SDO HMI 2011-08-18 04:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.07 | 109.25 | 20.81 | 102.53 | -20.78 | 56.80 | -52.12 | 119.66 | 0.8510 | 425.7 | 169.3 | |
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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 | 1.26 | 0.00 | 1.07 | -18.73 | 60.52 | -48.40 | 119.03 | 0.8122 | 624.0 | 481.6 | |
| 0.00 | 1.17 | 0.00 | 1.11 | -22.16 | 57.04 | -51.88 | 121.24 | 0.8543 | -440.0 | -454.6 | |
| 12.25 | 93.05 | 11.35 | 86.72 | -20.91 | 57.35 | -51.57 | 120.03 | 0.8472 | 843.7 | 181.1 | |
| 6.94 | -3.00 | 6.52 | -3.00 | -21.00 | 56.78 | -52.14 | 119.88 | 0.8521 | 403.1 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.57 | -18.55 | 57.18 | -51.74 | 117.36 | 0.8403 | 647.0 | 560.0 | |
| 0.00 | 1.26 | 0.00 | 1.17 | -18.89 | 56.45 | -52.47 | 117.43 | 0.8475 | 475.0 | 513.9 | |
| 1.17 | 1.98 | 1.10 | 1.86 | -19.32 | 56.15 | -52.77 | 117.78 | 0.8514 | 403.4 | 376.6 | |
| 0.00 | 0.90 | 0.00 | 0.84 | -18.74 | 56.31 | -52.61 | 117.21 | 0.8481 | 479.0 | 404.8 | |
| 0.00 | 1.26 | 0.00 | 1.18 | -18.86 | 56.09 | -52.83 | 117.25 | 0.8503 | 336.0 | 340.0 | |
| 0.00 | 0.54 | 0.00 | 0.51 | -18.59 | 55.46 | -53.46 | 116.71 | 0.8545 | 382.0 | 266.5 | |
| 0.00 | 1.62 | 0.00 | 1.58 | -19.68 | 54.83 | -54.09 | 117.65 | 0.8630 | 399.0 | 335.7 | |
| 0.00 | 1.08 | 0.00 | 1.07 | -19.92 | 54.49 | -54.43 | 117.78 | 0.8663 | 140.0 | 178.2 | |
| 0.00 | 0.99 | 0.00 | 1.06 | -20.94 | 52.02 | -56.90 | 117.95 | 0.8876 | -471.0 | -432.4 | |
| 1.71 | 2.43 | 1.84 | 2.61 | -20.77 | 51.70 | -57.22 | 117.65 | 0.8894 | -660.5 | -686.5 | |
| 0.00 | 1.08 | 0.00 | 1.18 | -20.76 | 51.16 | -57.77 | 117.45 | 0.8931 | -462.0 | -389.9 | |
| 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. | |