SDO HMI 2014-11-07 03:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.54 | 0.00 | 7.56 | -21.44 | 78.89 | 23.85 | 221.28 | 0.5722 | 555.2 | 419.2 | |
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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 | 1.73 | 0.00 | 1.06 | -20.04 | 82.85 | 27.81 | 227.86 | 0.5932 | 669.0 | 492.5 | |
| 0.00 | 1.21 | 0.00 | 0.74 | -19.84 | 82.56 | 27.52 | 227.85 | 0.5884 | 838.0 | 706.1 | |
| 0.00 | 1.47 | 0.00 | 0.90 | -19.97 | 82.48 | 27.43 | 227.60 | 0.5887 | 762.0 | 684.9 | |
| 0.00 | 1.64 | 0.00 | 1.01 | -20.42 | 82.53 | 27.49 | 227.04 | 0.5932 | 734.0 | 540.4 | |
| 0.00 | 1.04 | 0.00 | 0.64 | -21.88 | 82.03 | 26.99 | 224.66 | 0.6013 | 569.0 | 425.6 | |
| 0.00 | 0.78 | 0.00 | 0.48 | -22.88 | 80.37 | 25.32 | 221.68 | 0.5949 | 635.0 | 488.7 | |
| 0.00 | 0.78 | 0.00 | 0.46 | -20.65 | 78.31 | 23.27 | 222.16 | 0.5530 | 743.0 | 529.4 | |
| 0.00 | 0.78 | 0.00 | 0.46 | -21.28 | 76.21 | 21.17 | 218.75 | 0.5396 | 686.0 | 508.7 | |
| 0.00 | 1.04 | 0.00 | 0.62 | -23.73 | 76.47 | 21.42 | 216.16 | 0.5689 | 564.0 | 636.7 | |
| 0.00 | 0.52 | 0.00 | 0.30 | -21.47 | 73.18 | 18.14 | 214.40 | 0.5150 | 644.0 | 482.7 | |
| 0.00 | 1.55 | 0.00 | 0.89 | -24.86 | 65.60 | 10.56 | 199.17 | 0.5082 | -737.0 | -626.8 | |
| 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. | |