Lan Jian
0000-0002-6849-5527
NASA Goddard Space Flight Center
100 papers found
Refreshing results…
Validation for global solar wind prediction using Ulysses comparison: Multiple coronal and heliospheric models installed at the Community Coordinated Modeling Center
Shock Connectivity in the 2010 August and 2012 July Solar Energetic Particle Events Inferred From Observations and Enlil Modeling
A Proton-Cyclotron Wave Storm Generated by Unstable Proton Distribution Functions in the Solar Wind
Interplanetary shocks and foreshocks observed by STEREO during 2007–2010
Ion-driven instabilities in the solar wind: Wind observations of 19 March 2005
Electromagnetic Cyclotron Waves in the Solar Wind: Wind Observation and Wave Dispersion Analysis
MESSENGER survey of in situ low frequency wave storms between 0.3 and 0.7 AU
Propagation of the 2014 January 7 Cme and Resulting Geomagnetic Non-Event
Ensemble Modeling of CMEs Using the WSA–ENLIL+Cone Model
The impact of a slow interplanetary coronal mass ejection on Venus
Validation for solar wind prediction at Earth: Comparison of coronal and heliospheric models installed at the CCMC
Low-frequency waves within isolated magnetic clouds and complex structures: STEREO observations
Generation and propagation of ion cyclotron waves in nonuniform magnetic field: Application to the corona and solar wind
A statistical analysis of heliospheric plasma sheets, heliospheric current sheets, and sector boundaries observed in situ by STEREO
Ninety degrees pitch angle enhancements of suprathermal electrons associated with interplanetary shocks
An Ensemble Study of a January 2010 Coronal Mass Ejection (CME): Connecting a Non-obvious Solar Source with Its ICME/Magnetic Cloud
Electromagnetic Waves Near the Proton Cyclotron Frequency:stereoobservations
Generation of ion cyclotron waves in the corona and solar wind
Why have geomagnetic storms been so weak during the recent solar minimum and the rising phase of cycle 24?
Inner Heliospheric Evolution of a “stealth” Cme Derived From Multi-View Imaging and Multipoint in Situ Observations. I. Propagation to 1 Au
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