SDO HMI 2014-07-03 14:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.88 | 0.00 | 14.24 | 6.54 | 262.27 | -24.30 | 80.85 | 0.4149 | 579.0 | 436.2 | |
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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 | 3.09 | 0.00 | 1.56 | 4.25 | 276.12 | -10.45 | 83.50 | 0.1828 | -726.0 | -616.8 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 1.67 | 274.21 | -12.35 | 96.41 | 0.2162 | -680.0 | -540.0 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 10.78 | 267.42 | -19.15 | 67.09 | 0.3513 | 850.0 | 642.5 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 2.81 | 267.73 | -18.83 | 90.47 | 0.3238 | 742.0 | 604.1 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 6.77 | 267.53 | -19.04 | 78.40 | 0.3321 | 838.0 | 570.8 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 10.90 | 267.21 | -19.35 | 66.97 | 0.3551 | 837.0 | 644.7 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 9.60 | 265.12 | -21.45 | 72.08 | 0.3805 | 891.0 | 715.9 | |
| 0.00 | 5.00 | 0.00 | 2.75 | 8.60 | 260.97 | -25.59 | 76.73 | 0.4406 | 818.0 | 681.1 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 8.65 | 260.63 | -25.94 | 76.76 | 0.4461 | 786.0 | 596.8 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 8.56 | 260.43 | -26.14 | 77.05 | 0.4488 | 678.0 | 507.5 | |
| 0.00 | 1.45 | 0.00 | 0.82 | -1.17 | 258.60 | -27.97 | 98.30 | 0.4757 | 725.0 | 538.5 | |
| 0.00 | 1.82 | 0.00 | 1.03 | 7.70 | 257.85 | -28.71 | 79.71 | 0.4858 | 804.0 | 623.4 | |
| 0.00 | 1.73 | 0.00 | 1.00 | 5.20 | 255.71 | -30.86 | 85.09 | 0.5147 | 831.0 | 693.3 | |
| 0.00 | 1.36 | 0.00 | 0.85 | 4.51 | 249.07 | -37.49 | 86.65 | 0.6100 | 637.0 | 526.1 | |
| 0.00 | 1.27 | 0.00 | 0.81 | 6.45 | 247.48 | -39.08 | 83.61 | 0.6326 | 654.0 | 493.2 | |
| 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. | |