SDO HMI 2014-11-06 17:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.64 | 0.00 | 10.86 | -21.40 | 80.09 | 19.53 | 216.19 | 0.5279 | 581.1 | 368.3 | |
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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 | 0.60 | 0.00 | 0.35 | -16.18 | 85.09 | 24.53 | 229.87 | 0.5236 | 716.0 | 529.3 | |
| 0.00 | 2.33 | 0.00 | 1.47 | -27.01 | 84.38 | 23.82 | 215.34 | 0.6243 | -646.0 | -518.2 | |
| 0.00 | 0.69 | 0.00 | 0.40 | -19.82 | 82.70 | 22.14 | 221.83 | 0.5338 | 815.0 | 719.2 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -20.34 | 82.78 | 22.22 | 221.24 | 0.5401 | 607.0 | 490.7 | |
| 0.00 | 0.43 | 0.00 | 0.25 | -20.21 | 82.66 | 22.10 | 221.26 | 0.5375 | 807.0 | 647.8 | |
| 0.00 | 3.11 | 0.00 | 1.81 | -19.68 | 82.31 | 21.75 | 221.51 | 0.5285 | 560.0 | 424.1 | |
| 0.00 | 1.12 | 0.00 | 0.65 | -20.80 | 80.67 | 20.11 | 217.90 | 0.5252 | 581.0 | 489.8 | |
| 0.00 | 3.19 | 0.00 | 1.85 | -21.31 | 79.76 | 19.20 | 216.04 | 0.5228 | 468.0 | 372.5 | |
| 0.00 | 1.04 | 0.00 | 0.60 | -21.36 | 79.49 | 18.93 | 215.60 | 0.5212 | 665.0 | 501.0 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -21.26 | 76.14 | 15.58 | 210.70 | 0.4922 | 675.0 | 648.3 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -21.77 | 75.56 | 15.00 | 209.23 | 0.4944 | 836.0 | 665.1 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -18.19 | 75.09 | 14.53 | 212.61 | 0.4443 | 750.0 | 656.5 | |
| 0.00 | 1.04 | 0.00 | 0.59 | -21.77 | 75.27 | 14.71 | 208.75 | 0.4922 | 675.0 | 539.8 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -22.10 | 73.55 | 12.99 | 205.56 | 0.4846 | 627.0 | 542.8 | |
| 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. | |