SDO HMI 2011-11-25 07:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.43 | 64.16 | 24.22 | 60.83 | 16.33 | 298.43 | 57.52 | 288.24 | 0.8539 | -225.2 | -100.9 | |
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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 |
| 12.59 | 30.32 | 12.57 | 30.30 | 16.23 | 300.34 | 59.43 | 287.80 | 0.8703 | -660.1 | -254.4 | |
| 2.31 | 3.60 | 2.24 | 3.49 | 15.45 | 299.43 | 58.52 | 287.04 | 0.8618 | -520.9 | -380.7 | |
| 2.31 | 8.65 | 2.12 | 7.93 | 15.19 | 297.47 | 56.56 | 287.03 | 0.8444 | 223.6 | -102.5 | |
| 0.00 | 1.03 | 0.00 | 0.96 | 16.29 | 297.77 | 56.87 | 288.27 | 0.8486 | 256.0 | 287.7 | |
| 1.63 | -3.00 | 1.48 | -3.00 | 15.35 | 297.20 | 56.29 | 287.26 | 0.8422 | -392.5 | 999999 | |
| 0.00 | 1.11 | 0.00 | 1.01 | 16.07 | 296.83 | 55.93 | 288.17 | 0.8399 | -392.0 | -340.5 | |
| 0.00 | 1.03 | 0.00 | 0.93 | 16.22 | 296.73 | 55.83 | 288.37 | 0.8392 | -308.0 | -367.2 | |
| 0.00 | 1.97 | 0.00 | 1.77 | 16.08 | 296.40 | 55.49 | 288.26 | 0.8359 | -580.0 | -501.3 | |
| 0.00 | 0.60 | 0.00 | 0.54 | 16.72 | 296.57 | 55.66 | 288.99 | 0.8384 | 284.0 | 167.4 | |
| 0.00 | 0.77 | 0.00 | 0.69 | 17.45 | 295.80 | 54.89 | 289.99 | 0.8326 | 76.0 | 152.6 | |
| 1.28 | 8.74 | 1.13 | 7.70 | 17.33 | 295.42 | 54.51 | 289.93 | 0.8290 | 371.9 | 386.8 | |
| 5.31 | -11.00 | 4.68 | -11.00 | 17.61 | 295.44 | 54.53 | 290.26 | 0.8296 | 532.9 | 999999 | |
| 0.00 | 5.57 | 0.00 | 4.86 | 17.18 | 295.09 | 54.18 | 289.83 | 0.8257 | 560.0 | 495.7 | |
| 0.00 | 0.77 | 0.00 | 0.65 | 17.81 | 293.47 | 52.56 | 290.93 | 0.8116 | -497.0 | -463.9 | |
| 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. | |