Maisa Rojas
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Previous Organizations / Institutes
The organizations / institutes from the scholar's other articles in the past ten years
Research Subjects
Maisa Rojas has a total of 21 co-authors. Here are the top co-authors by number of shared publications:
- Patricio Iván Moreno
Departamento de Ciencias Ecológicas, Universidad de Chile, Santiago, Chile
2 shared publications - Ana Laura Berman
Centro de Investigaciones del Mar y la Atmósfera (CIMA), CONICET/UBA, Instituto Franco-Argentino de Estudios sobre el Clima y sus Impactos (IRL 3351 IFAECI/CNRS-CONICET-IRD-UBA), Buenos Aires, Argentina
1 shared publication Anji Seth
Department of Geography, University of Connecticut, Storrs, CT, USA
1 shared publication- Ayako Abe-Ouchi
Atmosphere and Ocean Research Institute, The University of Tokyo
1 shared publication Chris Hewitt
Met Office, Exeter, UK
1 shared publicationEsther C. Brady
Climate Change Research National Center for Atmospheric Research, Boulder, USA
1 shared publication
Latest Publications
- Open Access
- 19 August 2016
- Published by Copernicus GmbH in Climate of the Past
- Vol. 12 (8) , 1681-1691
The South American monsoon variability over the last millennium in climate models
In this paper we assess South American monsoon system (SAMS) variability in the last millennium as depicted by global coupled climate model simulations. High-resolution proxy records for the South American monsoon over this period show a coherent regional picture of a weak monsoon during the Medieval Climate Anomaly and a stronger monsoon during the Little Ice Age (LIA). Due to the small external forcing during the past 1000 years, model simulations do not show very strong temperature anomalies over these two specific periods, which in turn do not translate into clear precipitation anomalies, in contrast with the rainfall reconstructions in South America. Therefore, we used an ad hoc definition of these two periods for each model simulation in order to account for model-specific signals. Thereby, several coherent large-scale atmospheric circulation anomalies are identified. The models feature a stronger monsoon during the LIA associated with (i) an enhancement of the rising motion in the SAMS domain in austral summer; (ii) a stronger monsoon-related upper-tropospheric anticyclone; (iii) activation of the South American dipole, which results in a poleward shift of the South Atlantic Convergence Zone; and (iv) a weaker upper-level subtropical jet over South America. The diagnosed changes provide important insights into the mechanisms of these climate anomalies over South America during the past millennium.
- 19 August 2016
- Published by Copernicus GmbH in Climate of the Past
- Vol. 12 (8) , 1681-1691
Open AccessThe South American monsoon variability over the last millennium in climate models
In this paper we assess South American monsoon system (SAMS) variability in the last millennium as depicted by global coupled climate model simulations. High-resolution proxy records for the South American monsoon over this period show a coherent regional picture of a weak monsoon during the Medieval Climate Anomaly and a stronger monsoon during the Little Ice Age (LIA). Due to the small external forcing during the past 1000 years, model simulations do not show very strong temperature anomalies over these two specific periods, which in turn do not translate into clear precipitation anomalies, in contrast with the rainfall reconstructions in South America. Therefore, we used an ad hoc definition of these two periods for each model simulation in order to account for model-specific signals. Thereby, several coherent large-scale atmospheric circulation anomalies are identified. The models feature a stronger monsoon during the LIA associated with (i) an enhancement of the rising motion in the SAMS domain in austral summer; (ii) a stronger monsoon-related upper-tropospheric anticyclone; (iii) activation of the South American dipole, which results in a poleward shift of the South Atlantic Convergence Zone; and (iv) a weaker upper-level subtropical jet over South America. The diagnosed changes provide important insights into the mechanisms of these climate anomalies over South America during the past millennium.
- 19 March 2016
- Published by Springer Nature in Climate Dynamics
- Vol. 48 (1-2) , 387-404
Accelerated greenhouse gases versus slow insolation forcing induced climate changes in southern South America since the Mid-Holocene
- 19 March 2016
- Published by Springer Nature in Climate Dynamics
- Vol. 48 (1-2) , 387-404
Accelerated greenhouse gases versus slow insolation forcing induced climate changes in southern South America since the Mid-Holocene
- 30 June 2013
- Published by Springer Nature in Climate Dynamics
- Vol. 41 (3-4) , 551-571
Winter weather regimes over the Mediterranean region: their role for the regional climate and projected changes in the twenty-first century
- 30 June 2013
- Published by Springer Nature in Climate Dynamics
- Vol. 41 (3-4) , 551-571
Winter weather regimes over the Mediterranean region: their role for the regional climate and projected changes in the twenty-first century
- Open Access
- 27 January 2013
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 40 (5) , 965-970
Sensitivity of Southern Hemisphere circulation to LGM and 4 × CO2 climates
This paper investigates the effect of Last Glacial Maximum (LGM) versus high CO2 world boundary condition on the Southern Hemisphere atmospheric circulation, in particular on the strength and latitudinal position of the near surface Southern Westerly Winds (SWW). PMIP2 and PMIP3 experiments, as well as the “abrupt 4 × CO2” simulations from CMIP5, were analyzed. Robust findings include poleward expansion of the Mean Meridional Circulation (MMC) and intensified and poleward‐shifted SWW in the 4 × CO2 simulations (consistent with recent observations and 21st century climate change projections); and for the LGM, stronger and southward shifted northern hemisphere MMC, and weakened southern Hadley cell. However, six of the eight LGM simulations show a decrease in the SWW, the other two models simulate the opposite. A critical difference between the models is strong coupling between sea‐ice extent, surface temperature gradients, SWW, and Ferrel cell in the two models with stronger and poleward‐shifted SWW.
