cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.6084/m9.figshare.10250825.v1
title: Optimizing the recovery of disrupted single-sourced multi-echelon assembly supply chain networks

description: We consider optimization problems related to the scheduling of Multi-Echelon Assembly Supply Chain (MEASC) networks that find application in the recovery from large-scale disruptive events. Each manufacturer within this network assembles a component from a series of sub-components received from other manufacturers and, due to high qualification standards, each sub-component of the manufacturer is single-sourced. Our motivating industries for this problem are defense aircraft and biopharmaceutical manufacturing. We develop scheduling decision rules that are applied locally at each manufacturer and are proven to optimize two industry-relevant <i>global</i> recovery metrics: (i) minimizing the maximum tardiness of any order of the final product of the MEASC network, and (ii) and minimizing the time to recover from the disruptive event. Our approaches are applied to a data set based on an industrial partner’s supply chain to show their applicability as well as their advantages over Integer Programming (IP) models. The developed decision rules are proven to be optimal, faster, and more robust than the equivalent IP formulations. In addition, they provide conditions under which local manufacturer decisions will lead to globally optimal recovery efforts. These decision rules can help managers to make better production and shipping decisions to optimize the recovery after disruptions and quantitatively test the impact of different pre-event mitigation strategies against potential disruptions. They can be further useful in MEASCs with or expecting a large amount of backorders.
DOI: 10.6084/m9.figshare.10250819.v1
title: Dataset for: Hidden Markov random field models applied to color homogeneity evaluation in dyed textiles images

description: Color is one of the most important features in any textile material. Due to its competitive price, most of the colorants currently used for textile dyeing are synthetic, originated from non-renewable sources and highly pollutant. There is an increasing interest for natural processes to dye fabrics. When new textile dyeing technologies are developed, evaluating the quality of these techniques involves measuring the resulting color homogeneity using digital images. The presence of a texture effect, caused by the interlacing of warp and weft yarns as well as small displacement of the fabric, creates a sophisticated dependence structure in pixels coloring. A random effects model is emplyed in order to separate the signal from the dyeing effect (fixed effect described by smooth functions) and warp and weft texture effect (Gaussian mixture driven by a hidden Markov random field), allowing an evaluation of color homogeneity in dyed textiles regardless of the effect of the texture.
DOI: 10.6084/m9.figshare.10250816
title: Global sourcing decisions for a multinational firm with foreign tax credit planning

description: Various countries’ tax laws adopt certain forms of a so-called worldwide tax system which levy taxes on their countries’ multinational firms’ global incomes at home country tax rates. To avoid double taxation, they permit tax cross-crediting, i.e., a global firm can use excess foreign tax credits (the portion of foreign tax payments that exceed its home country tax liabilities) generated from a subsidiary (located in a high-tax country) to offset the tax obligations from another subsidiary (located in a low-tax country). This article studies a multinational firm’s global sourcing decisions at two subsidiaries located in low- and high-tax countries, respectively, with an objective of maximizing its expected worldwide after-tax profit. We characterize the optimal sourcing decisions under various decentralized and centralized after-tax profit-maximizing performance measures. We show that the global firm can devise an easily implementable incentive scheme to optimally coordinate the decentralized sourcing decisions made at the two subsidiaries. We also demonstrate that decentralized policies with after-tax performance measures are more advantageous than the traditional pretax policies when the “tax effects”, i.e., the impacts of certain features of the tax laws (such as tax cross-crediting) on supply chain decisions, are significant.
DOI: 10.25380/iastate.10250774
title: Glucocorticoid effects on mucosal microbiota in healthy dogs and dogs with IBD

description: Raw data for ileal and colonic mucosal bacterial counts by bacterial FISH probe in healthy dogs and in IBD dogs following treatment with glucocorticoids.The mucosal microbiota from endoscopic biopsies of inflammatory bowel disease (IBD) dogs (n=8) and healthy controls (HC; n=15 dogs) was evaluated by fluorescence in situ hybridization (FISH) targeting the 16S rRNA genes of total bacteria and bacterial species using a seven probe array. We also used immunohistochemical (IHC) techniques to evaluate the impact of steroid therapy on mucosal apical junction protein (AJP) expression in dogs with IBD.
DOI: 10.6084/m9.figshare.10250816.v1
title: Global sourcing decisions for a multinational firm with foreign tax credit planning

