SDO HMI 2014-09-16 12:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.95 | 31.80 | 1.63 | 26.43 | -15.89 | 64.75 | 48.63 | 244.06 | 0.8048 | 109.9 | 241.4 | |
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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 | 1.33 | 0.00 | 1.12 | -15.80 | 65.44 | 49.32 | 244.48 | 0.8108 | 414.0 | 401.7 | |
| 0.00 | 2.31 | 0.00 | 1.93 | -15.61 | 65.24 | 49.11 | 244.60 | 0.8083 | 748.0 | 606.5 | |
| 1.33 | 10.57 | 1.12 | 8.90 | -15.91 | 65.29 | 49.16 | 244.28 | 0.8098 | 744.1 | 480.6 | |
| 0.00 | 2.93 | 0.00 | 2.43 | -15.19 | 64.91 | 48.79 | 244.94 | 0.8037 | 814.0 | 647.0 | |
| 0.62 | 2.93 | 0.51 | 2.40 | -14.67 | 64.52 | 48.39 | 245.38 | 0.7979 | 737.3 | 599.3 | |
| 0.00 | 2.93 | 0.00 | 2.44 | -15.84 | 64.88 | 48.76 | 244.18 | 0.8058 | 595.0 | 438.2 | |
| 0.00 | 0.62 | 0.00 | 0.49 | -14.06 | 63.46 | 47.33 | 245.63 | 0.7853 | -487.0 | -469.6 | |
| 0.00 | 3.11 | 0.00 | 2.56 | -16.73 | 64.03 | 47.91 | 242.77 | 0.8015 | -546.0 | -390.9 | |
| 0.00 | 2.31 | 0.00 | 1.91 | -17.28 | 63.98 | 47.86 | 242.11 | 0.8033 | -626.0 | -472.8 | |
| 0.00 | 1.69 | 0.00 | 1.39 | -16.84 | 63.79 | 47.66 | 242.53 | 0.7997 | -474.0 | -484.9 | |
| 0.00 | 1.07 | 0.00 | 0.86 | -16.00 | 63.19 | 47.07 | 243.22 | 0.7906 | -479.0 | -390.5 | |
| 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. | |