SDO HMI 2014-05-18 13:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.67 | 274.11 | 25.31 | 151.76 | -24.31 | 191.12 | 15.23 | 212.43 | 0.4485 | 825.9 | 289.8 | |
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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 |
| 25.80 | 252.88 | 14.29 | 140.12 | -24.08 | 191.61 | 15.72 | 213.57 | 0.4492 | 1285.2 | 371.4 | |
| 18.88 | -1.00 | 10.47 | -1.00 | -24.38 | 191.41 | 15.51 | 212.84 | 0.4511 | 1199.5 | 999999 | |
| 0.99 | -1.00 | 0.55 | -1.00 | -23.73 | 191.12 | 15.23 | 213.24 | 0.4405 | 1175.8 | 999999 | |
| 0.00 | 2.07 | 0.00 | 1.15 | -25.93 | 190.49 | 14.60 | 209.39 | 0.4637 | 61.0 | 159.5 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -24.13 | 190.04 | 14.14 | 210.86 | 0.4366 | 824.0 | 674.9 | |
| 0.00 | 8.00 | 0.00 | 4.35 | -24.45 | 186.36 | 10.46 | 203.62 | 0.4142 | -872.0 | -759.7 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -25.70 | 186.16 | 10.26 | 201.96 | 0.4309 | -764.0 | -656.2 | |
| 0.00 | 2.34 | 0.00 | 1.28 | -25.83 | 185.65 | 9.76 | 200.87 | 0.4300 | -931.0 | -741.1 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -27.30 | 185.57 | 9.68 | 199.43 | 0.4508 | -867.0 | -679.8 | |
| 0.00 | 1.71 | 0.00 | 0.95 | -27.91 | 184.58 | 8.69 | 197.13 | 0.4549 | -778.0 | -610.6 | |
| 0.00 | 3.51 | 0.00 | 1.93 | -27.14 | 184.11 | 8.21 | 196.81 | 0.4413 | -733.0 | -524.8 | |
| 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. | |