SDO HMI 2014-10-01 09:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.03 | 114.12 | 14.70 | 76.84 | -10.05 | 140.54 | -39.25 | 112.81 | 0.6781 | 367.4 | 197.5 | |
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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 | 0.62 | 0.00 | 0.44 | -16.64 | 139.96 | -39.83 | 121.11 | 0.7191 | 551.0 | 485.9 | |
| 22.03 | 102.93 | 14.70 | 68.74 | -9.64 | 140.92 | -38.87 | 112.47 | 0.6719 | 973.2 | 288.2 | |
| 0.00 | 0.70 | 0.00 | 0.48 | -12.31 | 140.09 | -39.70 | 115.64 | 0.6945 | 96.0 | 115.4 | |
| 0.00 | 2.03 | 0.00 | 1.46 | -14.71 | 138.24 | -41.55 | 117.70 | 0.7268 | -761.0 | -669.7 | |
| 0.00 | 1.32 | 0.00 | 0.94 | -13.50 | 138.27 | -41.52 | 116.17 | 0.7206 | -667.0 | -609.3 | |
| 0.00 | 0.44 | 0.00 | 0.32 | -13.22 | 137.79 | -42.00 | 115.56 | 0.7244 | -543.0 | -475.0 | |
| 0.00 | 0.70 | 0.00 | 0.52 | -14.61 | 137.13 | -42.66 | 116.97 | 0.7380 | -492.0 | -429.0 | |
| 0.00 | 0.44 | 0.00 | 0.32 | -14.25 | 136.88 | -42.91 | 116.38 | 0.7389 | -326.0 | -298.4 | |
| 0.00 | 1.41 | 0.00 | 1.02 | -12.83 | 136.78 | -43.01 | 114.54 | 0.7335 | -644.0 | -516.9 | |
| 0.00 | 0.88 | 0.00 | 0.64 | -12.67 | 136.82 | -42.97 | 114.35 | 0.7324 | -656.0 | -560.5 | |
| 0.00 | 1.15 | 0.00 | 0.84 | -12.56 | 136.12 | -43.67 | 113.88 | 0.7394 | -362.0 | -375.2 | |
| 0.00 | 0.88 | 0.00 | 0.65 | -12.16 | 135.69 | -44.10 | 113.17 | 0.7423 | -417.0 | -370.4 | |
| 0.00 | 0.62 | 0.00 | 0.47 | -12.44 | 133.53 | -46.26 | 112.53 | 0.7662 | -274.0 | -230.0 | |
| 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. | |