SDO HMI 2014-07-22 10:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.76 | 135.03 | 21.39 | 88.16 | -20.97 | 69.06 | 31.72 | 229.04 | 0.6522 | 552.1 | 219.4 | |
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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 |
| 18.60 | 109.80 | 12.24 | 72.12 | -20.94 | 69.87 | 32.53 | 229.79 | 0.6600 | 1018.9 | 275.2 | |
| 1.63 | -1.00 | 1.07 | -1.00 | -21.09 | 69.48 | 32.14 | 229.29 | 0.6572 | 739.8 | 999999 | |
| 4.45 | -1.00 | 2.90 | -1.00 | -20.81 | 69.25 | 31.92 | 229.45 | 0.6528 | 994.1 | 999999 | |
| 3.63 | -1.00 | 2.36 | -1.00 | -20.80 | 69.06 | 31.73 | 229.30 | 0.6508 | 916.0 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.82 | -20.35 | 68.12 | 30.79 | 229.04 | 0.6377 | 786.0 | 633.4 | |
| 1.45 | 7.80 | 0.94 | 5.05 | -21.13 | 68.22 | 30.89 | 228.16 | 0.6450 | 800.2 | 636.6 | |
| 0.00 | 2.99 | 0.00 | 1.90 | -19.86 | 67.63 | 30.30 | 229.24 | 0.6288 | 725.0 | 482.4 | |
| 0.00 | 1.00 | 0.00 | 0.63 | -21.85 | 65.59 | 28.26 | 224.83 | 0.6255 | -723.0 | -628.0 | |
| 0.00 | 1.27 | 0.00 | 0.80 | -21.23 | 65.35 | 28.02 | 225.36 | 0.6176 | -791.0 | -693.6 | |
| 0.00 | 1.27 | 0.00 | 0.81 | -22.19 | 65.55 | 28.22 | 224.39 | 0.6282 | -369.0 | -459.4 | |
| 0.00 | 1.91 | 0.00 | 1.20 | -21.59 | 65.01 | 27.68 | 224.59 | 0.6176 | -590.0 | -559.2 | |
| 2.36 | 5.63 | 1.48 | 3.53 | -21.61 | 64.76 | 27.43 | 224.30 | 0.6153 | -889.6 | -760.5 | |
| 0.64 | 2.09 | 0.40 | 1.30 | -22.11 | 63.68 | 26.35 | 222.59 | 0.6098 | -790.3 | -654.2 | |
| 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. | |