SDO HMI 2014-09-13 20:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.23 | 84.72 | 12.38 | 47.08 | -15.73 | 65.77 | 14.46 | 211.87 | 0.4572 | 681.9 | 508.2 | |
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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 |
| 3.11 | 5.51 | 1.74 | 3.08 | -15.81 | 66.86 | 15.54 | 213.67 | 0.4669 | 873.5 | 598.1 | |
| 0.00 | 1.51 | 0.00 | 0.85 | -16.40 | 66.81 | 15.49 | 212.88 | 0.4740 | 686.0 | 572.4 | |
| 1.96 | 4.00 | 1.09 | 2.23 | -15.83 | 66.47 | 15.15 | 212.99 | 0.4638 | 870.1 | 601.1 | |
| 5.96 | 64.45 | 3.32 | 35.78 | -15.63 | 66.20 | 14.88 | 212.76 | 0.4589 | 976.2 | 572.4 | |
| 0.00 | 0.89 | 0.00 | 0.50 | -16.55 | 66.23 | 14.92 | 211.73 | 0.4711 | 664.0 | 549.3 | |
| 0.00 | 1.42 | 0.00 | 0.80 | -16.21 | 66.14 | 14.83 | 211.96 | 0.4661 | 764.0 | 686.9 | |
| 5.51 | -4.00 | 3.07 | -4.00 | -15.52 | 66.03 | 14.71 | 212.59 | 0.4561 | 1095.7 | 999999 | |
| 5.69 | -4.00 | 3.16 | -4.00 | -15.45 | 65.76 | 14.45 | 212.21 | 0.4530 | 1191.2 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.60 | -18.43 | 64.10 | 12.78 | 206.01 | 0.4805 | 602.0 | 485.0 | |
| 0.00 | 0.98 | 0.00 | 0.55 | -18.30 | 63.96 | 12.64 | 205.90 | 0.4777 | 652.0 | 493.5 | |
| 0.00 | 1.42 | 0.00 | 0.77 | -14.13 | 63.03 | 11.71 | 208.56 | 0.4134 | 627.0 | 547.0 | |
| 0.00 | 1.42 | 0.00 | 0.79 | -16.94 | 61.74 | 10.42 | 203.02 | 0.4444 | -843.0 | -659.9 | |
| 0.00 | 1.07 | 0.00 | 0.60 | -19.17 | 60.16 | 8.84 | 198.13 | 0.4682 | -679.0 | -526.6 | |
| 0.00 | 0.98 | 0.00 | 0.53 | -16.64 | 58.70 | 7.38 | 196.96 | 0.4237 | -732.0 | -611.8 | |
| 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. | |