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COSMIC RAY
Dr. Lev Pustil’nik
Geophysical Department of Tel Aviv University
Israel Cosmic Ray and Space Weather Center
1
Cosmic Ray 100-year history
Three faces of Cosmic Ray
Cosmic Ray as part of high energy particle
physics and high energy astrophysics
Cosmic Ray as Space Weather impact factor
(radiation, magnetic storms, …)
Cosmic Ray as Space Weather tool for diagnostic
of nearest space (solar wind, CME, and shock
waves; 3-D Heliosphere and jets; solar cosmic ray
from solar flares)
Cosmic Ray in Israel
2
What are Cosmic Rays?
• Corpuscular high energy emission (mostly protons and
nuclear) bombarded Earth from all directions
• Flux of CR is almost isotropy
• Flux of CR is almost constant in time
• Energy of CR are from 0.001 GeV up to 1011 GeV
• Main questions:
– Origin of cosmic ray and CR manifestation in space (synchrotron
radio emission, gamma ray, …)
– Propagation of cosmic ray from sources to the Earth
– CR impact on the Earth environment 3
Pre-history of CR discovery: CR and atmospheric
electricity
• First intimation – from William Gilbert (1600: “Magnet”), father of term
“electricity” and creator of electroscope - first equipment for quantitative
measurements of electricity.
• Discharge of electroscope in dry air – first unexpected fact!!!
• Answer – atmospheric electricity is result of any high energy emanation
what ionize atoms in atmosphere (ions and free electrons)
4
What does ionize atmosphere?
• Rentgen (1900) – discovery X-rays and its input
to ionization: accelerated e-=> target =>
secondary emission– “ray’s fever”
• Geitel (1900) – ionization of air has place in all
heights and location, on light and in darkness,
much stronger in grots an mines.
Discussion: what is the source? Natural
radioactivity or external radiation from space
•Marie Skłodowska-Curie (1899) – “radiation of
uranium and thorium is secondary emission caused
by rays, like to X-ray…. The possible source of this
radiation may be Sun”. After tests (absorption, day-
night) CR hypothesis of Uranium emission was
rejected – natural radioactivity! 1900 year –new era! 5
100 year of CR discovery (1912)
• Victor Hess (Nobel Prize 1936)
First attempt – 1911 – balloon 1,100 m – “no essential change” compared with ground level!
Second attempt (without oxygen tanks) during 7 expeditions up to h=5,350 m + included total
solar eclipse phase
Surprisingly, he found: 1) that the radiation levels increased with altitude from h=2 km, 2) it did not
depend on eclipse phase – non-solar origin – external space
Hess interpreted this result to mean that radiation is entering the atmosphere from above. He gave
this phenomenon the name “High Altitude Radiation", which later evolved to "Cosmic Rays" 6
CR tracks – Charles Wilson Chamber Camera –discover CR-
tracks (Nobel Prise 1927 with Arthur Compton)
Chamber camera for 10$ (CERN)
7
https://www.youtube.com/watch?v=SnKvtazt5So
8
CR today
• Definition – non-thermal (non-
Maxwell) part of particles population
with power spectrum.
• Source – explosions SuperNova and
solar flares
• Origin – acceleration in electrical
fields of turbulent current sheet and
magnetized shock waves.
• Universal power spectrum is
sequence of equilibrium between
acceleration and run-away (Fermi
acceleration) 9
Three Faces of Cosmic Rays
Vishnu
(the preserver/rajas)
Cosmic Ray as
diagnostic and
forecaster tools,
preserved from
dangerous space
weather storms
Trimurti (meaning ‘having three forms’)
Brahma (the creator/sattva)
Cosmic Ray as Particle Physics – Grand Unification Theory (GUT)
Shiva (the destroyer/tamas)
Cosmic Ray as Impact
Factor-destroyer of
technological,
economics and health
elements
10
Energy of Cosmic Rays and input in
Particle Physics
Accelerators
- CERN
Input of high energy CR ito
particle physics:
•Discovery in CR of
positrons (Cameron,
NobelPrize 1936), muons,
pions, hyperons,...
•Expected future result and
possibly Nobel Prize in CR
field – Pier Augre CR
observatory (J. Cronin – Nobel
Prizer 1980 – “violation CPT
symmetry” ) study CR
showers for particles energy
up to 1020 ev
Piere
Augre
CR
showers
collabora
tion
11
Two components of CR (Galaxy and solar)
12
Pierre Auger Cosmic Ray Observatory
• Prof. James Cronin (Nobel Prize 1980) and Alan Watson • Location – Pampa, Argentina.
• 1,600 water tanks that cover an enormous section of the Pampa and serve as
particle detectors. Each 3,000-gallon (12,000 liter) tank, separated from each of
its neighbors by 1.5 kilometers, is completely dark inside - except when
particles from a cosmic ray air shower pass through it. These energetic particles
are traveling faster than the speed of light in water when they reach the detector.
• Area -3,000 km2 = 60*60 km
• Energy of particles – up to 1019 ev – few events in year. 1020 – limit caused by
relic radio emission
13
Cosmic Ray as “Writing on the Wall” How does we obtain answer from “almost nothing”:(almost isotropy and
almost non-variable)?
