SDO HMI 2014-10-13 22:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.73 | 0.00 | 10.28 | 17.24 | 352.16 | -22.14 | 59.11 | 0.4111 | -284.2 | -223.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.40 | 0.00 | 0.71 | 14.57 | 3.54 | -10.77 | 50.09 | 0.2368 | -1016.0 | -793.7 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 14.51 | 3.14 | -11.17 | 51.31 | 0.2414 | -901.0 | -699.0 | |
| 0.00 | 1.31 | 0.00 | 0.68 | 14.69 | 0.12 | -14.19 | 56.93 | 0.2843 | -967.0 | -808.5 | |
| 0.00 | 1.75 | 0.00 | 0.90 | 14.92 | 359.94 | -14.37 | 56.51 | 0.2887 | -980.0 | -820.8 | |
| 0.00 | 1.49 | 0.00 | 0.77 | 14.47 | 359.94 | -14.37 | 57.89 | 0.2849 | -1091.0 | -941.0 | |
| 0.00 | 0.70 | 0.00 | 0.36 | 15.81 | 358.89 | -15.42 | 55.74 | 0.3110 | -554.0 | -615.1 | |
| 0.00 | 2.80 | 0.00 | 1.49 | 16.52 | 355.23 | -19.07 | 58.97 | 0.3672 | -882.0 | -637.2 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 15.25 | 352.58 | -21.73 | 64.79 | 0.3965 | -426.0 | -380.5 | |
| 0.00 | 1.57 | 0.00 | 0.91 | 17.50 | 344.61 | -29.70 | 65.77 | 0.5203 | 563.0 | 458.7 | |
| 0.00 | 1.84 | 0.00 | 1.11 | 22.82 | 342.52 | -31.79 | 57.94 | 0.5752 | 580.0 | 510.2 | |
| 0.00 | 1.05 | 0.00 | 0.64 | 23.35 | 342.30 | -32.01 | 57.25 | 0.5808 | 682.0 | 535.9 | |
| 0.00 | 1.75 | 0.00 | 1.04 | 17.15 | 341.92 | -32.38 | 67.77 | 0.5550 | 699.0 | 504.2 | |
| 0.00 | 0.79 | 0.00 | 0.48 | 21.38 | 340.66 | -33.65 | 61.36 | 0.5901 | 599.0 | 490.3 | |
| 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. | |