description: Various countries’ tax laws adopt certain forms of a so-called worldwide tax system which levy taxes on their countries’ multinational firms’ global incomes at home country tax rates. To avoid double taxation, they permit tax cross-crediting, i.e., a global firm can use excess foreign tax credits (the portion of foreign tax payments that exceed its home country tax liabilities) generated from a subsidiary (located in a high-tax country) to offset the tax obligations from another subsidiary (located in a low-tax country). This article studies a multinational firm’s global sourcing decisions at two subsidiaries located in low- and high-tax countries, respectively, with an objective of maximizing its expected worldwide after-tax profit. We characterize the optimal sourcing decisions under various decentralized and centralized after-tax profit-maximizing performance measures. We show that the global firm can devise an easily implementable incentive scheme to optimally coordinate the decentralized sourcing decisions made at the two subsidiaries. We also demonstrate that decentralized policies with after-tax performance measures are more advantageous than the traditional pretax policies when the “tax effects”, i.e., the impacts of certain features of the tax laws (such as tax cross-crediting) on supply chain decisions, are significant.
DOI: 10.25380/iastate.10250774.v1
title: Glucocorticoid effects on mucosal microbiota in healthy dogs and dogs with IBD

description: Raw data for ileal and colonic mucosal bacterial counts by bacterial FISH probe in healthy dogs and in IBD dogs following treatment with glucocorticoids.The mucosal microbiota from endoscopic biopsies of inflammatory bowel disease (IBD) dogs (n=8) and healthy controls (HC; n=15 dogs) was evaluated by fluorescence in situ hybridization (FISH) targeting the 16S rRNA genes of total bacteria and bacterial species using a seven probe array. We also used immunohistochemical (IHC) techniques to evaluate the impact of steroid therapy on mucosal apical junction protein (AJP) expression in dogs with IBD.
DOI: 10.6084/m9.figshare.10250699
title: D15_DDA_components_gridA.txt: MarsWRF-predicted dust devil activity and contributing variables as a function of time of sol, averaged over four seasons for the first three Mars years of the MSL mission, now using vertical grid A.

description: Renno et al. [1998] dust devil activity and contributing variables at the Curiosity Rover’s location, averaged over 90° of Ls (i.e., in each of four seasons) in the first three years of the mission, as a function of time of sol.<br><br>All variables are predicted using output from a MarsWRF simulation of the atmosphere over Gale Crater, but now using vertical Grid A (see paper referenced below for details).<br><br>These data are used to produce Figure S8 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon.<br>In the data file:Periods 1-4 refer to periods spanning 90∞ of Ls, centered on Ls=180, 270, 0 and 90 in MSL yr 1<br>Periods 5-8 refer to the same but in MSL yr 2<br>Periods 9-12 refer to the same but in MSL yr 3<br><br>ToD = local true solar time in hours <br>RHO = air density in kg/m3 <br>UST = drag velocity, u*, in m/s <br>TDF = surface temperature minus air temperature at 1.5m, in K <br>PDF = surface pressure minus pressure at top of planetary boundary layer in Pa <br>OMB = vertical thermodynamic efficiency <br>HFX = sensible heat flux in W/m2 <br>DDA = dust devil activity[see paper for more description of the last 3 variables]<br><br>
DOI: 10.6084/m9.figshare.10250690
title: D14_REMS_Pdrops_CENmethod_UsedInFigS6.txt: Measured vortex pressure drops over the first three years of the MSL mission using another method.

