SDO HMI 2014-06-05 00:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.17 | 17.63 | 1.28 | 10.82 | 4.15 | 269.30 | -35.58 | 82.60 | 0.5846 | -448.1 | -422.7 | |
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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 | 0.63 | 0.00 | 0.37 | 8.09 | 273.29 | -31.58 | 74.49 | 0.5402 | -661.0 | -522.9 | |
| 0.00 | 0.99 | 0.00 | 0.58 | 3.53 | 273.00 | -31.87 | 82.99 | 0.5331 | -770.0 | -612.0 | |
| 0.00 | 0.63 | 0.00 | 0.37 | 5.58 | 272.83 | -32.05 | 79.24 | 0.5396 | -551.0 | -496.3 | |
| 0.00 | 1.18 | 0.00 | 0.69 | 3.13 | 272.83 | -32.04 | 83.77 | 0.5349 | -844.0 | -689.0 | |
| 2.17 | 5.25 | 1.28 | 3.09 | 4.33 | 272.35 | -32.52 | 81.66 | 0.5439 | -938.9 | -646.4 | |
| 0.00 | 1.72 | 0.00 | 1.01 | 2.95 | 272.33 | -32.54 | 84.19 | 0.5420 | -746.0 | -602.8 | |
| 0.00 | 1.36 | 0.00 | 0.82 | 3.45 | 270.23 | -34.65 | 83.64 | 0.5731 | -919.0 | -766.5 | |
| 0.00 | 1.63 | 0.00 | 0.98 | 3.60 | 270.15 | -34.73 | 83.39 | 0.5745 | -660.0 | -630.4 | |
| 0.00 | 1.09 | 0.00 | 0.66 | 3.91 | 269.65 | -35.23 | 82.95 | 0.5820 | -631.0 | -465.2 | |
| 0.00 | 0.90 | 0.00 | 0.58 | -0.71 | 265.91 | -38.96 | 90.86 | 0.6311 | -666.0 | -496.5 | |
| 0.00 | 0.54 | 0.00 | 0.37 | 1.86 | 262.10 | -42.78 | 87.03 | 0.6820 | 700.0 | 593.0 | |
| 0.00 | 0.90 | 0.00 | 0.62 | 5.62 | 261.16 | -43.72 | 81.68 | 0.6974 | 440.0 | 371.0 | |
| 0.00 | 0.81 | 0.00 | 0.68 | 9.68 | 251.59 | -53.28 | 77.83 | 0.8105 | 559.0 | 505.0 | |
| 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. | |