SDO HMI 2014-10-15 10:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.24 | 407.57 | 38.81 | 246.26 | -21.17 | 17.05 | 22.51 | 218.61 | 0.5745 | 985.6 | 350.3 | |
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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 |
| 1.14 | 395.85 | 0.69 | 239.30 | -21.74 | 17.70 | 23.17 | 218.74 | 0.5862 | 350.7 | 364.6 | |
| 31.55 | -1.00 | 19.12 | -1.00 | -21.23 | 17.48 | 22.94 | 219.07 | 0.5788 | 1153.5 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.63 | -19.62 | 17.16 | 22.62 | 220.61 | 0.5588 | 262.0 | 210.2 | |
| 31.55 | -1.00 | 19.00 | -1.00 | -21.00 | 16.89 | 22.35 | 218.61 | 0.5710 | 1350.5 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.57 | -20.77 | 14.55 | 20.01 | 215.89 | 0.5481 | 674.0 | 535.4 | |
| 0.00 | 1.92 | 0.00 | 1.15 | -22.09 | 14.63 | 20.10 | 214.54 | 0.5639 | 747.0 | 565.8 | |
| 0.00 | 0.70 | 0.00 | 0.41 | -19.92 | 14.06 | 19.53 | 216.21 | 0.5341 | 724.0 | 552.2 | |
| 0.00 | 1.49 | 0.00 | 0.87 | -20.97 | 13.45 | 18.92 | 214.17 | 0.5411 | -645.0 | -559.2 | |
| 0.00 | 0.61 | 0.00 | 0.36 | -21.19 | 13.18 | 18.64 | 213.54 | 0.5416 | 815.0 | 652.7 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -25.72 | 11.30 | 16.77 | 206.58 | 0.5832 | -594.0 | -451.5 | |
| 0.00 | 1.14 | 0.00 | 0.66 | -21.33 | 10.34 | 15.80 | 209.24 | 0.5214 | -652.0 | -577.1 | |
| 0.00 | 1.40 | 0.00 | 0.82 | -22.77 | 9.83 | 15.30 | 207.09 | 0.5363 | -732.0 | -536.6 | |
| 0.00 | 1.31 | 0.00 | 0.80 | -29.03 | 3.98 | 9.44 | 194.11 | 0.5906 | -447.0 | -439.8 | |
| 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. | |