SDO HMI 2011-03-03 06:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 28.66 | 0.00 | 15.11 | -23.26 | 180.56 | 12.29 | 215.03 | 0.3434 | -356.6 | -184.4 | |
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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 | 5.18 | 0.00 | 2.73 | -21.45 | 183.04 | 14.77 | 223.58 | 0.3457 | 1274.0 | 906.8 | |
| 0.00 | 0.78 | 0.00 | 0.41 | -21.64 | 182.89 | 14.62 | 222.91 | 0.3462 | 949.0 | 775.1 | |
| 0.00 | 3.71 | 0.00 | 1.96 | -22.89 | 182.13 | 13.86 | 218.93 | 0.3528 | 910.0 | 683.9 | |
| 0.00 | 0.78 | 0.00 | 0.41 | -23.43 | 180.52 | 12.25 | 214.67 | 0.3438 | -605.0 | -494.6 | |
| 0.00 | 1.64 | 0.00 | 0.86 | -23.53 | 180.37 | 12.10 | 214.17 | 0.3436 | -758.0 | -613.0 | |
| 0.00 | 1.90 | 0.00 | 1.00 | -22.91 | 180.21 | 11.94 | 214.95 | 0.3342 | -732.0 | -533.0 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -23.54 | 179.97 | 11.70 | 213.30 | 0.3402 | -804.0 | -686.6 | |
| 0.00 | 1.55 | 0.00 | 0.82 | -23.83 | 179.47 | 11.20 | 211.69 | 0.3396 | -768.0 | -709.2 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -24.92 | 179.43 | 11.16 | 209.85 | 0.3542 | -815.0 | -729.5 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -24.64 | 179.41 | 11.14 | 210.23 | 0.3502 | -925.0 | -776.9 | |
| 0.00 | 4.06 | 0.00 | 2.15 | -24.80 | 179.22 | 10.95 | 209.58 | 0.3509 | -559.0 | -712.2 | |
| 0.00 | 5.27 | 0.00 | 2.76 | -23.53 | 179.01 | 10.74 | 211.17 | 0.3317 | -920.0 | -762.8 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -23.97 | 178.72 | 10.45 | 209.76 | 0.3353 | -883.0 | -706.1 | |
| 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. | |