SDO HMI 2014-05-15 23:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.31 | 41.87 | 6.41 | 21.82 | 8.48 | 195.62 | -14.42 | 52.00 | 0.3131 | -258.2 | 35.3 | |
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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 |
| 0.00 | 1.89 | 0.00 | 0.97 | 7.25 | 198.14 | -11.90 | 50.28 | 0.2671 | -863.0 | -680.2 | |
| 5.48 | 7.99 | 2.82 | 4.12 | 8.08 | 197.99 | -12.05 | 48.28 | 0.2781 | -1158.8 | -851.8 | |
| 0.00 | 2.33 | 0.00 | 1.20 | 6.67 | 198.03 | -12.01 | 52.27 | 0.2625 | -708.0 | -601.5 | |
| 0.00 | 1.89 | 0.00 | 0.97 | 8.61 | 197.76 | -12.28 | 47.43 | 0.2869 | -940.0 | -708.6 | |
| 0.00 | 1.71 | 0.00 | 0.88 | 8.58 | 197.54 | -12.50 | 48.00 | 0.2893 | -873.0 | -652.8 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 8.46 | 197.23 | -12.81 | 49.01 | 0.2919 | -952.0 | -841.2 | |
| 0.45 | 1.80 | 0.23 | 0.93 | 8.55 | 197.04 | -13.00 | 49.18 | 0.2953 | -1070.4 | -815.6 | |
| 0.00 | 1.53 | 0.00 | 0.79 | 8.34 | 196.67 | -13.37 | 50.52 | 0.2978 | -864.0 | -731.8 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 8.21 | 194.81 | -15.23 | 54.44 | 0.3211 | -936.0 | -749.1 | |
| 1.62 | 5.03 | 0.85 | 2.65 | 9.27 | 194.12 | -15.92 | 53.01 | 0.3403 | 1123.5 | 946.7 | |
| 2.15 | 8.08 | 1.14 | 4.26 | 9.25 | 193.74 | -16.30 | 53.71 | 0.3451 | 1029.4 | 787.4 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 8.79 | 193.41 | -16.63 | 55.35 | 0.3453 | 834.0 | 686.9 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 7.74 | 193.46 | -16.58 | 57.89 | 0.3354 | 745.0 | 565.2 | |
| 0.90 | 5.93 | 0.47 | 3.12 | 8.39 | 193.33 | -16.71 | 56.45 | 0.3427 | 1098.2 | 874.6 | |
| 1.71 | -14.00 | 0.90 | -14.00 | 8.45 | 193.20 | -16.84 | 56.50 | 0.3451 | 1002.9 | 999999 | |
| 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. | |