SDO HMI 2014-10-09 00:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.65 | 28.94 | 2.56 | 16.15 | -13.06 | 59.89 | -19.28 | 135.54 | 0.4601 | 408.3 | 240.3 | |
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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 | 0.88 | 0.00 | 0.49 | -15.29 | 62.83 | -16.34 | 143.28 | 0.4557 | 526.0 | 429.4 | |
| 0.96 | 7.72 | 0.53 | 4.25 | -12.85 | 61.55 | -17.62 | 137.60 | 0.4395 | 1025.0 | 783.3 | |
| 0.88 | -2.00 | 0.48 | -2.00 | -12.65 | 61.54 | -17.63 | 137.28 | 0.4373 | 1048.1 | 999999 | |
| 2.81 | 5.44 | 1.55 | 3.00 | -12.80 | 61.21 | -17.96 | 136.97 | 0.4424 | 887.6 | 692.9 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -13.99 | 60.01 | -19.16 | 136.96 | 0.4685 | 654.0 | 580.9 | |
| 0.00 | 2.28 | 0.00 | 1.27 | -13.16 | 60.29 | -18.88 | 136.12 | 0.4563 | 776.0 | 420.5 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -14.49 | 59.21 | -19.96 | 136.54 | 0.4824 | 623.0 | 544.0 | |
| 0.00 | 0.70 | 0.00 | 0.39 | -12.99 | 60.15 | -19.02 | 135.64 | 0.4560 | -510.0 | -525.4 | |
| 0.00 | 1.05 | 0.00 | 0.59 | -13.06 | 59.95 | -19.22 | 135.44 | 0.4589 | 446.0 | 336.5 | |
| 0.00 | 4.65 | 0.00 | 2.58 | -11.97 | 59.69 | -19.48 | 133.31 | 0.4501 | -750.0 | -697.7 | |
| 0.00 | 1.05 | 0.00 | 0.60 | -14.96 | 57.33 | -21.84 | 134.66 | 0.5073 | 559.0 | 446.4 | |
| 0.00 | 1.05 | 0.00 | 0.61 | -15.07 | 55.68 | -23.49 | 132.74 | 0.5262 | 411.0 | 434.9 | |
| 0.00 | 1.75 | 0.00 | 1.04 | -12.99 | 52.07 | -27.10 | 125.69 | 0.5486 | -669.0 | -480.9 | |
| 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. | |