SDO HMI 2014-10-01 00:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.24 | 107.21 | 15.30 | 77.62 | -9.89 | 140.79 | -43.94 | 110.37 | 0.7314 | 622.4 | 319.3 | |
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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 | 0.70 | 0.00 | 0.49 | -13.00 | 143.94 | -40.79 | 115.96 | 0.7103 | 528.0 | 444.8 | |
| 0.00 | 1.06 | 0.00 | 0.77 | -13.86 | 141.88 | -42.85 | 115.96 | 0.7367 | 522.0 | 457.4 | |
| 19.65 | 99.38 | 14.16 | 71.60 | -9.68 | 140.98 | -43.75 | 110.19 | 0.7286 | 972.9 | 349.9 | |
| 1.59 | -3.00 | 1.14 | -3.00 | -9.22 | 140.88 | -43.84 | 109.55 | 0.7278 | 687.2 | 999999 | |
| 0.00 | 1.06 | 0.00 | 0.78 | -10.98 | 140.06 | -44.66 | 111.45 | 0.7437 | 551.0 | 431.8 | |
| 0.00 | 0.79 | 0.00 | 0.59 | -11.76 | 139.77 | -44.95 | 112.30 | 0.7499 | 276.0 | 317.7 | |
| 0.00 | 0.79 | 0.00 | 0.59 | -11.86 | 139.71 | -45.02 | 112.40 | 0.7510 | 588.0 | 503.0 | |
| 0.00 | 0.70 | 0.00 | 0.55 | -13.44 | 138.18 | -46.54 | 113.67 | 0.7731 | -542.0 | -506.2 | |
| 0.00 | 0.79 | 0.00 | 0.64 | -14.69 | 137.02 | -47.71 | 114.65 | 0.7895 | -428.0 | -349.2 | |
| 0.00 | 0.79 | 0.00 | 0.63 | -12.49 | 136.41 | -48.31 | 111.76 | 0.7873 | -564.0 | -486.4 | |
| 0.00 | 1.15 | 0.00 | 0.98 | -12.70 | 133.43 | -51.29 | 110.86 | 0.8168 | -365.0 | -393.2 | |
| 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. | |