SDO HMI 2014-10-07 04:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.88 | 17.92 | 0.67 | 13.35 | -13.51 | 59.06 | -44.29 | 114.55 | 0.7480 | 259.1 | 217.4 | |
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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 | 1.23 | 0.00 | 0.87 | -12.74 | 61.85 | -41.51 | 114.95 | 0.7153 | 662.0 | 553.6 | |
| 0.00 | 3.16 | 0.00 | 2.24 | -12.82 | 61.63 | -41.73 | 114.94 | 0.7181 | 803.0 | 703.7 | |
| 0.00 | 0.26 | 0.00 | 0.19 | -13.00 | 61.34 | -42.02 | 115.02 | 0.7221 | 259.0 | 399.0 | |
| 0.00 | 2.46 | 0.00 | 1.76 | -12.81 | 60.96 | -42.39 | 114.58 | 0.7253 | 761.0 | 576.7 | |
| 0.00 | 1.76 | 0.00 | 1.26 | -12.97 | 60.89 | -42.47 | 114.75 | 0.7269 | 752.0 | 606.2 | |
| 0.00 | 0.88 | 0.00 | 0.65 | -15.44 | 59.87 | -43.49 | 117.32 | 0.7489 | 514.0 | 437.7 | |
| 0.00 | 0.79 | 0.00 | 0.60 | -13.45 | 58.12 | -45.24 | 114.01 | 0.7582 | -677.0 | -542.1 | |
| 0.00 | 2.99 | 0.00 | 2.28 | -13.30 | 57.58 | -45.77 | 113.58 | 0.7632 | -802.0 | -650.8 | |
| 0.88 | 2.02 | 0.67 | 1.55 | -12.27 | 57.12 | -46.24 | 112.10 | 0.7640 | -554.2 | -475.6 | |
| 0.00 | 1.76 | 0.00 | 1.42 | -15.63 | 55.57 | -47.79 | 115.49 | 0.7924 | 474.0 | 415.6 | |
| 0.00 | 0.61 | 0.00 | 0.53 | -18.03 | 53.68 | -49.67 | 117.43 | 0.8189 | 390.0 | 353.9 | |
| 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. | |