- 27 January 2013
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 40 (5) , 965-970
Open AccessSensitivity of Southern Hemisphere circulation to LGM and 4 × CO2 climates
This paper investigates the effect of Last Glacial Maximum (LGM) versus high CO2 world boundary condition on the Southern Hemisphere atmospheric circulation, in particular on the strength and latitudinal position of the near surface Southern Westerly Winds (SWW). PMIP2 and PMIP3 experiments, as well as the “abrupt 4 × CO2” simulations from CMIP5, were analyzed. Robust findings include poleward expansion of the Mean Meridional Circulation (MMC) and intensified and poleward‐shifted SWW in the 4 × CO2 simulations (consistent with recent observations and 21st century climate change projections); and for the LGM, stronger and southward shifted northern hemisphere MMC, and weakened southern Hadley cell. However, six of the eight LGM simulations show a decrease in the SWW, the other two models simulate the opposite. A critical difference between the models is strong coupling between sea‐ice extent, surface temperature gradients, SWW, and Ferrel cell in the two models with stronger and poleward‐shifted SWW.
- 24 June 2010
- Published by Springer Nature in Climate Dynamics
- Vol. 37 (1-2) , 357-375
Atmospheric circulation changes and neoglacial conditions in the Southern Hemisphere mid-latitudes: insights from PMIP2 simulations at 6 kyr
- 24 June 2010
- Published by Springer Nature in Climate Dynamics
- Vol. 37 (1-2) , 357-375
Atmospheric circulation changes and neoglacial conditions in the Southern Hemisphere mid-latitudes: insights from PMIP2 simulations at 6 kyr
- 3 June 2008
- Published by Springer Nature in Climate Dynamics
- Vol. 32 (4) , 525-548
The Southern Westerlies during the last glacial maximum in PMIP2 simulations
- 3 June 2008
- Published by Springer Nature in Climate Dynamics
- Vol. 32 (4) , 525-548
The Southern Westerlies during the last glacial maximum in PMIP2 simulations
- 27 June 2007
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research: Atmospheres
- Vol. 112 (D12)
Amplification of the 2‐day wave from mutual interaction of global Rossby‐gravity and local modes in the summer mesosphere
The 2‐day wave is a planetary‐scale wave recurrently observed in the summer mesosphere. It is predominantly zonal wave number 3 (though wave numbers 2 and 4 are also observed) and has a period of approximately 2 days. It is generally accepted that the 2‐day wave has characteristics of both global‐scale Rossby‐gravity normal mode and baroclinic/barotropic instability. Here we examine how local instability amplifies the global Rossby‐gravity mode. We perform a two‐dimensional instability calculation to calculate unstable modes. The fastest growing modes have wave number 3, a 35‐hour Rossby mode localized in the summer hemisphere at high latitudes, and a Rossby‐gravity mode with period 42 hours with similar characteristics to the observed 2‐day wave. The Rossby‐gravity mode was examined as the background state was changed from an isothermal atmosphere to realistic conditions. The wave was slowly Doppler shifted toward shorter periods and its spatial structure became distorted. Approaching realistic conditions the mode becomes weakly unstable. Near this point a localized Rossby mode also emerges which exists on the reversed potential vorticity gradients of the summer jet. This has the necessary characteristics to phase lock with the Rossby‐gravity mode. Hence we propose that the 2‐day wave amplifies from the interaction of global‐scale Rossby‐gravity and local modes. A nonlinear model was used to examine the unstable modes as they grow to finite amplitude. It was found that even though the 35‐hour Rossby wave had the largest growth rates, it did not reach large amplitude. It was the slower growing 42‐hour Rossby‐gravity mode which dominated the long time evolution.
