SDO HMI 2014-09-19 02:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.52 | 215.84 | 33.20 | 172.51 | 8.24 | 289.92 | -52.08 | 85.12 | 0.7860 | -694.9 | -254.6 | |
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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 | 1.86 | 0.00 | 1.33 | 9.06 | 295.60 | -46.40 | 84.29 | 0.7210 | -578.0 | -414.9 | |
| 0.00 | 0.62 | 0.00 | 0.47 | 12.16 | 292.24 | -49.76 | 80.08 | 0.7599 | -384.0 | -341.4 | |
| 0.00 | 0.89 | 0.00 | 0.70 | 16.31 | 290.31 | -51.69 | 74.79 | 0.7827 | -590.0 | -420.0 | |
| 0.27 | 78.33 | 0.21 | 61.53 | 5.00 | 291.03 | -50.97 | 89.38 | 0.7762 | -916.7 | -255.9 | |
| 16.32 | -4.00 | 12.81 | -4.00 | 5.25 | 290.86 | -51.14 | 89.03 | 0.7778 | -838.8 | 999999 | |
| 0.00 | 1.33 | 0.00 | 1.04 | 4.80 | 290.91 | -51.09 | 89.61 | 0.7777 | -217.0 | -281.0 | |
| 12.69 | 124.29 | 10.11 | 99.60 | 10.35 | 289.84 | -52.16 | 82.44 | 0.7860 | -1096.7 | -282.6 | |
| 5.59 | -7.00 | 4.48 | -7.00 | 10.20 | 289.62 | -52.38 | 82.62 | 0.7883 | -826.8 | 999999 | |
| 3.19 | -7.00 | 2.57 | -7.00 | 10.30 | 289.39 | -52.61 | 82.48 | 0.7907 | -658.9 | 999999 | |
| 1.60 | -7.00 | 1.29 | -7.00 | 10.44 | 289.26 | -52.74 | 82.30 | 0.7921 | -534.2 | 999999 | |
| 0.00 | 1.15 | 0.00 | 1.04 | 6.47 | 284.80 | -57.20 | 86.93 | 0.8385 | 419.0 | 288.0 | |
| 0.00 | 1.51 | 0.00 | 1.38 | 4.52 | 284.47 | -57.53 | 89.21 | 0.8432 | -143.0 | -45.9 | |
| 0.00 | 1.24 | 0.00 | 1.14 | 2.69 | 284.65 | -57.35 | 91.40 | 0.8434 | 22.0 | 79.3 | |
| 0.00 | 0.98 | 0.00 | 0.90 | 5.47 | 284.28 | -57.72 | 88.06 | 0.8441 | 364.0 | 341.2 | |
| 1.86 | 3.64 | 1.73 | 3.38 | 5.34 | 283.84 | -58.16 | 88.18 | 0.8483 | 468.3 | 326.6 | |
| 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. | |