SDO HMI 2014-09-13 19:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.34 | 91.21 | 14.07 | 50.55 | -15.73 | 65.67 | 13.80 | 210.67 | 0.4521 | 644.7 | 451.9 | |
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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 | 1.33 | 0.00 | 0.75 | -16.06 | 66.95 | 15.08 | 212.58 | 0.4661 | 500.0 | 422.7 | |
| 3.11 | 5.51 | 1.74 | 3.08 | -15.83 | 66.86 | 14.99 | 212.71 | 0.4624 | 891.4 | 629.1 | |
| 0.00 | 1.60 | 0.00 | 0.90 | -16.45 | 66.85 | 14.98 | 211.94 | 0.4703 | 673.0 | 517.2 | |
| 2.67 | 4.53 | 1.49 | 2.53 | -15.82 | 66.47 | 14.60 | 212.05 | 0.4590 | 898.5 | 572.0 | |
| 0.00 | 1.51 | 0.00 | 0.85 | -16.60 | 66.37 | 14.50 | 210.95 | 0.4685 | 578.0 | 534.1 | |
| 6.31 | 66.76 | 3.51 | 36.96 | -15.64 | 66.17 | 14.30 | 211.72 | 0.4543 | 987.8 | 557.6 | |
| 0.00 | 1.69 | 0.00 | 0.94 | -16.20 | 66.18 | 14.31 | 211.07 | 0.4617 | 833.0 | 658.8 | |
| 5.87 | -6.00 | 3.25 | -6.00 | -15.54 | 66.03 | 14.16 | 211.59 | 0.4518 | 1080.4 | 999999 | |
| 7.38 | -6.00 | 4.08 | -6.00 | -15.43 | 65.80 | 13.93 | 211.30 | 0.4485 | 1201.3 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.59 | -15.95 | 65.67 | 13.80 | 210.46 | 0.4544 | 607.0 | 485.3 | |
| 0.00 | 1.33 | 0.00 | 0.72 | -14.15 | 63.04 | 11.17 | 207.42 | 0.4097 | 748.0 | 653.2 | |
| 0.00 | 1.87 | 0.00 | 1.03 | -16.96 | 61.69 | 9.82 | 201.79 | 0.4411 | -929.0 | -713.0 | |
| 0.00 | 1.87 | 0.00 | 1.04 | -18.88 | 59.53 | 7.66 | 196.04 | 0.4586 | -828.0 | -651.4 | |
| 0.00 | 0.98 | 0.00 | 0.53 | -16.60 | 58.71 | 6.84 | 195.81 | 0.4207 | -713.0 | -595.4 | |
| 0.00 | 1.16 | 0.00 | 0.63 | -16.63 | 58.49 | 6.62 | 195.30 | 0.4202 | -721.0 | -633.2 | |
| 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. | |