SDO HMI 2014-01-11 16:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.73 | 0.00 | 9.73 | -23.79 | 55.54 | 6.52 | 200.21 | 0.4179 | -575.9 | -442.0 | |
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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 | 2.04 | 0.00 | 1.12 | -14.72 | 72.86 | 23.83 | 244.20 | 0.4359 | -873.0 | -696.5 | |
| 0.00 | 1.36 | 0.00 | 0.78 | -21.61 | 73.81 | 24.78 | 231.88 | 0.4974 | 693.0 | 503.3 | |
| 0.00 | 1.10 | 0.00 | 0.63 | -21.63 | 73.22 | 24.19 | 231.25 | 0.4905 | 802.0 | 619.5 | |
| 0.00 | 1.02 | 0.00 | 0.54 | -15.65 | 65.23 | 16.21 | 233.13 | 0.3375 | -812.0 | -644.6 | |
| 0.00 | 1.10 | 0.00 | 0.57 | -16.28 | 59.63 | 10.61 | 219.98 | 0.2763 | -759.0 | -682.5 | |
| 0.00 | 1.53 | 0.00 | 0.79 | -16.13 | 59.56 | 10.54 | 220.16 | 0.2736 | -928.0 | -720.8 | |
| 0.00 | 1.10 | 0.00 | 0.57 | -19.27 | 58.35 | 9.33 | 210.37 | 0.3040 | -809.0 | -700.2 | |
| 0.00 | 0.76 | 0.00 | 0.41 | -24.76 | 52.05 | 3.03 | 187.77 | 0.3564 | -828.0 | -635.8 | |
| 0.00 | 1.19 | 0.00 | 0.66 | -30.62 | 52.11 | 3.09 | 185.94 | 0.4495 | -786.0 | -607.6 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -29.50 | 42.41 | -6.62 | 166.82 | 0.4415 | -782.0 | -669.4 | |
| 0.00 | 1.44 | 0.00 | 0.80 | -29.76 | 42.32 | -6.70 | 166.81 | 0.4458 | -589.0 | -422.6 | |
| 0.00 | 1.78 | 0.00 | 1.03 | -34.22 | 41.08 | -7.94 | 167.16 | 0.5162 | -714.0 | -428.4 | |
| 0.00 | 1.10 | 0.00 | 0.62 | -31.57 | 39.15 | -9.88 | 162.41 | 0.4856 | -819.0 | -551.3 | |
| 0.00 | 0.85 | 0.00 | 0.46 | -26.01 | 38.34 | -10.68 | 155.93 | 0.4102 | -859.0 | -665.1 | |
| 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. | |