SDO HMI 2011-11-01 11:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.16 | 131.73 | 47.06 | 289.99 | -13.65 | 119.79 | -75.33 | 105.14 | 0.9743 | 159.6 | 54.5 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.33 | 76.94 | 8.29 | 146.49 | -15.42 | 122.03 | -73.09 | 107.25 | 0.9669 | 370.0 | 87.4 | |
| 4.59 | -1.00 | 8.44 | -1.00 | -14.67 | 122.49 | -72.64 | 106.55 | 0.9644 | 595.3 | 999999 | |
| 2.25 | -1.00 | 4.39 | -1.00 | -15.44 | 121.68 | -73.44 | 107.22 | 0.9684 | -237.8 | 999999 | |
| 2.51 | -1.00 | 4.77 | -1.00 | -14.98 | 122.00 | -73.13 | 106.80 | 0.9668 | 253.5 | 999999 | |
| 1.64 | -1.00 | 3.16 | -1.00 | -14.25 | 121.77 | -73.35 | 106.02 | 0.9673 | 231.9 | 999999 | |
| 0.00 | 1.30 | 0.00 | 3.30 | -17.33 | 118.32 | -76.80 | 108.65 | 0.9817 | -84.0 | -64.0 | |
| 0.00 | 1.30 | 0.00 | 2.71 | -13.74 | 120.42 | -74.71 | 105.29 | 0.9725 | -172.0 | -189.8 | |
| 0.00 | 1.82 | 0.00 | 4.59 | -15.58 | 118.21 | -76.91 | 106.86 | 0.9813 | -337.0 | -298.5 | |
| 1.90 | 4.76 | 5.41 | 13.52 | -15.81 | 116.89 | -78.23 | 106.92 | 0.9854 | -295.5 | -241.1 | |
| 0.00 | 5.80 | 0.00 | 16.01 | -15.36 | 117.04 | -78.09 | 106.49 | 0.9848 | 181.0 | 74.1 | |
| 0.00 | 0.78 | 0.00 | 1.78 | -13.47 | 119.06 | -76.06 | 104.84 | 0.9774 | -302.0 | -328.9 | |
| 3.81 | 39.03 | 9.64 | 101.59 | -10.91 | 117.51 | -77.61 | 102.05 | 0.9816 | 238.8 | 72.1 | |
| 1.13 | -12.00 | 2.96 | -12.00 | -11.00 | 117.13 | -77.99 | 102.10 | 0.9828 | -225.7 | 999999 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |