Your English writing platform
Discover LudwigExact(60)
Figure 6: Stellar wind model predictions for ξ1 CMa.
The winds so derived are compared with HWM07 wind model.
The calculated winds has been compared with HWM14 wind model.
Gravitational spreading of the umbrella cloud dominates tephra transport only within the first hundred kilometres due to strong stratospheric winds in our best-fit wind model.
These findings are consistent with the 'disk wind' model, in which the outflowing gas is launched by an extended disk wind from a Keplerian disk.
These wind features have similar patterns to those of the empirical HWM93 wind model.
In this paper we present the calculation of secondary antiproton spectrum in the Galactic Wind model.
Neutral wind simulations of present model agree well with those of horizontal wind model (HWM-93).
In this paper we present an application of the reduced basis method to a local high definition adjusted wind model.
Based on the external wind conditions, a new turbulent cyclone wind model is created with the associated load case(s).
This wind model was developed to explain entirely other phenomena: the narrow and broad quasar absorption lines (NALs and BALs).
Write better and faster with AI suggestions while staying true to your unique style.
Since I tried Ludwig back in 2017, I have been constantly using it in both editing and translation. Ever since, I suggest it to my translators at ProSciEditing.

Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com