Survey of large zenith angle muon data at high energies

Flint, R.W.; Nash, W.F.

doi:10.1016/0550-3213(72)90573-1

Survey of large zenith angle muon data at high energies

R.W. Flint
(
- Nottingham U.
)
,
W.F. Nash
(
- Nottingham U.
)

1971

11 pages

Published in:

Nucl.Phys.B 33 (1971) 632-642,
Nucl.Phys.B 40 (1972) 607 (erratum)

Published: 1971

DOI:

View in:

OSTI Information Bridge Server

reference search5 citations

Citations per year

Abstract: (Elsevier)

This paper presents a survey of muon-spectrum charge-ratio measurements with large zenith angle sea level spectrometers and underground telescopes, with particular reference to results from the Nottingham spectrometer.

cosmic radiation
muon: energy spectrum
energy spectrum: muon
flux
correction
charge
pi: production
production: pi
hyperon: decay
decay: hyperon

References(25)

Figures(0)

[1]

Evidence for a New Production Process for 1012-eV Muons

- Phys.Rev.Lett. 19 (1967) 1487-1491
•
DOI:
- 10.1103/PhysRevLett.19.1487

[2]

J.W. Keuffel
,
J.L. Osborne
,
G.L. Bolingbroke
,
G.W. Mason
,
M.O. Larson

et al.

[3]

in press

R.W. Flint
,
W.F. Nash

[4]

F. Ashton
,
Y. Kamiya
,
P.I. MacKeown
,
J.L. Osborne
,
J.B.M. Pattison

et al.

- Proc.Phys.Soc. 87 (1966) 79

[5]

The momentum spectrum of muons at sea-level in the range 3–1000 GeV/c

- Nucl.Phys.B 4 (1968) 539-548
•
DOI:
- 10.1016/0550-3213(68)90112-0

[6]

in press

Y. Kamiya
,
S. Kawaguchi
,
Z. Fujii
,
S. Iida
,
K. Mitsui

[7]

Cosmic-ray muon spectra near 1000 gev at large zenith angles

- Nuovo Cim.B 66 (1970) 169-182
•
DOI:
- 10.1007/BF02710256

[8]

Cosmic ray muon intensities at 80 degrees to the zenith

N.S. Palmer
(
- Nottingham U.
)
,
W.F. Nash
(
- Nottingham U.
)

- Nucl.Phys.B 9 (1969) 315-323
•
DOI:
- 10.1016/0550-3213(69)90105-9

[9]

O.C. Allkofer
,
K. Carstensen
,
W.D. Dau
,
J. Fricke
,
W. Heinrich

et al.

[10]

Observations on the cosmic ray angular distribution underground at 1500 hg/cm 2 (Kolar) and the question of muon production in the TeV energy region

et al.

- Phys.Lett.B 27 (1968) 535-538
•
DOI:
- 10.1016/0370-2693(68)90217-7

[11]

C.T. Stockel

- J.Phys. AII (1969) 639

[12]

in press

W.R. Sheldon
,
W.G. Cantrell
,
N.M. Duller
,
F. Cambou
,
G. Vedrenne

et al.

[13]

Z. Fujii
,
S. Iida
,
Y. Kamiya
,
S. Kawaguchi
,
A. Takenaka

- Nuovo Cimento Letters Ser. I (1969) 845

[14]

Ph.D.Thesis

R.W. Flint

[15]

Ph.D.Thesis

P.K. MacKeown

[16]

N.S. Palmer
,
W.F. Nash

- Can.J.Phys. 46 (1968) 313

[17]

private communication

O.C. Allkofer

[18]

London

S. Kawaguchi
,
T. Sakai
,
H. Oda
,
H. Ueno
,
Y. Kamiya

- Proc.Int.Conf.on cosmic rays 2 (1965) 941

[19]

A.M. Aurela
,
P.K. MacKeown
,
A.W. Wolfendale

- Proc.Phys.Soc. 89 (1966) 401

[20]

Y. Kamiya
,
H. Ueno
,
S. Sagisaka
,
Y. Sekido

- Nuovo Cim. 30 (1963) 1

[21]

H. Kasha
,
C.B.J. Hawkins
,
J.R. Stefanski

- Can.J.Phys. 46 (1967) 306

[22]

in press

D. Alexander
,
M.G. Thompson

[23]

private communication

J.H. Parker

[24]

Proc. Int. Conf. on cosmic rays, Hungary, in press

R.W. Flint
,
W.F. Nash

[25]

B. Peters

- Nuovo Cim. 23 (1962) 88