Coronal Field Opens at Lower Height During the Solar Cycles 22 and 23 Minimum Periods: IMF Comparison Suggests the Source Surface Should Be Lowered

Solar Physics

Volumn 269, Issue 2, 2011, Pages 367-388

  Lee, C O ^a,b   Luhmann, J G ^a   Hoeksema, J T ^c   Sun, X ^c   Arge, C N ^d   de Pater, I ^b  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c STANFORD UNIVERSITY   (United States)

^d AIR FORCE RESEARCH LABORATORY   (United States)

Author keywords

Corona, models; Coronal holes; Magnetic field, interplanetary; Magnetic field, observations; Solar cycle, observations

Indexed keywords

EID: 79952699726     PISSN: 00380938     EISSN: 1573093X     Source Type: Journal    
DOI: 10.1007/s11207-010-9699-9     Document Type: Article

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