SDO HMI 2011-06-25 04:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.63 | 53.49 | 9.56 | 59.87 | 17.11 | 166.34 | 63.04 | 288.06 | 0.8977 | 8.3 | -211.2 | |
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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 |
| 0.00 | 2.09 | 0.00 | 2.44 | 15.87 | 167.77 | 64.47 | 286.53 | 0.9072 | -339.0 | -315.4 | |
| 0.00 | 0.54 | 0.00 | 0.62 | 14.79 | 167.15 | 63.86 | 285.39 | 0.9020 | -565.0 | -492.0 | |
| 1.45 | 10.90 | 1.69 | 12.70 | 16.47 | 167.69 | 64.40 | 287.20 | 0.9070 | -557.6 | -529.8 | |
| 0.00 | 1.82 | 0.00 | 2.32 | 19.96 | 169.84 | 66.55 | 290.76 | 0.9238 | 449.0 | 269.1 | |
| 0.82 | -3.00 | 0.95 | -3.00 | 16.92 | 167.53 | 64.24 | 287.71 | 0.9062 | -468.3 | 999999 | |
| 0.00 | 1.36 | 0.00 | 1.54 | 16.15 | 166.84 | 63.55 | 286.93 | 0.9007 | -527.0 | -519.9 | |
| 0.00 | 0.54 | 0.00 | 0.60 | 15.95 | 166.23 | 62.93 | 286.77 | 0.8960 | -230.0 | -258.3 | |
| 0.00 | 2.09 | 0.00 | 2.29 | 15.99 | 165.90 | 62.61 | 286.85 | 0.8936 | 227.0 | 176.0 | |
| 0.00 | 3.45 | 0.00 | 3.80 | 16.21 | 166.02 | 62.73 | 287.08 | 0.8947 | -328.0 | -273.8 | |
| 0.00 | 0.82 | 0.00 | 0.96 | 19.29 | 167.51 | 64.22 | 290.31 | 0.9080 | -172.0 | -181.1 | |
| 0.00 | 1.00 | 0.00 | 1.10 | 17.93 | 165.93 | 62.64 | 289.01 | 0.8955 | 182.0 | 179.5 | |
| 6.36 | 27.61 | 6.92 | 30.18 | 17.37 | 165.52 | 62.22 | 288.44 | 0.8920 | 367.1 | -153.7 | |
| 0.00 | 1.27 | 0.00 | 1.32 | 18.22 | 163.99 | 60.70 | 289.59 | 0.8812 | 313.0 | 224.0 | |
| 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. | |