Cosmic Ray Energetics and Mass (CREAM) is an experiment to determine the composition of cosmic rays up to the 1015 eV (also known as the "knee prospect")...

Moreover, scientific balloons (such as the one used in Cosmic Ray Energetics and Mass Experiment) and satellites (such as China's Dark Matter Particle Explorer...

Heliospheric Observatory Voyager 1 and Voyager 2 Advanced Thin Ionization Calorimeter BESS Cosmic Ray Energetics and Mass (CREAM) HEAT (High Energy Antimatter...

Calorimeter) TRACER (cosmic ray detector) BOOMERanG experiment TIGER [1] Archived 2012-05-03 at the Wayback Machine Cosmic Ray Energetics and Mass (CREAM) AESOP...

cosmic ray (UHECR) is a cosmic ray with an energy greater than 1 EeV (1018 electronvolts, approximately 0.16 joules), far beyond both the rest mass and...

Solar energetic particles (SEP), formerly known as solar cosmic rays, are high-energy, charged particles originating in the solar atmosphere and solar...

occur when cosmic rays hit the Earth's atmosphere, or possibly in the Large Hadron Collider at CERN. These theories are very speculative, and the creation...

Retrieved 4 December 2018. Messier, Doug (7 February 2017). "DLR to Launch Cosmic Greenhouses into Orbit". Parabolic Arc. Retrieved 9 February 2017. "Hiber...

China Dark Matter Experiment Cosmic Ray Energetics and Mass Experiment General antiparticle spectrometer GlueX The E and B Experiment VIP2 experiment...

due to their favorable energetics of formation, described by the Oddo–Harkins rule. The abundance of elements in the Sun and outer planets is similar...

(disambiguation) Crème de la crème (disambiguation) Cosmic Ray Energetics and Mass (CREAM), a series of cosmic ray experiments Slang term for ejaculate or ejaculation...

interactions with cosmic ray particles. Natural terrestrial sources that produce gamma rays include lightning strikes and terrestrial gamma-ray flashes, which...

The Oh-My-God particle was an ultra-high-energy cosmic ray detected on 15 October 1991 by the Fly's Eye camera in Dugway Proving Ground, Utah, United States...

J. N; Piran, T; Piran, T (2010). "The Collimation and Energetics of the Brightest Swift Gamma-Ray Bursts". The Astrophysical Journal. 711 (2): 641–654...

MeV. The sites where cosmic rays are accelerated are expected to produce neutrinos that are at least one million times more energetic, produced from turbulent...

(66 lb) Computer resources: 53 kg (117 lb) External payloads: Cosmic-Ray Energetics and Mass (CREAM): 1,258 kg (2,773 lb) SpaceX CRS-12 Launch of CRS-12...

ELM-ES and the HTV Transfer Pallet. i-SEEP2 - IVA-replaceable Small Exposed Experiment Platform 2 Exposed Facility Slot 11. CREAM – Cosmic Ray Energetics and...

energy per nucleon, from solar wind to galactic cosmic ray energies, with sensitivity and with charge and mass resolution much better than heretofore possible...

standards) mixture of ions, atoms, molecules, larger dust grains, cosmic rays, and (galactic) magnetic fields. The energy that occupies the same volume...

forming a cosmic web at scales on which entire galaxies appear like tiny particles. In the standard Lambda-CDM model of cosmology, the mass–energy content...

In gamma-ray astronomy, gamma-ray bursts (GRBs) are extremely energetic events occurring in distant galaxies which represent the brightest and most powerful...

wind while others arrive as cosmic rays. By trapping the solar wind, the magnetic field deflects those energetic particles and protects the atmosphere from...

constitute the secondary cosmic rays that are produced after primary cosmic rays interact with Earth's atmosphere. Gamma rays, X-rays, and the higher energy...

source of cosmic rays. They might also produce gravitational waves. The word supernova has the plural form supernovae (/-viː/) or supernovas and is often...

particles produced after cosmic rays interact with Earth's atmosphere, including muons, mesons, and positrons. Cosmic rays may also produce radioisotopes...

2013. Baade, Walter & Zwicky, Fritz (1934). "Remarks on Super-Novae and Cosmic Rays" (PDF). Physical Review. 46 (1): 76–77. Bibcode:1934PhRv...46...76B...

atmosphere. In either case, the ultimate aim is to find the mass and energy of the primary cosmic ray which created the shower. Surface detectors accomplish...

(see CPT symmetry). Antimatter occurs in natural processes like cosmic ray collisions and some types of radioactive decay, but only a tiny fraction of these...

The cosmic microwave background (CMB, CMBR), or relic radiation, is microwave radiation that fills all space in the observable universe. With a standard...

the first evidence of antimatter and was discovered when Anderson allowed cosmic rays to pass through a cloud chamber and a lead plate. A magnet surrounded...