| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 78.95 | 430.48 | 72.44 | 393.44 | 7.81 | 344.02 | 57.73 | 274.74 | 0.8426 | -315.6 | -341.5 | |
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back to the solar disc SDO HMI 2014-08-27 01:00:37 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.24 | 0.00 | 2.31 | 8.23 | 348.14 | 61.84 | 275.52 | 0.8786 | -185.0 | -91.3 | |
| 0.00 | 1.53 | 0.00 | 1.56 | 7.71 | 347.87 | 61.57 | 274.91 | 0.8766 | -318.0 | -336.0 | |
| 1.97 | 13.28 | 1.99 | 13.36 | 8.40 | 347.41 | 61.11 | 275.67 | 0.8724 | -605.6 | -428.3 | |
| 4.04 | 5.92 | 4.02 | 5.89 | 9.64 | 347.06 | 60.77 | 277.06 | 0.8689 | 490.4 | 354.1 | |
| 0.00 | 2.78 | 0.00 | 2.69 | 7.39 | 345.97 | 59.67 | 274.40 | 0.8605 | 339.0 | 221.1 | |
| 23.42 | 393.68 | 21.70 | 358.06 | 6.97 | 344.45 | 58.15 | 273.78 | 0.8471 | 399.1 | -362.7 | |
| 0.00 | 0.81 | 0.00 | 0.75 | 11.06 | 344.69 | 58.39 | 278.62 | 0.8475 | -267.0 | -280.1 | |
| 47.64 | -6.00 | 43.08 | -6.00 | 8.10 | 343.59 | 57.30 | 275.06 | 0.8385 | -843.6 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.25 | 11.45 | 344.46 | 58.17 | 279.08 | 0.8453 | -259.0 | -341.7 | |
| 1.88 | -6.00 | 1.65 | -6.00 | 6.83 | 342.33 | 56.03 | 273.44 | 0.8271 | 249.9 | 999999 | |
| 0.00 | 3.32 | 0.00 | 2.88 | 10.34 | 342.08 | 55.78 | 277.69 | 0.8230 | 218.0 | 197.6 | |
| 0.00 | 1.97 | 0.00 | 1.69 | 8.29 | 341.52 | 55.23 | 275.15 | 0.8183 | -302.0 | -301.1 | |
| 0.00 | 0.45 | 0.00 | 0.39 | 8.70 | 341.61 | 55.32 | 275.67 | 0.8190 | -418.0 | -389.2 | |
| 0.00 | 1.08 | 0.00 | 0.93 | 10.61 | 341.87 | 55.58 | 278.01 | 0.8209 | 626.0 | 550.8 | |
| 0.00 | 1.08 | 0.00 | 0.92 | 10.21 | 341.60 | 55.31 | 277.51 | 0.8184 | 537.0 | 456.7 | |
| 0.00 | 0.90 | 0.00 | 0.77 | 10.45 | 341.66 | 55.37 | 277.80 | 0.8189 | 400.0 | 427.2 | |
| 0.00 | 1.17 | 0.00 | 0.99 | 8.61 | 341.00 | 54.71 | 275.52 | 0.8130 | -512.0 | -393.5 | |
| 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. | |