HelioWebUniversity of California, San Diego, Center for Astrophysics and Space Science
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I[University of California, San Diego, Center for Astrophysics and Space Science]
PI["Parent Institutions (1)"]
CI["Child Institutions (0)"]
AW["Affiliated Works (113)"]
CA["Linked Collaborating Authors (15)"]
I== skos:broader ==>PI
CI== skos:broader ==>I
AW== affil ==>I
AW== author ==>CA
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Child Institutions [?]
Affiliated Works
sorted by decreasing year, and then by display-name
- A Study of Interacting Plasma Phenomena Using the Tomographic 3-Dimensional Reconstruction Techniques Developed for the Solar Mass Ejection Imager (SMEI)
- Hybrid Simulations of solar wind interaction with magnetized asteroids: Comparisons with observations of the whistler wing
- Introduction of the CSSS Magnetic Field Model into the UCSD Tomographic Solar Wind Model
- Space Weather Using Remote Sensing Data
- Study of ICME Structure Using LASCO White Light and STE Lab IPS Observations of Halo CMEs
- Volume Rendering of Heliospheric Data
- Halo CME's - Will They Hit or Miss Earth?
- Visualization of Remotely-Sensed Heliospheric Plasmas
- IPS From LOFAR: A Complement to Thomson Scattering Studies
- IPS/SMEI potential joint observations
- Interactive Visualization of Transient Solar Wind Phenomena for Space Weather Applications
- Recent Comparative Analyses of the CSSS UCSD Tomographic Solar Wind Model with in situ Spacecraft Observations
- SMEI: First Results and Future Capabilities
- Space Performance of the Multistage Labyrinthine SMEI Baffle
- Stellar Variability Studies with SMEI
- The Solar Mass Ejection Imager (SMEI)
- The Solar Mass Ejection Imager (SMEI) Mission
- Comparison of Solar Mass Ejection Imager (SMEI) White Light Observations with IPS Velocity
- Compensating for the Effects of hot Pixels in the Sunward Camera of SMEI
- Heliospheric Photometric Images and 3D Reconstruction from the Solar Mass Ejection Imager (SMEI) Data
- Systematic Error Reduction and Photometric Calibration for the Solar Mass Ejection Imager (SMEI)
- The Deceleration of Interplanetary Transients Between the Sun and 5 AU
- Three-dimensional structure of compound interplanetary transients associated with 27-28 May 2003 coronal mass ejections
- Wind/WAVES and SMEI Observations of ICMEs
- Zodiacal Light Analysis and Removal From the Solar Mass Ejection Imager (SMEI) Data
- Global 3-D Solar Wind Analysis of Halo CMEs Using Interplanetary Scintillation (IPS) Remote Sensing and its Comparison at Mars
- SMEI: A Spaceborne Observatory for Heliospheric Remote Sensing
- Solar Mass Ejection Imager (SMEI) Solar Wind 3-D Analysis of the January 20, 2005 CME
- 3-D Magnetic Field Geometry of the October 28, 2003 ICME: Comparison with SMEI White-Light Observations
- An Empirical Description of Zodiacal Light as Measured by SMEI
- CME Brightness at Large Elongations: Application to LASCO and SMEI Observations
- Goals and Progress of the LWS Focused Science Topic on the CME--ICME Connection
- Off-radial flow of the solar wind from EISCAT and MERLIN IPS observations
- The 20 January 2005 CME Solar Mass Ejection Imager (SMEI) Analyses
- The Evolution of Comets in the Heliosphere as Observed by SMEI
- A 3D view of coronal mass ejections in interplanetary space
- Analysis and Interpretation of Comet Measurements from SMEI
- IPS observations of the inner-heliosphere and their comparison with multi-point in-situ measurements
- Inner-heliosphere SMEI observations and their comparison with multi-point in-situ measurements
- Measurements of the Gegenschein brightness from the Solar Mass Ejection Imager (SMEI)