Like to prophet Daniel on banquet hosted by king Belshazzar
…mene, mene, tekel,u parsi =מנא, מנא, תקל, ופרסי...
14
Cosmic Ray impacts on the Earth • Radiation impact on electronic equipment (up to loss of
satellites).
• Ionization of atmosphere with influence on weather and GPS
navigation
15
What is necessity of Space Weather Centers?
High price of space weather knowledge for space technology
1. Price of space technology (include space
stations) in 2013 is about 1000,000,000,000$
Only insurance claims is about 1 billion$/yearly
2. For example: 2014 year – more then
400 communication satellites provide above
2*109 users by mobile communication + GPS
As example of Space Weather impacts –
crash of SkyLab mission 25 m* 7 m with loss 600 millions $$
Impact 1- Satellites malfunction: Cosmic Rays
and magnetic storms generates malfunctions
(satellite’s anomalies) up to shut-down
17
Impact 1. Probability of satellite's malfunction in dependence of
protons flux for high altitude – high inclination satellites for
different energies of protons (10 MeV and 60 MeV|)
18
Impact 2: Cosmic rays influence on atmospheric processes
and global climate change Cosmic Ray and Cloudiness
19
Situation in the Maunder minimum: a) variation in
reconstructed solar irradiance from Lean et al. (1995); b)
variation in concentration from Beer et al. (1991); c)
reconstructed air surface temperature for the northern
hemisphere from Jones et al. (1998). According to
Swensmark (2000).
Impact 2. Cosmic Rays and ground
temperature for the northern
hemisphere
1. During Maunder Minimum cosmic ray
modulation (from Be10) correlate with
surface temperature in northern
hemisphere.
2. In opposite solar irradiation is very
stable and has not correlation with
surface temperature
20
Asymmetry in wheat prices during Maunder Minimum. White diamonds show prices averaged for three-year intervals centred on
moments of minimum CR intensity (maximum solar activity);
Black diamonds show the same for minimum solar activity. White and black triangles show prices at moments of minimum and maximum CR
intensity. 21
Impact 3. Atmospheric lightning - role of Cosmic Rays in
formation of breakthrough for electrical discharge’s
(lightnings) in the Earth’s atmosphere
1. Secondary CR electrons in atmospheric
avalanches of accelerated particles
initiate electrical discharge – lightning
(Gureveich et.al, 2000)
2. Without CR our Earth would not has
lightning!
Gurevich model’s maximal electric field
lead to discharge on different heights and
experimental results (L-lightning events)
22
Cosmic Ray in Israel
• Israel Cosmic Ray Observatory on the Mount Hermon organized
by Prof. Yuval Neeman and Prof Lev Dorman in 1998.
23
SPACE WEATHER and COSMIC RAYS –
factors of space influence on the Earth civilization 1. Radiation impact:
• safety of electronics and astronauts in
space;
• safety of crew and passengers in
high-altitude flights (cosmic rays).
2. Magnetosphere impact=“magnetic storms”:
• extra atmospheric drag of satellites and
space platform;
• failure of magnetic navigation and
altitude control;
• Electricity grids disruption by extra-currents
with global black-out on large territories;
• Telecommunication cable disruption.
3. Ionosphere impact:
• ionosphere currents and plasma bubbles
disturb GPS navigation and radio wave
communication (signal scintillation)
4. Atmospheric impact:
• disturbance of atmosphere by magnetic
storms;
• influence of cosmic ray on cloudiness
(precipitations) and on weather/climate
PARTICIPANTS and
EQUIPMENT
Israel Cosmic Ray and Space Weather
Center (ICRSWC) of Tel Aviv University
Prof. Lev. Dorman – Cosmic Rays
Geophysics and Planetary Sciences
Department (GPSD) of Tel Aviv University
Prof. Colin Price – Ionosphere
Research Department of Survey Of
Israel (SOI) - magnetometry group of
Dr. Boris Shirman – Magnetosphere
Departm. of Natural Science of Open
University (DNSOU)
Prof. Yoav Yair – Ionosphere
Wise Observatory of Tel Aviv University
(WOTAU) - ConCam meteors patrol
Prof. Noah Brosh – Meteors
Kinneret Limnological Laboratory (KLL)
team of Dr. Alon Rimmer - atmosphere
CR as tools for space weather diagnostic and
forecasting
26
4. FORECASTING OF EXPECTED FEP FLUXES AND
COMPARISON WITH OBSERVATIONS (2-nd CASE:
K(R, r) DEPENDS FROM DISTANCE TO THE SUN)
Fig. 2 . Calculation on line parameters , RK1 , RNo and forecasting
of total neutron intensity (time t is in minutes after 10.00 UT of September 29, 1989; curves – forecasting, circles – observed total neutron intensity) .
Fig. 2 . Calculation on line parameters , RK1 RK1 , RNo RNo and forecasting
of total neutron intensity (time t is in minutes after 10.00 UT of September 29, 1989; curves – forecasting, circles – observed total neutron intensity) .
27
28
Illustration of physical nature
of CR anisotropy formation in
result of scattering of galactic
CR on magnetic mirrors
before Coronal Mass Ejection
Above – scattering of GCR on
magnetic mirror, right –
manifestation of the scatters
particles as source of sporadic
anisotropy (x – dates, y –
asymptotic longitude.