The Sun’s Global Flows: Differential Rotation

Sushant Mahajan1, Lisa Upton2, H. M. Antia3, Sarbani Basu4, Marc L DeRosa5, J Todd Hoeksema6, Kiran Jain7, Rudolf Komm8, Alexei A Pevtsov7, Thierry Roudier9, Sushanta C Tripathy10, Roger K Ulrich11, Shea A. Hess Webber6 and Junwei Zhao1, (1)W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, United States, (2)Southwest Research Institute Boulder, Boulder, CO, United States, (3)Centre for Excellence in Basic Science, Mumbai, India, (4)Yale University, New Haven, CT, United States, (5)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (6)Stanford University, HEPL, Stanford, CA, United States, (7)National Solar Observatory, Boulder, United States, (8)National Solar Observatory, Sunspot, United States, (9)IRAP, Toulouse, France, (10)National Solar Observatory, Tucson, AZ, United States, (11)UCLA, Los Angeles, CA, United States