SDO HMI 2014-05-25 03:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.07 | 22.70 | 1.54 | 16.57 | -18.77 | 133.63 | 44.85 | 245.51 | 0.7359 | 32.9 | 4.9 | |
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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 | 2.16 | 0.00 | 1.63 | -18.65 | 135.34 | 46.56 | 246.27 | 0.7538 | 684.0 | 500.8 | |
| 0.00 | 1.53 | 0.00 | 1.15 | -18.94 | 135.21 | 46.43 | 245.85 | 0.7533 | 710.0 | 547.1 | |
| 2.07 | 3.70 | 1.54 | 2.74 | -18.31 | 134.75 | 45.98 | 246.52 | 0.7466 | 688.9 | 552.0 | |
| 0.00 | 0.81 | 0.00 | 0.60 | -18.76 | 134.72 | 45.95 | 245.93 | 0.7476 | 603.0 | 473.6 | |
| 0.00 | 1.80 | 0.00 | 1.33 | -18.34 | 134.53 | 45.76 | 246.40 | 0.7443 | 709.0 | 578.5 | |
| 0.00 | 1.17 | 0.00 | 0.86 | -17.69 | 133.99 | 45.22 | 247.08 | 0.7365 | 426.0 | 356.2 | |
| 0.00 | 1.17 | 0.00 | 0.87 | -19.18 | 134.36 | 45.59 | 245.26 | 0.7451 | -457.0 | -349.2 | |
| 0.00 | 1.08 | 0.00 | 0.79 | -19.64 | 133.56 | 44.79 | 244.37 | 0.7382 | 331.0 | 380.3 | |
| 0.00 | 4.24 | 0.00 | 2.99 | -17.72 | 131.91 | 43.13 | 246.30 | 0.7135 | -688.0 | -591.7 | |
| 0.00 | 0.72 | 0.00 | 0.52 | -20.65 | 132.83 | 44.06 | 242.78 | 0.7341 | -422.0 | -400.8 | |
| 0.00 | 1.62 | 0.00 | 1.17 | -20.72 | 132.45 | 43.68 | 242.53 | 0.7303 | -554.0 | -354.1 | |
| 0.00 | 1.08 | 0.00 | 0.77 | -20.11 | 132.06 | 43.28 | 243.16 | 0.7238 | -674.0 | -511.2 | |
| 0.00 | 0.27 | 0.00 | 0.19 | -18.81 | 131.54 | 42.76 | 244.69 | 0.7133 | -557.0 | -559.7 | |
| 0.00 | 1.35 | 0.00 | 0.96 | -19.41 | 131.60 | 42.83 | 243.91 | 0.7162 | -693.0 | -521.5 | |
| 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. | |