SDO HMI 2014-04-11 06:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.05 | 0.00 | 10.13 | -12.61 | 304.47 | -4.21 | 141.98 | 0.1891 | 137.0 | 76.9 | |
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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 | 1.15 | 0.00 | 0.58 | -11.86 | 320.85 | 12.17 | 242.82 | 0.2330 | 787.0 | 618.4 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -10.45 | 313.44 | 4.76 | 225.72 | 0.1145 | 742.0 | 606.9 | |
| 0.00 | 1.24 | 0.00 | 0.62 | -15.39 | 311.44 | 2.76 | 195.70 | 0.1721 | 796.0 | 697.0 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -12.06 | 310.20 | 1.52 | 193.62 | 0.1109 | 948.0 | 774.2 | |
| 0.00 | 1.24 | 0.00 | 0.63 | -19.82 | 308.66 | -0.02 | 179.91 | 0.2415 | 756.0 | 608.2 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -11.97 | 308.64 | -0.04 | 179.60 | 0.1062 | 792.0 | 651.4 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -17.84 | 308.15 | -0.53 | 177.58 | 0.2080 | 476.0 | 320.4 | |
| 0.00 | 1.85 | 0.00 | 0.92 | -5.10 | 305.14 | -3.53 | 77.23 | 0.0633 | 916.0 | 665.3 | |
| 0.00 | 2.47 | 0.00 | 1.23 | -1.40 | 304.74 | -3.94 | 41.21 | 0.1047 | 834.0 | 621.4 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -16.74 | 300.79 | -7.89 | 145.18 | 0.2311 | -840.0 | -686.8 | |
| 0.00 | 1.77 | 0.00 | 0.90 | -14.05 | 298.71 | -9.97 | 130.44 | 0.2218 | -955.0 | -834.2 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -14.14 | 298.54 | -10.14 | 130.31 | 0.2248 | -763.0 | -587.4 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -16.99 | 297.44 | -11.24 | 136.15 | 0.2703 | -848.0 | -655.2 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -16.84 | 296.48 | -12.19 | 133.51 | 0.2800 | -667.0 | -560.8 | |
| 0.00 | 2.12 | 0.00 | 1.10 | -17.15 | 295.40 | -13.28 | 132.01 | 0.2967 | -919.0 | -777.5 | |
| 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. | |