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1. Solar Neutrino Flux

   Linked via "interaction cross-section"

   Measurement Techniques and Detectors
   Measuring the incredibly low flux and low interaction cross-section of solar neutrinos requires massive, shielded detectors, often situated deep underground to shield against cosmic ray background. The history of measurement involves three generations of technology:
   | Detector Class | Primary Measurement Technique | Signature Particle Detected | Typical Energy Range (MeV) | Primary Observation |