SDO HMI 2014-07-08 08:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.36 | 21.18 | 0.21 | 12.61 | -21.90 | 201.62 | -22.06 | 141.12 | 0.5545 | 179.8 | 211.9 | |
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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 |
| 0.36 | 4.27 | 0.21 | 2.45 | -21.06 | 205.65 | -18.04 | 145.16 | 0.5078 | 906.2 | 783.0 | |
| 0.00 | 0.91 | 0.00 | 0.52 | -20.66 | 205.49 | -18.19 | 144.44 | 0.5044 | 719.0 | 571.5 | |
| 0.00 | 0.91 | 0.00 | 0.52 | -21.17 | 205.29 | -18.40 | 144.77 | 0.5121 | 482.0 | 444.5 | |
| 0.00 | 1.36 | 0.00 | 0.80 | -22.87 | 204.74 | -18.94 | 145.99 | 0.5369 | -810.0 | -746.5 | |
| 0.00 | 1.91 | 0.00 | 1.12 | -21.81 | 203.53 | -20.15 | 143.12 | 0.5350 | 809.0 | 678.4 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -21.65 | 203.52 | -20.16 | 142.90 | 0.5332 | 815.0 | 667.3 | |
| 0.00 | 2.18 | 0.00 | 1.28 | -21.69 | 202.99 | -20.70 | 142.25 | 0.5385 | 631.0 | 506.0 | |
| 0.00 | 0.91 | 0.00 | 0.54 | -22.31 | 202.68 | -21.00 | 142.60 | 0.5480 | 554.0 | 493.8 | |
| 0.00 | 0.91 | 0.00 | 0.58 | -28.59 | 199.86 | -23.82 | 146.14 | 0.6388 | -410.0 | -400.5 | |
| 0.00 | 2.09 | 0.00 | 1.27 | -22.82 | 199.84 | -23.84 | 139.78 | 0.5792 | 587.0 | 427.3 | |
| 0.00 | 1.00 | 0.00 | 0.62 | -20.88 | 195.62 | -28.07 | 132.87 | 0.6021 | -718.0 | -549.7 | |
| 0.00 | 2.82 | 0.00 | 1.76 | -20.93 | 195.01 | -28.68 | 132.36 | 0.6087 | -618.0 | -533.8 | |
| 0.00 | 0.64 | 0.00 | 0.41 | -21.73 | 193.06 | -30.63 | 131.61 | 0.6352 | -763.0 | -643.1 | |
| 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. | |