SDO HMI 2014-10-07 11:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.40 | 0.00 | 12.74 | 13.27 | 58.65 | -40.88 | 76.83 | 0.6551 | -14.7 | -11.4 | |
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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 | 1.32 | 0.00 | 0.77 | 14.67 | 67.36 | -32.16 | 72.67 | 0.5416 | -612.0 | -565.7 | |
| 0.00 | 1.58 | 0.00 | 0.94 | 11.77 | 65.45 | -34.08 | 78.40 | 0.5622 | -425.0 | -330.3 | |
| 0.00 | 2.02 | 0.00 | 1.28 | 16.52 | 61.15 | -38.37 | 71.51 | 0.6299 | -291.0 | -304.0 | |
| 0.00 | 1.67 | 0.00 | 1.07 | 14.81 | 60.30 | -39.23 | 74.39 | 0.6371 | -742.0 | -586.6 | |
| 0.00 | 0.79 | 0.00 | 0.51 | 13.75 | 60.36 | -39.17 | 76.04 | 0.6345 | -541.0 | -439.6 | |
| 0.00 | 1.40 | 0.00 | 0.90 | 14.52 | 60.16 | -39.37 | 74.86 | 0.6384 | -598.0 | -488.1 | |
| 0.00 | 1.67 | 0.00 | 1.07 | 13.63 | 59.94 | -39.59 | 76.30 | 0.6397 | -492.0 | -396.7 | |
| 0.00 | 0.44 | 0.00 | 0.29 | 14.09 | 58.67 | -40.86 | 75.81 | 0.6568 | -448.0 | -364.6 | |
| 0.00 | 1.67 | 0.00 | 1.10 | 12.82 | 58.40 | -41.13 | 77.78 | 0.6586 | 731.0 | 596.7 | |
| 0.00 | 1.23 | 0.00 | 0.82 | 13.47 | 57.35 | -42.17 | 76.93 | 0.6726 | 461.0 | 433.7 | |
| 0.00 | 1.14 | 0.00 | 0.77 | 13.45 | 56.60 | -42.92 | 77.07 | 0.6819 | 660.0 | 621.4 | |
| 0.00 | 0.70 | 0.00 | 0.48 | 13.39 | 55.85 | -43.68 | 77.24 | 0.6911 | 510.0 | 398.9 | |
| 0.00 | 1.40 | 0.00 | 1.01 | 10.50 | 52.93 | -46.60 | 81.55 | 0.7245 | 614.0 | 475.8 | |
| 0.00 | 1.23 | 0.00 | 0.90 | 12.25 | 52.06 | -47.47 | 79.19 | 0.7355 | 560.0 | 410.6 | |
| 0.00 | 1.14 | 0.00 | 0.83 | 8.90 | 51.79 | -47.74 | 83.76 | 0.7379 | 393.0 | 346.8 | |
| 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. | |