SDO HMI 2014-03-09 13:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.92 | 164.08 | 50.95 | 147.13 | -18.39 | 323.06 | -56.99 | 107.32 | 0.8349 | -78.3 | -175.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.18 | 20.10 | 7.50 | 16.40 | -17.76 | 327.04 | -53.01 | 106.86 | 0.7971 | 730.4 | 414.8 | |
| 2.34 | 3.64 | 1.94 | 3.02 | -17.68 | 326.28 | -53.77 | 106.70 | 0.8046 | 635.3 | 530.7 | |
| 0.00 | 4.50 | 0.00 | 3.77 | -17.86 | 325.94 | -54.11 | 106.89 | 0.8081 | 162.0 | 168.6 | |
| 0.00 | 0.61 | 0.00 | 0.51 | -18.39 | 325.64 | -54.41 | 107.51 | 0.8114 | 404.0 | 298.0 | |
| 0.00 | 1.47 | 0.00 | 1.23 | -17.44 | 326.02 | -54.03 | 106.37 | 0.8070 | 585.0 | 538.4 | |
| 0.00 | 1.21 | 0.00 | 1.03 | -18.61 | 325.37 | -54.68 | 107.76 | 0.8142 | 462.0 | 393.8 | |
| 0.00 | 1.13 | 0.00 | 0.95 | -17.69 | 325.47 | -54.58 | 106.64 | 0.8125 | -240.0 | -222.8 | |
| 4.76 | 6.93 | 4.03 | 5.85 | -17.45 | 325.48 | -54.57 | 106.34 | 0.8123 | 582.2 | 385.9 | |
| 0.00 | 1.39 | 0.00 | 1.19 | -18.57 | 324.95 | -55.10 | 107.67 | 0.8181 | -213.0 | -126.3 | |
| 0.00 | 0.87 | 0.00 | 0.75 | -19.12 | 324.57 | -55.48 | 108.31 | 0.8222 | 300.0 | 258.2 | |
| 1.47 | 6.58 | 1.27 | 5.67 | -17.71 | 324.70 | -55.35 | 106.60 | 0.8199 | 355.8 | -170.9 | |
| 0.00 | 2.51 | 0.00 | 2.18 | -17.83 | 324.42 | -55.63 | 106.73 | 0.8227 | -140.0 | -85.0 | |
| 0.00 | 1.04 | 0.00 | 0.91 | -18.77 | 323.90 | -56.15 | 107.83 | 0.8282 | -335.0 | -375.8 | |
| 0.00 | 1.91 | 0.00 | 1.66 | -17.99 | 324.17 | -55.88 | 106.91 | 0.8251 | -218.0 | -185.8 | |
| 1.21 | 2.77 | 1.08 | 2.46 | -19.14 | 323.54 | -56.51 | 108.24 | 0.8318 | -667.1 | -567.4 | |
| 3.21 | 5.98 | 2.88 | 5.36 | -19.27 | 323.06 | -56.99 | 108.36 | 0.8362 | -599.8 | -453.0 | |
| 5.98 | 42.27 | 5.30 | 37.76 | -18.26 | 323.47 | -56.58 | 107.18 | 0.8318 | -726.0 | -261.7 | |
| 1.65 | -17.00 | 1.47 | -17.00 | -18.73 | 323.18 | -56.87 | 107.72 | 0.8348 | -648.4 | 999999 | |
| 1.39 | -17.00 | 1.22 | -17.00 | -17.90 | 323.60 | -56.46 | 106.76 | 0.8304 | 228.3 | 999999 | |
| 0.00 | 1.39 | 0.00 | 1.27 | -20.05 | 322.44 | -57.61 | 109.24 | 0.8423 | -490.0 | -307.2 | |
| 2.51 | 4.07 | 2.28 | 3.69 | -19.45 | 322.67 | -57.38 | 108.54 | 0.8399 | -430.2 | -306.3 | |
| 7.02 | -17.00 | 6.28 | -17.00 | -18.19 | 323.11 | -56.94 | 107.07 | 0.8351 | 136.4 | 999999 | |
| 0.00 | 0.69 | 0.00 | 0.64 | -20.01 | 322.05 | -58.00 | 109.16 | 0.8457 | -260.0 | -224.4 | |
| 0.00 | 1.65 | 0.00 | 1.47 | -17.86 | 323.16 | -56.89 | 106.68 | 0.8344 | 532.0 | 441.0 | |
| 0.00 | 1.30 | 0.00 | 1.17 | -17.84 | 322.70 | -57.35 | 106.63 | 0.8386 | 238.0 | 229.0 | |
| 0.00 | 1.21 | 0.00 | 1.11 | -18.21 | 322.10 | -57.95 | 107.03 | 0.8442 | 284.0 | 164.8 | |
| 0.87 | 35.60 | 0.82 | 34.20 | -18.80 | 320.86 | -59.19 | 107.65 | 0.8553 | -748.7 | -516.8 | |
| 1.65 | -27.00 | 1.56 | -27.00 | -18.57 | 320.81 | -59.24 | 107.38 | 0.8556 | -726.4 | 999999 | |
| 0.00 | 1.91 | 0.00 | 1.80 | -18.04 | 321.04 | -59.01 | 106.77 | 0.8534 | -325.0 | -325.6 | |
| 0.00 | 0.95 | 0.00 | 0.90 | -18.30 | 320.90 | -59.15 | 107.07 | 0.8548 | -335.0 | -305.7 | |
| 0.43 | 9.62 | 0.42 | 9.45 | -19.37 | 320.15 | -59.91 | 108.28 | 0.8616 | -479.4 | -315.4 | |
| 0.00 | 0.78 | 0.00 | 0.73 | -17.15 | 321.39 | -58.66 | 105.74 | 0.8500 | 307.0 | 337.4 | |
| 9.44 | -27.00 | 9.14 | -27.00 | -18.81 | 320.17 | -59.88 | 107.63 | 0.8612 | -543.8 | 999999 | |
| 1.04 | -31.00 | 1.02 | -31.00 | -19.34 | 319.85 | -60.20 | 108.22 | 0.8641 | -535.5 | 999999 | |
| 2.77 | -31.00 | 2.74 | -31.00 | -19.27 | 319.44 | -60.61 | 108.11 | 0.8674 | -243.6 | 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. | |