SDO HMI 2014-09-19 03:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.15 | 0.00 | 10.06 | 8.18 | 338.11 | -3.34 | 172.95 | 0.1037 | -320.3 | -269.6 | |
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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 | 2.48 | 0.00 | 1.23 | 6.62 | 345.30 | 3.85 | 262.41 | 0.0676 | -885.0 | -606.1 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 8.11 | 343.82 | 2.37 | 292.41 | 0.0445 | -1002.0 | -799.8 | |
| 0.00 | 0.98 | 0.00 | 0.48 | 8.83 | 343.64 | 2.19 | 307.96 | 0.0482 | -716.0 | -523.5 | |
| 0.00 | 2.40 | 0.00 | 1.19 | 8.65 | 343.40 | 1.95 | 308.11 | 0.0429 | -1159.0 | -969.2 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 9.34 | 343.40 | 1.95 | 318.83 | 0.0513 | -749.0 | -466.2 | |
| 0.00 | 0.89 | 0.00 | 0.44 | 9.20 | 343.16 | 1.71 | 320.61 | 0.0466 | -899.0 | -756.7 | |
| 0.00 | 1.95 | 0.00 | 0.97 | 10.13 | 339.19 | -2.26 | 36.68 | 0.0654 | -868.0 | -611.2 | |
| 0.00 | 2.93 | 0.00 | 1.45 | 8.53 | 338.40 | -3.05 | 65.14 | 0.0582 | -778.0 | -722.2 | |
| 0.00 | 1.95 | 0.00 | 0.98 | 6.28 | 331.52 | -9.93 | 94.45 | 0.1727 | 744.0 | 670.0 | |
| 0.00 | 1.69 | 0.00 | 0.85 | 7.83 | 329.51 | -11.94 | 85.94 | 0.2065 | 778.0 | 614.5 | |
| 0.00 | 0.98 | 0.00 | 0.50 | 7.54 | 327.83 | -13.62 | 87.45 | 0.2347 | 884.0 | 727.3 | |
| 0.00 | 1.60 | 0.00 | 0.82 | 8.19 | 327.31 | -14.14 | 84.81 | 0.2439 | 806.0 | 712.3 | |
| 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. | |