SDO HMI 2014-11-30 12:00:25 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 86.77 | 400.73 | 74.68 | 346.29 | 3.62 | 161.80 | 54.85 | 273.80 | 0.8191 | -277.2 | -86.7 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-30 12:00:25 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 | 1.03 | 0.00 | 0.96 | 3.35 | 164.97 | 58.03 | 273.34 | 0.8504 | 399.0 | 323.6 | |
| 0.00 | 0.77 | 0.00 | 0.71 | 5.19 | 164.52 | 57.58 | 275.54 | 0.8467 | 591.0 | 523.0 | |
| 24.70 | 284.81 | 22.34 | 255.87 | 2.56 | 163.74 | 56.80 | 272.43 | 0.8388 | -806.2 | -199.4 | |
| 27.87 | -3.00 | 24.92 | -3.00 | 3.40 | 163.32 | 56.38 | 273.44 | 0.8349 | -874.0 | 999999 | |
| 0.60 | 2.74 | 0.52 | 2.40 | 4.21 | 162.50 | 55.55 | 274.44 | 0.8271 | -519.7 | -414.1 | |
| 5.39 | -3.00 | 4.70 | -3.00 | 3.71 | 162.39 | 55.45 | 273.84 | 0.8259 | -870.1 | 999999 | |
| 2.39 | -3.00 | 2.08 | -3.00 | 4.07 | 162.06 | 55.12 | 274.29 | 0.8228 | -687.7 | 999999 | |
| 1.62 | 3.76 | 1.38 | 3.20 | 4.20 | 161.30 | 54.36 | 274.47 | 0.8152 | -720.9 | -609.4 | |
| 0.00 | 1.62 | 0.00 | 1.36 | 0.71 | 160.78 | 53.84 | 270.17 | 0.8095 | -114.0 | -217.8 | |
| 0.00 | 0.94 | 0.00 | 0.79 | 4.12 | 160.93 | 53.99 | 274.38 | 0.8114 | -530.0 | -512.8 | |
| 0.00 | 1.03 | 0.00 | 0.85 | 3.27 | 160.20 | 53.26 | 273.35 | 0.8037 | 444.0 | 302.5 | |
| 0.00 | 2.48 | 0.00 | 2.04 | 4.16 | 159.94 | 52.99 | 274.48 | 0.8012 | -4.0 | 55.6 | |
| 6.33 | 8.63 | 5.15 | 7.03 | 4.49 | 159.43 | 52.48 | 274.92 | 0.7960 | 589.7 | 268.9 | |
| 0.00 | 0.43 | 0.00 | 0.34 | 3.67 | 158.67 | 51.73 | 273.91 | 0.7876 | 190.0 | 244.8 | |
| 0.00 | 1.54 | 0.00 | 1.23 | 5.13 | 158.72 | 51.78 | 275.76 | 0.7887 | 222.0 | 155.7 | |
| 1.71 | 7.86 | 1.36 | 6.27 | 5.16 | 158.44 | 51.49 | 275.82 | 0.7857 | -586.9 | -42.9 | |
| 0.00 | 1.71 | 0.00 | 1.36 | 4.36 | 158.25 | 51.31 | 274.81 | 0.7833 | 396.0 | 320.7 | |
| 0.00 | 1.20 | 0.00 | 0.94 | 2.94 | 158.09 | 51.15 | 273.00 | 0.7811 | 509.0 | 424.6 | |
| 0.00 | 2.14 | 0.00 | 1.69 | 3.21 | 158.06 | 51.12 | 273.34 | 0.7808 | 579.0 | 404.6 | |
| 0.00 | 0.94 | 0.00 | 0.74 | 4.57 | 158.18 | 51.24 | 275.08 | 0.7826 | 582.0 | 444.3 | |
| 0.00 | 0.77 | 0.00 | 0.61 | 4.01 | 158.03 | 51.09 | 274.37 | 0.7808 | 514.0 | 465.2 | |
| 0.00 | 0.68 | 0.00 | 0.53 | 3.72 | 157.44 | 50.50 | 274.02 | 0.7742 | 635.0 | 460.0 | |
| 0.00 | 0.68 | 0.00 | 0.53 | 5.54 | 156.74 | 49.79 | 276.43 | 0.7673 | 179.0 | 141.4 | |
| 0.00 | 1.88 | 0.00 | 1.43 | 3.65 | 156.28 | 49.33 | 273.98 | 0.7611 | 753.0 | 621.7 | |
| 0.00 | 1.03 | 0.00 | 0.78 | 4.01 | 156.08 | 49.13 | 274.46 | 0.7590 | 544.0 | 526.8 | |
| 7.27 | 63.59 | 5.52 | 48.28 | 5.58 | 156.14 | 49.20 | 276.53 | 0.7607 | 704.8 | 297.3 | |
| 0.00 | 0.85 | 0.00 | 0.65 | 4.84 | 156.06 | 49.12 | 275.55 | 0.7593 | 662.0 | 547.7 | |
| 2.39 | -26.00 | 1.82 | -26.00 | 6.02 | 156.06 | 49.12 | 277.12 | 0.7600 | 610.9 | 999999 | |
| 0.00 | 1.80 | 0.00 | 1.35 | 4.63 | 155.86 | 48.92 | 275.30 | 0.7569 | 727.0 | 573.7 | |
| 0.00 | 1.11 | 0.00 | 0.84 | 6.62 | 156.05 | 49.10 | 277.91 | 0.7604 | 277.0 | 223.6 | |
| 4.96 | -26.00 | 3.74 | -26.00 | 6.00 | 155.74 | 48.79 | 277.12 | 0.7564 | 961.0 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.77 | 4.52 | 155.44 | 48.50 | 275.17 | 0.7520 | 692.0 | 545.6 | |
| 1.54 | 3.68 | 1.15 | 2.74 | 3.93 | 155.21 | 48.27 | 274.40 | 0.7491 | 843.3 | 694.4 | |
| 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. | |