SDO HMI 2011-08-25 02:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.48 | 0.00 | 12.18 | 19.09 | 356.76 | -20.75 | 56.37 | 0.3997 | -342.7 | -173.3 | |
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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 | 0.63 | 0.00 | 0.33 | 18.02 | 3.55 | -13.96 | 49.77 | 0.3017 | -616.0 | -528.4 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 17.87 | 2.58 | -14.93 | 51.96 | 0.3127 | -890.0 | -702.6 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 20.88 | 1.55 | -15.96 | 46.50 | 0.3556 | -753.0 | -605.9 | |
| 0.00 | 1.26 | 0.00 | 0.66 | 20.25 | 1.45 | -16.06 | 48.06 | 0.3504 | -676.0 | -580.4 | |
| 0.00 | 1.17 | 0.00 | 0.62 | 19.63 | 0.51 | -17.00 | 50.99 | 0.3560 | -875.0 | -773.9 | |
| 0.00 | 1.44 | 0.00 | 0.75 | 16.70 | 0.67 | -16.84 | 58.08 | 0.3284 | -795.0 | -539.8 | |
| 0.00 | 1.71 | 0.00 | 0.90 | 17.57 | 0.02 | -17.49 | 56.70 | 0.3443 | -894.0 | -696.4 | |
| 0.00 | 2.78 | 0.00 | 1.47 | 18.37 | 359.94 | -17.57 | 54.82 | 0.3520 | -642.0 | -524.6 | |
| 0.00 | 1.62 | 0.00 | 0.85 | 18.15 | 359.86 | -17.65 | 55.47 | 0.3512 | -1037.0 | -819.0 | |
| 0.00 | 1.89 | 0.00 | 1.00 | 18.14 | 359.66 | -17.85 | 55.76 | 0.3538 | -716.0 | -573.0 | |
| 0.00 | 2.16 | 0.00 | 1.18 | 17.74 | 354.30 | -23.21 | 62.54 | 0.4248 | 1083.0 | 761.3 | |
| 0.00 | 1.71 | 0.00 | 0.95 | 17.58 | 352.44 | -25.07 | 64.34 | 0.4500 | 663.0 | 494.0 | |
| 0.00 | 2.42 | 0.00 | 1.43 | 22.19 | 347.48 | -30.03 | 59.16 | 0.5417 | 730.0 | 638.8 | |
| 0.00 | 1.62 | 0.00 | 0.96 | 22.84 | 347.21 | -30.30 | 58.25 | 0.5489 | 620.0 | 460.6 | |
| 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. | |