SDO HMI 2011-08-26 06:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.01 | 0.00 | 12.22 | 18.47 | 358.69 | -3.42 | 306.91 | 0.2208 | -400.0 | -383.7 | |
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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 | 4.04 | 0.00 | 2.02 | 14.52 | 4.53 | 2.42 | 342.52 | 0.1369 | -943.0 | -753.7 | |
| 0.00 | 1.62 | 0.00 | 0.82 | 19.58 | 2.60 | 0.50 | 357.85 | 0.2178 | -764.0 | -609.0 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 17.85 | 2.44 | 0.33 | 358.31 | 0.1880 | -893.0 | -706.5 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 20.82 | 1.96 | -0.15 | 0.58 | 0.2389 | -809.0 | -541.1 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 17.78 | 1.80 | -0.31 | 1.56 | 0.1869 | -1026.0 | -891.5 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 17.69 | 1.48 | -0.62 | 3.21 | 0.1856 | -1019.0 | -829.3 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 19.95 | 0.38 | -1.73 | 7.24 | 0.2258 | -804.0 | -593.5 | |
| 0.00 | 0.72 | 0.00 | 0.36 | 17.75 | 0.37 | -1.74 | 8.84 | 0.1886 | -957.0 | -790.5 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 16.98 | 0.31 | -1.79 | 9.85 | 0.1756 | -946.0 | -718.6 | |
| 0.00 | 2.96 | 0.00 | 1.51 | 19.70 | 0.22 | -1.89 | 8.06 | 0.2220 | -1140.0 | -841.9 | |
| 0.00 | 1.80 | 0.00 | 0.91 | 18.52 | 0.23 | -1.87 | 8.86 | 0.2020 | -891.0 | -592.8 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 17.66 | 354.40 | -7.70 | 34.63 | 0.2258 | 926.0 | 797.0 | |
| 0.00 | 1.62 | 0.00 | 0.82 | 15.91 | 352.98 | -9.13 | 44.49 | 0.2187 | 648.0 | 537.8 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 23.40 | 347.60 | -14.50 | 38.89 | 0.3677 | 815.0 | 601.7 | |
| 0.00 | 1.62 | 0.00 | 0.86 | 22.82 | 347.19 | -14.92 | 40.74 | 0.3651 | 772.0 | 575.7 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 22.36 | 345.57 | -16.53 | 44.42 | 0.3776 | 631.0 | 448.0 | |
| 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. | |