SDO HMI 2014-08-09 19:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.41 | 28.95 | 2.96 | 15.93 | -18.43 | 160.77 | 6.48 | 194.33 | 0.4341 | 832.9 | 707.5 | |
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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 | 1.08 | 0.00 | 0.60 | -17.27 | 165.27 | 10.98 | 204.53 | 0.4399 | 728.0 | 573.7 | |
| 1.08 | 3.70 | 0.60 | 2.05 | -19.40 | 161.23 | 6.94 | 194.73 | 0.4501 | 851.8 | 757.4 | |
| 0.00 | 2.26 | 0.00 | 1.25 | -19.02 | 161.12 | 6.83 | 194.72 | 0.4440 | 996.0 | 811.2 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -19.70 | 161.12 | 6.82 | 194.32 | 0.4542 | 548.0 | 463.2 | |
| 0.00 | 2.08 | 0.00 | 1.15 | -19.33 | 160.97 | 6.68 | 194.24 | 0.4480 | 856.0 | 753.8 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -19.12 | 160.90 | 6.60 | 194.21 | 0.4446 | 862.0 | 818.7 | |
| 0.00 | 1.62 | 0.00 | 0.90 | -19.59 | 160.88 | 6.59 | 193.91 | 0.4517 | 723.0 | 562.3 | |
| 4.33 | 9.93 | 2.36 | 5.40 | -17.18 | 160.76 | 6.47 | 195.12 | 0.4145 | 990.8 | 803.7 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -19.25 | 160.71 | 6.42 | 193.74 | 0.4459 | 891.0 | 698.4 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -19.46 | 160.62 | 6.33 | 193.45 | 0.4486 | 805.0 | 642.3 | |
| 0.00 | 1.17 | 0.00 | 0.66 | -20.71 | 160.51 | 6.21 | 192.56 | 0.4672 | 691.0 | 498.8 | |
| 0.00 | 1.44 | 0.00 | 0.80 | -19.61 | 159.59 | 5.29 | 191.25 | 0.4476 | 846.0 | 635.4 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -15.61 | 158.81 | 4.52 | 191.48 | 0.3827 | 762.0 | 594.2 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -17.57 | 155.76 | 1.47 | 183.44 | 0.4077 | 903.0 | 689.4 | |
| 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. | |