SDO HMI 2014-07-04 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.35 | 0.00 | 11.52 | 7.29 | 265.63 | -12.64 | 97.27 | 0.2358 | 330.8 | 403.6 | |
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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 | 1.09 | 0.00 | 0.54 | 6.20 | 279.59 | 1.32 | 336.33 | 0.0573 | -945.0 | -685.4 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 3.34 | 278.94 | 0.67 | 281.18 | 0.0120 | -957.0 | -776.8 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 2.91 | 275.55 | -2.72 | 96.10 | 0.0478 | -904.0 | -692.1 | |
| 0.00 | 0.91 | 0.00 | 0.45 | 3.13 | 275.55 | -2.72 | 91.62 | 0.0476 | -867.0 | -687.4 | |
| 0.00 | 3.09 | 0.00 | 1.56 | 9.33 | 269.72 | -8.55 | 53.82 | 0.1825 | 1022.0 | 719.2 | |
| 0.00 | 1.73 | 0.00 | 0.87 | 8.56 | 269.15 | -9.12 | 59.06 | 0.1836 | 901.0 | 727.3 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 8.43 | 268.56 | -9.71 | 61.17 | 0.1914 | 733.0 | 494.7 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 8.52 | 265.16 | -13.11 | 67.25 | 0.2444 | 896.0 | 773.9 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 8.97 | 261.53 | -16.74 | 70.15 | 0.3038 | 1048.0 | 835.6 | |
| 0.00 | 4.45 | 0.00 | 2.32 | 8.93 | 261.24 | -17.03 | 70.55 | 0.3081 | 895.0 | 800.4 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 1.46 | 259.52 | -18.75 | 94.91 | 0.3239 | 761.0 | 641.5 | |
| 0.00 | 1.64 | 0.00 | 0.87 | 7.56 | 258.06 | -20.21 | 76.96 | 0.3531 | 718.0 | 436.1 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 8.83 | 251.18 | -27.09 | 76.99 | 0.4638 | 709.0 | 584.2 | |
| 0.00 | 0.82 | 0.00 | 0.46 | 7.66 | 250.95 | -27.32 | 79.57 | 0.4644 | 621.0 | 640.8 | |
| 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. | |