Hapke parameters
The Hapke parameters are a set of parameters for an empirical model that is commonly used to describe the directional reflectance properties of the airless regolith surfaces of bodies in the solar system. The model has been developed by astronomer Bruce Hapke at the University of Pittsburgh. The parameters are: The Hapke parameters can be used to derive other albedo and scattering properties such as the geometric albedo, the phase integral, and the Bond albedo.
Wikipage redirect
Link from a Wikipage to another Wikipage
primaryTopic
Hapke parameters
The Hapke parameters are a set of parameters for an empirical model that is commonly used to describe the directional reflectance properties of the airless regolith surfaces of bodies in the solar system. The model has been developed by astronomer Bruce Hapke at the University of Pittsburgh. The parameters are: The Hapke parameters can be used to derive other albedo and scattering properties such as the geometric albedo, the phase integral, and the Bond albedo.
has abstract
The Hapke parameters are a set ...... integral, and the Bond albedo.
@en
哈普克參數(英語:Hapke parameters)是常用來 ...... 數。該組參數是由美國匹茲堡大學行星科學家布魯斯·哈普克提出。
@zh
Wikipage page ID
10,180,397
page length (characters) of wiki page
Wikipage revision ID
800,291,949
Link from a Wikipage to another Wikipage
comment
The Hapke parameters are a set ...... integral, and the Bond albedo.
@en
哈普克參數(英語:Hapke parameters)是常用來 ...... 數。該組參數是由美國匹茲堡大學行星科學家布魯斯·哈普克提出。
@zh
label
Hapke parameters
@en
哈普克參數
@zh