SDO HMI 2014-11-12 14:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.66 | 0.00 | 8.04 | -10.19 | 338.19 | -4.92 | 160.35 | 0.2529 | -156.2 | -66.0 | |
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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 | 0.34 | 0.00 | 0.17 | -6.52 | 343.20 | 0.10 | 180.58 | 0.1687 | 256.0 | 501.8 | |
| 0.00 | 1.38 | 0.00 | 0.70 | -9.51 | 342.21 | -0.90 | 175.97 | 0.2207 | 989.0 | 865.1 | |
| 0.00 | 1.72 | 0.00 | 0.88 | -9.81 | 342.12 | -0.99 | 175.66 | 0.2260 | 813.0 | 611.0 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -14.30 | 341.88 | -1.23 | 176.05 | 0.3020 | 772.0 | 595.9 | |
| 0.00 | 1.55 | 0.00 | 0.79 | -10.94 | 341.42 | -1.69 | 173.22 | 0.2463 | 945.0 | 782.3 | |
| 0.00 | 0.77 | 0.00 | 0.40 | -11.16 | 340.11 | -2.99 | 168.29 | 0.2535 | 768.0 | 558.6 | |
| 0.00 | 0.77 | 0.00 | 0.40 | -12.27 | 337.24 | -5.87 | 159.39 | 0.2851 | -694.0 | -516.1 | |
| 0.00 | 1.21 | 0.00 | 0.62 | -9.64 | 336.81 | -6.30 | 153.95 | 0.2473 | -870.0 | -661.0 | |
| 0.00 | 1.38 | 0.00 | 0.71 | -10.04 | 336.44 | -6.67 | 153.35 | 0.2561 | -905.0 | -707.3 | |
| 0.00 | 1.12 | 0.00 | 0.58 | -10.90 | 335.72 | -7.39 | 152.48 | 0.2745 | -828.0 | -566.8 | |
| 0.00 | 1.12 | 0.00 | 0.58 | -11.18 | 335.19 | -7.91 | 151.33 | 0.2828 | -803.0 | -549.6 | |
| 0.00 | 0.86 | 0.00 | 0.44 | -10.05 | 334.71 | -8.40 | 147.73 | 0.2707 | -859.0 | -701.3 | |
| 0.00 | 1.03 | 0.00 | 0.53 | -8.02 | 334.33 | -8.77 | 141.97 | 0.2463 | -823.0 | -628.6 | |
| 0.00 | 1.46 | 0.00 | 0.75 | -7.90 | 334.12 | -8.98 | 141.01 | 0.2469 | -948.0 | -656.6 | |
| 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. | |