SDO HMI 2014-04-04 13:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.58 | 0.00 | 9.14 | 5.75 | 24.80 | -12.43 | 45.07 | 0.3014 | -301.8 | -208.6 | |
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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 | 1.41 | 0.00 | 0.72 | 6.42 | 29.13 | -8.10 | 32.49 | 0.2618 | -657.0 | -511.8 | |
| 0.00 | 1.41 | 0.00 | 0.71 | 3.55 | 28.95 | -8.28 | 40.10 | 0.2241 | -1023.0 | -905.6 | |
| 0.00 | 1.32 | 0.00 | 0.68 | 7.95 | 28.43 | -8.80 | 31.67 | 0.2897 | -727.0 | -570.9 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 5.18 | 28.27 | -8.96 | 38.03 | 0.2530 | -730.0 | -607.4 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 1.56 | 28.21 | -9.03 | 49.03 | 0.2086 | -687.0 | -528.5 | |
| 0.00 | 1.67 | 0.00 | 0.86 | 6.19 | 27.06 | -10.17 | 39.21 | 0.2790 | -563.0 | -348.2 | |
| 0.00 | 1.93 | 0.00 | 0.99 | 3.26 | 26.98 | -10.25 | 47.13 | 0.2436 | -912.0 | -738.7 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 1.65 | 25.64 | -11.59 | 55.74 | 0.2440 | -957.0 | -818.0 | |
| 0.00 | 1.49 | 0.00 | 0.78 | 7.68 | 24.06 | -13.17 | 43.33 | 0.3305 | 741.0 | 620.4 | |
| 0.00 | 2.20 | 0.00 | 1.18 | 9.30 | 20.74 | -16.49 | 46.59 | 0.3873 | 352.0 | 211.8 | |
| 0.00 | 1.49 | 0.00 | 0.81 | 6.58 | 17.32 | -19.91 | 57.32 | 0.4036 | 751.0 | 616.2 | |
| 0.00 | 1.32 | 0.00 | 0.71 | 6.36 | 17.33 | -19.90 | 57.77 | 0.4017 | 791.0 | 601.9 | |
| 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. | |