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21 results on '"Whittlesey, Phyllis"'

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1. Erratum: “The Role of Alfvén Wave Dynamics on the Large-scale Properties of the Solar Wind: Comparing an MHD Simulation with Parker Solar Probe E1 data” (2020, ApJS, 246, 24)

2. Cross Helicity Reversals in Magnetic Switchbacks

3. The Enhancement of Proton Stochastic Heating in the Near-Sun Solar Wind

4. Analysis of the Internal Structure of the Streamer Blowout Observed by the Parker Solar Probe During the First Solar Encounter

5. Exploring Solar Wind Origins and Connecting Plasma Flows from the Parker Solar Probe to 1 au: Nonspherical Source Surface and Alfvénic Fluctuations

6. The Radial Dependence of Proton-scale Magnetic Spectral Break in Slow Solar Wind during PSP Encounter 2

7. Energetic Particle Increases Associated with Stream Interaction Regions

8. Sharp Alfvénic Impulses in the Near-Sun Solar Wind

9. Plasma Waves near the Electron Cyclotron Frequency in the Near-Sun Solar Wind

10. The Heliospheric Current Sheet in the Inner Heliosphere Observed by the Parker Solar Probe

11. Switchbacks in the Near-Sun Magnetic Field: Long Memory and Impact on the Turbulence Cascade

12. Magnetic Field Kinks and Folds in the Solar Wind

13. Source and Propagation of a Streamer Blowout Coronal Mass Ejection Observed by the Parker Solar Probe

14. The Solar Probe Cup on the Parker Solar Probe

15. The Solar Probe ANalyzers—Electrons on the Parker Solar Probe

16. Statistics and Polarization of Type III Radio Bursts Observed in the Inner Heliosphere

17. Kinetic-scale Spectral Features of Cross Helicity and Residual Energy in the Inner Heliosphere

18. Density Fluctuations in the Solar Wind Based on Type III Radio Bursts Observed by Parker Solar Probe

19. The Role of Alfvén Wave Dynamics on the Large-scale Properties of the Solar Wind: Comparing an MHD Simulation with Parker Solar Probe E1 Data

20. Magnetic Connectivity of the Ecliptic Plane within 0.5 au: Potential Field Source Surface Modeling of the First Parker Solar Probe Encounter

21. Relating Streamer Flows to Density and Magnetic Structures at the Parker Solar Probe

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