SDO HMI 2014-09-30 01:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 134.43 | 698.83 | 145.93 | 759.40 | 15.14 | 260.93 | 63.56 | 283.63 | 0.8899 | -47.0 | -81.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 9.43 | 0.00 | 12.77 | 12.63 | 266.83 | 69.46 | 280.95 | 0.9323 | 161.0 | 89.7 | |
| 0.97 | 128.45 | 1.29 | 163.66 | 12.96 | 266.41 | 69.04 | 281.28 | 0.9296 | -235.8 | -219.5 | |
| 15.34 | -2.00 | 19.78 | -2.00 | 13.44 | 265.68 | 68.30 | 281.77 | 0.9248 | -392.6 | 999999 | |
| 0.00 | 1.85 | 0.00 | 2.27 | 12.40 | 264.43 | 67.06 | 280.60 | 0.9167 | -425.0 | -335.2 | |
| 2.29 | -2.00 | 2.87 | -2.00 | 13.61 | 264.95 | 67.57 | 281.93 | 0.9199 | -618.2 | 999999 | |
| 4.32 | -2.00 | 5.42 | -2.00 | 13.94 | 265.06 | 67.69 | 282.29 | 0.9207 | -503.6 | 999999 | |
| 4.14 | -2.00 | 5.12 | -2.00 | 14.02 | 264.62 | 67.25 | 282.37 | 0.9177 | -741.1 | 999999 | |
| 0.00 | 0.97 | 0.00 | 1.13 | 13.84 | 263.10 | 65.73 | 282.14 | 0.9072 | -478.0 | -466.7 | |
| 0.00 | 2.20 | 0.00 | 2.54 | 13.66 | 262.78 | 65.41 | 281.93 | 0.9049 | -507.0 | -397.6 | |
| 0.00 | 0.79 | 0.00 | 0.90 | 13.62 | 262.31 | 64.94 | 281.88 | 0.9015 | -441.0 | -409.0 | |
| 0.00 | 0.97 | 0.00 | 1.09 | 14.38 | 262.13 | 64.76 | 282.72 | 0.9001 | -355.0 | -319.8 | |
| 19.92 | 225.95 | 22.62 | 251.41 | 15.16 | 262.28 | 64.91 | 283.60 | 0.9011 | -587.7 | -386.6 | |
| 0.00 | 0.79 | 0.00 | 0.86 | 13.30 | 260.93 | 63.56 | 281.50 | 0.8911 | 214.0 | 174.1 | |
| 9.43 | -12.00 | 10.36 | -12.00 | 15.13 | 261.39 | 64.02 | 283.56 | 0.8945 | -1007.4 | 999999 | |
| 8.02 | -12.00 | 8.91 | -12.00 | 15.81 | 261.71 | 64.34 | 284.32 | 0.8969 | -632.7 | 999999 | |
| 8.64 | -12.00 | 9.32 | -12.00 | 14.88 | 260.82 | 63.45 | 283.28 | 0.8902 | 149.5 | 999999 | |
| 0.00 | 1.06 | 0.00 | 1.16 | 16.88 | 261.35 | 63.98 | 285.51 | 0.8943 | -594.0 | -548.9 | |
| 0.00 | 0.53 | 0.00 | 0.55 | 13.46 | 259.37 | 62.00 | 281.66 | 0.8787 | 433.0 | 410.5 | |
| 0.00 | 2.47 | 0.00 | 2.51 | 13.47 | 258.98 | 61.61 | 281.67 | 0.8755 | 315.0 | 297.2 | |
| 0.53 | 3.35 | 0.54 | 3.42 | 13.90 | 259.04 | 61.67 | 282.16 | 0.8760 | 570.7 | 473.2 | |
| 0.00 | 5.20 | 0.00 | 5.31 | 14.42 | 259.09 | 61.72 | 282.75 | 0.8764 | 617.0 | 441.9 | |
| 4.50 | 12.78 | 4.57 | 13.01 | 15.02 | 258.92 | 61.55 | 283.44 | 0.8751 | 363.9 | 177.0 | |
| 0.00 | 1.85 | 0.00 | 1.87 | 14.64 | 258.74 | 61.36 | 283.01 | 0.8735 | 507.0 | 417.6 | |
| 0.00 | 0.62 | 0.00 | 0.64 | 17.12 | 259.67 | 62.30 | 285.82 | 0.8814 | -265.0 | -292.7 | |
| 0.00 | 1.59 | 0.00 | 1.66 | 17.32 | 259.79 | 62.42 | 286.05 | 0.8824 | -314.0 | -238.1 | |
| 0.53 | 2.56 | 0.55 | 2.65 | 17.35 | 259.53 | 62.16 | 286.09 | 0.8804 | 98.8 | 120.7 | |
| 2.82 | 273.56 | 2.83 | 268.49 | 15.50 | 258.45 | 61.08 | 284.00 | 0.8712 | 268.2 | 198.1 | |
| 3.17 | 21.51 | 3.13 | 21.16 | 14.62 | 257.95 | 60.58 | 283.00 | 0.8670 | 751.2 | 446.0 | |
| 6.26 | -27.00 | 6.19 | -27.00 | 15.45 | 258.03 | 60.66 | 283.95 | 0.8678 | 702.8 | 999999 | |
| 5.03 | -27.00 | 4.97 | -27.00 | 15.76 | 258.00 | 60.63 | 284.31 | 0.8676 | 575.7 | 999999 | |
| 32.88 | -27.00 | 32.01 | -27.00 | 16.35 | 257.41 | 60.04 | 285.01 | 0.8627 | 693.0 | 999999 | |
| 0.00 | 0.35 | 0.00 | 0.34 | 15.60 | 256.91 | 59.54 | 284.15 | 0.8582 | 523.0 | 537.0 | |
| 0.97 | -27.00 | 0.94 | -27.00 | 17.20 | 257.35 | 59.98 | 286.00 | 0.8625 | 438.1 | 999999 | |
| 2.64 | -27.00 | 2.58 | -27.00 | 17.59 | 257.50 | 60.13 | 286.44 | 0.8639 | 415.9 | 999999 | |
| 2.03 | -27.00 | 1.93 | -27.00 | 17.08 | 256.60 | 59.23 | 285.90 | 0.8560 | 709.3 | 999999 | |
| 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. | |