SDO HMI 2011-06-07 12:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.38 | 38.30 | 18.86 | 40.50 | -21.11 | 36.89 | 59.73 | 245.80 | 0.8847 | 391.8 | 150.2 | |
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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 | 1.18 | 0.00 | 1.35 | -19.14 | 40.01 | 62.84 | 248.65 | 0.9042 | 309.0 | 303.2 | |
| 12.49 | 17.74 | 14.06 | 19.95 | -19.21 | 39.34 | 62.18 | 248.47 | 0.8997 | 588.9 | 432.1 | |
| 0.00 | 0.81 | 0.00 | 0.88 | -20.47 | 37.87 | 60.70 | 246.80 | 0.8908 | 274.0 | 291.3 | |
| 0.00 | 1.00 | 0.00 | 1.13 | -22.40 | 38.85 | 61.69 | 244.88 | 0.9008 | 300.0 | 221.1 | |
| 0.00 | 1.27 | 0.00 | 1.31 | -22.23 | 36.05 | 58.88 | 244.44 | 0.8804 | 542.0 | 373.6 | |
| 0.00 | 1.45 | 0.00 | 1.45 | -21.87 | 34.80 | 57.64 | 244.55 | 0.8701 | 689.0 | 575.8 | |
| 4.89 | 6.61 | 4.80 | 6.50 | -23.08 | 33.88 | 56.71 | 242.94 | 0.8655 | 439.3 | 185.4 | |
| 0.00 | 1.00 | 0.00 | 0.96 | -23.58 | 32.88 | 55.71 | 242.11 | 0.8587 | 296.0 | 234.1 | |
| 0.00 | 1.18 | 0.00 | 1.16 | -24.85 | 33.62 | 56.45 | 240.90 | 0.8675 | -462.0 | -428.1 | |
| 0.00 | 2.26 | 0.00 | 2.17 | -23.95 | 32.76 | 55.59 | 241.67 | 0.8587 | 26.0 | -78.3 | |
| 0.00 | 2.71 | 0.00 | 2.60 | -24.18 | 32.56 | 55.39 | 241.35 | 0.8577 | -551.0 | -331.2 | |
| 0.00 | 1.09 | 0.00 | 1.04 | -24.48 | 32.64 | 55.47 | 241.03 | 0.8590 | -505.0 | -522.6 | |
| 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. | |