SDO HMI 2014-03-05 10:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.32 | 51.28 | 11.73 | 29.53 | -17.23 | 44.71 | -29.69 | 111.83 | 0.5114 | -66.1 | -15.1 | |
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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 |
| 5.71 | 9.86 | 3.23 | 5.58 | -16.89 | 46.51 | -27.89 | 112.08 | 0.4850 | 969.6 | 676.7 | |
| 3.03 | 5.62 | 1.72 | 3.19 | -17.17 | 46.14 | -28.25 | 112.44 | 0.4913 | 840.9 | 639.1 | |
| 0.00 | 1.38 | 0.00 | 0.79 | -17.18 | 45.89 | -28.50 | 112.33 | 0.4949 | 435.0 | 330.3 | |
| 0.00 | 2.16 | 0.00 | 1.23 | -16.14 | 45.75 | -28.65 | 110.22 | 0.4928 | 826.0 | 602.4 | |
| 0.86 | 2.59 | 0.50 | 1.49 | -17.63 | 45.32 | -29.08 | 112.89 | 0.5048 | 646.0 | 365.4 | |
| 0.00 | 4.76 | 0.00 | 2.73 | -17.35 | 45.15 | -29.25 | 112.26 | 0.5059 | -221.0 | -260.9 | |
| 0.00 | 1.82 | 0.00 | 1.05 | -17.37 | 44.40 | -30.00 | 111.91 | 0.5164 | 452.0 | 416.4 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -15.89 | 44.58 | -29.82 | 109.19 | 0.5084 | -648.0 | -527.6 | |
| 0.00 | 0.61 | 0.00 | 0.35 | -16.32 | 44.19 | -30.21 | 109.84 | 0.5155 | -598.0 | -527.9 | |
| 0.00 | 1.30 | 0.00 | 0.75 | -17.52 | 43.90 | -30.50 | 111.95 | 0.5239 | -283.0 | -226.7 | |
| 0.00 | 3.63 | 0.00 | 2.11 | -17.60 | 43.70 | -30.70 | 112.00 | 0.5269 | -581.0 | -594.6 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -16.31 | 43.47 | -30.93 | 109.51 | 0.5255 | -731.0 | -607.2 | |
| 10.72 | 15.65 | 6.28 | 9.16 | -17.56 | 43.09 | -31.31 | 111.64 | 0.5351 | -897.3 | -572.2 | |
| 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. | |