Experiments
Searchable full-text extractions: founding hypothesis, core claims, experimental setups, key results and statistics — pulled out of each paper as structure. Search a cell line, an assay or an entity (e.g. HUH7) and find every paper that worked with it. This corpus stands on its own: most entries carry no reproduction assessment (yet).
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Has reproduction
Advanced Methods for Analyzing in-Situ Observations of Magnetic Reconnection.
PMID 39234211 · PMC11369046 · Space science reviews · 2024 · 7 claims · 8 setups
Collisionless magnetic reconnection in geospace has multi-scale structure: MHD regions (ions and electrons frozen-in), ion diffusion regions (ions demagnetized, electrons magnetized), and electron diffusion regions (both demagnetized, magnetic topology changes).
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Has reproduction · 92
Electron Energy Partition across Interplanetary Shocks. I. Methodology and Data Product.
PMID 31806920 · PMC6894189 · The Astrophysical journal. Supplement series · 2019 · 7 claims · 3 setups
Solar wind electron VDFs below ~1.2 keV are best modeled as the sum of three components: a cold dense core, a hot tenuous halo, and a field-aligned beam/strahl.
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Has reproduction · 67
Downstream high-speed plasma jet generation as a direct consequence of shock reformation.
PMID 35105885 · PMC8807623 · Nature communications · 2022 · 7 claims · 6 setups
High-speed downstream jets at Earth's bow shock are generated as a direct consequence of shock reformation.
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Has reproduction · 94
Direct observations of cross-scale wave-particle energy transfer in space plasmas.
PMID 39919183 · PMC11804927 · Science advances · 2025 · 7 claims · 8 setups
Fluid-scale ULF waves resonate with reflected ions, modifying their velocity distributions and driving growth of ion-scale magnetosonic-whistler waves
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Has reproduction · 68
Revealing an unexpectedly low electron injection threshold via reinforced shock acceleration.
PMID 39805850 · PMC11730962 · Nature communications · 2025 · 8 claims · 4 setups
A reinforced shock acceleration model combining foreshock transients, wave-particle interactions, and variable stellar wind conditions operating across multiple scales enables electrons to consistently reach relativistic energies