SDO HMI 2014-02-26 04:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.61 | 115.36 | 22.02 | 75.34 | 8.37 | 132.34 | -37.55 | 68.06 | 0.6520 | 580.8 | 307.4 | |
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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 | 1.12 | 0.00 | 0.65 | 7.19 | 142.05 | -27.83 | 63.22 | 0.5210 | -630.0 | -497.4 | |
| 0.00 | 1.03 | 0.00 | 0.60 | 7.04 | 141.01 | -28.88 | 64.34 | 0.5338 | -779.0 | -713.2 | |
| 0.00 | 0.95 | 0.00 | 0.56 | 8.18 | 140.48 | -29.41 | 62.88 | 0.5482 | -708.0 | -572.8 | |
| 0.00 | 1.72 | 0.00 | 1.03 | 6.34 | 138.67 | -31.22 | 67.27 | 0.5607 | -611.0 | -441.0 | |
| 0.00 | 0.60 | 0.00 | 0.38 | 7.34 | 134.09 | -35.79 | 68.60 | 0.6253 | 613.0 | 507.1 | |
| 0.00 | 1.03 | 0.00 | 0.66 | 7.32 | 133.91 | -35.97 | 68.73 | 0.6275 | 630.0 | 527.1 | |
| 0.00 | 1.12 | 0.00 | 0.71 | 6.92 | 133.58 | -36.31 | 69.52 | 0.6298 | -501.0 | -470.2 | |
| 0.00 | 1.12 | 0.00 | 0.72 | 6.02 | 132.94 | -36.94 | 71.20 | 0.6337 | -518.0 | -338.2 | |
| 9.74 | 30.68 | 6.33 | 19.96 | 8.65 | 132.57 | -37.31 | 67.55 | 0.6507 | 1086.9 | 462.2 | |
| 0.00 | 1.55 | 0.00 | 1.01 | 8.63 | 132.12 | -37.76 | 67.84 | 0.6561 | 764.0 | 632.1 | |
| 0.00 | 1.72 | 0.00 | 1.12 | 7.25 | 132.12 | -37.77 | 69.83 | 0.6496 | 755.0 | 597.7 | |
| 0.00 | 1.12 | 0.00 | 0.73 | 7.44 | 132.02 | -37.86 | 69.60 | 0.6516 | 647.0 | 448.5 | |
| 23.87 | 68.76 | 15.69 | 45.32 | 8.41 | 131.73 | -38.16 | 68.37 | 0.6598 | 824.4 | 316.6 | |
| 0.00 | 1.81 | 0.00 | 1.20 | 9.53 | 131.28 | -38.60 | 67.05 | 0.6706 | 276.0 | 267.5 | |
| 0.00 | 1.03 | 0.00 | 0.69 | 9.18 | 131.02 | -38.87 | 67.68 | 0.6720 | 585.0 | 459.5 | |
| 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. | |