SDO HMI 2014-07-04 04:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 27.70 | 0.00 | 14.31 | 6.95 | 265.51 | -13.31 | 109.55 | 0.2417 | 367.9 | 423.2 | |
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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 | 0.95 | 3.67 | 279.12 | 0.31 | 326.84 | 0.0098 | -683.0 | -548.7 | |
| 0.00 | 2.36 | 0.00 | 1.17 | 3.43 | 278.97 | 0.15 | 325.67 | 0.0047 | -932.0 | -714.9 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 4.03 | 276.31 | -2.51 | 71.52 | 0.0462 | -880.0 | -704.0 | |
| 0.00 | 0.73 | 0.00 | 0.36 | 3.15 | 275.52 | -3.30 | 90.83 | 0.0577 | -790.0 | -707.4 | |
| 0.00 | 2.45 | 0.00 | 1.24 | 9.35 | 269.71 | -9.11 | 55.40 | 0.1907 | 1046.0 | 806.7 | |
| 0.00 | 2.09 | 0.00 | 1.05 | 8.52 | 269.13 | -9.68 | 60.68 | 0.1917 | 851.0 | 717.8 | |
| 0.00 | 2.54 | 0.00 | 1.29 | 8.42 | 268.64 | -10.18 | 62.29 | 0.1984 | 861.0 | 666.7 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 8.51 | 265.07 | -13.75 | 68.19 | 0.2542 | 903.0 | 761.8 | |
| 0.00 | 6.90 | 0.00 | 3.60 | 8.92 | 261.34 | -17.48 | 71.01 | 0.3151 | 936.0 | 817.9 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 1.58 | 260.65 | -18.17 | 94.68 | 0.3142 | 525.0 | 477.5 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 8.34 | 259.78 | -19.04 | 74.00 | 0.3373 | 752.0 | 563.6 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 1.50 | 259.49 | -19.33 | 94.59 | 0.3334 | 895.0 | 686.5 | |
| 0.00 | 0.73 | 0.00 | 0.41 | 8.84 | 251.14 | -27.68 | 77.18 | 0.4727 | 670.0 | 580.9 | |
| 0.00 | 1.27 | 0.00 | 0.71 | 7.67 | 251.01 | -27.80 | 79.67 | 0.4718 | 807.0 | 635.6 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 7.69 | 250.77 | -28.05 | 79.69 | 0.4756 | 557.0 | 426.2 | |
| 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. | |