SOT: HOP 101(polar helioseismology)
2009-03-07T16:09:45 to 2009-03-08T08:08:55
Science Goal: Helioseismology Observations of the Sun's polar regions with SOT
Program: Ca 2x2, 5576 DG 4x4 for helioseismology (Q50, Q65)
Target: South Pole
xcen=-7 ycen=-911
Instrument: SOT
HOP/JOP: 101
Description:
The solar polar regions play a critical role in the solar dynamo and activity cycle. Magnetic field of active regions is transported by meridional flows from low latitudes to the polar regions. This flux transport causes reversals of the global magnetic field of the Sun around the time of activity maxima. The amount of magnetic flux accumulated in the polar regions determines the strength of the future sunspot cycle. For understanding the mechanism of the cyclic magnetic activity it is very important to measure the properties of the meridional flows and supergranular dynamics in the high-latitude regions, and their variations during the solar cycle. XRT joins the campaign for detection of waves propagating into corona.
wavelength: TF Fe I 5576 cadence: 1 min fov: 327,163 images: 960 JavaScript Landing Page
