SDO HMI 2014-07-17 02:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.62 | 0.00 | 11.44 | -20.36 | 146.92 | 39.05 | 233.84 | 0.7318 | -84.5 | 62.4 | |
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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 | 1.09 | 0.00 | 0.92 | -20.42 | 156.69 | 48.81 | 240.66 | 0.8112 | 261.0 | 209.2 | |
| 0.00 | 1.27 | 0.00 | 1.08 | -21.23 | 156.74 | 48.87 | 239.76 | 0.8148 | 374.0 | 336.9 | |
| 0.00 | 1.54 | 0.00 | 1.11 | -9.16 | 152.41 | 44.54 | 252.81 | 0.7271 | 489.0 | 488.4 | |
| 0.00 | 1.00 | 0.00 | 0.72 | -9.63 | 152.35 | 44.48 | 252.17 | 0.7279 | 602.0 | 557.8 | |
| 0.00 | 1.45 | 0.00 | 1.13 | -18.66 | 153.34 | 45.46 | 241.20 | 0.7729 | 253.0 | 344.0 | |
| 0.00 | 1.27 | 0.00 | 1.03 | -21.77 | 154.05 | 46.18 | 237.90 | 0.7932 | 550.0 | 414.1 | |
| 0.00 | 1.36 | 0.00 | 1.00 | -21.35 | 148.63 | 40.76 | 235.46 | 0.7405 | 635.0 | 536.7 | |
| 0.00 | 0.91 | 0.00 | 0.61 | -17.75 | 144.57 | 36.70 | 237.39 | 0.6779 | -475.0 | -417.3 | |
| 0.00 | 0.91 | 0.00 | 0.66 | -24.57 | 146.31 | 38.44 | 230.23 | 0.7379 | -571.0 | -428.9 | |
| 0.00 | 0.82 | 0.00 | 0.59 | -24.18 | 145.41 | 37.54 | 230.07 | 0.7271 | -463.0 | -449.8 | |
| 0.00 | 0.45 | 0.00 | 0.33 | -24.54 | 145.11 | 37.24 | 229.44 | 0.7268 | -351.0 | -399.6 | |
| 0.00 | 0.73 | 0.00 | 0.51 | -24.60 | 143.55 | 35.67 | 228.25 | 0.7129 | -536.0 | -453.9 | |
| 0.00 | 0.82 | 0.00 | 0.57 | -27.09 | 140.38 | 32.51 | 223.01 | 0.7038 | -782.0 | -652.2 | |
| 0.00 | 0.82 | 0.00 | 0.48 | -23.98 | 124.28 | 16.41 | 208.56 | 0.5419 | -624.0 | -474.3 | |
| 0.00 | 1.18 | 0.00 | 0.70 | -29.07 | 109.40 | 1.53 | 182.42 | 0.5557 | -630.0 | -529.8 | |
| 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. | |