1985 Coronal Synoptic Maps

With CME Lat/Long Overlay

These 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.

NOTE: These synoptic data are ONLY available for single-rotation maps.

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:

7-Rotation Maps [No CME overlay]

[ CR 1758-1764 2.0 Rsun ] [ CR 1758-1764 2.8 Rsun ] [ CR 1758-1764 3.4 Rsun ]
[ CR 1764-1770 2.0 Rsun ] [ CR 1764-1770 2.8 Rsun ] [ CR 1764-1770 3.4 Rsun ]

6-Rotation Maps [No CME overlay]

[ CR 1758-1763 2.0 Rsun ] [ CR 1758-1763 2.8 Rsun ] [ CR 1758-1763 3.4 Rsun ]
[ CR 1765-1770 2.0 Rsun ] [ CR 1765-1770 2.8 Rsun ] [ CR 1765-1770 3.4 Rsun ]

3-Rotation Maps [No CME overlay]

[ CR 1758-1760 2.0 Rsun ] [ CR 1758-1760 2.8 Rsun ] [ CR 1758-1760 3.4 Rsun ]
[ CR 1761-1763 2.0 Rsun ] [ CR 1761-1763 2.8 Rsun ] [ CR 1761-1763 3.4 Rsun ]
[ CR 1764-1766 2.0 Rsun ] [ CR 1764-1766 2.8 Rsun ] [ CR 1764-1766 3.4 Rsun ]
[ CR 1767-1769 2.0 Rsun ] [ CR 1767-1769 2.8 Rsun ] [ CR 1767-1769 3.4 Rsun ]

1-Rotation Maps [no CME overlay]

The synoptic maps below 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