Downward surface flux computations in a vertically inhomogeneous grey planetary atmosphere
Autor(a) principal: | |
---|---|
Data de Publicação: | 2008 |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Revista Brasileira de Meteorologia (Online) |
Texto Completo: | http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0102-77862008000100004 |
Resumo: | We describe an efficient computational scheme for downward surface flux computations in a vertically inhomogeneous grey planetary atmosphere for different values of solar zenith angle. We start with the basic equations of a recently developed discrete ordinates spectral nodal method, and we derive suitable bidirectional functions whose diffuse components do not depend on the solar zenith angle. We then make use of these bidirectional functions to construct an efficient scheme for computing the downward surface fluxes in a given model atmosphere for a number of solar zenith angles. We illustrate the merit of the computational scheme described here with downward surface flux computations in a three-layer grey model atmosphere for four values of solar zenith angle, and we conclude this article with general remarks and directions for future work. |
id |
SBMET-1_11019642d3b4a84d90125e1fb748f78c |
---|---|
oai_identifier_str |
oai:scielo:S0102-77862008000100004 |
network_acronym_str |
SBMET-1 |
network_name_str |
Revista Brasileira de Meteorologia (Online) |
repository_id_str |
|
spelling |
Downward surface flux computations in a vertically inhomogeneous grey planetary atmosphereatmospheric radiationdiscrete ordinatesspectral nodal methodbidirectional functionsradiative fluxcomputational efficiencyWe describe an efficient computational scheme for downward surface flux computations in a vertically inhomogeneous grey planetary atmosphere for different values of solar zenith angle. We start with the basic equations of a recently developed discrete ordinates spectral nodal method, and we derive suitable bidirectional functions whose diffuse components do not depend on the solar zenith angle. We then make use of these bidirectional functions to construct an efficient scheme for computing the downward surface fluxes in a given model atmosphere for a number of solar zenith angles. We illustrate the merit of the computational scheme described here with downward surface flux computations in a three-layer grey model atmosphere for four values of solar zenith angle, and we conclude this article with general remarks and directions for future work.Sociedade Brasileira de Meteorologia2008-03-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersiontext/htmlhttp://old.scielo.br/scielo.php?script=sci_arttext&pid=S0102-77862008000100004Revista Brasileira de Meteorologia v.23 n.1 2008reponame:Revista Brasileira de Meteorologia (Online)instname:Sociedade Brasileira de Meteorologia (SBMET)instacron:SBMET10.1590/S0102-77862008000100004info:eu-repo/semantics/openAccessAbreu,Marcos Pimenta deeng2008-04-18T00:00:00Zoai:scielo:S0102-77862008000100004Revistahttp://www.rbmet.org.br/port/index.phpONGhttps://old.scielo.br/oai/scielo-oai.php||rbmet@rbmet.org.br1982-43510102-7786opendoar:2008-04-18T00:00Revista Brasileira de Meteorologia (Online) - Sociedade Brasileira de Meteorologia (SBMET)false |
dc.title.none.fl_str_mv |
Downward surface flux computations in a vertically inhomogeneous grey planetary atmosphere |
title |
Downward surface flux computations in a vertically inhomogeneous grey planetary atmosphere |
spellingShingle |
Downward surface flux computations in a vertically inhomogeneous grey planetary atmosphere Abreu,Marcos Pimenta de atmospheric radiation discrete ordinates spectral nodal method bidirectional functions radiative flux computational efficiency |
title_short |
Downward surface flux computations in a vertically inhomogeneous grey planetary atmosphere |
title_full |
Downward surface flux computations in a vertically inhomogeneous grey planetary atmosphere |
title_fullStr |
Downward surface flux computations in a vertically inhomogeneous grey planetary atmosphere |
title_full_unstemmed |
Downward surface flux computations in a vertically inhomogeneous grey planetary atmosphere |
title_sort |
Downward surface flux computations in a vertically inhomogeneous grey planetary atmosphere |
author |
Abreu,Marcos Pimenta de |
author_facet |
Abreu,Marcos Pimenta de |
author_role |
author |
dc.contributor.author.fl_str_mv |
Abreu,Marcos Pimenta de |
dc.subject.por.fl_str_mv |
atmospheric radiation discrete ordinates spectral nodal method bidirectional functions radiative flux computational efficiency |
topic |
atmospheric radiation discrete ordinates spectral nodal method bidirectional functions radiative flux computational efficiency |
description |
We describe an efficient computational scheme for downward surface flux computations in a vertically inhomogeneous grey planetary atmosphere for different values of solar zenith angle. We start with the basic equations of a recently developed discrete ordinates spectral nodal method, and we derive suitable bidirectional functions whose diffuse components do not depend on the solar zenith angle. We then make use of these bidirectional functions to construct an efficient scheme for computing the downward surface fluxes in a given model atmosphere for a number of solar zenith angles. We illustrate the merit of the computational scheme described here with downward surface flux computations in a three-layer grey model atmosphere for four values of solar zenith angle, and we conclude this article with general remarks and directions for future work. |
publishDate |
2008 |
dc.date.none.fl_str_mv |
2008-03-01 |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0102-77862008000100004 |
url |
http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0102-77862008000100004 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
10.1590/S0102-77862008000100004 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
text/html |
dc.publisher.none.fl_str_mv |
Sociedade Brasileira de Meteorologia |
publisher.none.fl_str_mv |
Sociedade Brasileira de Meteorologia |
dc.source.none.fl_str_mv |
Revista Brasileira de Meteorologia v.23 n.1 2008 reponame:Revista Brasileira de Meteorologia (Online) instname:Sociedade Brasileira de Meteorologia (SBMET) instacron:SBMET |
instname_str |
Sociedade Brasileira de Meteorologia (SBMET) |
instacron_str |
SBMET |
institution |
SBMET |
reponame_str |
Revista Brasileira de Meteorologia (Online) |
collection |
Revista Brasileira de Meteorologia (Online) |
repository.name.fl_str_mv |
Revista Brasileira de Meteorologia (Online) - Sociedade Brasileira de Meteorologia (SBMET) |
repository.mail.fl_str_mv |
||rbmet@rbmet.org.br |
_version_ |
1752122083500883968 |