- 27 June 2007
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research: Atmospheres
- Vol. 112 (D12)
Amplification of the 2‐day wave from mutual interaction of global Rossby‐gravity and local modes in the summer mesosphere
The 2‐day wave is a planetary‐scale wave recurrently observed in the summer mesosphere. It is predominantly zonal wave number 3 (though wave numbers 2 and 4 are also observed) and has a period of approximately 2 days. It is generally accepted that the 2‐day wave has characteristics of both global‐scale Rossby‐gravity normal mode and baroclinic/barotropic instability. Here we examine how local instability amplifies the global Rossby‐gravity mode. We perform a two‐dimensional instability calculation to calculate unstable modes. The fastest growing modes have wave number 3, a 35‐hour Rossby mode localized in the summer hemisphere at high latitudes, and a Rossby‐gravity mode with period 42 hours with similar characteristics to the observed 2‐day wave. The Rossby‐gravity mode was examined as the background state was changed from an isothermal atmosphere to realistic conditions. The wave was slowly Doppler shifted toward shorter periods and its spatial structure became distorted. Approaching realistic conditions the mode becomes weakly unstable. Near this point a localized Rossby mode also emerges which exists on the reversed potential vorticity gradients of the summer jet. This has the necessary characteristics to phase lock with the Rossby‐gravity mode. Hence we propose that the 2‐day wave amplifies from the interaction of global‐scale Rossby‐gravity and local modes. A nonlinear model was used to examine the unstable modes as they grow to finite amplitude. It was found that even though the 35‐hour Rossby wave had the largest growth rates, it did not reach large amplitude. It was the slower growing 42‐hour Rossby‐gravity mode which dominated the long time evolution.
- 1 August 2006
- Published by American Meteorological Society in Monthly Weather Review
- Vol. 134 (8) , 2208-2223
Multiply Nested Regional Climate Simulation for Southern South America: Sensitivity to Model Resolution
Results are reported from two 5-month-long simulations for southern South America using the fifth-generation Pennsylvania State University–NCAR Mesoscale Model (MM5). The periods of simulation correspond to May–September 1997 and 1998, which were anomalously wet and dry winters for central Chile, respectively. The model setup includes triply nested, two-way-interacting domains centered over the eastern South Pacific and the western coast of southern South America, with horizontal grid intervals of 135, 45, and 15 km. Boundary conditions are provided from NCEP–NCAR reanalyzed fields. The analysis focuses on two subregions of central Chile (30°–41°S). Region 1 (32°–35°S), which is where the observed interannual precipitation differences are largest, is topographically very complex, with a mean height of the Andes Cordillera around 4500 m. Region 2 (35°–39°S) has relatively smooth terrain, as the mean height of the Andes drops to 3000 m. Station precipitation and temperature data are used for model ... Abstract Results are reported from two 5-month-long simulations for southern South America using the fifth-generation Pennsylvania State University–NCAR Mesoscale Model (MM5). The periods of simulation correspond to May–September 1997 and 1998, which were anomalously wet and dry winters for central Chile, respectively. The model setup includes triply nested, two-way-interacting domains centered over the eastern South Pacific and the western coast of southern South America, with horizontal grid intervals of 135, 45, and 15 km. Boundary conditions are provided from NCEP–NCAR reanalyzed fields. The analysis focuses on two subregions of central Chile (30°–41°S). Region 1 (32°–35°S), which is where the observed interannual precipitation differences are largest, is topographically very complex, with a mean height of the Andes Cordillera around 4500 m. Region 2 (35°–39°S) has relatively smooth terrain, as the mean height of the Andes drops to 3000 m. Station precipitation and temperature data are used for model ...
- 1 August 2006
- Published by American Meteorological Society in Monthly Weather Review
- Vol. 134 (8) , 2208-2223
Multiply Nested Regional Climate Simulation for Southern South America: Sensitivity to Model Resolution
Results are reported from two 5-month-long simulations for southern South America using the fifth-generation Pennsylvania State University–NCAR Mesoscale Model (MM5). The periods of simulation correspond to May–September 1997 and 1998, which were anomalously wet and dry winters for central Chile, respectively. The model setup includes triply nested, two-way-interacting domains centered over the eastern South Pacific and the western coast of southern South America, with horizontal grid intervals of 135, 45, and 15 km. Boundary conditions are provided from NCEP–NCAR reanalyzed fields. The analysis focuses on two subregions of central Chile (30°–41°S). Region 1 (32°–35°S), which is where the observed interannual precipitation differences are largest, is topographically very complex, with a mean height of the Andes Cordillera around 4500 m. Region 2 (35°–39°S) has relatively smooth terrain, as the mean height of the Andes drops to 3000 m. Station precipitation and temperature data are used for model ... Abstract Results are reported from two 5-month-long simulations for southern South America using the fifth-generation Pennsylvania State University–NCAR Mesoscale Model (MM5). The periods of simulation correspond to May–September 1997 and 1998, which were anomalously wet and dry winters for central Chile, respectively. The model setup includes triply nested, two-way-interacting domains centered over the eastern South Pacific and the western coast of southern South America, with horizontal grid intervals of 135, 45, and 15 km. Boundary conditions are provided from NCEP–NCAR reanalyzed fields. The analysis focuses on two subregions of central Chile (30°–41°S). Region 1 (32°–35°S), which is where the observed interannual precipitation differences are largest, is topographically very complex, with a mean height of the Andes Cordillera around 4500 m. Region 2 (35°–39°S) has relatively smooth terrain, as the mean height of the Andes drops to 3000 m. Station precipitation and temperature data are used for model ...