SDO HMI 2014-01-11 19:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.22 | 0.00 | 12.10 | -20.39 | 60.23 | 12.87 | 214.29 | 0.4065 | -692.6 | -552.4 | |
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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 | 2.12 | 0.00 | 1.25 | -12.31 | 79.53 | 32.16 | 253.70 | 0.5440 | -841.0 | -612.4 | |
| 0.00 | 3.31 | 0.00 | 1.84 | -14.57 | 72.82 | 25.46 | 245.81 | 0.4580 | -722.0 | -483.2 | |
| 0.00 | 1.44 | 0.00 | 0.82 | -22.67 | 71.50 | 24.13 | 229.46 | 0.4985 | 741.0 | 601.5 | |
| 0.00 | 1.78 | 0.00 | 0.95 | -15.39 | 65.35 | 17.98 | 236.43 | 0.3588 | -840.0 | -673.6 | |
| 0.00 | 2.38 | 0.00 | 1.23 | -16.24 | 59.54 | 12.17 | 223.91 | 0.2932 | -1083.0 | -767.1 | |
| 0.00 | 0.76 | 0.00 | 0.40 | -19.26 | 58.50 | 11.13 | 214.92 | 0.3199 | -697.0 | -580.3 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -19.14 | 57.76 | 10.40 | 213.35 | 0.3115 | -842.0 | -764.1 | |
| 0.00 | 1.78 | 0.00 | 0.95 | -23.98 | 56.25 | 8.88 | 202.58 | 0.3691 | -776.0 | -650.2 | |
| 0.00 | 0.59 | 0.00 | 0.32 | -24.38 | 52.56 | 5.19 | 193.42 | 0.3567 | -851.0 | -710.4 | |
| 0.00 | 2.21 | 0.00 | 1.17 | -24.14 | 51.90 | 4.54 | 191.94 | 0.3504 | -826.0 | -674.9 | |
| 0.00 | 1.02 | 0.00 | 0.57 | -30.72 | 51.93 | 4.57 | 188.71 | 0.4539 | -699.0 | -572.9 | |
| 0.00 | 0.93 | 0.00 | 0.51 | -29.66 | 42.68 | -4.68 | 170.63 | 0.4378 | -688.0 | -543.2 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -29.33 | 42.33 | -5.04 | 169.78 | 0.4337 | -752.0 | -674.1 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -26.01 | 38.29 | -9.08 | 159.15 | 0.4002 | -820.0 | -681.8 | |
| 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. | |