Melagen University

Learn about risks of radiation and how to shield your space assets.

Melagen University

Learn about risks of radiation and how to shield your space assets.

Melagen University

Learn about risks of radiation and how to shield your space assets.

Glossary

Total Ionizing Dose

TID

Total Ionizing Dose (TID) is the cumulative energy deposited by ionizing radiation in a material over time, expressed in units of rads or grays (1 rad = 0.01 Gy = 0.01 J/kg). In spacecraft engineering, TID is typically measured in krad(Si), where the reference is silicon, the bas

Single-Event Effects

SEE

Single-Event Effects (SEEs) are instantaneous, localized disruptions in an electronic device caused by a single energetic particle strike. Unlike Total Ionizing Dose (TID), which accumulates slowly over time, SEEs are probabilistic and can occur at any moment once a particle depo

Displacement Damage

DD

Displacement Damage (DD) refers to the physical disruption of a semiconductor’s crystal lattice caused by energetic particles, primarily protons, neutrons, and high-energy heavy ions. Unlike Total Ionizing Dose (TID), which is driven by trapped charge in oxides, displacement dama

Non-Ionizing Energy Loss

NIEL

Non-Ionizing Energy Loss (NIEL) describes the portion of a particle’s energy deposition that goes into displacing atoms in a solid rather than ionizing it. It is the primary figure of merit used to quantify displacement damage (DD) in semiconductors.

Linear Energy Transfer

LET

Linear Energy Transfer (LET) is a measure of the amount of energy an ionizing particle deposits per unit path length as it travels through matter. It is typically expressed in MeV·cm²/mg.

Solar Particle Events

SPE

Solar Particle Events (SPEs) are bursts of high-energy protons and heavier ions released during solar flares and coronal mass ejections (CMEs). Unlike the steady background of trapped radiation or galactic cosmic rays, SPEs are episodic but intense, delivering large doses of radi

Galactic Cosmic Rays

GCR

Galactic Cosmic Rays (GCRs) are high-energy charged particles—primarily protons (\~85%), helium nuclei (\~14%), and a small fraction of heavy ions—originating from outside the solar system, accelerated by supernovae and other astrophysical phenomena.

Van Allen Radiation Belts

VAB

The Van Allen Belts are zones of trapped charged particles (protons and electrons) held in place by Earth’s magnetic field. They form two primary regions and are among the most hazardous environments for satellites orbiting near Earth.

Dose Rate Effects and ELDRS

ELDRS

Dose rate effects describe how the rate at which radiation is delivered influences the severity of damage in electronic devices. While Total Ionizing Dose (TID) usually depends only on the integrated dose, certain devices—especially bipolar transistors—show greater degradation at

Cumulative vs. Stochastic Radiation Effects

Radiation effects in space electronics can be broadly divided into cumulative effects—which build up predictably over time—and stochastic (or single-event) effects, which occur randomly and suddenly when an individual particle strike disrupts device operation.

Reach out to learn more

We work closely with our customers to design and build purpose-specific radiation shield solutions for your exact mission parameters and requirements.


We want to ensure you have the radiation protection you need for enhanced mission success.

Reach out to learn more

We work closely with our customers to design and build purpose-specific radiation shield solutions for your exact mission parameters and requirements.


We want to ensure you have the radiation protection you need for enhanced mission success.

Reach out to learn more

We work closely with our customers to design and build purpose-specific radiation shield solutions for your exact mission parameters and requirements.


We want to ensure you have the radiation protection you need for enhanced mission success.