps [no CME overlay]

The synoptic maps are similar to the standard versions. What's different is that Coronal Mass Ejections (CMEs) are indicated by marking the start/stop times with two vertical dashed red lines, and the minimum/maximum latitudes are represented by solid red horizontal lines.

1-Rotation Maps [With CME overlay]

Detailed information on all SMM mass ejections is available in the SMM Catalogue of Coronal Mass Ejections