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- ...tric equation|parameterizes]] the energy [[Spectrum|spectra]] of primary [[cosmic ray]]s in the "knee" region (<math>10^{15}-10^{17}</math> eV) by the contin ...n|parametrized]] solutions of [[inverse problem]] to reconstruct primary [[cosmic ray]] energy spectra.<ref name=sam/><ref name="samo"> ...4 KB (573 words) - 10:14, 8 August 2022
- {{Short description|Cosmic stream of charged particles}} ...date=2016-09-28}}</ref> Because new stars and planets form from gases, the cosmic winds that push the gases away are preventing new stars from forming and ar ...5 KB (791 words) - 05:22, 17 November 2024
- ...nergy neutrinos are produced from interactions of utlra-high-energy cosmic rays, the observed rate of production of the latter places a limit on the former == Cosmic rays == ...16 KB (2,400 words) - 10:42, 10 February 2025
- ...etration, the m.w.e. provides a convenient and consistent way of comparing cosmic ray levels in different underground locations.<ref>{{cite web |url=http://w ...me="Grieder2001">{{cite book|first=Peter K. F. |last=Grieder |title=Cosmic Rays at Earth: Researcher's Reference Manual and Data Book |url=https://books.go ...6 KB (873 words) - 11:00, 10 February 2025
- ...his kind would be a third electron arriving on the 1s level. The emitted X-rays are detected by [[silicon drift detector]]s. [[File:Non-Paulian atomic tran ...e journal |last1=Bellini |first1=G.|display-authors=etal |year=2012 |title=Cosmic-muon flux and annual modulation in Borexino at 3800 m water-equivalent dept ...6 KB (774 words) - 01:05, 29 November 2023
- ...Bothe and Bruno Rossi: The birth and development of coincidence methods in cosmic-ray physics." Italian Association for the Teaching of Physics, ''arXiv'', 2 ...s]] or "vetos" are often used to filter common backgrounds, such as cosmic rays, from interacting with the primary detection medium. For instance, such a v ...14 KB (1,917 words) - 18:46, 6 August 2024
- ...dies measured intensity and composition of the nuclear component of cosmic rays at altitude 2000 meters above sea level in the energy range 100-300 GeV.<re ...8 KB (1,073 words) - 13:19, 9 November 2024
- ...eavy dark matter using diffuse backgrounds of neutrinos and cascaded gamma rays." ''Journal of Cosmology and Astroparticle Physics'' 2012, no. 10 (2012): 0 ...In general, indirect detection searches focus on either gamma-rays, cosmic-rays, or neutrinos.<ref name=":1" /> There are many instruments that have been u ...23 KB (3,587 words) - 11:13, 12 February 2025
- ...are [[volts]]. This definition is often utilised in the study of [[cosmic rays]], where the mass and charge of each particle is generally unknown. ...3 KB (424 words) - 18:39, 16 December 2024
- ...and global temperatures. As for the latter it was hypothesised that cosmic rays may impact cloud formation, therefore cloudiness, therefore global temperat ...8 KB (1,155 words) - 22:09, 2 January 2024
- {{Short description|Elliptical galaxy emitting very-high-energy gamma rays}} ...''') is a [[galaxy]] with a spectrum extending to the highest energy gamma rays.<ref name="Aharonian">{{cite journal|last=Aharonian|first=F. A.|author-link ...16 KB (2,295 words) - 01:47, 30 December 2024
- {{Short description|Cosmic ray acceleration mechanism}} ...n for [[ultra-high-energy cosmic ray]]s (UHECRs) and extreme-energy cosmic rays (EECRs) exceeding the [[Greisen–Zatsepin–Kuzmin limit]]. ...12 KB (1,654 words) - 05:24, 5 January 2025
- *'''[[Artem Alikhanian]]''', a prominent researcher of [[cosmic rays]], inventor of wide-gap track [[spark chamber]] ...Alikhanov]]''', [[nuclear physicist]], a prominent researcher of [[cosmic rays]], built the first [[nuclear reactor]]s in the [[USSR]], founder of [[Insti ...13 KB (1,753 words) - 19:51, 11 December 2024
- ...after the [[Big Bang]] and from more recent epochs. Observations of the [[cosmic microwave background]] and [[Big Bang nucleosynthesis]] studies have set co ...isotropies) in the [[cosmic microwave background]] (CMB), especially the [[Cosmic microwave background#Data reduction and analysis|second peak of the CMB pow ...20 KB (3,008 words) - 20:01, 5 January 2025
- ...10<sup>−4</sup> of the total. Further, the uniformly terrene nature of the cosmic ray flux indicates that nowhere in the Milky Way are there any sources of h * {{cite journal|title=Comet Kohoutek and Penetrating Rays|first=Vladimir|last=Rojansky|author-link=Vladimir Rojansky|journal=[[Physic ...19 KB (2,701 words) - 04:10, 17 November 2024
- ...y by taking samples from the interior that have not been exposed to cosmic rays, though the latter requires large samples.<ref>{{cite journal |last1=Kruije ...18 KB (2,464 words) - 06:59, 6 February 2025
- ...cretion disks]] are supported by [[magnetic field]]s, that [[extragalactic cosmic ray]]s are accelerated in them, and he estimates to within an order of magn ...6 KB (868 words) - 23:20, 21 September 2024
- '''Alpha particles''', also called '''alpha rays''' or '''alpha radiation''', consist of two [[proton]]s and two [[neutron]] ...and penetrate three times as far. The helium nuclei that form 10–12% of [[cosmic ray]]s are also usually of much higher energy than those produced by nuclea ...33 KB (4,877 words) - 10:36, 21 February 2025
- ...entified scalar force-carrier that is presumed to have physically caused [[cosmic inflation]]. |240 EeV cosmic ray ...16 KB (2,149 words) - 23:20, 3 February 2025
- ...ravity to act. However, the [[gas]] in star forming regions is heated by [[cosmic ray]]s and is cooled by radiative processes. The net result is that a gas i In this process, we can study the dynamics of the cosmic gas and understand the formation of stars. This is just one example. Even m ...11 KB (1,746 words) - 18:28, 6 August 2024