Parents

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Louis George Henyey grad student 1968 UC Berkeley
 (Convective energy transport in stellar atmospheres)

Children

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Allen W Shafter grad student UCLA (Physics Tree)
John M. Scalo grad student 1974 UCLA
Aimee A. Norton grad student 2000 UCLA (Physics Tree)
Tham Tran grad student 2009 UCLA (Physics Tree)
Daryl G. Parker grad student 2011 UCLA (Physics Tree)
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Publications

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Pevtsov AA, Tlatova KA, Pevtsov AA, et al. (2019) Reconstructing solar magnetic fields from historical observations. V. Sunspot magnetic field measurements at Mount Wilson Observatory Astronomy and Astrophysics. 628
Ulrich RK, Riley P, Tran T. (2018) Solar Sources of Interplanetary Magnetic Clouds Leading to Helicity Prediction. Space Weather : the International Journal of Research & Applications. 16: 1668-1685
Fossat E, Boumier P, Corbard T, et al. (2017) Asymptoticgmodes: Evidence for a rapid rotation of the solar core Astronomy & Astrophysics. 604: A40
Ulrich RK, Tran T. (2016) Generation of a North/South Magnetic Field Component from Variations in the Photospheric Magnetic Field Solar Physics. 291: 1059-1076
McIntosh SW, Leamon RJ, Krista LD, et al. (2015) The solar magnetic activity band interaction and instabilities that shape quasi-periodic variability. Nature Communications. 6: 6491
Riley P, Ben-Nun M, Linker JA, et al. (2014) A Multi-Observatory Inter-Comparison of Line-of-Sight Synoptic Solar Magnetograms Solar Physics. 289: 769-792
Ulrich RK, Tran T. (2013) THE GLOBAL SOLAR MAGNETIC FIELD—IDENTIFICATION OF TRAVELING, LONG-LIVED RIPPLES The Astrophysical Journal. 768: 189
Li J, Ulrich RK. (2012) LONG-TERM MEASUREMENTS OF SUNSPOT MAGNETIC TILT ANGLES The Astrophysical Journal. 758: 115
McIntosh SW, Leamon RJ, Hock RA, et al. (2011) Observing evolution in the supergranular network length scale during periods of low solar activity Astrophysical Journal Letters. 730
Ulrich RK. (2010) Solar meridional circulation from doppler shifts of the Fe I line at 5250Å as measured by the 150-foot solar tower telescope at the MT. Wilson observatory Astrophysical Journal. 725: 658-669
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