SDO HMI 2014-03-08 14:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.87 | 36.72 | 13.07 | 49.92 | -18.60 | 322.81 | -69.87 | 107.20 | 0.9327 | 79.7 | -74.1 | |
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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 |
| 4.24 | 6.75 | 5.17 | 8.22 | -18.08 | 325.62 | -67.06 | 106.62 | 0.9153 | 535.1 | 422.7 | |
| 0.00 | 0.61 | 0.00 | 0.76 | -18.37 | 324.81 | -67.87 | 106.93 | 0.9206 | 145.0 | 124.3 | |
| 0.00 | 0.61 | 0.00 | 0.79 | -19.08 | 323.94 | -68.74 | 107.70 | 0.9262 | -373.0 | -388.4 | |
| 0.00 | 1.56 | 0.00 | 1.98 | -17.93 | 324.57 | -68.11 | 106.46 | 0.9222 | 397.0 | 344.6 | |
| 0.00 | 1.99 | 0.00 | 2.55 | -18.22 | 324.34 | -68.34 | 106.77 | 0.9237 | 126.0 | 147.3 | |
| 0.00 | 0.87 | 0.00 | 1.15 | -19.23 | 323.35 | -69.33 | 107.87 | 0.9298 | -237.0 | -254.4 | |
| 0.00 | 1.04 | 0.00 | 1.33 | -18.05 | 324.22 | -68.46 | 106.59 | 0.9244 | 190.0 | 149.2 | |
| 1.73 | 8.40 | 2.32 | 11.18 | -18.90 | 323.20 | -69.47 | 107.51 | 0.9307 | -184.4 | -226.7 | |
| 0.00 | 6.15 | 0.00 | 9.30 | -19.64 | 320.40 | -72.28 | 108.33 | 0.9466 | -256.0 | -159.2 | |
| 1.13 | 2.16 | 1.65 | 3.17 | -18.75 | 321.15 | -71.53 | 107.38 | 0.9426 | -445.1 | -360.1 | |
| 0.00 | 1.47 | 0.00 | 2.21 | -19.25 | 320.61 | -72.06 | 107.92 | 0.9454 | -303.0 | -243.1 | |
| 0.00 | 0.69 | 0.00 | 1.02 | -18.35 | 321.16 | -71.52 | 106.95 | 0.9426 | -449.0 | -387.9 | |
| 2.77 | 4.42 | 3.93 | 6.26 | -17.28 | 321.89 | -70.79 | 105.80 | 0.9386 | 232.9 | 84.9 | |
| 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. | |