SDO HMI 2014-10-08 06:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.76 | 0.00 | 10.72 | -16.90 | 106.33 | 17.26 | 215.97 | 0.4927 | 338.4 | 350.0 | |
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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 | 1.49 | 0.00 | 0.86 | -14.53 | 111.26 | 22.19 | 226.40 | 0.5070 | 759.0 | 575.5 | |
| 0.00 | 1.40 | 0.00 | 0.80 | -13.38 | 110.48 | 21.41 | 227.12 | 0.4868 | 788.0 | 637.9 | |
| 0.00 | 1.05 | 0.00 | 0.60 | -13.53 | 110.33 | 21.26 | 226.68 | 0.4866 | 835.0 | 632.8 | |
| 0.00 | 0.61 | 0.00 | 0.36 | -17.70 | 110.48 | 21.42 | 221.01 | 0.5322 | 737.0 | 667.0 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -17.89 | 110.44 | 21.37 | 220.70 | 0.5339 | 665.0 | 553.7 | |
| 0.00 | 2.28 | 0.00 | 1.29 | -14.15 | 109.27 | 20.20 | 224.27 | 0.4816 | 767.0 | 673.1 | |
| 0.00 | 1.84 | 0.00 | 1.06 | -18.18 | 107.99 | 18.92 | 216.96 | 0.5144 | 746.0 | 573.0 | |
| 0.00 | 0.97 | 0.00 | 0.54 | -15.52 | 107.29 | 18.22 | 219.39 | 0.4767 | 619.0 | 540.0 | |
| 0.00 | 1.84 | 0.00 | 1.04 | -15.32 | 107.21 | 18.14 | 219.53 | 0.4736 | 771.0 | 591.6 | |
| 0.00 | 1.32 | 0.00 | 0.81 | -25.91 | 107.01 | 17.94 | 207.66 | 0.5992 | 709.0 | 563.5 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -23.90 | 106.71 | 17.65 | 209.05 | 0.5729 | 592.0 | 478.5 | |
| 0.00 | 1.49 | 0.00 | 0.79 | -9.21 | 102.93 | 13.86 | 221.77 | 0.3566 | -652.0 | -572.1 | |
| 0.00 | 0.70 | 0.00 | 0.40 | -21.97 | 93.62 | 4.56 | 188.83 | 0.4816 | -782.0 | -677.1 | |
| 0.00 | 0.70 | 0.00 | 0.39 | -19.31 | 93.42 | 4.35 | 189.40 | 0.4403 | -755.0 | -655.1 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -19.79 | 91.65 | 2.58 | 185.49 | 0.4442 | -723.0 | -599.7 | |
| 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. | |