SDO HMI 2014-11-07 02:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.83 | 126.04 | 25.00 | 131.50 | 13.48 | 117.29 | 61.69 | 283.27 | 0.8811 | -451.7 | -181.1 | |
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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 |
| 21.41 | 109.90 | 22.85 | 117.33 | 13.97 | 118.01 | 62.41 | 283.81 | 0.8876 | -684.8 | -208.3 | |
| 0.35 | 1.47 | 0.31 | 1.33 | 7.82 | 112.50 | 56.91 | 276.88 | 0.8382 | -535.0 | -453.2 | |
| 0.86 | 2.07 | 0.78 | 1.87 | 8.06 | 112.44 | 56.85 | 277.17 | 0.8377 | -634.3 | -531.1 | |
| 0.43 | 1.90 | 0.39 | 1.70 | 7.89 | 112.24 | 56.65 | 276.98 | 0.8357 | -697.6 | -626.8 | |
| 0.00 | 1.12 | 0.00 | 1.06 | 13.27 | 113.83 | 58.24 | 283.28 | 0.8524 | -532.0 | -461.9 | |
| 0.00 | 1.21 | 0.00 | 1.09 | 11.55 | 112.49 | 56.90 | 281.34 | 0.8392 | 407.0 | 289.9 | |
| 0.78 | 2.16 | 0.67 | 1.85 | 8.32 | 110.45 | 54.86 | 277.53 | 0.8184 | 534.8 | 428.4 | |
| 0.00 | 0.86 | 0.00 | 0.74 | 10.89 | 110.28 | 54.69 | 280.68 | 0.8177 | 396.0 | 369.3 | |
| 0.00 | 0.69 | 0.00 | 0.58 | 7.92 | 109.54 | 53.95 | 277.06 | 0.8091 | 570.0 | 445.8 | |
| 0.00 | 1.12 | 0.00 | 0.96 | 10.71 | 110.13 | 54.54 | 280.48 | 0.8161 | 490.0 | 432.8 | |
| 0.00 | 1.38 | 0.00 | 1.16 | 8.10 | 109.47 | 53.88 | 277.29 | 0.8085 | 420.0 | 289.2 | |
| 0.00 | 2.16 | 0.00 | 1.83 | 10.72 | 109.93 | 54.33 | 280.50 | 0.8141 | 348.0 | 352.3 | |
| 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. | |