SDO HMI 2014-03-06 13:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.43 | 24.11 | 0.31 | 17.37 | 17.13 | 99.65 | 40.07 | 302.02 | 0.7277 | 347.5 | 380.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.04 | 0.00 | 0.80 | 16.66 | 103.94 | 44.36 | 298.96 | 0.7679 | -274.0 | -300.3 | |
| 0.00 | 0.52 | 0.00 | 0.40 | 17.05 | 104.02 | 44.44 | 299.38 | 0.7705 | -566.0 | -525.7 | |
| 0.00 | 0.95 | 0.00 | 0.74 | 17.52 | 103.76 | 44.19 | 300.06 | 0.7703 | -453.0 | -419.0 | |
| 0.00 | 1.12 | 0.00 | 0.81 | 15.52 | 100.51 | 40.93 | 299.50 | 0.7276 | 445.0 | 474.5 | |
| 0.00 | 0.95 | 0.00 | 0.69 | 15.77 | 100.45 | 40.87 | 299.85 | 0.7283 | 461.0 | 371.2 | |
| 0.00 | 0.86 | 0.00 | 0.62 | 15.79 | 100.29 | 40.71 | 299.96 | 0.7268 | 519.0 | 387.4 | |
| 0.00 | 0.52 | 0.00 | 0.37 | 14.74 | 100.00 | 40.42 | 298.83 | 0.7181 | 530.0 | 439.3 | |
| 0.00 | 1.12 | 0.00 | 0.81 | 17.12 | 99.69 | 40.11 | 301.96 | 0.7281 | -569.0 | -498.5 | |
| 0.00 | 4.58 | 0.00 | 3.25 | 16.49 | 99.12 | 39.54 | 301.55 | 0.7187 | 778.0 | 659.4 | |
| 0.00 | 0.52 | 0.00 | 0.37 | 16.85 | 99.13 | 39.55 | 301.98 | 0.7208 | 394.0 | 394.7 | |
| 0.00 | 2.68 | 0.00 | 1.90 | 16.96 | 98.87 | 39.30 | 302.28 | 0.7188 | 838.0 | 667.8 | |
| 0.00 | 1.38 | 0.00 | 1.00 | 18.16 | 99.19 | 39.61 | 303.52 | 0.7291 | 424.0 | 431.4 | |
| 0.00 | 1.64 | 0.00 | 1.18 | 17.59 | 99.00 | 39.42 | 302.96 | 0.7238 | 690.0 | 566.2 | |
| 0.00 | 2.25 | 0.00 | 1.63 | 18.79 | 99.33 | 39.75 | 304.19 | 0.7342 | 544.0 | 378.8 | |
| 0.43 | 1.38 | 0.31 | 0.99 | 18.01 | 99.07 | 39.49 | 303.43 | 0.7270 | 719.2 | 644.3 | |
| 0.00 | 0.78 | 0.00 | 0.56 | 18.63 | 99.00 | 39.42 | 304.21 | 0.7300 | 537.0 | 520.9 | |
| 0.00 | 0.78 | 0.00 | 0.56 | 20.82 | 97.44 | 37.86 | 307.83 | 0.7287 | 501.0 | 417.9 | |
| 0.00 | 1.04 | 0.00 | 0.69 | 15.06 | 95.70 | 36.12 | 302.03 | 0.6738 | 621.0 | 529.8 | |
| 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. | |