SDO HMI 2014-09-06 02:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 79.14 | 467.95 | 95.88 | 566.64 | 14.92 | 86.72 | -66.93 | 76.86 | 0.9145 | 109.5 | -133.2 | |
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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 |
| 53.14 | 448.04 | 62.36 | 541.21 | 15.34 | 87.63 | -66.02 | 76.42 | 0.9083 | 577.3 | -129.5 | |
| 0.00 | 0.71 | 0.00 | 0.90 | 17.41 | 85.70 | -67.95 | 74.12 | 0.9211 | 212.0 | 181.8 | |
| 0.00 | 0.80 | 0.00 | 1.00 | 16.12 | 85.98 | -67.67 | 75.53 | 0.9194 | -212.0 | -177.2 | |
| 0.00 | 1.43 | 0.00 | 1.71 | 13.13 | 87.10 | -66.55 | 78.83 | 0.9124 | -155.0 | -155.6 | |
| 0.00 | 6.79 | 0.00 | 8.68 | 15.92 | 85.36 | -68.29 | 75.73 | 0.9235 | -266.0 | -242.9 | |
| 0.00 | 2.41 | 0.00 | 2.90 | 12.84 | 87.02 | -66.63 | 79.14 | 0.9130 | -565.0 | -505.2 | |
| 0.00 | 1.88 | 0.00 | 2.45 | 15.98 | 84.79 | -68.86 | 75.65 | 0.9271 | -343.0 | -313.2 | |
| 0.00 | 1.79 | 0.00 | 2.34 | 15.69 | 84.74 | -68.91 | 75.96 | 0.9275 | -428.0 | -405.5 | |
| 5.54 | -1.00 | 7.09 | -1.00 | 14.17 | 85.35 | -68.31 | 77.63 | 0.9240 | -790.5 | 999999 | |
| 3.13 | -1.00 | 3.98 | -1.00 | 13.85 | 85.55 | -68.11 | 77.98 | 0.9227 | -714.1 | 999999 | |
| 10.36 | -1.00 | 13.48 | -1.00 | 14.60 | 84.98 | -68.67 | 77.15 | 0.9262 | -756.4 | 999999 | |
| 0.00 | 1.16 | 0.00 | 1.46 | 12.66 | 85.91 | -67.74 | 79.30 | 0.9207 | -382.0 | -343.3 | |
| 6.97 | -1.00 | 8.97 | -1.00 | 13.45 | 85.28 | -68.37 | 78.41 | 0.9245 | -465.7 | 999999 | |
| 0.00 | 0.80 | 0.00 | 1.07 | 14.22 | 84.44 | -69.21 | 77.54 | 0.9297 | 244.0 | 251.6 | |
| 0.00 | 2.14 | 0.00 | 2.92 | 14.68 | 83.85 | -69.80 | 77.02 | 0.9332 | 311.0 | 267.5 | |
| 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. | |