SDO HMI 2014-04-29 09:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.05 | 160.20 | 25.12 | 117.18 | -23.54 | 114.25 | 44.96 | 241.61 | 0.7385 | 482.5 | 249.9 | |
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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 | 0.89 | 0.00 | 0.68 | -25.29 | 116.47 | 47.17 | 240.22 | 0.7663 | 71.0 | 87.0 | |
| 0.98 | 143.97 | 0.73 | 106.05 | -23.66 | 115.20 | 45.91 | 241.85 | 0.7484 | 201.9 | 326.0 | |
| 33.07 | -2.00 | 24.39 | -2.00 | -23.36 | 114.78 | 45.49 | 242.10 | 0.7431 | 969.4 | 999999 | |
| 0.00 | 1.43 | 0.00 | 1.00 | -21.19 | 112.63 | 43.33 | 244.21 | 0.7129 | -561.0 | -468.8 | |
| 0.00 | 0.98 | 0.00 | 0.72 | -24.76 | 114.09 | 44.80 | 240.04 | 0.7408 | 507.0 | 425.1 | |
| 0.00 | 1.34 | 0.00 | 0.93 | -21.43 | 111.65 | 42.35 | 243.53 | 0.7029 | -706.0 | -627.7 | |
| 0.00 | 1.43 | 0.00 | 1.07 | -28.13 | 113.95 | 44.65 | 235.71 | 0.7524 | 437.0 | 333.8 | |
| 0.00 | 0.89 | 0.00 | 0.61 | -22.37 | 110.80 | 41.51 | 241.91 | 0.6970 | -539.0 | -479.8 | |
| 0.00 | 1.25 | 0.00 | 0.86 | -22.98 | 110.68 | 41.38 | 241.02 | 0.6980 | -508.0 | -463.2 | |
| 0.00 | 0.80 | 0.00 | 0.54 | -20.96 | 109.46 | 40.16 | 243.31 | 0.6764 | -512.0 | -459.8 | |
| 0.00 | 1.25 | 0.00 | 0.84 | -24.79 | 107.85 | 38.55 | 237.22 | 0.6753 | -495.0 | -365.9 | |
| 0.00 | 1.07 | 0.00 | 0.72 | -25.56 | 108.06 | 38.76 | 236.27 | 0.6814 | -586.0 | -508.4 | |
| 0.00 | 1.43 | 0.00 | 0.95 | -27.59 | 106.18 | 36.89 | 232.51 | 0.6728 | -747.0 | -533.1 | |
| 0.00 | 0.98 | 0.00 | 0.64 | -27.63 | 104.34 | 35.05 | 231.30 | 0.6541 | -643.0 | -565.8 | |
| 0.00 | 0.80 | 0.00 | 0.52 | -27.83 | 104.25 | 34.95 | 230.97 | 0.6545 | -465.0 | -427.1 | |
| 0.00 | 1.69 | 0.00 | 1.05 | -30.32 | 97.58 | 28.28 | 222.53 | 0.6072 | -166.0 | -313.1 | |
| 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. | |