SDO HMI 2014-10-03 08:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.90 | 108.98 | 22.34 | 98.69 | 7.02 | 211.18 | 57.23 | 274.07 | 0.8382 | -95.4 | -72.8 | |
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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 | 0.97 | 0.00 | 0.92 | 6.43 | 212.79 | 58.84 | 273.51 | 0.8540 | -369.0 | -291.4 | |
| 6.51 | 64.61 | 6.18 | 61.02 | 7.30 | 212.91 | 58.96 | 274.53 | 0.8546 | -732.1 | -252.2 | |
| 6.95 | -2.00 | 6.54 | -2.00 | 7.21 | 212.59 | 58.64 | 274.40 | 0.8518 | -894.3 | 999999 | |
| 0.00 | 4.58 | 0.00 | 4.14 | 7.13 | 211.20 | 57.25 | 274.22 | 0.8389 | -730.0 | -564.3 | |
| 0.00 | 0.70 | 0.00 | 0.61 | 6.76 | 209.42 | 55.48 | 273.65 | 0.8220 | 132.0 | 89.2 | |
| 0.00 | 1.58 | 0.00 | 1.35 | 6.69 | 208.88 | 54.93 | 273.52 | 0.8166 | 93.0 | 104.6 | |
| 0.00 | 2.38 | 0.00 | 2.02 | 7.19 | 208.65 | 54.70 | 274.13 | 0.8140 | 523.0 | 397.8 | |
| 7.66 | 16.02 | 6.47 | 13.55 | 6.40 | 208.46 | 54.51 | 273.13 | 0.8126 | 599.2 | 225.2 | |
| 0.70 | 2.02 | 0.59 | 1.69 | 6.41 | 207.99 | 54.05 | 273.11 | 0.8079 | 581.8 | 470.3 | |
| 0.00 | 3.35 | 0.00 | 2.80 | 6.86 | 208.07 | 54.12 | 273.67 | 0.8083 | 502.0 | 424.9 | |
| 0.00 | 1.94 | 0.00 | 1.62 | 6.18 | 207.91 | 53.96 | 272.82 | 0.8071 | 503.0 | 396.9 | |
| 2.29 | 9.86 | 1.90 | 8.18 | 6.62 | 207.72 | 53.77 | 273.35 | 0.8049 | 847.7 | 686.0 | |
| 0.79 | -12.00 | 0.66 | -12.00 | 6.89 | 207.71 | 53.76 | 273.69 | 0.8047 | 691.7 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.79 | 7.15 | 206.89 | 52.94 | 273.96 | 0.7960 | 536.0 | 545.3 | |
| 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. | |