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  2. Solar neutrino - Wikipedia

    en.wikipedia.org/wiki/Solar_neutrino

    Diagram showing the Sun's components. The core is where nuclear fusion takes place, creating solar neutrinos. A solar neutrino is a neutrino originating from nuclear fusion in the Sun's core, and is the most common type of neutrino passing through any source observed on Earth at any particular moment.

  3. Neutrino - Wikipedia

    en.wikipedia.org/wiki/Neutrino

    Solar neutrinos originate from the nuclear fusion powering the Sun and other stars. The details of the operation of the Sun are explained by the Standard Solar Model. In short: when four protons fuse to become one helium nucleus, two of them have to convert into neutrons, and each such conversion releases one electron neutrino.

  4. Neutrino astronomy - Wikipedia

    en.wikipedia.org/wiki/Neutrino_astronomy

    Neutrinos are very hard to detect due to their non-interactive nature. In order to detect neutrinos, scientists have to shield the detectors from cosmic rays, which can penetrate hundreds of meters of rock. Neutrinos, on the other hand, can go through the entire planet without being absorbed, like "ghost particles".

  5. Neutrinos from our Sun hold the secrets to nuclear fusion

    www.aol.com/neutrinos-sun-hold-secrets-nuclear...

    Most people realize our Sun is producing light and heat from the fusion of hydrogen into helium. Typically, there are two processes by which smaller stars create fusion. The first of these, the ...

  6. Homestake experiment - Wikipedia

    en.wikipedia.org/wiki/Homestake_experiment

    After Bahcall calculated the rate at which the detector should capture neutrinos, Davis's experiment turned up only one third of this figure. The experiment was the first to successfully detect and count solar neutrinos, and the discrepancy in results created the solar neutrino problem. The experiment operated continuously from 1970 until 1994.

  7. Neutrino oscillation - Wikipedia

    en.wikipedia.org/wiki/Neutrino_oscillation

    Neutrinos produced in nuclear reactors have energies similar to solar neutrinos, of around a few MeV. The baselines of these experiments have ranged from tens of meters to over 100 km (parameter θ 12). Mikaelyan and Sinev proposed to use two identical detectors to cancel systematic uncertainties in reactor experiment to measure the parameter ...

  8. Mikheyev–Smirnov–Wolfenstein effect - Wikipedia

    en.wikipedia.org/wiki/Mikheyev–Smirnov...

    The 4 vertical strips indicate the values of the energies at which the survival probability was measured, by means of pp, 7 Be, pep, and 8 B solar neutrinos, respectively. For the low-energy solar neutrinos, on the other hand, the matter effect is negligible, and the formalism of oscillations in vacuum is valid.

  9. 30 things to do when you’re bored (that are actually good for ...

    www.aol.com/lifestyle/30-things-bored-actually...

    Escape the monotony of everyday life and go someplace new — like a park, museum or cool local landmark you’ve been meaning to check out. Or just hop in your car and see where the day takes you ...