![Page 1: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/1.jpg)
Review of direct measurements of cosmic rays
Sources of Galactic cosmic rays APC, Paris - December 7-9, 2016
![Page 2: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/2.jpg)
CR astrophуsics main problems
Sources ?
- Accelerators?
![Page 3: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/3.jpg)
The basic paradigm of CR acceleration
![Page 4: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/4.jpg)
Supernovae
1052 erg ! Energy balance
equation ( Ginzburg & Syrovatskii 1964)
~ 10% of SN kinetic energy
should go to cosmic rays
to maintain observed wcr
at Wsn=1051 erg, νsn = 1/(30 yr)
Ginzburg Syrovatskii
![Page 5: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/5.jpg)
SN 1987
Standard Model of Cosmic Ray Acceleration
Shock wave
Accelerated particles
Emax~BLZ ≈ 1014Z eV
Diffusive shock acceleration Fermi 1949, Krymsky 1977, Bell 1978,....
![Page 6: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/6.jpg)
LET’S FOLLOW THIS PARADIGM
AND FORGET (FOR A WHILE ) OTHERS ONES…
![Page 7: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/7.jpg)
Energy, eV
New component
F
lux
«The knee»
Fe
He
H
E
lgA
MEAN MASS
E~Z Emax~BLZ ≈ 10 14Z eV
Definition of average mass below “the knee” – the real test for current models
![Page 8: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/8.jpg)
Völk et al. magnetic field amplification in Tycho and other shell-type SNRs
very strong magnetic field in young SNRs is indirect but strong evidence of proton acceleration
Similar amplification in all other SNRs where such data are available: Cas A, SN 1006, Tycho, RCW 86, Kepler, RX J1713.7-3946, Vela Jr
shock profile in hard X-rays
diffusive shock acceleration of electrons, including
synchrotron losses gives observed scale
B ~ 300 µG, for Tycho’s SNR consistent with synchrotron spectrum from acceleration theory
Tycho’s SNR
Strong magnetic field in young SNRs
![Page 9: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/9.jpg)
SN 1987
Standard Model of Cosmic Ray Acceleration
Shock wave
Accelerated particles
Emax~BLZ ≈ 10 14Z eV
Diffusive shock acceleration Fermi 1949, Krymsky 1977, Bell 1978,....
17
![Page 10: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/10.jpg)
HE CR Balloons Satellites
HE CR on ground installations
Mostly, GCR can be measured using “off-ground” instruments: balloons&satellites
![Page 11: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/11.jpg)
«Proton» experiment : 1965 – 1966
Experimental instruments – ionization calorimeters were designed at Moscow State University
Proton 4
Proton 1-3
S. Vernov N. Grigorov
Эксперименты « Протон»
![Page 12: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/12.jpg)
«Proton 1-4»
«Proton’s» results
“Proton”: all particle from 10*11 till 10*15
eV
Up to now we had no such possibility!
.
Grigorov
4 orders
![Page 13: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/13.jpg)
The beginning of 21 century gave us
absolutely new results from CR experiments
![Page 14: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/14.jpg)
ATIC 2000-2007
![Page 15: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/15.jpg)
Proton and helium spectra: thin structure
Spectra for energy per particle
10 TeV
There is no single power law!
ATIC
H
He
![Page 16: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/16.jpg)
CREAM 2007 -2009
US + Korea
![Page 17: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/17.jpg)
CREAM-III has confirmed ATIC result
Y.S. Yoon et al. ICRC31 (2009, Lodz)
PROTONS
HELIUM
![Page 18: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/18.jpg)
In the middle of 2000’ : CR elemental composition
THE KNEE
Chemical composition in Multi-TeV energy region: ???
![Page 19: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/19.jpg)
PAMELA 2006
Pamela confirmed ATIC& CREAM data In comparison to the previous experiments PAMELA found the break position
![Page 20: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/20.jpg)
AMS-02 2012
![Page 21: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/21.jpg)
AMS-02 (ICRC2013): no slope’s change!
PAMELA PAMELA
AMS
AMS
H He
![Page 22: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/22.jpg)
During 2 years AMS team changed their conclusions
![Page 23: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/23.jpg)
AMS 02
Today:in TeV’s energy range spectra is changing
![Page 24: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/24.jpg)
The basic questions around “no-single - power spectrum”
1/ Is it specific source acceleration? 2/ Is it propagation effect? 3/ Is it effect of multiply sources of GCR?
SNR1 SNR2 SNR3
“interference of local (different)
sources”
![Page 25: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/25.jpg)
Based on the basic paradigm of CR acceleration we have to follow the conclusion that Diffusive Shock Acceleration produces the power law of
CR
![Page 26: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/26.jpg)
HEAVY NUCLEI BEFORE THE KNEE
Average mass definition below “the knee” – the real test for current models
![Page 27: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/27.jpg)
Average mass definition below “the knee” – the real test for current models
The knee
p
Fe
IRON KNEE ???
Panasyuk, 1998
![Page 28: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/28.jpg)
ICRC 2015: Heavier nuclei
Heavier elements energy dependence: HARDENING!
![Page 29: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/29.jpg)
On Dec., 26, 2014 satellite RESOURSE-P #2 was launched with NUCLEON instrument to study
chemical composition of high-energy galactic cosmic rays
Skobeltsyn Institute of Nuclear Physics of Lomonosov Moscow State University
Listen Podorozhnyi talk during this session!
![Page 30: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/30.jpg)
NUCLEON: THE FIRST RESULTS (2016)
Nucleon: multi-TeV energy range approaching
![Page 31: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/31.jpg)
Космические лучи.
Cosmic Rays
1015eV
1020
109 Since 2000 – ATIC CREAM PAMELA AMS 02 NUCLEON 2014 DAMPE 2015 CALET 2015 ISS CREAM 2017?
![Page 32: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/32.jpg)
Why is there such an interest in this energy range of GCR (1011- 1015 eV),
in spite of more than 50 years of research?
![Page 33: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/33.jpg)
The elemental composition of cosmic rays (till 2016)
Extragalactic component Galactic component Протоны The answer (1): Abnormal
behavior(non –consistent with the main paradigm)
of the elemental composition of cosmic rays
![Page 34: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/34.jpg)
The answer (2):
“Application of new nuclear-physical technologies in practice of the space experiment
allowed us to receive new PRECISION experimental information about the nuclear
composition of cosmic rays in terms of quality comparable to ground-based accelerator
experiments".
![Page 35: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/35.jpg)
Currently, direct measurements tend to higher energies , and indirect - to the lower ones. However statistics, below the knee is still not good enough to
draw final conclusions about the elemental composition near the knee.
CONCLUSION
This means that the mechanism of acceleration of cosmic rays in supernova remnants definitively
experimentally proven.
direct
indirect
![Page 36: Review of direct measurements of cosmic rayssemikoz/CosmicRays2016/Dec7/...Supernovae 1052 erg ! Energy balance equation ( Ginzburg & Syrovatskii 1964) ~ 10% of SN kinetic energy should](https://reader035.vdocuments.us/reader035/viewer/2022071405/60fa8a52ce71f35f236b95fe/html5/thumbnails/36.jpg)
Thank you