SDO HMI 2014-09-02 22:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.05 | 59.27 | 16.63 | 41.35 | -17.94 | 158.01 | -37.47 | 124.71 | 0.7060 | 284.4 | -168.9 | |
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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 |
| 11.00 | 25.84 | 7.49 | 17.60 | -17.67 | 159.60 | -35.88 | 125.49 | 0.6882 | 886.9 | 419.3 | |
| 5.63 | -1.00 | 3.83 | -1.00 | -17.39 | 159.39 | -36.09 | 124.99 | 0.6884 | 878.7 | 999999 | |
| 0.00 | 1.43 | 0.00 | 0.98 | -17.54 | 159.12 | -36.36 | 124.98 | 0.6922 | 225.0 | 156.1 | |
| 0.00 | 1.61 | 0.00 | 1.10 | -17.17 | 159.16 | -36.31 | 124.56 | 0.6894 | 678.0 | 555.4 | |
| 0.00 | 1.61 | 0.00 | 1.09 | -16.21 | 158.91 | -36.57 | 123.17 | 0.6858 | 410.0 | 275.9 | |
| 0.00 | 0.98 | 0.00 | 0.67 | -16.98 | 158.74 | -36.74 | 124.01 | 0.6925 | 230.0 | 269.6 | |
| 0.00 | 1.07 | 0.00 | 0.75 | -17.50 | 157.57 | -37.90 | 123.85 | 0.7078 | 472.0 | 352.9 | |
| 1.79 | 17.70 | 1.27 | 12.69 | -18.33 | 156.71 | -38.77 | 124.27 | 0.7216 | -843.6 | -618.7 | |
| 0.00 | 4.38 | 0.00 | 3.15 | -18.95 | 156.50 | -38.98 | 124.87 | 0.7275 | -687.0 | -533.4 | |
| 1.07 | -8.00 | 0.77 | -8.00 | -18.58 | 156.52 | -38.96 | 124.44 | 0.7251 | -782.7 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.76 | -17.98 | 156.60 | -38.88 | 123.77 | 0.7206 | -744.0 | -548.0 | |
| 3.84 | -8.00 | 2.76 | -8.00 | -18.53 | 156.28 | -39.20 | 124.23 | 0.7271 | -641.8 | 999999 | |
| 0.72 | 3.58 | 0.51 | 2.56 | -18.14 | 156.27 | -39.21 | 123.75 | 0.7248 | -834.2 | -654.5 | |
| 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. | |