SDO HMI 2014-03-11 04:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.11 | 0.00 | 10.45 | -10.57 | 15.64 | 17.02 | 256.52 | 0.2969 | 227.1 | 323.2 | |
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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 | 1.47 | 0.00 | 0.79 | -9.97 | 21.78 | 23.16 | 261.53 | 0.3933 | 765.0 | 542.3 | |
| 0.00 | 1.56 | 0.00 | 0.83 | -9.15 | 19.35 | 20.73 | 263.23 | 0.3534 | 790.0 | 589.6 | |
| 0.00 | 1.39 | 0.00 | 0.73 | -9.75 | 17.20 | 18.58 | 260.90 | 0.3194 | 766.0 | 637.2 | |
| 0.00 | 2.86 | 0.00 | 1.49 | -9.90 | 17.02 | 18.40 | 260.35 | 0.3168 | 726.0 | 732.2 | |
| 0.00 | 1.30 | 0.00 | 0.68 | -10.21 | 16.94 | 18.32 | 259.37 | 0.3161 | 848.0 | 658.6 | |
| 0.00 | 3.04 | 0.00 | 1.58 | -10.46 | 16.60 | 17.98 | 258.42 | 0.3113 | 1046.0 | 829.1 | |
| 0.00 | 3.12 | 0.00 | 1.62 | -10.57 | 15.97 | 17.35 | 257.73 | 0.3014 | 858.0 | 707.2 | |
| 0.00 | 1.91 | 0.00 | 0.97 | -11.65 | 10.78 | 12.17 | 248.87 | 0.2223 | -998.0 | -901.2 | |
| 0.00 | 1.47 | 0.00 | 0.75 | -12.10 | 10.65 | 12.03 | 246.75 | 0.2228 | -742.0 | -677.9 | |
| 0.00 | 1.30 | 0.00 | 0.66 | -11.87 | 10.54 | 11.93 | 247.59 | 0.2198 | -797.0 | -629.2 | |
| 0.00 | 0.69 | 0.00 | 0.35 | -12.32 | 9.23 | 10.61 | 243.25 | 0.2023 | -764.0 | -581.5 | |
| 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. | |