SDO HMI 2014-10-06 18:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.74 | 0.00 | 11.66 | -18.44 | 76.03 | -32.84 | 128.41 | 0.6556 | 274.8 | 265.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.97 | 0.00 | 0.59 | -20.92 | 84.98 | -23.89 | 139.98 | 0.5904 | 546.0 | 473.4 | |
| 0.00 | 0.79 | 0.00 | 0.50 | -23.72 | 83.34 | -25.53 | 141.29 | 0.6332 | 502.0 | 432.1 | |
| 0.00 | 1.05 | 0.00 | 0.62 | -15.84 | 84.40 | -24.47 | 132.82 | 0.5454 | 618.0 | 470.1 | |
| 0.00 | 0.70 | 0.00 | 0.45 | -21.91 | 80.81 | -28.06 | 136.66 | 0.6382 | 148.0 | 242.0 | |
| 0.00 | 2.19 | 0.00 | 1.36 | -15.75 | 79.37 | -29.50 | 127.49 | 0.5995 | 343.0 | 240.6 | |
| 0.00 | 0.97 | 0.00 | 0.59 | -14.73 | 79.10 | -29.77 | 125.84 | 0.5945 | 627.0 | 520.3 | |
| 0.00 | 1.32 | 0.00 | 0.84 | -16.87 | 77.36 | -31.51 | 127.21 | 0.6302 | 830.0 | 644.2 | |
| 0.00 | 0.70 | 0.00 | 0.45 | -17.03 | 76.81 | -32.06 | 126.96 | 0.6374 | 596.0 | 570.5 | |
| 0.00 | 2.37 | 0.00 | 1.52 | -16.91 | 76.65 | -32.22 | 126.67 | 0.6382 | 857.0 | 495.9 | |
| 0.00 | 0.53 | 0.00 | 0.34 | -16.50 | 75.39 | -33.48 | 125.11 | 0.6489 | 654.0 | 563.3 | |
| 0.00 | 1.32 | 0.00 | 0.86 | -16.71 | 75.27 | -33.60 | 125.28 | 0.6516 | 647.0 | 559.7 | |
| 0.00 | 0.79 | 0.00 | 0.55 | -20.07 | 71.67 | -37.20 | 126.80 | 0.7115 | -673.0 | -529.8 | |
| 0.00 | 0.97 | 0.00 | 0.70 | -22.01 | 70.80 | -38.06 | 128.47 | 0.7324 | 363.0 | 368.5 | |
| 0.00 | 1.14 | 0.00 | 0.84 | -22.01 | 69.39 | -39.48 | 127.52 | 0.7455 | -733.0 | -648.3 | |
| 0.00 | 0.70 | 0.00 | 0.55 | -24.89 | 67.49 | -41.37 | 129.52 | 0.7795 | -467.0 | -391.2 | |
| 0.00 | 0.26 | 0.00 | 0.20 | -20.82 | 67.76 | -41.11 | 125.11 | 0.7536 | -698.0 | -556.3 | |
| 0.00 | 0.97 | 0.00 | 0.70 | -15.34 | 67.20 | -41.67 | 118.19 | 0.7297 | 512.0 | 366.1 | |
| 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. | |