SDO HMI 2014-10-06 13:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.93 | 26.09 | 1.04 | 13.82 | 13.37 | 92.65 | -18.97 | 68.33 | 0.3411 | -119.3 | 76.8 | |
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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 | 1.58 | 0.00 | 0.79 | 9.27 | 102.73 | -8.90 | 71.55 | 0.1616 | -758.0 | -665.2 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 10.86 | 99.37 | -12.26 | 69.07 | 0.2243 | -682.0 | -601.8 | |
| 0.00 | 1.76 | 0.00 | 0.90 | 12.87 | 99.12 | -12.51 | 61.47 | 0.2414 | -790.0 | -637.6 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 10.71 | 98.09 | -13.54 | 71.34 | 0.2438 | -856.0 | -641.7 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 10.64 | 97.59 | -14.03 | 72.17 | 0.2515 | -835.0 | -714.5 | |
| 0.00 | 2.11 | 0.00 | 1.08 | 10.35 | 96.88 | -14.74 | 73.97 | 0.2617 | -881.0 | -720.2 | |
| 0.00 | 1.32 | 0.00 | 0.68 | 10.36 | 96.12 | -15.50 | 74.59 | 0.2740 | -879.0 | -758.6 | |
| 0.00 | 1.67 | 0.00 | 0.87 | 14.31 | 95.14 | -16.48 | 62.76 | 0.3106 | -885.0 | -730.7 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 16.85 | 93.00 | -18.63 | 58.61 | 0.3597 | 827.0 | 570.4 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 15.43 | 91.55 | -20.07 | 63.76 | 0.3704 | 910.0 | 714.2 | |
| 1.93 | 8.78 | 1.04 | 4.73 | 13.47 | 89.42 | -22.20 | 70.42 | 0.3917 | 1085.3 | 848.7 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 13.58 | 86.95 | -24.67 | 71.67 | 0.4292 | 753.0 | 636.2 | |
| 0.00 | 1.32 | 0.00 | 0.74 | 18.46 | 86.31 | -25.32 | 61.68 | 0.4627 | 587.0 | 390.8 | |
| 0.00 | 1.05 | 0.00 | 0.62 | 20.60 | 80.81 | -30.81 | 61.57 | 0.5473 | 685.0 | 591.8 | |
| 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. | |