- Tmt India
A composite image of the Sun that depicts the range of scientific research -- The interior image from MDI/SoHO illustrates the rivers of plasma discovered flowing under the Sun’s surface. The surface image was taken with the Extreme ultraviolet Imaging Telescope (EIT) at 304Å. Both were superimposed on a Large Angle Spectroscopic Coronograph (LASCO) C2 image, which blocks the Sun so that it can view the corona in visible. The image suggests the range of our research, from the solar interior, to the surface and corona, and out to the solar wind.
Solar Physics Discussion Meetings
Magnetic fields are present almost everywhere on the Sun. Without these fields the Sun would have been a rather dull object. One of the major challenges of solar physics is to understand the role of magnetic fields. Magnetohydrodynamics (MHD) describes the behaviour of plasma in the presence of magnetic field. Solar MHD attempts to explain the magnetic Sun.
IIA scientists are involved in studying the structure and dynamics of the magnetized solar chromosphere, wave propagation in magnetic network, mode coupling and conversion in magnetic flux tubes and energy transport mechanisms in the solar atmosphere.
Waves and Oscillations
Waves permeate the entire Sun. Studying these waves give us a clue about different properties of the solar atmosphere. Using various ground based and space based telescopes to observe the Sun in different wavelengths, IIA scientists try to identify and study various wave modes that are present on the solar atmosphere.
Helioseismology is the study of wave oscillations in the Sun. We use the techniques of local helioseismology to understand the interior of the Sun, especially the sub-surface structure of sunspots.
Solar Coronal Studies