Questions tagged [cosmic-rays]

Cosmic rays are highly energetic, charged particles (protons, alphas, electrons, etc, with energies ranging from $\sim10^9\text{ eV}$ to at least $10^{20}\text{ eV}$) from various galactic and extragalactic sources, that often interact with our atmosphere. Consider adding other tags to specify the origin you're interested in (i.e., solar or galactic).

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Could the observed GZK limit exceeding cosmic rays be due to hawking radiation?

In this question here, it was asked whether a black hole could emit protons with energies exceeding the GZK limit via Hawking radiation, the answer given was yes. So I ask, what proportion if observed ...
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How localised in space versus momentum are particles from the Sun?

In quantum mechanics, unbound states will tend to spread out in space over time according to the Shrodinger equation. So it seems to me there is a degree of freedom for "wild" particles (i.e....
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What’s the most energetic particles that can theoretically reach the earth?

In recent years several ultra high energy cosmic ray events are observed on Earth. These particles carry energies way beyond even the most powerful particle accelerators we can realistically build. ...
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Quantitatively, how much would radiation levels increase without the geomagnetic field?

Many, many popular science articles claim that if the Earth didn't have a magnetic field, then the much higher concentration of cosmic rays that reached the surface would cause health damage to humans....
tparker's user avatar
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Could a Relativistic Rocket convert the heat of Doppler shifted Cosmic Background Radiation into usable energy? [closed]

This page on mathdept.ucr.edu about relativistic rockets states: As you approach the speed of light you will be heading into an increasingly energetic and intense bombardment of cosmic rays and other ...
Ben Warner's user avatar
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Impact of distance from galactic centre on the value of energy in the cosmic ray spectrum where knee is observed?

This question is based on the recommendation and great explanation by @Kyle_Kanos. Is it known what causes the "knee" in the observed Cosmic Ray spectrum? Accepting the reason for the ...
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Shock when a supernova explodes

I have been reading that when supernovae explode, they produce (Shockwaves) which act as cosmic accelerators. I do not understand, what is meant with "shock" (partially because I do not ...
Mad's user avatar
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Understanding the graph of cosmic rays flux

This graph is to be found in various Articles, Papers, and websites. I am trying to understand, what the "y axis" represent. Are they refering to electromagnetic Flux ? What is this unit ...
Mad's user avatar
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Confusion in proper length and how to use the formula of contraction of length

Suppose a muon particle (imagine it does not decay) is moving towards earth with velocity $v=0.998c$ from point M. Distance between earth and point M is 10km. Now, I want find the distance covered by ...
Isteak Ahamed Imon's user avatar
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What exactly is the "Yield Function" of a neutron monitor?

I have been reading papers related to the theoretical computation of a neutron monitor count rate, which is defined as the integral of the "yield function" of the specific neutron monitor ...
Oscar Batalla Cruz's user avatar
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How does the local zenith angle evolve as a function of atmospheric vertical depth?

From Gaisser's Cosmic Rays and Particle Physics (ed. 2016). I know $\theta$ and I have the vertical depths $X_{v}$. I want to solve for $X$ via a simple trigonometric relation. However, theta evolves ...
Fred's user avatar
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How does cosmic rays influence aerosol growth?

I have read about aerosol formation increasing due to ionisation but unable to understand what actually goes into the process? Can someone please explain how cosmic rays help in aerosol formation? ...
25 Simran Tiwari's user avatar
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Cosmic ray GZK limit calculation: subtleties with four-vectors

I'm considering an ultra-relativistic cosmic proton colliding with a CMB photon, creating a neutral pion, as depicted by this equation: $$\tag{1} p + \gamma \rightarrow p + \pi. $$ This process is ...
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Energy and pressure relationship for cosmic rays [closed]

How to prove $E = 3P$ for cosmic rays? In other words $\gamma = \tfrac43$ for cosmic rays. Whereas for $\gamma=\tfrac53$ we have $E = \tfrac32 P$.
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How much energy does a cosmic ray lose before it hits a detector? [closed]

The origin of extremely high energy cosmic rays is still unclear, by my understanding. But say that they are produced by whatever local source does it: how much energy is lost to environmental effects ...
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Solar modulation of cosmic rays

Whilst studying cosmic rays (CRs) and the influence of the sun on the intensity of the CRs, I read that solar modulation mainly affects low-energy CR-particles. Could someone maybe explain to me why ...
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Source spectral index

Whilst studying the propagation of cosmic rays (CRs) through our galaxy, I was comparing simulated data to data measured by the Alpha Magnetic Spectrometer 02. I am studying the proton flux within CRs ...
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On "cosmic flux" units

I've trouble understanding the following graph, taken from Wikipedia: It's supposed to show the cosmic ray flux vs particle energy. I've never seen a "flux" written in these units... Why ${...
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Are there any plans for cosmic ray detectors as part of the new ARTEMIS program?

