SDO HMI 2014-11-05 01:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.27 | 24.71 | 3.01 | 13.91 | -17.54 | 100.40 | 17.89 | 218.27 | 0.4754 | -140.6 | -128.2 | |
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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 | 3.37 | 0.00 | 1.90 | -14.93 | 104.27 | 21.76 | 228.26 | 0.4820 | -790.0 | -675.3 | |
| 3.63 | 10.02 | 2.07 | 5.72 | -16.85 | 104.08 | 21.57 | 225.05 | 0.4992 | 854.7 | 787.0 | |
| 1.64 | -2.00 | 0.94 | -2.00 | -16.69 | 104.03 | 21.52 | 225.22 | 0.4970 | 1025.8 | 999999 | |
| 0.00 | 1.64 | 0.00 | 0.96 | -21.18 | 103.04 | 20.52 | 217.81 | 0.5354 | -561.0 | -376.9 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -16.74 | 100.90 | 18.39 | 220.74 | 0.4647 | 849.0 | 673.9 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -16.40 | 99.85 | 17.34 | 219.62 | 0.4503 | 728.0 | 596.7 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -17.89 | 96.56 | 14.04 | 211.92 | 0.4386 | -703.0 | -580.2 | |
| 0.00 | 1.04 | 0.00 | 0.57 | -17.16 | 95.35 | 12.83 | 210.57 | 0.4191 | -745.0 | -652.7 | |
| 0.00 | 0.95 | 0.00 | 0.52 | -18.52 | 93.84 | 11.33 | 206.02 | 0.4264 | -547.0 | -468.9 | |
| 0.00 | 1.04 | 0.00 | 0.56 | -18.03 | 93.49 | 10.98 | 205.85 | 0.4171 | -774.0 | -648.8 | |
| 0.00 | 1.21 | 0.00 | 0.66 | -18.51 | 93.49 | 10.98 | 205.33 | 0.4239 | -685.0 | -528.4 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -19.51 | 90.96 | 8.45 | 199.19 | 0.4233 | -765.0 | -656.2 | |
| 0.00 | 1.30 | 0.00 | 0.73 | -23.05 | 89.83 | 7.32 | 194.47 | 0.4710 | -711.0 | -559.0 | |
| 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. | |