SDO HMI 2014-04-03 07:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.31 | 343.98 | 42.80 | 236.66 | 12.45 | 13.82 | -39.89 | 64.54 | 0.6959 | -834.7 | -309.5 | |
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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 |
| 54.93 | 333.25 | 37.64 | 228.90 | 12.44 | 14.08 | -39.63 | 64.42 | 0.6929 | -1253.5 | -340.5 | |
| 7.38 | -1.00 | 5.16 | -1.00 | 12.63 | 12.83 | -40.88 | 64.86 | 0.7078 | -574.5 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.57 | 14.51 | 12.27 | -41.44 | 62.74 | 0.7231 | 530.0 | 471.4 | |
| 0.00 | 0.97 | 0.00 | 0.67 | 11.86 | 12.61 | -41.10 | 65.98 | 0.7066 | -365.0 | -287.2 | |
| 0.00 | 0.53 | 0.00 | 0.39 | 14.87 | 10.97 | -42.74 | 62.99 | 0.7386 | 496.0 | 424.5 | |
| 0.00 | 0.35 | 0.00 | 0.25 | 10.48 | 11.83 | -41.88 | 68.20 | 0.7094 | 520.0 | 484.0 | |
| 0.00 | 0.97 | 0.00 | 0.69 | 11.66 | 11.12 | -42.59 | 66.99 | 0.7224 | 633.0 | 486.2 | |
| 0.00 | 1.32 | 0.00 | 0.94 | 11.03 | 11.20 | -42.51 | 67.78 | 0.7188 | 672.0 | 589.9 | |
| 0.00 | 0.88 | 0.00 | 0.63 | 11.65 | 10.83 | -42.88 | 67.14 | 0.7256 | 629.0 | 506.0 | |
| 0.00 | 0.35 | 0.00 | 0.25 | 11.50 | 10.82 | -42.89 | 67.35 | 0.7250 | 258.0 | 206.2 | |
| 0.00 | 0.97 | 0.00 | 0.69 | 11.28 | 10.73 | -42.98 | 67.66 | 0.7251 | 539.0 | 461.4 | |
| 0.00 | 1.58 | 0.00 | 1.14 | 11.64 | 10.54 | -43.17 | 67.29 | 0.7288 | 628.0 | 503.8 | |
| 0.00 | 2.02 | 0.00 | 1.54 | 12.95 | 8.01 | -45.70 | 66.81 | 0.7611 | 698.0 | 557.8 | |
| 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. | |