SDO HMI 2014-05-18 03:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.35 | 42.81 | 9.77 | 24.20 | -17.24 | 156.35 | -25.03 | 122.99 | 0.4828 | 263.6 | 68.7 | |
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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 | 4.50 | 0.00 | 2.51 | -17.55 | 158.33 | -23.05 | 125.43 | 0.4600 | 696.0 | 683.9 | |
| 0.27 | 19.60 | 0.15 | 10.91 | -16.89 | 158.35 | -23.03 | 124.20 | 0.4545 | 1155.7 | 725.6 | |
| 5.21 | -2.00 | 2.90 | -2.00 | -16.98 | 158.16 | -23.22 | 124.18 | 0.4576 | 1005.3 | 999999 | |
| 6.02 | -2.00 | 3.35 | -2.00 | -16.82 | 158.04 | -23.33 | 123.76 | 0.4579 | 1069.2 | 999999 | |
| 1.44 | -2.00 | 0.80 | -2.00 | -16.95 | 157.89 | -23.49 | 123.83 | 0.4609 | 726.2 | 999999 | |
| 0.00 | 1.80 | 0.00 | 1.00 | -16.53 | 157.53 | -23.85 | 122.68 | 0.4624 | 679.0 | 498.0 | |
| 0.00 | 0.72 | 0.00 | 0.40 | -17.06 | 157.32 | -24.06 | 123.47 | 0.4691 | -583.0 | -455.2 | |
| 0.00 | 0.72 | 0.00 | 0.40 | -16.27 | 157.01 | -24.37 | 121.68 | 0.4673 | 157.0 | 172.8 | |
| 0.00 | 1.53 | 0.00 | 0.87 | -19.03 | 156.25 | -25.13 | 125.93 | 0.4978 | 531.0 | 409.9 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -16.18 | 155.45 | -25.93 | 120.09 | 0.4873 | -816.0 | -707.4 | |
| 0.81 | 10.70 | 0.47 | 6.23 | -17.43 | 153.08 | -28.30 | 120.37 | 0.5263 | -978.9 | -779.2 | |
| 3.60 | -11.00 | 2.10 | -11.00 | -17.61 | 153.01 | -28.37 | 120.64 | 0.5283 | -852.8 | 999999 | |
| 0.00 | 2.25 | 0.00 | 1.32 | -18.24 | 152.79 | -28.59 | 121.53 | 0.5352 | -894.0 | -685.0 | |
| 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. | |