SDO HMI 2014-03-12 14:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.37 | 35.30 | 16.64 | 43.99 | -18.40 | 47.60 | 67.64 | 253.01 | 0.9189 | -50.1 | 2.1 | |
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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 |
| 2.26 | 3.56 | 3.18 | 5.02 | -18.04 | 50.67 | 70.70 | 253.38 | 0.9381 | 47.8 | 1.9 | |
| 0.00 | 0.43 | 0.00 | 0.60 | -17.71 | 50.00 | 70.03 | 253.75 | 0.9342 | 286.0 | 229.2 | |
| 0.00 | 1.47 | 0.00 | 1.97 | -17.01 | 49.31 | 69.34 | 254.51 | 0.9301 | 141.0 | 102.8 | |
| 0.00 | 1.04 | 0.00 | 1.38 | -17.04 | 49.07 | 69.10 | 254.48 | 0.9286 | 99.0 | 194.0 | |
| 1.21 | 2.60 | 1.65 | 3.53 | -18.05 | 49.74 | 69.78 | 253.39 | 0.9326 | 555.1 | 429.6 | |
| 0.00 | 2.43 | 0.00 | 3.05 | -17.65 | 47.83 | 67.86 | 253.84 | 0.9207 | 552.0 | 450.8 | |
| 0.00 | 0.78 | 0.00 | 0.96 | -18.16 | 47.40 | 67.43 | 253.28 | 0.9179 | 264.0 | 196.2 | |
| 0.00 | 0.95 | 0.00 | 1.20 | -19.21 | 47.85 | 67.88 | 252.15 | 0.9208 | -21.0 | 12.6 | |
| 0.00 | 1.13 | 0.00 | 1.40 | -19.09 | 47.49 | 67.53 | 252.27 | 0.9185 | -126.0 | -211.5 | |
| 2.86 | 6.42 | 3.41 | 7.63 | -18.31 | 46.38 | 66.41 | 253.12 | 0.9110 | -20.7 | 120.5 | |
| 2.26 | 3.30 | 2.77 | 4.05 | -19.46 | 47.23 | 67.26 | 251.86 | 0.9168 | -187.8 | -150.3 | |
| 3.04 | 7.98 | 3.57 | 9.38 | -18.66 | 46.02 | 66.05 | 252.73 | 0.9086 | -512.9 | -424.1 | |
| 1.74 | 3.21 | 2.06 | 3.82 | -19.12 | 46.38 | 66.41 | 252.23 | 0.9111 | -497.4 | -282.9 | |
| 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. | |