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 |
| 2.65 | 32.20 | 1.34 | 16.39 | 7.74 | 207.91 | 13.28 | 275.35 | 0.2298 | -0.4 | 126.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.32 | 0.00 | 0.68 | 6.68 | 211.49 | 16.87 | 270.72 | 0.2895 | -715.0 | -492.5 | |
| 0.00 | 1.23 | 0.00 | 0.64 | 7.55 | 210.64 | 16.02 | 273.83 | 0.2753 | -838.0 | -644.3 | |
| 0.00 | 2.38 | 0.00 | 1.22 | 7.71 | 210.33 | 15.71 | 274.46 | 0.2703 | -1000.0 | -784.3 | |
| 0.00 | 1.50 | 0.00 | 0.77 | 7.41 | 210.26 | 15.63 | 273.36 | 0.2689 | -952.0 | -808.5 | |
| 0.00 | 1.50 | 0.00 | 0.77 | 7.25 | 209.66 | 15.03 | 272.79 | 0.2587 | -979.0 | -768.7 | |
| 0.00 | 1.68 | 0.00 | 0.86 | 6.68 | 208.86 | 14.23 | 270.49 | 0.2452 | -484.0 | -342.0 | |
| 0.00 | 1.94 | 0.00 | 0.99 | 6.60 | 208.42 | 13.79 | 270.13 | 0.2379 | -1119.0 | -878.8 | |
| 0.00 | 1.68 | 0.00 | 0.85 | 6.70 | 208.08 | 13.45 | 270.52 | 0.2321 | -900.0 | -741.9 | |
| 1.94 | 7.94 | 0.98 | 4.03 | 8.17 | 207.04 | 12.41 | 277.31 | 0.2154 | 1077.2 | 884.7 | |
| 0.71 | 2.91 | 0.36 | 1.47 | 8.66 | 206.68 | 12.05 | 279.80 | 0.2104 | 1002.8 | 788.4 | |
| 0.00 | 2.56 | 0.00 | 1.30 | 7.79 | 206.65 | 12.02 | 275.66 | 0.2084 | 985.0 | 732.4 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 7.31 | 206.48 | 11.86 | 273.40 | 0.2051 | 906.0 | 680.1 | |
| 0.00 | 1.85 | 0.00 | 0.94 | 8.34 | 206.39 | 11.76 | 278.43 | 0.2048 | 1123.0 | 973.6 | |
| 0.00 | 1.59 | 0.00 | 0.80 | 8.68 | 205.97 | 11.34 | 280.40 | 0.1985 | 830.0 | 640.7 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 8.20 | 205.83 | 11.20 | 278.08 | 0.1951 | 718.0 | 576.0 | |
| 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. | |