SDO HMI 2011-11-24 13:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.55 | 51.37 | 24.19 | 61.68 | 18.77 | 315.56 | 64.75 | 289.89 | 0.9116 | -141.9 | -130.5 | |
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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 |
| 0.00 | 2.74 | 0.00 | 3.60 | 18.50 | 317.99 | 67.18 | 289.29 | 0.9278 | -23.0 | -53.4 | |
| 0.43 | 17.47 | 0.57 | 22.78 | 18.77 | 318.13 | 67.33 | 289.57 | 0.9288 | -281.8 | -324.6 | |
| 0.00 | 0.77 | 0.00 | 0.97 | 17.40 | 316.92 | 66.12 | 288.22 | 0.9203 | -451.0 | -390.3 | |
| 4.54 | -2.00 | 5.91 | -2.00 | 18.81 | 317.76 | 66.95 | 289.65 | 0.9266 | -686.2 | 999999 | |
| 0.00 | 1.03 | 0.00 | 1.28 | 17.53 | 316.71 | 65.90 | 288.38 | 0.9190 | -292.0 | -378.1 | |
| 3.51 | 5.39 | 4.39 | 6.76 | 17.81 | 316.83 | 66.02 | 288.67 | 0.9200 | -544.6 | -341.8 | |
| 0.00 | 1.03 | 0.00 | 1.17 | 17.97 | 314.22 | 63.41 | 289.15 | 0.9023 | 160.0 | 161.9 | |
| 4.28 | 6.59 | 5.00 | 7.71 | 19.20 | 314.78 | 63.97 | 290.43 | 0.9074 | -496.9 | -82.0 | |
| 2.05 | 2.48 | 2.22 | 2.68 | 18.48 | 312.50 | 61.69 | 289.96 | 0.8903 | 342.5 | 175.0 | |
| 0.00 | 1.28 | 0.00 | 1.39 | 18.67 | 312.55 | 61.74 | 290.16 | 0.8908 | 217.0 | 186.0 | |
| 0.00 | 0.77 | 0.00 | 0.81 | 18.01 | 311.62 | 60.81 | 289.55 | 0.8831 | 363.0 | 285.7 | |
| 5.74 | 10.19 | 6.10 | 10.86 | 19.47 | 311.87 | 61.06 | 291.15 | 0.8867 | 546.0 | 199.9 | |
| 0.00 | 1.63 | 0.00 | 1.67 | 19.37 | 310.84 | 60.04 | 291.21 | 0.8787 | 600.0 | 461.3 | |
| 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. | |