SDO HMI 2014-05-18 22:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.52 | 71.21 | 9.52 | 36.59 | 9.93 | 180.30 | 9.39 | 322.78 | 0.2678 | -299.3 | -318.5 | |
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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 | 1.35 | 0.00 | 0.69 | 7.35 | 183.10 | 12.18 | 308.41 | 0.2683 | -769.0 | -606.1 | |
| 0.00 | 1.71 | 0.00 | 0.88 | 10.30 | 181.53 | 10.62 | 320.09 | 0.2839 | -392.0 | -404.7 | |
| 11.78 | 47.73 | 6.06 | 24.55 | 9.74 | 181.26 | 10.35 | 319.49 | 0.2738 | -1099.3 | -713.7 | |
| 5.39 | -3.00 | 2.77 | -3.00 | 9.43 | 181.10 | 10.18 | 319.18 | 0.2680 | -1173.4 | 999999 | |
| 0.00 | 3.15 | 0.00 | 1.62 | 10.76 | 179.14 | 8.23 | 327.97 | 0.2663 | -813.0 | -802.2 | |
| 0.00 | 1.62 | 0.00 | 0.83 | 10.72 | 178.92 | 8.01 | 328.60 | 0.2639 | -848.0 | -673.2 | |
| 0.00 | 2.07 | 0.00 | 1.09 | 15.57 | 178.83 | 7.92 | 336.53 | 0.3348 | 972.0 | 809.2 | |
| 1.35 | 4.40 | 0.69 | 2.25 | 10.22 | 178.19 | 7.28 | 329.97 | 0.2503 | 790.9 | 648.8 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 10.53 | 177.73 | 6.82 | 332.16 | 0.2511 | 761.0 | 644.9 | |
| 0.00 | 3.15 | 0.00 | 1.61 | 10.07 | 177.60 | 6.69 | 331.72 | 0.2431 | 848.0 | 761.5 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 11.25 | 177.53 | 6.62 | 334.13 | 0.2604 | 897.0 | 712.6 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 7.10 | 177.42 | 6.51 | 325.29 | 0.1984 | 844.0 | 662.2 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 8.98 | 176.10 | 5.18 | 335.37 | 0.2151 | 817.0 | 664.9 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 11.55 | 174.09 | 3.18 | 347.16 | 0.2458 | 908.0 | 754.7 | |
| 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. | |