SDO HMI 2014-04-11 01:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.80 | 0.00 | 9.63 | -15.99 | 303.36 | -8.07 | 148.15 | 0.2418 | 141.1 | -39.6 | |
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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 | 1.41 | 0.00 | 0.71 | -14.30 | 311.35 | -0.08 | 179.48 | 0.1461 | 959.0 | 660.7 | |
| 0.00 | 0.62 | 0.00 | 0.31 | -14.06 | 311.28 | -0.14 | 179.04 | 0.1419 | 775.0 | 567.4 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -14.88 | 311.16 | -0.27 | 178.35 | 0.1562 | 756.0 | 573.2 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -13.81 | 311.10 | -0.33 | 177.70 | 0.1378 | 563.0 | 523.2 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -12.03 | 310.18 | -1.24 | 168.71 | 0.1087 | 947.0 | 714.2 | |
| 0.00 | 1.24 | 0.00 | 0.63 | -18.88 | 309.47 | -1.96 | 171.78 | 0.2274 | 863.0 | 588.7 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -19.03 | 309.34 | -2.09 | 171.36 | 0.2303 | 739.0 | 557.3 | |
| 0.00 | 2.03 | 0.00 | 1.03 | -19.28 | 309.30 | -2.12 | 171.38 | 0.2345 | 46.0 | 80.0 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -6.58 | 305.91 | -5.52 | 96.99 | 0.0967 | 974.0 | 805.0 | |
| 0.00 | 1.41 | 0.00 | 0.73 | -17.01 | 297.48 | -13.94 | 130.24 | 0.3032 | -777.0 | -677.8 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -14.46 | 296.67 | -14.76 | 121.56 | 0.2907 | -593.0 | -600.5 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -16.68 | 296.40 | -15.02 | 127.39 | 0.3138 | -814.0 | -662.3 | |
| 0.00 | 2.12 | 0.00 | 1.11 | -16.82 | 296.20 | -15.23 | 127.42 | 0.3180 | -708.0 | -637.2 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -17.08 | 295.59 | -15.84 | 127.07 | 0.3284 | -771.0 | -533.9 | |
| 0.00 | 1.85 | 0.00 | 0.97 | -16.98 | 295.27 | -16.15 | 126.30 | 0.3316 | -842.0 | -693.4 | |
| 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. | |