2015
DOI: 10.1016/j.atmosenv.2015.01.048
|View full text |Cite
|
Sign up to set email alerts
|

Numerical simulation of the interaction between ammonium nitrate aerosol and convective boundary-layer dynamics

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

1
17
0

Year Published

2015
2015
2021
2021

Publication Types

Select...
7
1

Relationship

0
8

Authors

Journals

citations
Cited by 13 publications
(18 citation statements)
references
References 61 publications
1
17
0
Order By: Relevance
“…Figure 2 shows the burden of fine NO − 3 , NO − 3 on dust, NH + 4 , and NH 3 in AM3N. The simulated global burdens fall within the range of previous estimates (Bauer et al, 2007;Feng and Penner, 2007;Pye et al, 2009;Pringle et al, 2010;Bellouin et al, 2011;Xu and Penner, 2012;Hauglustaine et al, 2014) for fine NO − 3 (0.04-0.11 Tg N), NO − 3 on dust (0.07-0.41 Tg N), NH + 4 (0.21-0.27 Tg N), and NH 3 (0.07-0.29 Tg N). The burden of fine NO − 3 peaks over China where it reaches over 5 mg N m −2 , with a secondary maximum over India.…”
Section: Budget and Global Distributionsupporting
confidence: 70%
See 1 more Smart Citation
“…Figure 2 shows the burden of fine NO − 3 , NO − 3 on dust, NH + 4 , and NH 3 in AM3N. The simulated global burdens fall within the range of previous estimates (Bauer et al, 2007;Feng and Penner, 2007;Pye et al, 2009;Pringle et al, 2010;Bellouin et al, 2011;Xu and Penner, 2012;Hauglustaine et al, 2014) for fine NO − 3 (0.04-0.11 Tg N), NO − 3 on dust (0.07-0.41 Tg N), NH + 4 (0.21-0.27 Tg N), and NH 3 (0.07-0.29 Tg N). The burden of fine NO − 3 peaks over China where it reaches over 5 mg N m −2 , with a secondary maximum over India.…”
Section: Budget and Global Distributionsupporting
confidence: 70%
“…In AM3N, the dry deposition of NH 4 NO 3 is slow, similar to other fine aerosols. Several field observations have reported steeper vertical gradients and faster deposition velocities Huebert et al, 1988;Wyers and Duyzer, 1997;Van Oss et al, 1998;Rattray and Sievering, 2001;Nemitz et al, 2004;Fowler et al, 2009;Wolff et al, 2010;Barbaro et al, 2015). This difference stems from gradients in temperature, RH, and HNO 3 within the boundary layer, which reduce the stability of NH 4 NO 3 near the surface.…”
Section: Surface Removal Of Fine No −mentioning
confidence: 99%
“…Results also indicated that the model overestimated nitrate and ammonium and underestimated sulfate when SIA was relatively high. Positive biases of nitrate and ammonium were also found in other simulation studies (Fountoukis et al, 2011;Walker et al, 2012;Wang et al, 2013;Barbaro et al, 2015) which might be caused by the uncertainties in NO x emissions, •OH concentration, oxidation rate of NO 2 by •OH, removal rate of HNO 3 and under-predicted planet boundary layer (PBL) Pirovano et al, 2012;Walker et al, 2012). Table S2 of SI.…”
Section: Model Performancementioning
confidence: 74%
“…Figure shows the diurnal cycle of the O 3 , NO, and NO 2 mixing ratios for this particular day calculated with initial mixed‐layer and free‐tropospheric conditions and emission and deposition rates based on observations and previous research by Barbaro et al . []. The satisfactory agreement of modeled mixing ratios in combination with the ability of the model to represent the diurnal cycle of dynamics [ Van Heerwaarden et al ., ] gives enough confidence to use the fully coupled MXLCH model for more extensive studies.…”
Section: Methodsmentioning
confidence: 98%