SDO HMI 2014-04-05 21:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74.38 | 419.88 | 39.15 | 221.07 | 12.56 | 13.66 | -5.96 | 17.46 | 0.3397 | -1053.3 | -406.1 | |
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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 | 0.97 | 0.00 | 0.51 | 14.52 | 15.67 | -3.96 | 10.66 | 0.3627 | 602.0 | 424.6 | |
| 72.28 | 404.03 | 38.03 | 212.75 | 12.56 | 13.79 | -5.84 | 17.11 | 0.3389 | -1457.4 | -438.0 | |
| 0.26 | -2.00 | 0.14 | -2.00 | 13.33 | 13.43 | -6.19 | 17.40 | 0.3527 | -477.7 | 999999 | |
| 1.49 | -2.00 | 0.79 | -2.00 | 13.11 | 13.37 | -6.25 | 17.75 | 0.3495 | -781.9 | 999999 | |
| 0.35 | -2.00 | 0.19 | -2.00 | 12.87 | 12.54 | -7.08 | 20.17 | 0.3501 | -708.5 | 999999 | |
| 0.00 | 1.06 | 0.00 | 0.55 | 11.48 | 12.58 | -7.05 | 21.56 | 0.3285 | -676.0 | -526.4 | |
| 0.00 | 1.23 | 0.00 | 0.64 | 9.85 | 12.22 | -7.41 | 24.64 | 0.3061 | 764.0 | 538.6 | |
| 0.00 | 1.41 | 0.00 | 0.73 | 9.67 | 12.13 | -7.50 | 25.16 | 0.3039 | 813.0 | 580.5 | |
| 0.00 | 1.41 | 0.00 | 0.76 | 15.34 | 11.81 | -7.82 | 19.63 | 0.3919 | 696.0 | 470.2 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 12.31 | 11.85 | -7.78 | 22.59 | 0.3457 | -408.0 | -359.3 | |
| 0.00 | 1.41 | 0.00 | 0.73 | 10.04 | 11.87 | -7.75 | 25.36 | 0.3114 | 838.0 | 685.8 | |
| 0.00 | 2.55 | 0.00 | 1.34 | 12.06 | 11.67 | -7.96 | 23.35 | 0.3431 | -750.0 | -604.4 | |
| 0.00 | 3.17 | 0.00 | 1.67 | 11.79 | 10.59 | -9.03 | 26.45 | 0.3466 | 953.0 | 756.1 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 9.66 | 9.08 | -10.55 | 33.47 | 0.3286 | 722.0 | 559.2 | |
| 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. | |