|
Size: 96
Comment:
|
Size: 2449
Comment:
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 4: | Line 4: |
| === Nicole Meyer | === Nicole Meyer-Vernet PSULib QB529.M485 2007 === . [[ https://observatoiredeparis.psl.eu/ | Observatoire de Paris ]] and [[ https://en.wikipedia.org/wiki/French_National_Centre_for_Scientific_Research | Centre National de la Rechereche Scientifique ]] [[ https://www.cnrs.fr/fr | website ]] .p009 Sun: mass 1.98892e30 kg, radius 695700 km, Luminosity 3.828e26 W +/-0.1% .p054 plasmas interact less with radiation than with plasmas .p057 [[ https://en.wikipedia.org/wiki/Fermi_energy | Fermi energy ]] . book's "comet-like" heliosphere model [[ https://www.science.org/doi/10.1126/science.1181079 | obsolete ]] . [[ https://www.science.org/doi/10.1126/science.1181079 | Imaging the Interaction of the Heliosphere with the Interstellar Medium from Saturn with Cassini ]] .p057 [[ https://pmc.ncbi.nlm.nih.gov/articles/PMC9726803/pdf/11214_2022_Article_939.pdf | heliospheric dust grains ]] .p057 plasma particle collisional free path increases strongly with speed, fast particles nearly collisionless .p064 Magnetic mirrors: particle moving towards converging/increasing field mirrors and reflects .p066 transverse gradient produces a small transverse drift .p069 [[ https://en.wikipedia.org/wiki/Vlasov_equation | Vlasov equation ]] [[ https://en.wikipedia.org/wiki/Liouville's_theorem_(Hamiltonian) | Liouville's theorem ]] .p080 "upstream kinetic energy converted to downstream [[ https://en.wikipedia.org/wiki/Enthalpy | enthalpy ]], high temperature .p083 viscous forces generally much less important than inertial effects, but . see E. M. Purcell [[ https://www.damtp.cam.ac.uk/user/tong/fluids/lowreynolds.pdf | Life at low Reynolds number ]] Am. J. Phys. 45, 3–11 (1977) .p083 ions transport momentum, determining viscosity; electrons transport heat, determining thermal conductivity .p084 [[ | Reynolds number very large for space plasmas, viscosity generally negligable .p084 1e6 K (kelvin) solar corona heat conductivity 1e4 W/m-K "same order of magnitude as brass" . [[ https://www.researchgate.net/profile/Anastasia_Vasileiou2/publication/263155220/figure/fig4/AS:550876301492239@1508350553460/Brass-CuZn33-properties-as-a-function-of-temperature-a-thermal-conductivity-b_W640.jpg | NO, brass is around 150 1e4 W/m-K ]] [[ | ]] [[ | ]] [[ | ]] [[ | ]] [[ | ]] [[ | ]] [[ | ]] [[ | ]] |
http://wiki.keithl.com/SolarWind
Basics of the Solar Wind
Nicole Meyer-Vernet PSULib QB529.M485 2007
Observatoire de Paris and Centre National de la Rechereche Scientifique website
- p009 Sun: mass 1.98892e30 kg, radius 695700 km, Luminosity 3.828e26 W +/-0.1%
- p054 plasmas interact less with radiation than with plasmas
p057 Fermi energy
book's "comet-like" heliosphere model obsolete
Imaging the Interaction of the Heliosphere with the Interstellar Medium from Saturn with Cassini
- p057 plasma particle collisional free path increases strongly with speed, fast particles nearly collisionless
- p064 Magnetic mirrors: particle moving towards converging/increasing field mirrors and reflects
- p066 transverse gradient produces a small transverse drift
p080 "upstream kinetic energy converted to downstream enthalpy, high temperature
- p083 viscous forces generally much less important than inertial effects, but
see E. M. Purcell Life at low Reynolds number Am. J. Phys. 45, 3–11 (1977)
- p083 ions transport momentum, determining viscosity; electrons transport heat, determining thermal conductivity
- p084 [[ | Reynolds number very large for space plasmas, viscosity generally negligable
- p084 1e6 K (kelvin) solar corona heat conductivity 1e4 W/m-K "same order of magnitude as brass"
