SDO HMI 2014-12-11 00:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.43 | 307.83 | 36.12 | 181.22 | -3.93 | 1.10 | 32.56 | 263.29 | 0.5428 | 892.7 | 360.8 | |
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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 |
| 35.44 | 280.48 | 20.94 | 165.35 | -4.12 | 1.42 | 32.88 | 263.00 | 0.5477 | 1094.6 | 369.1 | |
| 1.45 | 2.90 | 0.85 | 1.71 | -1.40 | 1.23 | 32.69 | 267.97 | 0.5424 | -868.1 | -702.5 | |
| 1.02 | -1.00 | 0.60 | -1.00 | -4.41 | 1.05 | 32.50 | 262.38 | 0.5427 | 819.8 | 999999 | |
| 2.81 | 9.20 | 1.65 | 5.39 | -2.85 | 0.88 | 32.34 | 265.26 | 0.5382 | 775.1 | 536.7 | |
| 4.69 | -1.00 | 2.75 | -1.00 | -4.03 | 0.89 | 32.34 | 263.06 | 0.5398 | 1216.6 | 999999 | |
| 11.16 | -1.00 | 6.55 | -1.00 | -3.79 | 0.77 | 32.23 | 263.48 | 0.5377 | 1274.7 | 999999 | |
| 0.77 | -4.00 | 0.45 | -4.00 | -2.55 | 0.70 | 32.15 | 265.79 | 0.5352 | 684.1 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.65 | -2.79 | 0.60 | 32.05 | 265.33 | 0.5340 | 669.0 | 603.8 | |
| 0.00 | 1.45 | 0.00 | 0.84 | -1.90 | 0.37 | 31.82 | 266.98 | 0.5299 | -538.0 | -523.1 | |
| 0.00 | 0.68 | 0.00 | 0.40 | -5.63 | 359.51 | 30.96 | 259.73 | 0.5224 | 684.0 | 598.6 | |
| 0.00 | 2.47 | 0.00 | 1.42 | -2.85 | 359.21 | 30.67 | 265.03 | 0.5135 | 629.0 | 508.6 | |
| 0.77 | 2.22 | 0.44 | 1.27 | -2.11 | 358.99 | 30.44 | 266.45 | 0.5094 | 876.4 | 752.7 | |
| 0.00 | 0.85 | 0.00 | 0.49 | -1.90 | 358.95 | 30.41 | 266.85 | 0.5087 | 862.0 | 789.7 | |
| 0.00 | 1.02 | 0.00 | 0.59 | -4.03 | 358.70 | 30.16 | 262.62 | 0.5074 | 763.0 | 647.8 | |
| 3.32 | 5.45 | 1.89 | 3.11 | -3.30 | 358.06 | 29.52 | 263.96 | 0.4967 | -838.3 | -636.3 | |
| 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. | |