SDO HMI 2014-07-04 13:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.35 | 0.00 | 10.03 | 6.18 | 259.17 | -14.71 | 70.97 | 0.2734 | 796.8 | 624.3 | |
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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 | 1.73 | 0.00 | 0.86 | 9.28 | 270.06 | -3.82 | 31.95 | 0.1249 | 925.0 | 634.3 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 8.70 | 269.85 | -4.03 | 36.08 | 0.1186 | 761.0 | 633.1 | |
| 0.00 | 1.91 | 0.00 | 0.95 | 8.67 | 269.60 | -4.28 | 37.87 | 0.1208 | 874.0 | 711.9 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 8.35 | 268.06 | -5.82 | 48.25 | 0.1352 | 869.0 | 682.5 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -0.29 | 262.62 | -11.26 | 107.15 | 0.2052 | 749.0 | 463.5 | |
| 0.00 | 0.64 | 0.00 | 0.32 | 9.62 | 261.59 | -12.29 | 61.79 | 0.2393 | 813.0 | 653.0 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 1.61 | 260.09 | -13.79 | 96.39 | 0.2408 | 863.0 | 743.5 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 7.30 | 259.10 | -14.78 | 73.95 | 0.2645 | 913.0 | 686.6 | |
| 0.00 | 1.18 | 0.00 | 0.62 | -5.35 | 257.14 | -16.75 | 117.11 | 0.3237 | 707.0 | 531.3 | |
| 0.00 | 3.27 | 0.00 | 1.76 | 8.64 | 251.36 | -22.52 | 75.42 | 0.3929 | 642.0 | 594.9 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 8.24 | 251.25 | -22.63 | 76.48 | 0.3933 | 802.0 | 589.8 | |
| 0.00 | 0.55 | 0.00 | 0.29 | 8.25 | 250.55 | -23.33 | 76.77 | 0.4043 | 659.0 | 564.5 | |
| 0.00 | 2.00 | 0.00 | 1.09 | 4.41 | 249.22 | -24.66 | 86.47 | 0.4185 | 782.0 | 626.0 | |
| 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. | |