SDO HMI 2014-04-22 14:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.97 | 0.00 | 12.38 | -19.39 | 163.65 | 4.61 | 197.73 | 0.2754 | -775.9 | -608.3 | |
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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 | 1.42 | 0.00 | 0.74 | -13.39 | 175.61 | 16.57 | 241.66 | 0.3166 | -815.0 | -530.9 | |
| 0.00 | 1.95 | 0.00 | 1.00 | -12.22 | 171.42 | 12.39 | 238.60 | 0.2467 | -743.0 | -661.0 | |
| 0.00 | 1.69 | 0.00 | 0.91 | -25.95 | 167.93 | 8.89 | 201.17 | 0.3864 | -682.0 | -504.8 | |
| 0.00 | 0.89 | 0.00 | 0.44 | -10.39 | 165.38 | 6.35 | 228.94 | 0.1448 | -806.0 | -658.5 | |
| 0.00 | 1.42 | 0.00 | 0.79 | -30.88 | 165.12 | 6.09 | 191.76 | 0.4483 | -744.0 | -637.4 | |
| 0.00 | 3.11 | 0.00 | 1.59 | -19.56 | 162.25 | 3.21 | 191.84 | 0.2585 | -563.0 | -539.7 | |
| 0.00 | 1.24 | 0.00 | 0.63 | -16.44 | 162.04 | 3.00 | 194.19 | 0.2059 | -901.0 | -731.6 | |
| 0.00 | 1.95 | 0.00 | 1.00 | -18.66 | 161.85 | 2.81 | 191.12 | 0.2422 | -878.0 | -690.7 | |
| 0.00 | 0.98 | 0.00 | 0.49 | -16.32 | 161.57 | 2.53 | 192.16 | 0.2020 | -870.0 | -694.1 | |
| 0.00 | 1.69 | 0.00 | 0.87 | -19.91 | 161.55 | 2.51 | 189.09 | 0.2621 | -756.0 | -584.7 | |
| 0.00 | 1.33 | 0.00 | 0.68 | -18.82 | 161.44 | 2.40 | 189.42 | 0.2436 | -871.0 | -666.2 | |
| 0.00 | 1.69 | 0.00 | 0.88 | -23.81 | 161.09 | 2.05 | 185.79 | 0.3259 | -941.0 | -705.1 | |
| 0.00 | 3.37 | 0.00 | 1.72 | -18.54 | 159.56 | 0.52 | 182.12 | 0.2357 | -650.0 | -577.8 | |
| 0.00 | 1.24 | 0.00 | 0.64 | -22.20 | 157.68 | -1.36 | 175.77 | 0.2981 | -642.0 | -465.7 | |
| 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. | |