SDO HMI 2014-09-30 06:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.76 | 43.91 | 10.57 | 27.97 | -11.68 | 160.47 | -34.16 | 118.37 | 0.6280 | -96.9 | 221.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.44 | 0.00 | 0.28 | -24.56 | 172.89 | -21.74 | 146.67 | 0.6153 | 532.0 | 471.8 | |
| 0.00 | 1.06 | 0.00 | 0.69 | -23.47 | 166.36 | -28.27 | 138.48 | 0.6576 | 547.0 | 464.6 | |
| 0.00 | 1.68 | 0.00 | 0.99 | -12.13 | 166.93 | -27.70 | 124.35 | 0.5526 | 842.0 | 664.7 | |
| 0.00 | 1.32 | 0.00 | 0.79 | -12.45 | 166.82 | -27.81 | 124.73 | 0.5565 | 798.0 | 597.3 | |
| 0.00 | 2.82 | 0.00 | 1.67 | -10.40 | 166.31 | -28.31 | 121.08 | 0.5469 | 718.0 | 541.4 | |
| 0.00 | 0.97 | 0.00 | 0.61 | -13.92 | 162.55 | -32.08 | 123.08 | 0.6174 | 468.0 | 416.4 | |
| 0.00 | 1.15 | 0.00 | 0.80 | -23.07 | 160.29 | -34.34 | 132.68 | 0.7083 | 777.0 | 623.7 | |
| 16.05 | 23.99 | 10.12 | 15.12 | -10.15 | 160.25 | -34.38 | 115.97 | 0.6205 | -861.3 | -271.3 | |
| 0.71 | 3.17 | 0.45 | 2.03 | -10.12 | 158.95 | -35.68 | 115.07 | 0.6362 | 844.8 | 738.5 | |
| 0.00 | 2.82 | 0.00 | 1.84 | -10.65 | 158.04 | -36.58 | 115.27 | 0.6500 | 766.0 | 634.7 | |
| 0.00 | 0.79 | 0.00 | 0.52 | -10.82 | 157.83 | -36.80 | 115.38 | 0.6535 | 260.0 | 223.6 | |
| 0.00 | 1.23 | 0.00 | 0.81 | -11.25 | 157.53 | -37.10 | 115.79 | 0.6593 | 606.0 | 461.0 | |
| 0.00 | 0.88 | 0.00 | 0.65 | -16.16 | 152.29 | -42.34 | 119.09 | 0.7427 | -609.0 | -573.1 | |
| 0.00 | 1.59 | 0.00 | 1.17 | -15.92 | 152.05 | -42.58 | 118.67 | 0.7438 | -498.0 | -415.2 | |
| 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. | |