Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Longkang Dai"'
Publikováno v:
Earth and Planetary Physics, Vol 5, Iss 1, Pp 1-10 (2021)
Solar Wind (SW) electron precipitation is able to deposit a substantial amount of energy in the nightside Martian upper atmosphere, potentially exerting an influence on its thermal structure. This study serves as the first investigation of such an is
Externí odkaz:
https://doaj.org/article/a1a1a48853ce4911af89ad987f14d06d
Autor:
Hao Gu, Jun Cui, DanDan Niu, LongKang Dai, JianPing Huang, XiaoShu Wu, YongQiang Hao, Yong Wei
Publikováno v:
Earth and Planetary Physics, Vol 4, Iss 4, Pp 396-402 (2020)
Doubly charged positive ions (dications) are an important component of planetary ionospheres because of the large energy required for their formation. Observations of these ions are exceptionally difficult due to their low abundances; until now, only
Externí odkaz:
https://doaj.org/article/9d2d53dc9e1c4a52b9a251d4f4316e2a
Publikováno v:
Buildings, Vol 13, Iss 3, p 679 (2023)
Understanding the actual heating patterns of air-to-air heat pumps (AAHP) in rural areas is crucial for energy planning and clean-heating policy optimization. To explore the influence of outdoor climate change on occupants’ heating patterns when us
Externí odkaz:
https://doaj.org/article/c9b247cc51394a689f3b4708bf743931
Publikováno v:
Earth and Planetary Physics. 4:1-7
Doubly charged positive ions (dications) are an important component of planetary ionospheres because of the large energy required for their formation. Observations of these ions are exceptionally difficult due to their low abundances; until now, only
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ad45ddc380a5f18272b491fa132642c4
https://doi.org/10.26464/epp2020036
https://doi.org/10.26464/epp2020036
The current Venus climate is largely regulated by globally-covered concentrated sulfuric acid clouds from binary condensation of sulfuric acid (H2SO4) and water (H2O). To understand this complicated H2SO4-H2O gas-cloud system, previous theoretical st
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c97f424c4f8950c92843bd107e9ec87f
Publikováno v:
Earth and Planetary Physics.
Solar Wind (SW) electron precipitation is able to deposit a substantial amount of energy in the nightside Martian upper atmosphere, potentially exerting an influence on its thermal structure. This study serves as the first investigation of such an is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a0e92579bd67bca70c0a14904b2d8042
https://doi.org/10.26464/epp2021012
https://doi.org/10.26464/epp2021012
Publikováno v:
E3S Web of Conferences. 356:03002
Residents mainly set the temperature at the range of 25°C to 27°C under cooling conditions. However, they may feel uncomfortable after staying a period in a steady-temperature environment. To make themselves more comfortable, residents will change
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ba39197869537b1f5e64427f2a1f005d
https://doi.org/10.1051/e3sconf/202235603002
https://doi.org/10.1051/e3sconf/202235603002
Autor:
X. S. Wu, LongKang Dai, Y. ‐T. Cao, T. L. Zhang, Jun Cui, Zhaojin Rong, Yong Wei, Mingyu Wu, D.-D. Niu, H. Gu
Publikováno v:
The Astrophysical Journal. 909:108
In the absence of solar radiation, precipitating electrons from the solar wind (SW) are generally thought to be the dominant source of energy deposition in the nightside Martian upper atmosphere, creating a patchy ionosphere and possibly also affecti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8e425a1609ace2839f20ab13d4aaad03
https://doi.org/10.3847/1538-4357/abdbb0
https://doi.org/10.3847/1538-4357/abdbb0