SDO HMI 2014-11-03 18:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.27 | 39.23 | 6.51 | 20.96 | -17.23 | 98.05 | -1.51 | 176.63 | 0.3753 | -88.0 | -290.5 | |
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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 |
| 9.42 | 14.26 | 5.00 | 7.56 | -16.45 | 103.85 | 4.28 | 191.53 | 0.3601 | 1036.5 | 774.9 | |
| 2.85 | 5.19 | 1.51 | 2.75 | -16.85 | 100.38 | 0.81 | 182.17 | 0.3598 | 1100.1 | 803.6 | |
| 0.00 | 1.30 | 0.00 | 0.69 | -17.30 | 94.52 | -5.05 | 167.04 | 0.3763 | -803.0 | -676.5 | |
| 0.00 | 1.12 | 0.00 | 0.60 | -17.46 | 94.36 | -5.21 | 166.75 | 0.3794 | -872.0 | -695.3 | |
| 0.00 | 3.54 | 0.00 | 1.90 | -17.66 | 94.16 | -5.40 | 166.40 | 0.3832 | -668.0 | -719.1 | |
| 0.00 | 4.58 | 0.00 | 2.47 | -18.20 | 93.80 | -5.77 | 165.89 | 0.3931 | -727.0 | -656.4 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -17.08 | 93.68 | -5.88 | 164.83 | 0.3761 | -779.0 | -667.6 | |
| 0.00 | 1.30 | 0.00 | 0.69 | -17.28 | 93.55 | -6.02 | 164.65 | 0.3797 | -787.0 | -714.7 | |
| 0.00 | 1.90 | 0.00 | 1.02 | -18.11 | 93.36 | -6.20 | 164.80 | 0.3935 | -890.0 | -709.5 | |
| 0.00 | 1.38 | 0.00 | 0.73 | -14.05 | 93.22 | -6.35 | 161.01 | 0.3310 | -781.0 | -680.9 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -16.30 | 91.65 | -7.92 | 159.22 | 0.3743 | -811.0 | -700.0 | |
| 0.00 | 1.90 | 0.00 | 1.04 | -19.74 | 91.29 | -8.27 | 161.47 | 0.4279 | -900.0 | -726.1 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -21.75 | 91.08 | -8.48 | 162.54 | 0.4586 | -367.0 | -381.9 | |
| 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. | |