SDO HMI 2014-09-14 03:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.60 | 0.00 | 11.44 | -23.97 | 73.16 | 25.70 | 217.62 | 0.6494 | 8.5 | -27.4 | |
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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 |
| 0.00 | 1.60 | 0.00 | 1.11 | -21.54 | 82.15 | 34.69 | 228.98 | 0.7039 | 691.0 | 583.9 | |
| 0.00 | 0.89 | 0.00 | 0.61 | -21.17 | 81.81 | 34.35 | 229.14 | 0.6981 | 566.0 | 490.2 | |
| 0.00 | 0.44 | 0.00 | 0.30 | -20.33 | 81.44 | 33.98 | 229.83 | 0.6882 | 414.0 | 450.0 | |
| 0.00 | 0.53 | 0.00 | 0.36 | -23.54 | 78.94 | 31.48 | 224.07 | 0.6906 | 556.0 | 521.7 | |
| 0.00 | 0.89 | 0.00 | 0.60 | -23.04 | 78.81 | 31.35 | 224.50 | 0.6854 | 483.0 | 449.5 | |
| 0.00 | 1.25 | 0.00 | 0.82 | -23.12 | 76.47 | 29.01 | 222.26 | 0.6655 | 190.0 | 256.2 | |
| 0.00 | 0.80 | 0.00 | 0.54 | -25.08 | 75.78 | 28.32 | 219.52 | 0.6775 | 451.0 | 429.7 | |
| 0.00 | 1.42 | 0.00 | 0.93 | -23.45 | 75.09 | 27.63 | 220.56 | 0.6566 | 749.0 | 554.7 | |
| 0.00 | 2.49 | 0.00 | 1.60 | -25.22 | 70.41 | 22.94 | 213.77 | 0.6368 | -215.0 | -235.1 | |
| 0.00 | 0.89 | 0.00 | 0.56 | -24.57 | 69.67 | 22.21 | 213.54 | 0.6244 | -619.0 | -471.0 | |
| 0.00 | 0.89 | 0.00 | 0.56 | -24.22 | 69.60 | 22.14 | 213.81 | 0.6200 | -678.0 | -492.1 | |
| 0.00 | 0.89 | 0.00 | 0.56 | -24.86 | 69.11 | 21.65 | 212.61 | 0.6234 | -523.0 | -462.0 | |
| 0.00 | 1.33 | 0.00 | 0.84 | -24.77 | 68.74 | 21.28 | 212.25 | 0.6197 | -666.0 | -657.9 | |
| 0.00 | 0.89 | 0.00 | 0.56 | -24.80 | 68.53 | 21.07 | 211.98 | 0.6185 | -663.0 | -558.9 | |
| 0.00 | 2.40 | 0.00 | 1.49 | -25.74 | 64.97 | 17.51 | 206.69 | 0.6055 | -608.0 | -523.7 | |
| 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. | |