Add to ORKGWe present a new time-dependent model of the interplanetary heavy ion environment and a new set of software based on this model to calculate energy deposit (LET) spectra and resulting single event upset rates. © 1994 IEE
The proposed model generalizes the differential D(E) and integral D(>E) spectra of galactic and a...
In spite of strong magnetic shielding by the geomagnetic field, small fractions (1-10%) of the total...
Using the Langley Research Center galactic osmic ray (GCR) transport computer code (HZETRN) and the ...
The Cosmic Ray Effects on MicroElectronics (CREME) model that is currently in use to estimate single...
The high-energy charged particles entering the Earth’s environment from interplanetary space have th...
We present Linear Energy Transfer (LET) spectra calculated for the 1990-1991 CRRES mission using the...
The effects of radiation environment in interplanetary space must be taken into account for spacecra...
The galactic cosmic rays (GCR) contain fully stripped nuclei, from Hydrogen to beyond the Iron group...
The physical processes affecting the dynamics of the Earth's particle radiation environment are revi...
Times for accumulation of chemically significant dosages on icy surfaces of Centaur, Kuiper Belt, an...
A probabilistic model of cumulative solar heavy ion energy and LET spectra is developed for spacecra...
Ionizing radiation is harmful to biological organisms and technological systems. In space, this radi...
Our solar system is bombarded by galactic cosmic rays (GCR). These consist of electrons and nearly a...
For future human missions to Mars, it is important to study the surface radiation environment during...
A model of solar energetic particles (SEP) has been developed and is applied to solar flares during ...
The proposed model generalizes the differential D(E) and integral D(>E) spectra of galactic and a...
In spite of strong magnetic shielding by the geomagnetic field, small fractions (1-10%) of the total...
Using the Langley Research Center galactic osmic ray (GCR) transport computer code (HZETRN) and the ...
The Cosmic Ray Effects on MicroElectronics (CREME) model that is currently in use to estimate single...
The high-energy charged particles entering the Earth’s environment from interplanetary space have th...
We present Linear Energy Transfer (LET) spectra calculated for the 1990-1991 CRRES mission using the...
The effects of radiation environment in interplanetary space must be taken into account for spacecra...
The galactic cosmic rays (GCR) contain fully stripped nuclei, from Hydrogen to beyond the Iron group...
The physical processes affecting the dynamics of the Earth's particle radiation environment are revi...
Times for accumulation of chemically significant dosages on icy surfaces of Centaur, Kuiper Belt, an...
A probabilistic model of cumulative solar heavy ion energy and LET spectra is developed for spacecra...
Ionizing radiation is harmful to biological organisms and technological systems. In space, this radi...
Our solar system is bombarded by galactic cosmic rays (GCR). These consist of electrons and nearly a...
For future human missions to Mars, it is important to study the surface radiation environment during...
A model of solar energetic particles (SEP) has been developed and is applied to solar flares during ...
The proposed model generalizes the differential D(E) and integral D(>E) spectra of galactic and a...
In spite of strong magnetic shielding by the geomagnetic field, small fractions (1-10%) of the total...
Using the Langley Research Center galactic osmic ray (GCR) transport computer code (HZETRN) and the ...