description: Binned pressure drops measured by the Rover Environmental Monitoring Station (REMS) over the first three Mars years of the Mars Science Laboratory (MSL) Curiosity Rover mission, using the secondary method described in the Supplementary Material of “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon.<br>These data are used to produce Figure S6 in that paper.<br><br>Periods 1-4 refer to periods spanning 90° of Ls, centered on Ls=180, 270, 0 and 90 in MSL yr 1<br>Periods 5-8 refer to the same but in MSL yr 2<br>Periods 9-12 refer to the same but in MSL yr 3<br><br>Pdrop bins are (1) 0.5-0.8Pa; (2) 0.8-1.4Pa; (3) 1.4-2.6Pa; (4) 2.6-5.5Pa<br><br>REMS Pdrop (#) is the inferred number of pressure drops in that bin per hour<br><br><br><br>
DOI: 10.6084/m9.figshare.10250693
title: Statistical approaches in surface finishing. Part 3. Design-of-experiments

description: This paper is the third and final part of a short series of articles aimed towards describing some of the various statistical methods and approaches that have been used in surface finishing. Here, various types of Design-of-Experiments (DOE) techniques are described, such as full and fractional factorial design, central composite design, response surface methodology and Taguchi methods. Their application in the design of surface finishing related experiments are then reviewed, ending with a worked example of a two-level 2<sup>4</sup> full factorial DOE.
DOI: 10.6084/m9.figshare.10250690.v1
title: D14_REMS_Pdrops_CENmethod_UsedInFigS6.txt: Measured vortex pressure drops over the first three years of the MSL mission using another method.

description: Binned pressure drops measured by the Rover Environmental Monitoring Station (REMS) over the first three Mars years of the Mars Science Laboratory (MSL) Curiosity Rover mission, using the secondary method described in the Supplementary Material of “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon.<br>These data are used to produce Figure S6 in that paper.<br><br>Periods 1-4 refer to periods spanning 90° of Ls, centered on Ls=180, 270, 0 and 90 in MSL yr 1<br>Periods 5-8 refer to the same but in MSL yr 2<br>Periods 9-12 refer to the same but in MSL yr 3<br><br>Pdrop bins are (1) 0.5-0.8Pa; (2) 0.8-1.4Pa; (3) 1.4-2.6Pa; (4) 2.6-5.5Pa<br><br>REMS Pdrop (#) is the inferred number of pressure drops in that bin per hour<br><br><br><br>
DOI: 10.6084/m9.figshare.10250699.v1
title: D15_DDA_components_gridA.txt: MarsWRF-predicted dust devil activity and contributing variables as a function of time of sol, averaged over four seasons for the first three Mars years of the MSL mission, now using vertical grid A.

description: Renno et al. [1998] dust devil activity and contributing variables at the Curiosity Rover’s location, averaged over 90° of Ls (i.e., in each of four seasons) in the first three years of the mission, as a function of time of sol.<br><br>All variables are predicted using output from a MarsWRF simulation of the atmosphere over Gale Crater, but now using vertical Grid A (see paper referenced below for details).<br><br>These data are used to produce Figure S8 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon.<br>In the data file:Periods 1-4 refer to periods spanning 90∞ of Ls, centered on Ls=180, 270, 0 and 90 in MSL yr 1<br>Periods 5-8 refer to the same but in MSL yr 2<br>Periods 9-12 refer to the same but in MSL yr 3<br><br>ToD = local true solar time in hours <br>RHO = air density in kg/m3 <br>UST = drag velocity, u*, in m/s <br>TDF = surface temperature minus air temperature at 1.5m, in K <br>PDF = surface pressure minus pressure at top of planetary boundary layer in Pa <br>OMB = vertical thermodynamic efficiency <br>HFX = sensible heat flux in W/m2 <br>DDA = dust devil activity[see paper for more description of the last 3 variables]<br><br>
DOI: 10.6084/m9.figshare.10250681
title: D13_MarsWRF_MSLddac3yrs_gridA.txt: MarsWRF-predicted dust devil activity along MSL's traverse over 3 Mars years, now using vertical grid A.

