SDO HMI 2014-09-10 06:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.73 | 56.08 | 16.65 | 41.62 | 9.74 | 147.23 | 48.60 | 276.60 | 0.7461 | 84.4 | -74.7 | |
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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 | 4.28 | 0.00 | 3.43 | 9.82 | 151.06 | 52.43 | 276.82 | 0.7888 | -751.0 | -473.2 | |
| 0.00 | 3.48 | 0.00 | 2.77 | 10.82 | 150.84 | 52.21 | 278.08 | 0.7862 | -538.0 | -444.3 | |
| 5.71 | 15.87 | 4.34 | 12.07 | 10.19 | 148.58 | 49.95 | 277.22 | 0.7617 | -741.1 | -561.4 | |
| 0.00 | 0.89 | 0.00 | 0.68 | 9.90 | 148.33 | 49.70 | 276.85 | 0.7589 | -750.0 | -548.4 | |
| 0.53 | -3.00 | 0.41 | -3.00 | 10.48 | 148.41 | 49.77 | 277.61 | 0.7597 | -624.5 | 999999 | |
| 1.69 | -3.00 | 1.28 | -3.00 | 10.28 | 148.27 | 49.63 | 277.34 | 0.7582 | -821.3 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.93 | 9.45 | 147.39 | 48.76 | 276.21 | 0.7484 | -632.0 | -553.7 | |
| 0.00 | 2.41 | 0.00 | 1.74 | 8.91 | 146.00 | 47.37 | 275.43 | 0.7325 | 458.0 | 368.5 | |
| 11.95 | 25.23 | 8.58 | 18.12 | 9.31 | 145.53 | 46.90 | 275.98 | 0.7268 | 739.9 | 485.7 | |
| 2.85 | -9.00 | 2.04 | -9.00 | 9.16 | 145.24 | 46.60 | 275.76 | 0.7233 | 880.9 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.76 | 10.05 | 145.17 | 46.54 | 276.99 | 0.7224 | 600.0 | 456.4 | |
| 0.00 | 1.60 | 0.00 | 1.12 | 10.04 | 143.93 | 45.30 | 276.97 | 0.7074 | 696.0 | 562.8 | |
| 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. | |