SDO HMI 2011-09-05 10:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.22 | 99.97 | 15.75 | 65.04 | -19.60 | 258.72 | 30.90 | 228.06 | 0.6525 | 322.1 | 387.2 | |
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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 | 2.32 | 0.00 | 1.61 | -22.02 | 261.82 | 34.01 | 227.89 | 0.7013 | 546.0 | 467.9 | |
| 0.00 | 1.07 | 0.00 | 0.73 | -21.09 | 260.80 | 32.98 | 228.11 | 0.6845 | 658.0 | 553.2 | |
| 0.00 | 1.16 | 0.00 | 0.79 | -21.26 | 260.72 | 32.91 | 227.86 | 0.6851 | 579.0 | 443.1 | |
| 0.00 | 1.34 | 0.00 | 0.93 | -23.03 | 260.88 | 33.06 | 225.99 | 0.7005 | 686.0 | 436.9 | |
| 1.97 | 3.66 | 1.29 | 2.41 | -19.96 | 259.19 | 31.37 | 228.07 | 0.6601 | 455.0 | 323.7 | |
| 13.31 | 74.96 | 8.70 | 48.74 | -19.50 | 258.98 | 31.16 | 228.42 | 0.6543 | 924.2 | 547.9 | |
| 4.56 | -6.00 | 2.97 | -6.00 | -19.77 | 258.40 | 30.58 | 227.58 | 0.6508 | 735.2 | 999999 | |
| 3.13 | 4.02 | 2.00 | 2.58 | -18.50 | 258.03 | 30.21 | 228.79 | 0.6366 | -488.2 | -361.2 | |
| 0.00 | 0.98 | 0.00 | 0.63 | -18.72 | 257.33 | 29.52 | 227.87 | 0.6315 | -560.0 | -475.4 | |
| 0.00 | 5.54 | 0.00 | 3.54 | -18.96 | 257.34 | 29.53 | 227.58 | 0.6336 | -616.0 | -544.3 | |
| 0.00 | 0.98 | 0.00 | 0.63 | -19.48 | 256.56 | 28.75 | 226.20 | 0.6305 | -319.0 | -250.1 | |
| 1.25 | 1.52 | 0.79 | 0.95 | -18.38 | 256.25 | 28.43 | 227.23 | 0.6177 | -758.1 | -675.3 | |
| 0.00 | 0.54 | 0.00 | 0.34 | -19.48 | 255.54 | 27.73 | 225.18 | 0.6206 | -565.0 | -513.5 | |
| 0.00 | 0.63 | 0.00 | 0.39 | -19.50 | 255.36 | 27.55 | 224.97 | 0.6191 | -734.0 | -653.1 | |
| 0.00 | 1.25 | 0.00 | 0.77 | -17.57 | 254.88 | 27.07 | 226.88 | 0.5965 | -618.0 | -480.4 | |
| 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. | |