D. Mullan
2000–2002
A researcher in the Science corpus: 2 papers; trusts 1 researcher and is trusted by 4 researchers here, as inferred from the citation graph.
Whom D. Mullan trusts overall
Their strongest outbound trust, strongest first, inferred from their citations.
Who trusts D. Mullan overall
Papers from D. Mullan's perspective
Ordered by how strongly the researchers D. Mullan trusts endorse each paper. Same corpus, a different order for every researcher.
- Ion Cyclotron Wave Dissipation in the Solar Corona: The Summed Effect of More than 2000 Ion Species
- Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics
- Solar cycle changes in coronal holes and space weather cycles
- Current Theoretical Models and Future High Resolution Solar Observations: Preparing for ATST
- Simulations of Incompressible Magnetohydrodynamic Turbulence
- Differences between CME‐driven storms and CIR‐driven storms
- Turbulent Heating of the Solar Wind by Newborn Interstellar Pickup Protons
- Recent progress in astrophysical plasma turbulence from solar wind observations (Journal of Plasma Physics)
- The Solar Wind as a Turbulence Laboratory
- The mass-loss rates of red supergiants and the de Jager prescription
Their papers
- Coronal Heating Distribution Due to Low-Frequency, Wave-driven Turbulence (2002) — 165 citations
- MHD-driven Kinetic Dissipation in the Solar Wind and Corona (2000) — 242 citations