SDO HMI 2014-07-02 18:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.61 | 0.00 | 11.18 | 6.40 | 264.68 | -32.91 | 82.28 | 0.5428 | 314.9 | 275.2 | |
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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 | 1.91 | 0.00 | 0.99 | 4.71 | 279.56 | -18.02 | 84.09 | 0.3114 | -1120.0 | -927.9 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 6.29 | 279.16 | -18.43 | 79.26 | 0.3212 | -835.0 | -635.4 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 3.68 | 274.49 | -23.09 | 87.72 | 0.3933 | -621.0 | -488.0 | |
| 0.00 | 2.45 | 0.00 | 1.40 | 8.74 | 268.41 | -29.17 | 77.58 | 0.4953 | 615.0 | 527.2 | |
| 0.00 | 0.73 | 0.00 | 0.42 | 10.64 | 266.97 | -30.61 | 74.41 | 0.5216 | 688.0 | 627.6 | |
| 0.00 | 1.27 | 0.00 | 0.74 | 10.78 | 266.63 | -30.95 | 74.27 | 0.5269 | 766.0 | 635.1 | |
| 0.00 | 1.36 | 0.00 | 0.80 | 11.53 | 265.78 | -31.80 | 73.23 | 0.5414 | 792.0 | 598.7 | |
| 0.00 | 1.45 | 0.00 | 0.86 | 9.61 | 264.35 | -33.24 | 77.16 | 0.5564 | 733.0 | 626.7 | |
| 0.00 | 0.54 | 0.00 | 0.33 | 9.60 | 264.05 | -33.53 | 77.25 | 0.5605 | 586.0 | 501.8 | |
| 0.00 | 1.18 | 0.00 | 0.70 | 1.85 | 264.41 | -33.18 | 91.25 | 0.5492 | 521.0 | 444.9 | |
| 0.00 | 1.27 | 0.00 | 0.80 | 9.49 | 260.26 | -37.32 | 78.35 | 0.6128 | 658.0 | 598.6 | |
| 0.00 | 1.45 | 0.00 | 0.92 | 1.58 | 259.45 | -38.14 | 91.30 | 0.6197 | 649.0 | 507.4 | |
| 0.00 | 0.64 | 0.00 | 0.44 | -6.39 | 254.66 | -42.92 | 102.47 | 0.6954 | 376.0 | 371.4 | |
| 0.00 | 0.91 | 0.00 | 0.68 | 6.05 | 249.27 | -48.32 | 84.59 | 0.7483 | 521.0 | 435.9 | |
| 0.00 | 1.18 | 0.00 | 0.89 | 4.35 | 248.79 | -48.79 | 86.87 | 0.7536 | 394.0 | 346.5 | |
| 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. | |