| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.43 | 0.00 | 14.92 | -19.03 | 77.47 | -36.89 | 125.97 | 0.7004 | 402.9 | 363.2 | |
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back to the solar disc SDO HMI 2014-10-06 08:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.81 | 0.00 | 1.78 | -18.74 | 85.03 | -29.33 | 131.60 | 0.6226 | 278.0 | 287.8 | |
| 0.00 | 0.79 | 0.00 | 0.52 | -20.81 | 82.70 | -31.66 | 132.03 | 0.6629 | 631.0 | 536.3 | |
| 0.00 | 1.67 | 0.00 | 1.14 | -20.18 | 79.48 | -34.88 | 128.64 | 0.6896 | 501.0 | 393.2 | |
| 0.00 | 2.81 | 0.00 | 1.88 | -18.18 | 79.70 | -34.66 | 126.35 | 0.6733 | 860.0 | 695.1 | |
| 0.00 | 1.32 | 0.00 | 0.86 | -15.57 | 79.83 | -34.53 | 123.09 | 0.6540 | 741.0 | 609.5 | |
| 0.00 | 1.49 | 0.00 | 0.97 | -15.09 | 79.81 | -34.55 | 122.43 | 0.6511 | 777.0 | 649.9 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -20.22 | 78.33 | -36.03 | 127.83 | 0.7012 | 683.0 | 669.0 | |
| 0.00 | 1.05 | 0.00 | 0.73 | -19.07 | 77.76 | -36.60 | 126.03 | 0.6991 | 528.0 | 429.4 | |
| 0.00 | 1.58 | 0.00 | 1.08 | -16.78 | 77.22 | -37.14 | 122.80 | 0.6901 | 770.0 | 668.3 | |
| 0.00 | 1.49 | 0.00 | 1.13 | -23.44 | 74.48 | -39.89 | 128.87 | 0.7580 | 630.0 | 371.3 | |
| 0.00 | 0.79 | 0.00 | 0.57 | -19.58 | 75.65 | -38.71 | 125.19 | 0.7234 | 728.0 | 538.2 | |
| 0.00 | 1.14 | 0.00 | 0.82 | -19.44 | 74.95 | -39.41 | 124.56 | 0.7293 | 463.0 | 438.3 | |
| 0.00 | 0.88 | 0.00 | 0.61 | -16.93 | 75.63 | -38.73 | 121.94 | 0.7076 | 538.0 | 413.2 | |
| 0.00 | 0.62 | 0.00 | 0.45 | -19.59 | 74.62 | -39.74 | 124.54 | 0.7335 | 287.0 | 290.1 | |
| 0.00 | 0.44 | 0.00 | 0.33 | -19.63 | 72.84 | -41.52 | 123.48 | 0.7509 | -600.0 | -602.0 | |
| 0.00 | 1.32 | 0.00 | 1.09 | -22.37 | 68.71 | -45.65 | 124.28 | 0.8026 | -556.0 | -400.9 | |
| 0.00 | 0.97 | 0.00 | 0.78 | -19.59 | 68.43 | -45.93 | 121.00 | 0.7920 | -409.0 | -352.1 | |
| 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. | |