SDO HMI 2014-01-13 02:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.98 | 170.39 | 19.37 | 86.89 | -17.93 | 30.05 | -0.30 | 178.84 | 0.2374 | 218.8 | 104.0 | |
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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 | 1.44 | 0.00 | 0.73 | -15.51 | 33.03 | 2.68 | 193.11 | 0.1998 | 759.0 | 626.8 | |
| 2.72 | 90.60 | 1.39 | 46.19 | -18.11 | 31.51 | 1.17 | 184.65 | 0.2398 | 1069.8 | 545.4 | |
| 6.88 | -2.00 | 3.51 | -2.00 | -17.78 | 31.48 | 1.13 | 184.63 | 0.2341 | 1298.6 | 999999 | |
| 13.00 | -2.00 | 6.63 | -2.00 | -18.05 | 31.17 | 0.82 | 183.30 | 0.2383 | 1212.6 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -17.29 | 30.83 | 0.48 | 182.05 | 0.2252 | 746.0 | 523.1 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -17.05 | 30.77 | 0.42 | 181.82 | 0.2210 | 785.0 | 610.1 | |
| 0.00 | 0.68 | 0.00 | 0.35 | -17.41 | 30.67 | 0.33 | 181.38 | 0.2272 | 795.0 | 569.1 | |
| 0.00 | 0.76 | 0.00 | 0.39 | -17.90 | 30.55 | 0.20 | 180.83 | 0.2354 | 622.0 | 492.4 | |
| 0.00 | 4.76 | 0.00 | 2.43 | -18.32 | 30.27 | -0.08 | 179.70 | 0.2426 | 801.0 | 692.5 | |
| 0.00 | 1.87 | 0.00 | 0.95 | -18.02 | 29.90 | -0.45 | 178.20 | 0.2375 | 283.0 | 218.6 | |
| 0.00 | 1.70 | 0.00 | 0.87 | -18.23 | 29.12 | -1.22 | 175.17 | 0.2419 | -901.0 | -739.5 | |
| 0.76 | 3.99 | 0.39 | 2.04 | -18.41 | 28.87 | -1.47 | 174.27 | 0.2453 | -1050.1 | -783.7 | |
| 0.51 | 62.72 | 0.26 | 31.99 | -17.74 | 28.72 | -1.62 | 173.36 | 0.2343 | -959.7 | -539.2 | |
| 1.02 | -13.00 | 0.52 | -13.00 | -17.77 | 28.41 | -1.93 | 172.13 | 0.2355 | -1135.5 | 999999 | |
| 13.09 | -13.00 | 6.67 | -13.00 | -17.92 | 28.13 | -2.21 | 171.11 | 0.2387 | -1242.6 | 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. | |