Struct nyx_space::dynamics::solarpressure::SolarPressure [−][src]
pub struct SolarPressure { pub phi: f64, pub e_loc: EclipseLocator, }
Expand description
Computation of solar radiation pressure is based on STK: http://help.agi.com/stk/index.htm#gator/eq-solar.htm .
Fields
phi: f64
solar flux at 1 AU, in W/m^2
e_loc: EclipseLocator
Implementations
Will set the solar flux at 1 AU to: Phi = 1367.0
Accounts for the shadowing of only one body and will set the solar flux at 1 AU to: Phi = 1367.0
Trait Implementations
Defines the equations of motion for this force model from the provided osculating state.
Force models must implement their partials, although those will only be called if the propagation requires the
computation of the STM. The osc_ctx
is the osculating context, i.e. it changes for each sub-step of the integrator. Read more
Auto Trait Implementations
impl !RefUnwindSafe for SolarPressure
impl Send for SolarPressure
impl Sync for SolarPressure
impl Unpin for SolarPressure
impl !UnwindSafe for SolarPressure
Blanket Implementations
Mutably borrows from an owned value. Read more
type Output = T
type Output = T
Should always be Self
The inverse inclusion map: attempts to construct self
from the equivalent element of its
superset. Read more
pub fn is_in_subset(&self) -> bool
pub fn is_in_subset(&self) -> bool
Checks if self
is actually part of its subset T
(and can be converted to it).
pub fn to_subset_unchecked(&self) -> SS
pub fn to_subset_unchecked(&self) -> SS
Use with care! Same as self.to_subset
but without any property checks. Always succeeds.
pub fn from_subset(element: &SS) -> SP
pub fn from_subset(element: &SS) -> SP
The inclusion map: converts self
to the equivalent element of its superset.
pub fn vzip(self) -> V