Construct · 1 fields · 1 citations

Parker transport equation: a standalone construct

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Space physics

the equation for energetic particle transport in the heliosphere combining diffusion, convection with the solar wind, drifts and adiabatic energy change.

In space physics, Parker transport equation refers to the equation for energetic particle transport in the heliosphere combining diffusion, convection with the solar wind, drifts and adiabatic energy change. This meaning comes from Parker (1965) in Planetary and Space Science.[1]

Unit
Recovery means
Measured by

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Nearby constructs

convection3 fields · 3 citationsinvariant · one construct, three systems diffusion6 fields · 12 citationsjingle · one name, six constructs energy5 fields · 10 citationsjingle · one word, five constructs

References

Parker, E. N. (1965). The passage of energetic charged particles through interplanetary space. Planetary and Space Science, 13(1), 9-49. https://doi.org/10.1016/0032-0633(65)90131-5

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