SDO HMI 2014-09-04 19:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.36 | 188.16 | 54.07 | 248.28 | -19.42 | 107.17 | -63.55 | 114.39 | 0.9286 | 525.7 | 232.7 | |
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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 | 0.80 | 0.00 | 1.05 | -22.02 | 108.48 | -62.24 | 117.46 | 0.9261 | 384.0 | 401.6 | |
| 0.00 | 2.14 | 0.00 | 2.85 | -21.73 | 107.78 | -62.94 | 116.95 | 0.9296 | 396.0 | 327.9 | |
| 1.70 | 95.64 | 2.27 | 127.10 | -20.62 | 107.27 | -63.45 | 115.65 | 0.9304 | 312.5 | 163.9 | |
| 19.83 | -3.00 | 26.35 | -3.00 | -20.03 | 107.20 | -63.52 | 115.02 | 0.9296 | 539.0 | 999999 | |
| 1.79 | 63.32 | 2.29 | 80.26 | -18.83 | 107.84 | -62.88 | 113.97 | 0.9236 | 541.6 | 425.2 | |
| 13.13 | -5.00 | 16.71 | -5.00 | -18.56 | 107.87 | -62.85 | 113.70 | 0.9228 | 772.8 | 999999 | |
| 4.91 | 13.04 | 6.45 | 17.22 | -19.04 | 107.19 | -63.53 | 113.99 | 0.9278 | 390.9 | -20.2 | |
| 0.00 | 0.54 | 0.00 | 0.76 | -20.62 | 105.84 | -64.88 | 115.24 | 0.9383 | 149.0 | 180.7 | |
| 0.00 | 0.27 | 0.00 | 0.37 | -19.22 | 106.17 | -64.55 | 113.89 | 0.9341 | 150.0 | 82.0 | |
| 0.00 | 0.27 | 0.00 | 0.39 | -19.19 | 104.49 | -66.23 | 113.40 | 0.9432 | 323.0 | 317.3 | |
| 0.00 | 7.95 | 0.00 | 11.70 | -18.77 | 104.42 | -66.30 | 112.95 | 0.9430 | 373.0 | 287.3 | |
| 0.00 | 0.80 | 0.00 | 1.24 | -17.82 | 103.12 | -67.60 | 111.64 | 0.9484 | -381.0 | -366.3 | |
| 0.00 | 3.39 | 0.00 | 5.34 | -17.36 | 102.54 | -68.18 | 111.03 | 0.9507 | -348.0 | -251.3 | |
| 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. | |