Zobrazeno 1 - 10
of 12
pro vyhledávání: '"M. V. K. Appa Rao"'
Autor:
George Joseph, M. V. K. Appa Rao, R. R. Daniel, R. U. Kundapurkar, S. V. Damle, G. S. Gokhale, P. J. Lavakare
Publikováno v:
Proceedings of the Indian Academy of Sciences Section C: Engineering Sciences. 1:313-319
A payload for the detection and measurement of high energy neutrons and gamma rays from the sun was flown onboard the first Indian satelliteAryabhata. The payload system for this neutron-gamma experiment was designed for detecting energetic neutrons
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::75e8abbb427e62e20917cc479840291f
https://doi.org/10.1007/bf02842879
https://doi.org/10.1007/bf02842879
Autor:
M. V. K. Appa Rao, S. Mitra
Publikováno v:
Proceedings of the Indian Academy of Sciences - Section A. 41:30-35
A K-meson is found to decay at rest into a nearly relativistic secondary particle. The secondary particle produces a nuclear disintegration in flight and is identified as a π-meson of kinetic energy ∼ 110 MeV. The event is interpreted as the decay
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5e2098d4edc06580fa658360b6a90ede
https://doi.org/10.1007/bf03050592
https://doi.org/10.1007/bf03050592
Autor:
P. J. Lavakare, M. V. K. Appa Rao
Publikováno v:
Il Nuovo Cimento. 26:740-747
An attempt has been made to determine the abundance of low-energy tritons and deuterons in a nuclear emulsion stack exposed at a geomagnetic latitude, λ =61° N on August 3, 1958 under 3.8 g/cm2 of matter. The grain density versus range method has b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1016fae09b1ab24fadd222ee2206efa2
https://doi.org/10.1007/bf02781799
https://doi.org/10.1007/bf02781799
Autor:
M. V. K. Appa Rao, M. F. Kaplon
Publikováno v:
Il Nuovo Cimento. 21:369-372
The maximum often observed at low energies in primary cosmic ray spectra is examined with respect to the possible effect of isotopic composition. It is shown that a maximum can arise if He/sup 3/ and He/sup 4/ are not distinguished and spectra are pl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c079f35a8f22e1d7b3e4dd553e49db05
https://doi.org/10.1007/bf02832562
https://doi.org/10.1007/bf02832562
The influence of ionization loss on the shape of the differential primary cosmic ray energy-spectrum
Autor:
M. V. K. Appa Rao, M. F. Kaplon
Publikováno v:
Il Nuovo Cimento. 27:700-717
The effect of ionization loss on a primary cosmic ray spectrum of the formN A, Z (e)=K(A, Z)γ/eγ+1 is calculated for1H,9Be,12C,19F,27Al,40Ca and56Fe as representative of the charge spectrum of primary cosmic rays. The calculation is carried out for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c9a266dc34dfb32a4bb0628d58c12cf7
https://doi.org/10.1007/bf02784575
https://doi.org/10.1007/bf02784575
Publikováno v:
Proceedings of the Indian Academy of Sciences - Section A. 43:181-201
A study of nuclear disintegrations caused by α-particles of primary cosmic radiation with energies > 5 BeV per nucleon, has been carried out. In a systematic survey in nuclear emulsions using ‘along the track’ scanning method, 479 α-particles w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::00f5dbccc5b89aae7f4473c64b6ee1da
https://doi.org/10.1007/bf03052778
https://doi.org/10.1007/bf03052778
Autor:
M. V. K. Appa Rao
Publikováno v:
Il Nuovo Cimento. 27:693-699
It is proposed that the characteristics of nuclear interactions of primary cosmic-ray nuclei (in-out interaction) be used to obtain the isotope abundance ratios for different charges. The applications of the procedure to singly and doubly charged nuc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5c69ff56cb282eb88613890e29150d5c
https://doi.org/10.1007/bf02784574
https://doi.org/10.1007/bf02784574
Autor:
M. V. K. Appa Rao
Publikováno v:
Il Nuovo Cimento. 32:1158-1165
The effect of spallation and ionization loss on the relative abundances and energy spectra of cosmic-ray nuclei of charge greater than two, during their propagation in the interstellar and interplanetary space, has been determined. Comparison of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::38da9c931afc29cf43bcc322a084b660
https://doi.org/10.1007/bf02726058
https://doi.org/10.1007/bf02726058
Autor:
M. V. K. Appa Rao, P. J. Lavakare
Publikováno v:
Il Nuovo Cimento. 29:321-325
Nuclear interactions produced in nuclear emulsions by douterons of mean energy 275 MeV have been studied. The mean free path for douterons of this energy is found to be (16.6 ±1.8) cm.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fac0e29b4b83471195c580ad385db2d7
https://doi.org/10.1007/bf02750354
https://doi.org/10.1007/bf02750354
Autor:
M. V. K. Appa Rao
Publikováno v:
Journal of Geophysical Research. 67:1289-1293
The ratio R = He3/(He3 + He4) is determined using a nuclear emulsion stack exposed at the geomagnetic latitude 61°N on August 3, 1958, under 3.8 g/cm2 of matter. The ratio R found at the top of the atmosphere is 0.31±0.08 for the same energy per nu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3db5beeaad2fbbc32e3f7f543a003f2e
https://doi.org/10.1029/jz067i004p01289
https://doi.org/10.1029/jz067i004p01289