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David M. Malaspina

Identifiers

  • name variant David M. Malaspina 0.60 · backfill

Papers (40)

  1. How long-lived grains dominate the shape of the Zodiacal Cloud astro-ph.EP · 2024 · author #5
  2. Variability of Antenna Signals From Dust Impacts physics.space-ph · 2023 · author #3
  3. Laboratory Study of Antenna Signals Generated by Dust Impacts on Spacecraft physics.space-ph · 2023 · author #5
  4. Electrostatic Model for Antenna Signal Generation From Dust Impacts physics.space-ph · 2023 · author #4
  5. New Observations of Solar Wind 1/f Turbulence Spectrum from Parker Solar Probe astro-ph.SR · 2023 · author #21
  6. On the evolution of the Anisotropic Scaling of Magnetohydrodynamic Turbulence in the Inner Heliosphere physics.space-ph · 2023 · author #18
  7. Magnetic field spectral evolution in the inner heliosphere astro-ph.SR · 2022 · author #19
  8. Correlation between bandwidth and frequency of plasmaspheric hiss uncovered with unsupervised machine learning physics.space-ph · 2022 · author #2
  9. Patches of magnetic switchbacks and their origins astro-ph.SR · 2022 · author #16
  10. Parker Solar Probe observations of near-$f_{\rm ce}$ harmonics emissions in the near-Sun solar wind and their dependence on the magnetic field direction astro-ph.SR · 2022 · author #3
  11. MMS Observations of a Compressed Current Sheet: Importance of the Ambipolar Electric Field physics.space-ph · 2022 · author #4
  12. Exploring the Solar Wind from its Source on the Corona into the Inner Heliosphere during the First Solar Orbiter - Parker Solar Probe Quadrature astro-ph.SR · 2021 · author #44
  13. A novel machine learning technique to identify and categorize plasma waves in spacecraft measurements physics.space-ph · 2021 · author #2
  14. Ambipolar electric field and potential in the solar wind estimated from electron velocity distribution functions astro-ph.SR · 2021 · author #18
  15. A powerful machine learning technique to extract proton core, beam and alpha-particle parameters from velocity distribution functions in space plasmas physics.space-ph · 2021 · author #4
  16. Alfv\'enic versus non-Alfv\'enic turbulence in the inner heliosphere as observed by Parker Solar Probe astro-ph.SR · 2021 · author #11
  17. Encounter of Parker Solar Probe and a Comet-like Object During Their Perihelia: Model Predictions and Measurements astro-ph.EP · 2020 · author #18
  18. The Contribution of Alpha Particles to the Solar Wind Angular Momentum Flux in the Inner Heliosphere astro-ph.SR · 2020 · author #16
  19. Wave-particle energy transfer directly observed in an ion cyclotron wave physics.space-ph · 2020 · author #4
  20. Measurement of the Open Magnetic Flux in the Inner Heliosphere down to 0.13AU astro-ph.SR · 2020 · author #9
  21. Small-scale Magnetic Flux Ropes in the First two Parker Solar Probe Encounters physics.space-ph · 2020 · author #16
  22. Parker Solar Probe observations of proton beams simultaneous with ion-scale waves physics.space-ph · 2020 · author #12
  23. Coronal Electron Temperature inferred from the Strahl Electrons in the Inner Heliosphere: Parker Solar Probe and Helios observations astro-ph.SR · 2020 · author #18
  24. The Radial Dependence of Proton-scale Magnetic Spectral Break in Slow Solar Wind during PSP Encounter 2 physics.space-ph · 2020 · author #19
  25. Inner-Heliosphere Signatures of Ion-Scale Dissipation and Nonlinear Interaction astro-ph.SR · 2020 · author #19
  26. A Merged Search-Coil and Fluxgate Magnetometer Data Product for Parker Solar Probe FIELDS astro-ph.IM · 2020 · author #11
  27. Density Fluctuations in the Solar Wind Based on Type III Radio Bursts Observed by Parker Solar Probe astro-ph.SR · 2020 · author #10
  28. Cross Helicity Reversals In Magnetic Switchbacks physics.space-ph · 2019 · author #18
  29. Proton Temperature Anisotropy Variations in Inner Heliosphere Estimated with First Parker Solar Probe Observations physics.space-ph · 2019 · author #26
  30. The role of Alfv\'en wave dynamics on the large scale properties of the solar wind: comparing an MHD simulation with PSP E1 data astro-ph.SR · 2019 · author #18
  31. Observations of Energetic-Particle Population Enhancements along Intermittent Structures near the Sun from Parker Solar Probe physics.space-ph · 2019 · author #27
  32. Statistics and Polarization of Type III Radio Bursts Observed in the Inner Heliosphere astro-ph.SR · 2019 · author #18
  33. Magnetic field kinks and folds in the solar wind physics.space-ph · 2019 · author #18
  34. Enhanced Energy Transfer Rate in Solar Wind Turbulence Observed near the Sun from Parker Solar Probe physics.space-ph · 2019 · author #17
  35. Switchbacks in the near-Sun magnetic field: long memory and impact on the turbulence cascade astro-ph.SR · 2019 · author #13
  36. The Enhancement of Proton Stochastic Heating in the near-Sun Solar Wind astro-ph.SR · 2019 · author #16
  37. First in-situ Measurements of Electron Density and Temperature from Quasi-Thermal Noise Spectroscopy with Parker Solar Probe/FIELDS astro-ph.SR · 2019 · author #13
  38. Ion Scale Electromagnetic Waves in the Inner Heliosphere astro-ph.SR · 2019 · author #5
  39. Magnetic connectivity of the ecliptic plane within 0.5 AU : PFSS modeling of the first PSP encounter astro-ph.SR · 2019 · author #19
  40. On the role of wave-particle interactions in the macroscopic dynamics of collisionless plasmas physics.space-ph · 2015 · author #4

Mentions

  • 2401.13776 #5 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2301.03896 #18 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2303.00843 #21 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2304.00452 #4 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2304.00454 #3 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2304.00453 #5 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2209.02451 #19 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2207.10505 #2 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2201.07720 #4 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2205.11356 #3 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2206.03807 #16 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 1912.03777 #18 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2108.08528 #18 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2110.11031 #44 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2108.08925 #2 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2105.08651 #4 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2010.15189 #4 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2101.00830 #11 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2011.00016 #16 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2009.06844 #9 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2012.00005 #18 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2007.04551 #16 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2001.05081 #19 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2001.04587 #11 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2004.03009 #12 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2003.04016 #18 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 1912.03871 #26 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 1912.07823 #18 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 1912.02361 #5 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2001.08239 #19 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 2001.03476 #10 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 1912.03424 #27 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 1912.02959 #17 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 1912.02653 #16 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 1912.02518 #13 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 1912.03240 #18 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 1912.03371 #18 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 1912.02856 #13 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 1912.02244 #19 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 1510.06904 #4 · arxiv_oai · confidence 0.70 David M. Malaspina
  • 1510.06904 #4 · backfill · confidence 0.70 David M. Malaspina

Frequent Coauthors