The colors of the bullets convey the main topics of the papers: YELLOW for the Sun, BLUE for hot stars, RED for cool stars, and GREEN for planets and asteroids.

Refereed Journals

  • Shoda, M., Suzuki, T. K., Matt, S. P., Cranmer, S. R., Vidotto, A. A., Strugarek, A., See, V., Reville, V., Finley, A. J., and Brun, A. S. 2020, "Alfven-wave Driven Magnetic Rotator Winds from Low-mass Stars I: Rotation Dependences of Magnetic Braking and Mass-loss Rate," Ap. J., submitted.

  • Schiff, A. J., and Cranmer, S. R. 2019, "Thermal Conduction in the Solar Corona and Solar Wind: The Eight-Moment Approximation," Ap. J., submitted.

  • Cranmer, S. R. 2018, "Low-frequency Alfven Waves Produced by Magnetic Reconnection in the Sun's Magnetic Carpet," Ap. J., 862, 6. [see also arXiv:1805.12184]

  • Cranmer, S. R. 2017, "Mass Loss Rates from Coronal Mass Ejections: A Predictive Theoretical Model for Solar-Type Stars," Ap. J., 840, 114. [see also arXiv:1704.06689]

  • Cranmer, S. R. 2016, "Predictions for Dusty Mass Loss from Asteroids during Close Encounters with Solar Probe Plus," Earth, Moon, and Planets, 118, 51. [see also arXiv:1606.01785]

  • Cranmer, S. R. 2014, "Suprathermal Electrons in the Solar Corona: Can Nonlocal Transport Explain Heliospheric Charge States?" Ap. J. Letters, 791, L31. [see also arXiv:1407.5941]

  • Cranmer, S. R. 2014, "Ensemble Simulations of Proton Heating in the Solar Wind via Turbulence and Ion Cyclotron Resonance," Ap. J. Suppl., 213, 16. [see also arXiv:1406.0678]

  • Cranmer, S. R. 2010, "An Efficient Approximation of the Coronal Heating Rate for Use in Global Sun-Heliosphere Simulations," Ap. J., 710, 676. [see also arXiv:0912.5333]

  • Cranmer, S. R. 2009, "Testing Models of Accretion-driven Coronal Heating and Stellar Wind Acceleration for T Tauri Stars," Ap. J., 706, 824. [see also arXiv:0910.2686]

  • Cranmer, S. R. 2008, "Turbulence-driven Polar Winds from T Tauri Stars Energized by Magnetospheric Accretion," Ap. J., 689, 316. [see also arXiv:0808.2250]

  • Cranmer, S. R. 2005, "A Statistical Study of Threshold Rotation Rates for the Formation of Disks around Be Stars," Ap. J., 634, 585 (November 20, 2005). [see also astro-ph/0507718]

  • Cranmer, S. R. 2002, "Coronal Holes and the High-Speed Solar Wind," Space Sci. Rev., 101, 229 (65-page review paper).

  • Cranmer, S. R. 2001, "Ion Cyclotron Diffusion of Velocity Distributions in the Extended Solar Corona," J. Geophys. Res., 106, 24937.

  • Cranmer, S. R. 1998, "Non-Maxwellian Redistribution in Solar Coronal Lyman Alpha Emission," Ap. J., 508, 925.

  • Cranmer, S. R. and Owocki, S. P. 1996, "Hydrodynamical Simulations of Corotating Interaction Regions and Discrete Absorption Components in Rotating O-Star Winds," Ap. J., 462, 469.

  • Cranmer, S. R. and Owocki, S. P. 1995, "The Effect of Oblateness and Gravity Darkening on the Radiation Driving in Winds from Rapidly Rotating B Stars," Ap. J., 440, 308.

  • Cranmer, S. R. 1993, "Some Aspects of Illuminated Model Atmosphere Theory as Applied to Close Binary Systems," Mon. Not. R. Astr. Soc., 263, 989.