- Modeling the Corona-Heliosphere Interface in Anticipation of the Murchison Wide-field Array
- Observation and Modeling of Ion Upwelling Above Aurora
- SMEI Remote Sensing and the 3D Reconstruction of Corotating Heliospheric Structures
- Solar Wind 3D Reconstructions of the Whole Heliospheric Interval
- About the Solar Mass Ejection Imager (SMEI) 3D-Reconstruction-and-Display of Co-rotating Heliospheric Structure during the Present Deep Solar Minimum
- Coronal Mass Ejections in the Declining and Minimum Phase between Solar Cycles 23 and 24
- Measurements of Zodiacal-light brightness from the Solar Mass Ejection Imager (SMEI)
- Spectroscopy of the LCROSS Ejecta Plume from Keck, Gemini, and NASA IRTF Observatories
- The 26 April 2008 CME; a Case Study Tracking a CME into the Heliosphere
- A Heliospheric Imager for Deep Space: Lessons Learned from Helios, SMEI, and STEREO
- End-to-End Observations and Modeling of the 17-21 January 2010 CME/ICME
- Imaging Coronal Mass Ejections and Large-Scale Solar Wind Structure Using IPS and Thomson-Scattered Sunlight (Invited)
- Remote-Sensing Studies of Heliospheric Solar-Wind Structure Around Two Solar Minima
- Solar Mass Ejection Imager (SMEI) 3-D Reconstructions of CMEs, CIRs and Interplanetary Shocks, and Comparison with In-situ Data
- Type III Metric Radio-Wave Activity Prior to and During Active Region Flaring and CMEs (Invited)
- A Study of Long-Term Heliospheric Brightness Using SMEI Data
- Comparative Validation of Realtime Solar Wind Forecasting Using the UCSD Heliospheric Tomography Model
- Current and Planned Solar Wind Observations Using the EISCAT and LOFAR Radio-Telescope Systems
- Imaging Coronal Mass Ejections and Large-Scale Solar Wind Structure Using Thomson-Scattering Measurements from SMEI
- Necessity of 2D image data for determining 3D configurations of magnetic clouds
- SMEI and IPS 3-D CME Reconstructions, and What They Indicate of Heliospheric Solar Wind Acceleration
- UCSD Time-Dependent Tomographic Forecasting with Interplanetary Scintillation and White-Light Observations
- Using Global Heliospheric Reconstructions to Separate Multiple CME and CIR Flows
- Implicit Predictor-Corrector finite difference scheme for the ideal MHD simulations
- Precise Gravity Measurements for Lunar Laser Ranging at Apache Point Observatory
- Remote Sensing of Solar Wind Velocity Applying IPS Technique using MEXART
- The Ability of Radio Heliospheric Remote Sensing Observations to Provide Global Solar Wind Parameters
- Tracing Polar Jets into the Inner Heliosphere by Using Images from the LASCO C2 and STEREO COR2 Coronagraphs and 3D Tomographic Reconstructions from Interplanetary Scintillation and the Solar Mass Ejection Imager (SMEI)
- Comet C/2012 S1 (ISON): Observations of the Dust Grains from SOFIA and of the Atomic Gas from NSO Dunn and McMath-Pierce Solar Telescopes (Invited)
- Constraining Cometary Crystal Shapes from IR Spectral Features
- IPS-based time-dependent boundary conditions for modeling the heliosphere
- Remote Sensing of Solar Wind Speeds using Observations of IPS at 140 and 327 MHz: MEXART and STELab
- Simulation of Magnetic Cloud Erosion and Deformation During Propagation
- Using Interplanetary Scintillation (IPS) For Space-Weather Forecasting
- Faraday Rotation (FR) and Interplanetary Scintillation (IPS) Case Studies Using the LOw Frequency ARray (LOFAR)
- Heliospheric Tomography from IPS Data at 140 MHz
- Using IPS Magnetic Modeling to Determine Bz
- 3D Analysis of Remote-Sensed Heliospheric Data for Space Weather Forecasting
- Determination of the North-South Heliospheric Magnetic-Field Component from Inner-Corona Closed-Loop Propagation
- How Reliable Is the Solar Wind Prediction from the Models Installed at the CCMC?
