SDO HMI 2014-08-05 00:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.60 | 0.00 | 12.20 | -18.69 | 239.93 | 22.29 | 221.06 | 0.5487 | 235.6 | 331.2 | |
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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 | 0.72 | 0.00 | 0.44 | -16.84 | 244.04 | 26.40 | 228.35 | 0.5718 | 558.0 | 428.2 | |
| 0.00 | 0.81 | 0.00 | 0.49 | -17.47 | 243.32 | 25.68 | 226.73 | 0.5699 | 653.0 | 535.1 | |
| 0.00 | 1.81 | 0.00 | 1.08 | -17.67 | 242.61 | 24.97 | 225.67 | 0.5644 | 754.0 | 624.4 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -17.21 | 242.12 | 24.48 | 225.72 | 0.5550 | 631.0 | 520.8 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -17.18 | 241.35 | 23.71 | 224.87 | 0.5466 | 514.0 | 369.6 | |
| 0.00 | 0.81 | 0.00 | 0.49 | -19.33 | 241.06 | 23.42 | 221.74 | 0.5656 | 644.0 | 486.8 | |
| 0.00 | 4.34 | 0.00 | 2.58 | -19.19 | 240.31 | 22.67 | 220.99 | 0.5570 | 818.0 | 729.9 | |
| 0.00 | 4.43 | 0.00 | 2.64 | -19.77 | 239.73 | 22.09 | 219.56 | 0.5577 | 670.0 | 618.8 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -18.26 | 238.83 | 21.19 | 220.28 | 0.5329 | 681.0 | 530.2 | |
| 0.00 | 1.54 | 0.00 | 0.90 | -20.11 | 237.11 | 19.47 | 215.72 | 0.5381 | -786.0 | -680.2 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -18.45 | 236.87 | 19.23 | 217.36 | 0.5168 | -700.0 | -573.5 | |
| 0.00 | 0.63 | 0.00 | 0.37 | -18.51 | 236.61 | 18.96 | 216.91 | 0.5151 | -585.0 | -551.4 | |
| 0.00 | 1.54 | 0.00 | 0.88 | -17.46 | 236.22 | 18.58 | 217.66 | 0.4994 | -789.0 | -660.8 | |
| 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. | |