SDO HMI 2014-04-09 12:01:18 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.82 | 0.00 | 10.72 | -19.61 | 326.41 | -5.37 | 163.50 | 0.2616 | 242.4 | 227.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.85 | 0.00 | 0.93 | -14.54 | 332.23 | 0.44 | 182.88 | 0.1490 | 885.0 | 640.5 | |
| 0.00 | 1.59 | 0.00 | 0.81 | -19.71 | 331.88 | 0.10 | 180.39 | 0.2377 | 814.0 | 635.5 | |
| 0.00 | 2.56 | 0.00 | 1.31 | -20.08 | 331.79 | 0.00 | 180.00 | 0.2440 | 624.0 | 506.9 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -17.83 | 331.73 | -0.06 | 179.72 | 0.2056 | 907.0 | 717.9 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -17.00 | 330.98 | -0.81 | 175.93 | 0.1919 | 769.0 | 545.6 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -14.71 | 330.24 | -1.54 | 170.22 | 0.1541 | 854.0 | 654.0 | |
| 0.00 | 0.79 | 0.00 | 0.40 | -17.61 | 329.18 | -2.61 | 167.81 | 0.2065 | 980.0 | 762.7 | |
| 0.00 | 3.53 | 0.00 | 1.79 | -17.28 | 327.10 | -4.68 | 158.27 | 0.2116 | 727.0 | 582.1 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -25.53 | 325.55 | -6.24 | 163.66 | 0.3501 | 5.0 | 0.6 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -21.78 | 320.10 | -11.69 | 145.49 | 0.3335 | -820.0 | -669.1 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -21.93 | 319.92 | -11.87 | 145.38 | 0.3372 | -728.0 | -675.6 | |
| 0.00 | 1.15 | 0.00 | 0.61 | -22.84 | 319.84 | -11.95 | 146.79 | 0.3499 | -26.0 | -8.3 | |
| 0.00 | 1.41 | 0.00 | 0.75 | -23.54 | 317.59 | -14.20 | 143.51 | 0.3798 | -806.0 | -595.4 | |
| 0.00 | 1.50 | 0.00 | 0.80 | -22.59 | 316.18 | -15.61 | 139.30 | 0.3826 | -792.0 | -623.2 | |
| 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. | |