Analysis of Photospheric Convection Flows Over a Solar Cycle

Details Analysis of Photospheric Convection Flows Over a Solar Cycle Analysis of Photospheric Convection Flows Over a Solar Cycle

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.0919w&link_type=abstract

American Astronomical Society, SPD meeting #40, #9.19; Bulletin of the American Astronomical Society, Vol. 41, p.820

Astronomy and Astrophysics

Astronomy

Scientific paper

Convection in the Sun plays an important role as a mechanism responsible for the 11-year solar cycle. Magnetic field phenomena are thus inextricably linked to the convective process, an example being the gathering of magnetic field lines around supergranule boundaries observed as the chromospheric network.
Our research asks to what extent variations in the global magnetic field affect particular characteristics of photospheric convection features, using Dopplergrams derived from SOHO/MDI data during the course of Solar Cycle 23.
We look ahead to the higher resolution data that SDO/HMI will provide and any further insight such data may provide.

Affiliated with

Also associated with

No associations

Rating

Analysis of Photospheric Convection Flows Over a Solar Cycle does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Analysis of Photospheric Convection Flows Over a Solar Cycle, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Analysis of Photospheric Convection Flows Over a Solar Cycle will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1112017