description: Mean DDA is the Renno et al. [1998] dust devil activity at the Curiosity Rover’s location, averaged over 90° of Ls for the given period, at the time of sol shown (LTST = local true solar time). <br><br>DDA is predicted using output from a MarsWRF simulation of the atmosphere over Gale Crater, now using vertical Grid A [see paper referenced below for details].<br><br>These data are used to produce Figure 12 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br><br>
DOI: 10.6084/m9.figshare.10250633
title: D12_DDA_components.txt: MarsWRF-predicted dust devil activity and contributing variables as a function of time of sol, averaged over four seasons for the first three Mars years of the MSL mission.

description: Renno et al. [1998] dust devil activity and contributing variables at the Curiosity Rover’s location, averaged over 90° of Ls (i.e., in each of four seasons) in the first three years of the mission, as a function of time of sol.<br><br>All variables are predicted using output from a MarsWRF simulation of the atmosphere over Gale Crater.<br><br>These data are used to produce Figure 10 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon.<br>In the data file:Periods 1-4 refer to periods spanning 90∞ of Ls, centered on Ls=180, 270, 0 and 90 in MSL yr 1<br>Periods 5-8 refer to the same but in MSL yr 2<br>Periods 9-12 refer to the same but in MSL yr 3<br><br>ToD = local true solar time in hours <br>RHO = air density in kg/m3 <br>UST = drag velocity, u*, in m/s <br>TDF = surface temperature minus air temperature at 1.5m, in K <br>PDF = surface pressure minus pressure at top of planetary boundary layer in Pa <br>OMB = vertical thermodynamic efficiency <br>HFX = sensible heat flux in W/m2 <br>DDA = dust devil activity[see paper for more description of the last 3 variables]<br><br>
DOI: 10.6084/m9.figshare.10250693.v1
title: Statistical approaches in surface finishing. Part 3. Design-of-experiments

description: This paper is the third and final part of a short series of articles aimed towards describing some of the various statistical methods and approaches that have been used in surface finishing. Here, various types of Design-of-Experiments (DOE) techniques are described, such as full and fractional factorial design, central composite design, response surface methodology and Taguchi methods. Their application in the design of surface finishing related experiments are then reviewed, ending with a worked example of a two-level 2<sup>4</sup> full factorial DOE.
DOI: 10.6084/m9.figshare.10250573
title: D11_DDs_sol_1_to_sol_1975_.txt: Measured vortex pressure drops over the first three years of the MSL mission.

description: List of pressure drops measured by the Rover Environmental Monitoring Station (REMS) over the first three Mars years of the Mars Science Laboratory (MSL) Curiosity Rover mission, using the primary method described in “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon.<br>These data are used to produce Figures 9, 11 and 12 in that paper.<br><br>MSL sol = sol of the mission<br>Ls = areocentric solar longitudeLMST = local mean solar time <br>LTST = local true solar time <br>Ps drop = drop in surface pressure <br>FWHM duration = duration of pressure drop in terms of its full width at half maximum <br><br>
DOI: 10.6084/m9.figshare.10250633.v1
title: D12_DDA_components.txt: MarsWRF-predicted dust devil activity and contributing variables as a function of time of sol, averaged over four seasons for the first three Mars years of the MSL mission.

description: Renno et al. [1998] dust devil activity and contributing variables at the Curiosity Rover’s location, averaged over 90° of Ls (i.e., in each of four seasons) in the first three years of the mission, as a function of time of sol.<br><br>All variables are predicted using output from a MarsWRF simulation of the atmosphere over Gale Crater.<br><br>These data are used to produce Figure 10 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon.<br>In the data file:Periods 1-4 refer to periods spanning 90∞ of Ls, centered on Ls=180, 270, 0 and 90 in MSL yr 1<br>Periods 5-8 refer to the same but in MSL yr 2<br>Periods 9-12 refer to the same but in MSL yr 3<br><br>ToD = local true solar time in hours <br>RHO = air density in kg/m3 <br>UST = drag velocity, u*, in m/s <br>TDF = surface temperature minus air temperature at 1.5m, in K <br>PDF = surface pressure minus pressure at top of planetary boundary layer in Pa <br>OMB = vertical thermodynamic efficiency <br>HFX = sensible heat flux in W/m2 <br>DDA = dust devil activity[see paper for more description of the last 3 variables]<br><br>
DOI: 10.6084/m9.figshare.10250567
title: D10_MarsWRF_MSLddac3yrs_gridB.txt: MarsWRF-predicted dust devil activity along MSL's traverse over 3 Mars years.