NASA's new Artemis program involves building several temporary waypoints around and on the moon. One of the side-bonuses for scientists is that this has opened a few new funding avenues for studying ...
honeste_vivere's user avatar
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How are the other components related?

Often, the tensor of diffusion of cosmic rays in the inner heliosphere is given in terms of $k_{\parallel}$ and $k_\perp$, the coefficients of diffusion along and perpendicular to the magnetic field. ...
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What energy range is considered as a "high-energy" or "low energy" cosmic ray?

I have been studying cosmic ray muons lately, and I'm having trouble with making sense of all the eV values. What is the approxamate range (in eV) for "high-energy" and "low energy"...
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What is wrong with my cloud chamber? [closed]

Ive been trying to make a cloud chamber for a few days. I seem to have gotten most of the way there, but cant quite see any tracks, only mist. Im using isopropanol with cooling from salted water ice ...
DFined's user avatar
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Why is interstellar cosmic radiation more energetic than radiation from our sun?

I just watched an interesting minidoc about cosmic radiation. The video, and other resources I've read afterward, explains that the most energetic cosmic radiation comes from supernovae and black ...
Pink Sweetener's user avatar
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Why is space radiation mainly positively charged? Where are all the electrons?

I've heard that space radiation is mainly, overwhelmingly positively charged. Wikipedia (Cosmic ray - Composition) says ...about 99% are the bare nuclei of well-known atoms (stripped of their ...
Tim Cooper's user avatar
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Measure cosmic ray pions and protons below surface of the Earth?

In my particle physics lecture, the prof asserted that apparently cosmic ray muons can still be measured 1km below the surface of the earth (e.g. in a mine). This led me to ask the following two ...
Philippe Knecht's user avatar
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What is the acceleration rate of a neutrino? [closed]

I understand that photons do not have acceleration because they are massless. But what about neutrinos, which have been proven to have mass due to oscillation? Let's assume a typical Solar neutrino ...
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Did Victor Hess discover cosmic rays directly, or muons with his gold-leaf electroscope?

Most histories just mention cosmic rays themselves, but I also read that cosmic rays themselves rarely make it far into Earth's atmosphere, and it is usually muons, (or tauons or electrons) detected ...
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How to check the particle rate of $1\ m^{-2}.s^{-1}$ at an energy of $10^{12}\ TeV$ from the "Swordy plot"? [duplicate]

On this web page, we see the so-called "swordy plot" https://www.quantamagazine.org/ultrahigh-energy-cosmic-rays-traced-to-hotspot-20150514/ At an energy of $10^{12}\ eV=1\ TeV$, we read ...
Mathieu Krisztian's user avatar
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What is the current status or resolution of Greisen–Zatsepin–Kuzmin (GZK) cosmic-ray paradox?

The Greisen–Zatsepin–Kuzmin limit (GZK limit) is a theoretical upper limit on the energy of cosmic ray protons traveling from other galaxies through the intergalactic medium to our galaxy. A number of ...
ann marie cœur's user avatar
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What happens to extra-galactic rays when they arrive at the solar system?

Quazars send baryons from other galaxies towards us which are deflected from by the local magnetosphere. The early solar system probably picked up many millions of extragalactic cosmic rays for every ...
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How do you convert between different units of particle flux?

Charts of particle flux tend to show the flux rate in units of particles per metre squared per second per steradian per MeV. I don't understand what the "per MeV" is referring to. How do I ...
joe_deniable's user avatar
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What happens when chemical elements are struck by cosmic rays?

When struck by cosmic rays, chemical elements in soils and rocks emit uniquely identifiable signatures of energy in the form of gamma rays. These data can help scientists look for geologically ...
DarkLumiere's user avatar
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Radiation and windows for building of a great project in a low Earth orbit: reference request or exercise as a ficticious need to build it

I know about the existence of certain windows for which it is more suitable to launch a probe for the exploration of a cellestial body in our Solar System (see the Wikipedia Launch window). I wondered ...
user250478's user avatar
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Could A Stray Radioactive Particle Collide With an Atom in a Human, Causing a Cascade?

