| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.78 | 197.94 | 21.57 | 117.16 | -10.14 | 359.25 | -33.43 | 97.47 | 0.5489 | 554.5 | 370.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-08 14:00:28 UT
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 | 1.30 | 0.00 | 0.74 | -14.19 | 2.63 | -30.05 | 105.83 | 0.5066 | 789.0 | 571.0 | |
| 0.00 | 2.77 | 0.00 | 1.59 | -14.24 | 2.41 | -30.27 | 105.84 | 0.5099 | 756.0 | 671.8 | |
| 0.69 | 2.86 | 0.40 | 1.64 | -13.91 | 2.35 | -30.32 | 105.17 | 0.5098 | 971.1 | 822.0 | |
| 0.52 | 1.73 | 0.30 | 1.00 | -14.07 | 1.58 | -31.10 | 105.24 | 0.5214 | 890.0 | 740.5 | |
| 0.00 | 1.39 | 0.00 | 0.81 | -14.11 | 0.89 | -31.79 | 105.13 | 0.5313 | 609.0 | 498.4 | |
| 0.00 | 1.30 | 0.00 | 0.75 | -5.41 | 1.36 | -31.32 | 88.50 | 0.5197 | 846.0 | 771.8 | |
| 0.00 | 1.30 | 0.00 | 0.76 | -5.67 | 0.85 | -31.82 | 89.08 | 0.5269 | 788.0 | 671.6 | |
| 0.00 | 1.04 | 0.00 | 0.61 | -5.04 | 0.75 | -31.93 | 87.90 | 0.5293 | 816.0 | 698.0 | |
| 15.32 | 150.38 | 8.96 | 88.10 | -9.51 | 0.24 | -32.44 | 96.38 | 0.5344 | 1096.1 | 431.1 | |
| 18.18 | -9.00 | 10.67 | -9.00 | -10.06 | 359.96 | -32.71 | 97.39 | 0.5387 | 1063.6 | 999999 | |
| 0.43 | -9.00 | 0.25 | -9.00 | -9.80 | 359.63 | -33.04 | 96.88 | 0.5434 | 507.8 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.52 | -15.59 | 358.65 | -34.03 | 107.13 | 0.5662 | 610.0 | 513.2 | |
| 0.00 | 0.69 | 0.00 | 0.41 | -8.23 | 359.47 | -33.20 | 93.99 | 0.5454 | 688.0 | 521.2 | |
| 0.00 | 0.78 | 0.00 | 0.46 | -7.64 | 359.46 | -33.22 | 92.89 | 0.5458 | 579.0 | 541.6 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -8.37 | 359.35 | -33.32 | 94.25 | 0.5472 | 614.0 | 509.1 | |
| 0.00 | 1.13 | 0.00 | 0.67 | -9.66 | 358.08 | -34.59 | 96.55 | 0.5656 | 875.0 | 722.2 | |
| 0.00 | 2.16 | 0.00 | 1.30 | -10.02 | 357.71 | -34.97 | 97.17 | 0.5710 | 781.0 | 644.1 | |
| 0.00 | 1.30 | 0.00 | 0.78 | -9.75 | 357.74 | -34.94 | 96.71 | 0.5705 | 802.0 | 631.9 | |
| 1.64 | 4.59 | 0.99 | 2.76 | -9.30 | 357.65 | -35.03 | 95.90 | 0.5717 | 692.1 | 647.5 | |
| 0.00 | 0.87 | 0.00 | 0.52 | -9.51 | 357.62 | -35.05 | 96.27 | 0.5721 | 504.0 | 429.7 | |
| 0.00 | 1.39 | 0.00 | 0.85 | -14.10 | 356.86 | -35.82 | 104.11 | 0.5875 | 567.0 | 429.4 | |
| 0.00 | 0.69 | 0.00 | 0.42 | -9.85 | 357.47 | -35.21 | 96.87 | 0.5743 | 521.0 | 381.4 | |
| 0.00 | 2.51 | 0.00 | 1.52 | -10.96 | 357.06 | -35.61 | 98.77 | 0.5807 | 638.0 | 638.6 | |
| 0.00 | 1.73 | 0.00 | 1.05 | -10.14 | 356.91 | -35.76 | 97.34 | 0.5823 | -219.0 | -211.7 | |
| 0.00 | 1.13 | 0.00 | 0.69 | -13.65 | 356.37 | -36.31 | 103.25 | 0.5934 | 549.0 | 456.9 | |
| 0.00 | 0.87 | 0.00 | 0.54 | -15.58 | 355.60 | -37.07 | 106.29 | 0.6072 | -674.0 | -575.5 | |
| 0.00 | 0.87 | 0.00 | 0.56 | -16.19 | 352.52 | -40.15 | 106.57 | 0.6484 | -631.0 | -528.1 | |
| 0.00 | 0.26 | 0.00 | 0.17 | -14.77 | 351.81 | -40.87 | 104.26 | 0.6552 | -438.0 | -376.3 | |
| 0.00 | 0.78 | 0.00 | 0.50 | -7.95 | 352.55 | -40.13 | 93.75 | 0.6420 | -526.0 | -458.3 | |
| 0.00 | 0.95 | 0.00 | 0.62 | -7.54 | 352.32 | -40.35 | 93.13 | 0.6452 | -805.0 | -763.0 | |
| 0.00 | 2.16 | 0.00 | 1.44 | -13.00 | 350.43 | -42.25 | 101.41 | 0.6707 | -752.0 | -638.2 | |
| 0.00 | 1.13 | 0.00 | 0.74 | -4.34 | 351.58 | -41.09 | 88.30 | 0.6580 | -626.0 | -507.2 | |
| 0.00 | 2.25 | 0.00 | 1.50 | -12.91 | 350.16 | -42.52 | 101.27 | 0.6740 | -617.0 | -574.9 | |
| 0.00 | 0.87 | 0.00 | 0.57 | -10.87 | 350.51 | -42.16 | 98.23 | 0.6684 | -631.0 | -484.9 | |
| 0.00 | 1.73 | 0.00 | 1.17 | -12.35 | 349.61 | -43.07 | 100.40 | 0.6805 | -500.0 | -410.0 | |
| 0.00 | 1.21 | 0.00 | 0.84 | -11.53 | 348.13 | -44.55 | 99.13 | 0.6985 | -661.0 | -545.9 | |
| 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. | |