Measuring Direct and Return Albedo Proton Fluxes in the PAMELA Experiment

2021 ◽  
Vol 85 (4) ◽  
pp. 350-352
Author(s):  
O. A. Golub ◽  
A. G. Mayorov
Keyword(s):  
Pamela Experiment ◽  
Proton Fluxes

scholarly journals Proton Fluxes Measured by the PAMELA Experiment from the Minimum to the Maximum Solar Activity for Solar Cycle 24

2018 ◽  
Vol 854 (1) ◽  
pp. L2 ◽  
Author(s):  
M. Martucci ◽  
R. Munini ◽  
M. Boezio ◽  
V. Di Felice ◽  
O. Adriani ◽  
...  
Keyword(s):  
Solar Activity ◽  
Solar Cycle ◽  
Pamela Experiment ◽  
Proton Fluxes ◽  
Solar Cycle 24 ◽  
Cycle 24 ◽  
Maximum Solar Activity

scholarly journals TRAPPED PROTON FLUXES AT LOW EARTH ORBITS MEASURED BY THE PAMELA EXPERIMENT

2015 ◽  
Vol 799 (1) ◽  
pp. L4 ◽  
Author(s):  
O. Adriani ◽  
G. C. Barbarino ◽  
G. A. Bazilevskaya ◽  
R. Bellotti ◽  
M. Boezio ◽  
...  
Keyword(s):  
Pamela Experiment ◽  
Proton Fluxes ◽  
Low Earth Orbits ◽  
Earth Orbits

scholarly journals Reentrant albedo proton fluxes measured by the PAMELA experiment

2015 ◽  
Vol 120 (5) ◽  
pp. 3728-3738 ◽  
Author(s):  
O. Adriani ◽  
G. C. Barbarino ◽  
G. A. Bazilevskaya ◽  
R. Bellotti ◽  
M. Boezio ◽  
...  
Keyword(s):  
Pamela Experiment ◽  
Proton Fluxes

Detection and Prediction of Absorbed Radiation Doses from Solar Proton Fluxes onboard Orbital Stations

2004 ◽  
Vol 42 (3) ◽  
pp. 203-209 ◽  
Author(s):  
N. V. Kuznetsov ◽  
R. A. Nymmik ◽  
M. I. Panasyuk ◽  
E. N. Sosnovets ◽  
M. V. Teltsov
Keyword(s):  
Solar Proton ◽  
Radiation Doses ◽  
Proton Fluxes

scholarly journals Excitation And Ionization By Auroral Protons

1966 ◽  
Vol 19 (3) ◽  
pp. 309 ◽  
Keyword(s):  
Magnetic Field ◽  
Energy Range ◽  
Pitch Angle ◽  
Proton Energy ◽  
Ionization Rate ◽  
Energy Spectra ◽  
Proton Fluxes ◽  
Atmospheric Ionization ◽  
The Magnetic Field

Height distributions are presented for the atmospheric ionization rate and Balmer radiation resulting from precipitation of auroral protons. These results have been computed assuming proton fluxes with several different energy spectra and pitch-angle distributions about the magnetic field, the total proton energy range being restricted to 1-1000 keY.

scholarly journals Variation of Proton Flux with Atmospheric Depth Between 10 and 50 g/cm2 at l = 47° S. Geomagnetic

1965 ◽  
Vol 18 (1) ◽  
pp. 59 ◽  
Author(s):  
KKM Wu ◽  
BSK Chow
Keyword(s):  
Proton Flux ◽  
Atmospheric Depth ◽  
Nuclear Emulsions ◽  
Proton Fluxes

Proton fluxes at atmospheric depths between 10 and 50 g/cm2 have been measured using nuclear emulsions during a series of balloon flights over Melbourne (A = 47� S. geomagnetic) in the period November 1961-April 1962. The proton flux J(x) decreases with increasing depth within this region. It can be represented by the relation log J(x) = (3�05�0�02)-(2�36�0�66)xlO-3x and, when extrapolated, gives the flux at the top of the atmosphere to be 1120�50 protons m-2 steradian-1 S-l.

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