| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 200 | 1122 | 116 | 643 | 18.46 | 32.41 | -26.80 | 58.04 | 0.5053 | 299.4 | 22.2 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-07-06 01:35:31 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 6 | 0 | 3 | 18.34 | 41.15 | -18.07 | 48.65 | 0.3938 | 747.0 | 690.2 | |
| 0 | 4 | 0 | 2 | 18.54 | 40.69 | -18.53 | 48.94 | 0.4014 | 871.0 | 724.9 | |
| 0 | 3 | 0 | 2 | 16.28 | 37.76 | -21.45 | 57.32 | 0.4189 | 574.0 | 522.8 | |
| 32 | 533 | 18 | 300 | 19.05 | 35.59 | -23.62 | 54.23 | 0.4688 | 1705.3 | 409.8 | |
| 6 | -4 | 4 | -4 | 18.68 | 35.60 | -23.61 | 54.90 | 0.4657 | 2067.9 | 999999 | |
| 0 | 5 | 0 | 3 | 20.61 | 34.97 | -24.24 | 52.10 | 0.4891 | 675.0 | 528.3 | |
| -4 | -4 | -4 | -4 | 18.83 | 35.21 | -24.00 | 55.01 | 0.4719 | 999999 | 999999 | |
| 32 | -4 | 18 | -4 | 18.05 | 35.06 | -24.16 | 56.63 | 0.4679 | 1617.5 | 999999 | |
| 11 | 81 | 6 | 46 | 19.80 | 34.23 | -24.99 | 54.26 | 0.4917 | 1436.9 | 617.0 | |
| 12 | -9 | 7 | -9 | 20.00 | 33.91 | -25.30 | 54.21 | 0.4971 | 1106.9 | 999999 | |
| 2 | -4 | 1 | -4 | 18.93 | 34.00 | -25.22 | 56.03 | 0.4879 | 934.6 | 999999 | |
| 0 | 5 | 0 | 3 | 20.72 | 32.84 | -26.37 | 53.99 | 0.5157 | 577.0 | 383.0 | |
| 0 | 3 | 0 | 2 | 16.98 | 33.06 | -26.16 | 60.45 | 0.4867 | -526.0 | -405.7 | |
| 6 | -4 | 3 | -4 | 19.63 | 32.34 | -26.88 | 56.30 | 0.5139 | -1104.9 | 999999 | |
| 0 | 5 | 0 | 3 | 18.88 | 32.14 | -27.08 | 57.77 | 0.5112 | -611.0 | -605.5 | |
| 0 | 12 | 0 | 7 | 17.45 | 32.38 | -26.84 | 60.13 | 0.4987 | -508.0 | -342.1 | |
| 7 | -4 | 4 | -4 | 19.86 | 31.77 | -27.44 | 56.38 | 0.5226 | 927.6 | 999999 | |
| 15 | 88 | 8 | 50 | 16.67 | 32.13 | -27.09 | 61.76 | 0.4971 | -1416.9 | -856.8 | |
| 4 | 14 | 3 | 8 | 20.63 | 31.15 | -28.07 | 55.62 | 0.5357 | 754.4 | 454.3 | |
| 0 | 3 | 0 | 2 | 19.97 | 31.18 | -28.04 | 56.69 | 0.5307 | 372.0 | 442.8 | |
| 0 | 5 | 0 | 3 | 21.04 | 30.92 | -28.30 | 55.14 | 0.5414 | -492.0 | -410.1 | |
| 7 | -18 | 4 | -18 | 16.52 | 31.36 | -27.86 | 62.60 | 0.5066 | -1242.1 | 999999 | |
| 5 | -18 | 3 | -18 | 16.84 | 31.03 | -28.19 | 62.27 | 0.5128 | -1243.4 | 999999 | |
| 0 | 5 | 0 | 3 | 21.06 | 30.14 | -29.08 | 55.74 | 0.5509 | 675.0 | 456.8 | |
| 0 | 6 | 0 | 4 | 19.94 | 30.13 | -29.09 | 57.58 | 0.5435 | -813.0 | -596.4 | |
| 0 | 5 | 0 | 3 | 21.01 | 29.61 | -29.60 | 56.24 | 0.5568 | 430.0 | 266.9 | |
| 0 | 6 | 0 | 3 | 16.41 | 30.25 | -28.97 | 63.58 | 0.5208 | -800.0 | -739.8 | |
| 15 | 38 | 9 | 22 | 17.25 | 29.68 | -29.54 | 62.48 | 0.5330 | -1235.3 | -717.6 | |
| 0 | 7 | 0 | 4 | 20.48 | 28.85 | -30.37 | 57.65 | 0.5628 | 732.0 | 580.6 | |
| 0 | 8 | 0 | 5 | 19.70 | 29.02 | -30.20 | 58.80 | 0.5558 | -636.0 | -632.1 | |
| 0 | 4 | 0 | 2 | 19.57 | 28.65 | -30.56 | 59.28 | 0.5595 | -672.0 | -540.8 | |
| 0 | 4 | 0 | 2 | 16.30 | 29.27 | -29.95 | 64.41 | 0.5333 | -714.0 | -646.7 | |
| 0 | 6 | 0 | 3 | 16.01 | 28.94 | -30.28 | 65.14 | 0.5362 | -619.0 | -600.8 | |
| 33 | 254 | 20 | 151 | 17.79 | 28.62 | -30.60 | 62.25 | 0.5498 | -1464.9 | -485.3 | |
| -34 | -34 | -34 | -34 | 18.16 | 28.50 | -30.72 | 61.71 | 0.5533 | 999999 | 999999 | |
| 0 | 5 | 0 | 3 | 16.61 | 28.69 | -30.53 | 64.23 | 0.5426 | -749.0 | -648.7 | |
| 13 | -34 | 8 | -34 | 18.34 | 27.83 | -31.39 | 61.83 | 0.5629 | 1109.4 | 999999 | |
| 0 | 3 | 0 | 2 | 16.66 | 27.52 | -31.69 | 64.85 | 0.5582 | -220.0 | -255.0 | |
| 0 | 4 | 0 | 2 | 17.22 | 27.37 | -31.85 | 63.98 | 0.5630 | -396.0 | -398.7 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |