SDO HMI 2014-08-17 10:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 85.33 | 480.53 | 78.16 | 440.10 | -17.68 | 105.91 | 52.40 | 243.79 | 0.8419 | 56.4 | -33.8 | |
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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 | 1.80 | 0.00 | 1.85 | -18.05 | 110.09 | 56.58 | 245.06 | 0.8772 | -124.0 | -111.8 | |
| 43.70 | 244.82 | 43.16 | 241.63 | -16.97 | 109.18 | 55.67 | 245.91 | 0.8672 | 830.9 | 196.3 | |
| 0.00 | 0.27 | 0.00 | 0.25 | -16.64 | 106.15 | 52.64 | 245.16 | 0.8413 | 526.0 | 447.3 | |
| 0.81 | 1.89 | 0.75 | 1.74 | -17.40 | 106.24 | 52.74 | 244.35 | 0.8446 | 497.3 | 451.1 | |
| 0.54 | 1.44 | 0.49 | 1.32 | -17.63 | 105.92 | 52.41 | 243.96 | 0.8426 | 413.0 | 352.1 | |
| 0.00 | 0.27 | 0.00 | 0.25 | -18.69 | 106.27 | 52.76 | 242.93 | 0.8490 | -397.0 | -411.3 | |
| 0.00 | 2.43 | 0.00 | 2.22 | -17.84 | 105.69 | 52.18 | 243.64 | 0.8414 | 555.0 | 351.6 | |
| 0.00 | 1.26 | 0.00 | 1.12 | -18.00 | 104.61 | 51.11 | 243.02 | 0.8328 | -428.0 | -366.1 | |
| 0.00 | 0.63 | 0.00 | 0.57 | -19.21 | 104.45 | 50.95 | 241.60 | 0.8358 | -427.0 | -364.3 | |
| 0.81 | 10.63 | 0.73 | 9.55 | -19.78 | 104.19 | 50.69 | 240.85 | 0.8357 | -650.8 | -420.6 | |
| 0.90 | 214.46 | 0.77 | 179.05 | -18.64 | 102.32 | 48.81 | 241.29 | 0.8152 | -266.7 | -328.8 | |
| 0.00 | 0.63 | 0.00 | 0.55 | -19.64 | 102.67 | 49.16 | 240.33 | 0.8223 | -383.0 | -316.1 | |
| 38.57 | -11.00 | 32.26 | -11.00 | -18.50 | 101.54 | 48.03 | 241.08 | 0.8077 | -949.5 | 999999 | |
| 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. | |