description: Mean DDA is the Renno et al. [1998] dust devil activity at the Curiosity Rover’s location, averaged over 90° of Ls for the given period, at the time of sol shown (LTST = local true solar time). <br><br>DDA is predicted using output from a MarsWRF simulation of the atmosphere over Gale Crater.<br>These data are used to produce Figures 9 and 11 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br><br>
DOI: 10.6084/m9.figshare.10250567.v2
title: D10_MarsWRF_MSLddac3yrs_gridB.txt: MarsWRF-predicted dust devil activity along MSL's traverse over 3 Mars years.

description: Mean DDA is the Renno et al. [1998] dust devil activity at the Curiosity Rover’s location, averaged over 90° of Ls for the given period, at the time of sol shown (LTST = local true solar time). <br><br>DDA is predicted using output from a MarsWRF simulation of the atmosphere over Gale Crater.<br>These data are used to produce Figures 9 and 11 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br><br>
DOI: 10.6084/m9.figshare.10250573.v1
title: D11_DDs_sol_1_to_sol_1975_.txt:

description: List of pressure drops measured by the Rover Environmental Monitoring Station (REMS) over the first three Mars years of the Mars Science Laboratory (MSL) Curiosity Rover mission, using the primary method described in “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon.<br>These data are used to produce Figures 9, 11 and 12 in that paper.<br><br>MSL sol = sol of the mission<br>Ls = areocentric solar longitudeLMST = local mean solar time <br>LTST = local true solar time <br>Ps drop = drop in surface pressure <br>FWHM duration = duration of pressure drop in terms of its full width at half maximum <br><br>
DOI: 10.6084/m9.figshare.10250567.v1
title: MarsWRF-predicted dust devil activity along MSL's traverse over 3 Mars years.

description: Mean DDA is the Renno et al. [1998] dust devil activity at the Curiosity Rover’s location, averaged over 90° of Ls for the given period, at the time of sol shown (LTST = local true solar time). <br><br>DDA is predicted using output from a MarsWRF simulation of the atmosphere over Gale Crater.<br>These data are used to produce Figures 9 and 11 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br><br>
DOI: 10.6084/m9.figshare.10250441
title: D8_2pm_winds_d05.txt: MarsWRF-predicted 2pm winds at 1.5m altitude for southern summer solstice in a domain covering Gale Crater.

description: <br>This file provides 2pm zonal and meridional winds averaged over 7 sols at southern summer solstice (Ls~270°) for a region covering Gale Crater, output from domain 5 of a MarsWRF simulation.<br><br>Variables included are: Lon (longitude in deg E), Lat (latitude in deg N), U (zonal wind in m/s), V (meridional wind in m/s). Every second domain 4 wind output is included.<br><br>These data are used to produce Figure 6 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br>
DOI: 10.6084/m9.figshare.10250435
title: D7_2pm_winds_d04.txt: MarsWRF-predicted 2pm winds at 1.5m altitude for southern summer solstice in a domain 9 times bigger than Gale Crater.

description: This file provides 2pm zonal and meridional winds averaged over 7 sols at southern summer solstice (Ls~270°) for a region centered on but 9 times larger than Gale Crater, output from domain 4 of a MarsWRF simulation.<br><br>Variables included are: Lon (longitude in deg E), Lat (latitude in deg N), U (zonal wind in m/s), V (meridional wind in m/s). Every second domain 4 wind output is included.<br><br>These data are used to produce Figure 6 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br>