SDO HMI 2014-05-26 06:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.17 | 193.76 | 74.81 | 415.93 | -18.84 | 150.05 | 76.15 | 250.88 | 0.9710 | 89.9 | -30.4 | |
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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 | 2.71 | 0.00 | 6.81 | -17.34 | 152.41 | 78.51 | 252.59 | 0.9812 | 321.0 | 265.3 | |
| 13.53 | 76.77 | 38.65 | 223.85 | -18.43 | 153.76 | 79.86 | 251.53 | 0.9854 | 138.0 | -19.0 | |
| 0.00 | 0.99 | 0.00 | 2.33 | -17.61 | 151.56 | 77.66 | 252.27 | 0.9784 | 389.0 | 377.2 | |
| 0.63 | 6.40 | 1.26 | 12.73 | -17.47 | 149.15 | 75.25 | 252.30 | 0.9694 | -354.1 | 179.3 | |
| 2.98 | 30.58 | 4.86 | 49.45 | -17.51 | 145.76 | 71.86 | 252.04 | 0.9540 | -245.9 | -291.3 | |
| 2.80 | -5.00 | 4.51 | -5.00 | -17.74 | 145.57 | 71.67 | 251.79 | 0.9531 | -333.5 | 999999 | |
| 4.69 | -5.00 | 7.45 | -5.00 | -18.10 | 145.20 | 71.30 | 251.38 | 0.9514 | -336.4 | 999999 | |
| 0.00 | 5.68 | 0.00 | 9.41 | -19.98 | 145.83 | 71.93 | 249.47 | 0.9554 | -410.0 | -230.0 | |
| 9.74 | 31.57 | 15.18 | 49.39 | -19.26 | 144.66 | 70.76 | 250.11 | 0.9492 | 414.3 | 310.1 | |
| 0.00 | 0.90 | 0.00 | 1.36 | -18.67 | 144.07 | 70.17 | 250.69 | 0.9458 | 602.0 | 526.3 | |
| 1.53 | 38.16 | 2.46 | 60.60 | -21.07 | 145.09 | 71.19 | 248.26 | 0.9523 | -169.9 | -195.0 | |
| 0.27 | -11.00 | 0.44 | -11.00 | -21.49 | 145.26 | 71.37 | 247.84 | 0.9534 | 501.7 | 999999 | |
| 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. | |