Cranmer, Steven R. - Harvard-Smithsonian Center for Astrophysics

Advanced Search

Cranmer, Steven R. - Harvard-Smithsonian Center for Astrophysics

The Sun is often highlighted as a benchmark for the study of other stars, and as a stepping stone to the study of galaxies and cosmic dis-
STELLAR EVOLUTION [Contents] [Next Article] Winds that Sail on Starlight
CORONAL HOLES AND THE SOLAR WIND Steven R. Cranmer1
SOLAR WIND PHYSICS WITH SOLAR PROBE: How will our first mission to the nearest star contribute to our
New views of the solar wind with the Lambert W function Steven R. Cranmera)
Multi-wavelength Observations of Coronal Structure and Dynamics: Yohkoh 10th Anniversary Meeting,
IUGG XXIII General Assembly, GAIV.02 Sapporo, Japan . . . July 4, 2003
Biographical Sketch: Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics Phone: 6174957271, Fax: 6174957455
Coronal Holes E N CYC LO PE D IA O F AS T R O N O MY AN D AS T R O PHYS I C S Coronal Holes
Originally written July 30, 1997 A Simple Approach to Mutual Irradiation Heating in Close Binary Systems
UVCS/SOHO Observations of Jupiter in January 1997: An Independent Calibration of the White Light Channel
Potential Hot/Massive Star Areas of Interest for Stellar Imager Steven R. Cranmer (scranmer@cfa.harvard.edu)
13th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, Hamburg, Germany, July 59, 2004
To be published in the proceedings of the 14th Topical Conference on Radio Frequency Power in Plasmas, May 79, 2001, Oxnard, California, AIP Press.
Coronal Holes E NCYCLOPED I A O F A S TRONOMY AND A S TROPHYS I C S Coronal Holes
SPECTROSCOPIC CONSTRAINTS ON MODELS OF IONCYCLOTRON RESONANCE HEATING IN THE POLAR SOLAR CORONA
Potential Hot/Massive Star Areas of Interest for Stellar Imager Steven R. Cranmer (scranmer@cfa.harvard.edu)
To be published in the proceedings of the 14th Topical Conference on Radio Frequency Power in Plasmas, May 7--9, 2001, Oxnard, California, AIP Press.
ALFVE NIC TURBULENCE IN THE EXTENDED SOLAR CORONA: KINETIC EFFECTS AND PROTON HEATING
On the Synthesis of Coronal WhiteLight Polarization Diagnostics Steven R. Cranmer
The Impact of IonCyclotron Wave Dissipation on Heating and Accelerating the Fast Solar Wind
Effect of Gravity Darkening on Radiatively Driven Mass Loss from Rapidly Rotating HotStars
SOLAR WIND PHYSICS WITH SOLAR PROBE: How will our first mission to the nearest star contribute to our
UVCS/SOHO Observations of Jupiter in January 1997: An Independent Calibration of the White Light Channel
An Introduction to Coronal Velocity Distributions and the Modeling of UVCS/SOHO Emission Lines
CORONAL HOLES AND THE SOLAR WIND Steven R. Cranmer 1
On the Synthesis of Solar Coronal Emission Diagnostics Steven R. Cranmer
THE IMPACT OF UVCS/SOHO OBSERVATIONS ON MODELS OF IONCYCLOTRON RESONANCE HEATING OF THE SOLAR CORONA
New views the solar wind with the Lambert function Steven Cranmer
November 10, 2010 Ultraviolet Coronagraph Spectroscopy: A Key Capability for Understanding
CORONAL HOLES AND THE HIGH-SPEED SOLAR WIND STEVEN R. CRANMER
ALFVE NIC TURBULENCE IN THE EXTENDED SOLAR CORONA: KINETIC EFFECTS AND PROTON HEATING
Plasma Conditions in Polar Plumes and Interplume Regions
ON THE GENERATION, PROPAGATION, AND REFLECTION OF ALFVEN WAVES FROM THE SOLAR PHOTOSPHERE TO THE DISTANT HELIOSPHERE
43rd Annual Meeting of the Division of Plasma Physics October 29November 2, 2001, Long Beach, California
SOHO15: Coronal Heating, 69 September 2004, University of St. Andrews, Scotland
IMPROVED CONSTRAINTS ON THE PREFERENTIAL HEATING AND ACCELERATION OF OXYGEN IONS IN THE EXTENDED SOLAR CORONA
Monte Carlo Solutions to Diffusion-Like Equations: A Practical Application of the It^o Calculus
SELF-CONSISTENT CORONAL HEATING AND SOLAR WIND ACCELERATION FROM ANISOTROPIC MAGNETOHYDRODYNAMIC TURBULENCE
TURBULENCE-DRIVEN POLAR WINDS FROM T TAURI STARS ENERGIZED BY MAGNETOSPHERIC ACCRETION
UVCS Observations of the Solar Wind and its Modeling
An Introduction to Coronal Velocity Distributions and the Modeling of UVCS SOHO Emission Lines