- Measurements and an Empirical Model of the Zodiacal Brightness as Observed by the Solar Mass Ejection Imager (SMEI)
- Observations of Heliospheric Faraday Rotation (FR) and Interplanetary Scintillation (IPS) with the LOw Frequency ARray (LOFAR): Steps Towards Improving Space-Weather Forecasting Capabilities
- Phase-Angle Dependence of Determinations of Diameter, Albedo, and Taxonomy: A case study of NEO 3691 Bede
- Requirements for an Operational Coronagraph
- The first super geomagnetic storm of solar cycle 24: "The St. Patrick day (17 March 2015)" event
- Using In Situ and Remote Sensing Data to Model the Plasma Flow throughout the Heliosphere
- ASHI, an All Sky Heliospheric Imager for Future NASA Missions
- Imaging and characterizing exo-Earths at 10 microns - The TIKI project
- Interplanetary Scintillation Observations with a New Generation of Radio Telescopes: First results from the MWA
- Modeling the Solar Wind throughout Interplanetary Space Using Ground-based and Spacecraft Observational Data
- Observations of Heliospheric Faraday Rotation of a CME Using LOFAR and Space-Based Imaging
- Observations of the Variable Coronal Solar Wind, and its Implications for Solar Probe Plus and Solar Orbiter
- Potential Use of Observations of Interplanetary Scintillation (IPS) and Faraday Rotation (FR) in Support of the Solar Orbiter and Solar Probe Plus Missions
- The Eulerian solver of Vlasov-Ampère system for electrostatic plasma
- The UCSD Time-dependent Tomography and IPS use for Exploring Space Weather Events
- The Worldwide Interplanetary Scintillation (IPS) Stations (WIPSS) Network in support of Space-Weather Science and Forecasting
- ASHI: An All Sky Heliospheric Imager for Viewing Thomson-Scattered Light
- An Iterative Interplanetary Scintillation (IPS) Analysis Using Time-dependent 3-D MHD Models as Kernels
- The Worldwide Interplanetary Scintillation (IPS) Stations (WIPSS) Network October 2016 Observing Campaign: Initial WIPSS Data Analyses
- The variable nature of the solar wind
- ASHI: An All Sky Heliospheric Imager for viewing Thomson-scattered sunlight
- The Prediction of Bz Fields Using the CSSS Model and UCSD IPS Tomography
- The UCSD Iterative Interplanetary Scintillation (IPS) Analysis Using an ENLIL 3-D MHD Model Kernel in Near Real Time
- ASHI: An All Sky Heliospheric Imager to Provide Space Weather Forecasting Using Thomson-Scattered Sunlight
- The UCSD Iterative Interplanetary Scintillation (IPS) Analysis Using an ENLIL 3-D MHD Model Kernel
- The Worldwide Interplanetary Scintillation (IPS) Stations (WIPSS) Network: A Ground-Based Heliospheric Observatory for Science and Space Weather
- Validating the Alfven Wave Solar Atmosphere (AWSoM) Model from the Low Corona to 1 AU
- Finite Temperature and Ion Inertia Induced multiple convective fluid instabilities in Polar Patches
- Highly absorbing refractory carbonaceous matter in cometary comae dust from the perspective of thermal IR spectroscopy
- SOFIA Exploration of Refractory Dust Species in Comets
- UCSD Iterative Tomography Analyses Applied to STEREO HI Observations
- Ionospheric Drivers Induced Multiple Convective Fluid Instabilities In Polar Patches
- Convective interchange mix-modes and phase scintillation In polar patches.