I'm not thinking of even particles from a nuclear power-plant or man-made event. If a high-velocity highly-interacting particle made it through all the natural protections that keep life in a non-...
Taylor Blackstone's user avatar
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1 answer
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Why is the GZK cutoff at such high energies?

Why is the GZK cutoff at such high energies? The threshold energy for Compton scattering is 0.511 MeV. But the inverse Compton scattering has a very high energy threshold. For example in ...
flammmes's user avatar
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The net charge of Earth

Shouldn't the earth have an over all small positive net charge? Cosmic rays in the form of light or high energy particles can ionize atoms, when that happens the electron and the positive ion recoils ...
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How much higher is muon flux at Earth's poles?

https://futurism.com/make-a-cosmic-ray-detector-at-home-and-test-relativity-2 This article states that the Earth's magnetic field funnels incoming muons towards the magnetic poles. Quantitatively, ...
DJG's user avatar
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Why don't we see/feel charged particles, penetrating our brains/retina?

If we see tracks in bubble or Wilson chamber, it means that particles are everywhere and can leave tracks in gases and liquids. They can also penetrate concrete of the building levels in the lab. So ...
Dims's user avatar
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Energy distribution of incoming muons from cosmic rays

I believe there has been research done which provides data on the kinetic energies of muons which result from incoming cosmic rays. I'm looking for a graph of counts (vertical axis) vs. kinetic energy ...
DJG's user avatar
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Shouldn't cosmic rays slow down Earth's movement around the Sun?

Maybe a dumb question. Are cosmic rays slowing down earth's (or any planets) movement around the sun? To me it sounds like an analogy of moving a mass through air and being slowed down by the impact ...
rst's user avatar
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Why the geomagnetic field become stronger when solar wind is stronger?

The following description is from the webpage of Niels Bohr Institue's Former Centre for Ice and Climate The Earth reacts to the solar wind by increasing the strength of the shielding magnetic ...
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What affects the propagation of secondary cosmic rays?

Primary cosmic rays produce, upon entering the Earth's atmosphere, a whole load of secondary particles. These primary particles are necessarily stable particles such as protons, electrons, and ...
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Do space-borne cosmic ray experiments publish all-particle spectra?

I was trying to gather data to produce my own cosmic ray (CR) spectrum plot. I have relied on this very useful French database collecting past space-based CR measurements. If I try to insert the ...
cosimoNigro's user avatar
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Does an atom or proton (cosmic ray) get stretched when traveling through expanding space?

I have read this question: Why does space expansion not expand matter? I do understand that matter inside galaxies will not get stretched because inside galaxies, gravity dominates over dark energy. ...
Árpád Szendrei's user avatar
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1 answer
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Galactic or Extra-galactic Cosmic Rays?

If we want to show whether or not a specific Cosmic Ray particle is confined to our galaxy we must use the Larmor radius (relativistic version), $$r = \gamma \, \frac{ m c}{q B}$$ Considering a $10^...
LightningStrike's user avatar
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What exactly is delta-14C and why are there periodic plateaus in the delta-14C curve?

I downloaded the IntCal13, IntCal09, and IntCal04 datasets (parent site), and when I plotted the last 24k years was surprised to see a plateau or even reversal appear every ~5300 years. Apparently we ...
Livid's user avatar
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What is the difference between an interaction and a decay in particle physics?

While studying secondary cosmic rays, I have encountered sentences like: Charged pions and kaons can either initiate further interactions or decay. or Because of the low area density at large ...
Awais Mirza's user avatar
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Why are neutrino flavors equal to 1:1:1 after a long travel?

Neutrinos produced in the interaction of very high energy cosmic rays with the CMB are produced in the proportion $\nu_\mu:\nu_e:\nu_\tau=2:1:0$ because of the decays produced after the cosmic ray ...
Juanjo's user avatar
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A good reference on cosmic ray?

I am looking for a good reference on cosmic ray, both galactic and solar. Does anyone have any suggestion? I'm looking for a reference that covers the production and propagation of cosmic rays in a ...
2 votes
1 answer
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What are SEP events in this article?

I am studying this paper; at page 5 it says: The occurrence of SEP events with fluences larger than the saturation limit was estimated to be less tha n one per year for the period the LPF ...
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