SDO HMI 2014-10-11 00:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.22 | 0.00 | 12.69 | 14.53 | 55.98 | 3.20 | 328.50 | 0.1682 | 77.5 | 46.8 | |
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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 | 0.62 | 14.79 | 60.74 | 7.96 | 318.37 | 0.2025 | -766.0 | -621.8 | |
| 0.00 | 4.73 | 0.00 | 2.42 | 18.20 | 60.67 | 7.88 | 328.07 | 0.2475 | -848.0 | -707.2 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 18.47 | 60.52 | 7.74 | 329.16 | 0.2502 | -781.0 | -605.5 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 17.65 | 60.29 | 7.51 | 328.05 | 0.2365 | -951.0 | -801.5 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 16.54 | 59.11 | 6.33 | 329.63 | 0.2101 | -837.0 | -608.4 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 12.67 | 58.81 | 6.03 | 317.94 | 0.1537 | 823.0 | 650.6 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 15.51 | 58.77 | 5.99 | 328.30 | 0.1921 | -768.0 | -615.3 | |
| 0.00 | 1.93 | 0.00 | 0.96 | 13.31 | 54.58 | 1.79 | 346.21 | 0.1284 | 875.0 | 800.8 | |
| 0.00 | 1.31 | 0.00 | 0.66 | 12.53 | 54.23 | 1.45 | 347.41 | 0.1138 | 942.0 | 729.5 | |
| 0.00 | 1.31 | 0.00 | 0.66 | 14.06 | 54.09 | 1.31 | 350.84 | 0.1396 | 906.0 | 653.1 | |
| 0.00 | 2.01 | 0.00 | 1.00 | 12.83 | 53.04 | 0.26 | 357.85 | 0.1164 | 828.0 | 701.3 | |
| 0.00 | 1.93 | 0.00 | 0.96 | 13.61 | 52.67 | -0.11 | 0.84 | 0.1300 | 821.0 | 590.3 | |
| 0.00 | 1.66 | 0.00 | 0.83 | 14.79 | 52.27 | -0.51 | 3.31 | 0.1507 | 876.0 | 699.2 | |
| 0.00 | 2.19 | 0.00 | 1.09 | 11.81 | 51.05 | -1.73 | 16.80 | 0.1030 | 782.0 | 520.6 | |
| 0.00 | 1.40 | 0.00 | 0.70 | 6.96 | 47.78 | -5.01 | 80.75 | 0.0882 | -740.0 | -476.2 | |
| 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. | |