SDO HMI 2014-04-22 08:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.42 | 0.00 | 8.64 | -21.33 | 166.98 | 4.66 | 191.47 | 0.3107 | -717.7 | -503.7 | |
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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 | 2.40 | 0.00 | 1.40 | -31.30 | 181.27 | 18.94 | 211.82 | 0.5281 | 604.0 | 335.5 | |
| 0.00 | 1.07 | 0.00 | 0.54 | -11.69 | 173.22 | 10.89 | 237.49 | 0.2204 | -735.0 | -592.4 | |
| 0.00 | 1.51 | 0.00 | 0.76 | -12.29 | 171.33 | 9.01 | 230.10 | 0.2003 | -1021.0 | -868.7 | |
| 0.00 | 1.33 | 0.00 | 0.69 | -20.48 | 167.79 | 5.46 | 198.46 | 0.2829 | -780.0 | -592.7 | |
| 0.00 | 1.15 | 0.00 | 0.62 | -26.01 | 167.61 | 5.28 | 192.99 | 0.3698 | -800.0 | -624.5 | |
| 0.00 | 0.80 | 0.00 | 0.43 | -27.90 | 166.43 | 4.10 | 189.23 | 0.3960 | -712.0 | -585.9 | |
| 0.00 | 1.07 | 0.00 | 0.55 | -19.87 | 161.55 | -0.78 | 177.14 | 0.2580 | -836.0 | -653.2 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -24.00 | 161.38 | -0.94 | 177.36 | 0.3272 | -867.0 | -624.0 | |
| 0.00 | 0.80 | 0.00 | 0.41 | -18.69 | 161.39 | -0.93 | 176.26 | 0.2381 | -781.0 | -612.1 | |
| 0.00 | 1.24 | 0.00 | 0.65 | -23.90 | 161.02 | -1.30 | 176.32 | 0.3260 | -726.0 | -614.9 | |
| 0.00 | 1.24 | 0.00 | 0.64 | -19.43 | 160.75 | -1.58 | 174.05 | 0.2516 | -828.0 | -599.6 | |
| 0.00 | 1.51 | 0.00 | 0.75 | -10.12 | 159.51 | -2.82 | 151.54 | 0.1020 | -793.0 | -645.9 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -23.34 | 158.20 | -4.12 | 168.16 | 0.3231 | -1055.0 | -894.5 | |
| 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. | |