Measurements of cosmic-ray Li, Be and B nuclei in the energy range 100 Mev/nuc to greater than 22 Bev/nuc.
Cosmic ray Li, Be and B nuclei measurements, analyzing differential energy spectra, L-M ratio, atmospheric and solar modulation
Ormes, J. F.↗
Engineering topics
Ormes, J. F.
Publications and source records attributed to Ormes, J. F..
Proton and helium nuclei cosmic-ray spectra and modulations between 100 and 2000 Mev/nucleon.
Proton and He nuclei cosmic ray differential energy spectra, examining functional form of 11 year solar modulation
Ormes, J. F.↗
A method of measuring the cosmic ray charge composition between 10 super 10 and 10 super 14 ev.
Event collection, energy measurement and charge identification methods for measuring primary cosmic ray charge composition from Z equals one to 50
Balasubrahmanyan, V. K.↗
Cosmic-ray proton and helium spectra and solar modulation effects in the new solar cycle measured with a four-element counter telescope.
Primary cosmic ray proton and He energy spectra and solar modulation effects during sunspot minimum from balloon-borne scintillation counter telescope data
Ormes, J. F.↗
Proton and helium nuclei cosmic ray spectra and modulations between 100 and 2,000 MeV/nucleon
Combination Cerenkov and scintillation detector, and range scintillator for proton and helium nuclei cosmic ray spectra between 100 and 2000 MeV/nucleon
Ormes, J. F.↗
Cerenkov-scintillation counter measurements of nuclei heavier than helium in the primary cosmic radiation. I.
Energy spectra and charge composition of nuclei heavier than helium in primary cosmic radiation from Cerenkov scintillation counter measurements
Ormes, J. F.↗
An upper limit on the quiet time solar neutron flux at energies greater than 60 Mev.
New lower upper limit on solar neutron flux at energies greater than 60 mev for emission during quiet times
SOLAR RADIATION↗
Observations on nuclei heavier than iron in the primary by cosmic radiation.
Primary cosmic radiation abundance measurements on iron and heavier nuclei, using Cerenkov counter on balloon flights
CERENKOV COUNTER↗
Observations of nuclei heavier than iron in the primary cosmic radiation
Charge and energy spectra of primary cosmic rays made with large area Cerenkov scintillation counter on baloon flights - heavier than iron nuclei
SPECTRAL ENERGY DISTRIBUTION↗
An upper limit on the quiet time solar neutron flux at energies greater than 60 MeV
Upper limit on quiet time solar neutron flux at energies above 60 MeV determined by using balloon flights with Cerenkov scintillation counters
CERENKOV COUNTER↗
Measurements of the primary proton and helium spectra and their modulations using a balloon- borne Cerenkov-scintillation counter.
Balloon-borne Cerenkov scintillation counter for measurements of primary proton and helium spectra and modulations
CERENKOV COUNTER↗
Measurements of the energy spectrum of nuclei with Z greater than 3 in the primary radiation using a balloon borne Cerenkov-scintillation counter.
Balloon-borne Cerenkov scintillation counter measurements of energy spectra of primary cosmic radiation heavy nuclei at various geomagnetic latitudes
GEOMAGNETIC LATITUDE↗