SDO HMI 2014-07-14 00:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.00 | 358.81 | 116.85 | 648.65 | -7.76 | 222.02 | 73.35 | 260.70 | 0.9629 | 489.9 | 201.4 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.81 | 0.00 | 4.80 | -4.66 | 221.34 | 72.67 | 263.83 | 0.9582 | -50.0 | -0.3 | |
| 60.64 | 326.96 | 111.64 | 599.45 | -7.79 | 222.26 | 73.59 | 260.70 | 0.9642 | 550.5 | 207.2 | |
| 0.00 | 2.90 | 0.00 | 4.74 | -7.21 | 220.24 | 71.57 | 261.05 | 0.9541 | 398.0 | 362.3 | |
| 2.27 | 5.81 | 3.58 | 9.15 | -6.18 | 219.69 | 71.01 | 262.06 | 0.9506 | -382.2 | -326.2 | |
| 0.00 | 1.54 | 0.00 | 2.36 | -7.40 | 218.97 | 70.30 | 260.70 | 0.9475 | 429.0 | 423.9 | |
| 1.09 | 10.53 | 1.63 | 15.92 | -6.93 | 218.54 | 69.86 | 261.13 | 0.9447 | 464.4 | 319.5 | |
| 0.00 | 5.72 | 0.00 | 8.88 | -9.85 | 218.90 | 70.23 | 258.12 | 0.9489 | 199.0 | 122.0 | |
| 0.00 | 1.09 | 0.00 | 1.60 | -8.88 | 217.92 | 69.25 | 259.00 | 0.9427 | -320.0 | -294.1 | |
| 0.00 | 0.27 | 0.00 | 0.35 | -12.22 | 214.20 | 65.53 | 254.85 | 0.9232 | 261.0 | 264.0 | |
| 0.00 | 0.27 | 0.00 | 0.34 | -12.36 | 213.44 | 64.77 | 254.56 | 0.9184 | 148.0 | 185.3 | |
| 0.00 | 0.27 | 0.00 | 0.32 | -11.64 | 212.11 | 63.44 | 255.09 | 0.9084 | -101.0 | -137.3 | |
| 0.00 | 0.64 | 0.00 | 0.74 | -12.84 | 211.65 | 62.98 | 253.69 | 0.9067 | -150.0 | -202.9 | |
| 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. | |