climatic responses
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2021 ◽  
Vol 932 (1) ◽  
pp. 012003
Author(s):  
E A Kurbanov ◽  
O N Vorobev ◽  
S A Lezhnin ◽  
D M Dergunov ◽  
Y Wang

Abstract This study assesses whether MODIS NDVI satellite data time series can be used to detect changes in forest phenology over the different forest types of the Mari El Republic of Russia. Due to the severe climatic conditions, coniferous and deciduous forests of this region are especially vulnerable to climate change, which can lead to stresses from droughts and increase the frequency of wild fires in the long term. Time series analysis was applied to 16-day composite MODIS (MOD13Q1) (250 m) satellite data records (2000-2020) for the investigated territory, based on understanding that the NDVI trend vectors would enable detection of phenological changes in forest cover. There was also the determination of land cover/land use change for the area and examination of meteorological data for the investigated period. For the study, we utilized four phenological metrics: start of season (SOS), end of season (EOS), length of season (LOS), and Maximum vegetation index (MVI). The NDVI MODIS data series were smoothed in the TimeSAT software using the Savitsky-Golay filter. The results of the study show that over the 20-years period variations in phenological metrics do not have a significant impact on the productivity and growth of forest ecosystems in the Mari El Republic.


Universe ◽  
2021 ◽  
Vol 7 (2) ◽  
pp. 36
Author(s):  
Xinhua Zhao ◽  
Willie Soon ◽  
Victor M. Velasco Herrera

The solar impact on Earth’s climate is both a rich and open-ended topic with intense debates. In this study, we use the reconstructed data available to investigate periodicities of solar variability (i.e., variations of sunspot numbers) and temperature changes (10 sites spread all over the Earth) as well as the statistical inter-relations between them on the millennial scale during the past 8640 years (BC 6755–AD 1885) before the modern industrial era. We find that the variations of the Earth’s temperatures show evidence for the Eddy cycle component, i.e., the 1000-year cyclicity, which was discovered in variations of sunspot numbers and believed to be an intrinsic periodicity of solar variability. Further wavelet time-frequency analysis demonstrates that the co-variation between the millennium cycle components of solar variability and the temperature change held stable and statistically strong for five out of these 10 sites during our study interval. In addition, the Earth’s climatic response to solar forcing could be different region-by-region, and the temperatures in the southern hemisphere seemed to have an opposite changing trend compared to those in the northern hemisphere on this millennial scale. These findings reveal not only a pronounced but also a complex relationship between solar variability and climatic change on Earth on the millennial timescale. More data are needed to further verify these preliminary results in the future.


2021 ◽  
Vol 12 (1) ◽  
Author(s):  
Nicola Maher ◽  
Scott B. Power ◽  
Jochem Marotzke

AbstractSeparating how model-to-model differences in the forced response (UMD) and internal variability (UIV) contribute to the uncertainty in climate projections is important, but challenging. Reducing UMD increases confidence in projections, while UIV characterises the range of possible futures that might occur purely by chance. Separating these uncertainties is limited in traditional multi-model ensembles because most models have only a small number of realisations; furthermore, some models are not independent. Here, we use six largely independent single model initial-condition large ensembles to separate the contributions of UMD and UIV in projecting 21st-century changes of temperature, precipitation, and their temporal variability under strong forcing (RCP8.5). We provide a method that produces similar results using traditional multi-model archives. While UMD is larger than UIV for both temperature and precipitation changes, UIV is larger than UMD for the changes in temporal variability of both temperature and precipitation, between 20° and 80° latitude in both hemispheres. Over large regions and for all variables considered here except temporal temperature variability, models agree on the sign of the forced response whereas they disagree widely on the magnitude. Our separation method can readily be extended to other climate variables.


2020 ◽  
Vol 64 ◽  
pp. 125763
Author(s):  
V.V. Kukarskih ◽  
N.M. Devi ◽  
A.Y. Surkov ◽  
M.O. Bubnov ◽  
L.A. Gorlanova ◽  
...  

2020 ◽  
Vol 474 ◽  
pp. 118351
Author(s):  
Rafael Zas ◽  
Roberto Touza ◽  
Luis Sampedro ◽  
Francisco José Lario ◽  
Gloria Bustingorri ◽  
...  

2020 ◽  
Vol 10 (8) ◽  
pp. 777-780 ◽  
Author(s):  
Lei Chen ◽  
Heikki Hänninen ◽  
Sergio Rossi ◽  
Nicholas G. Smith ◽  
Stephanie Pau ◽  
...  

2020 ◽  
Author(s):  
Sergey Osipov ◽  
Georgiy Stenchikov ◽  
Kostas Tsigaridis ◽  
Allegra LeGrande ◽  
Susanne Bauer ◽  
...  

<p>Volcanic eruptions trigger a broad spectrum of climatic responses. For example, the Mount Pinatubo eruption in 1991 forced an El Niño and global cooling, and the Tambora eruption in 1815 caused the "Year Without a Summer." Especially grand eruptions such as Toba around 74,000 years ago can push the Earth's climate into a volcanic winter state, significantly lowering the surface temperature and precipitation globally. Here we present a new, previously overlooked element of the volcanic effects spectrum: the radiative mechanism of stratospheric ozone depletion. We found that the volcanic plume of Toba enhanced the UV optical depth and suppressed the primary formation of stratospheric ozone from O<sub>2</sub> photolysis. Sulfate aerosols additionally reflect the photons needed to break the O<sub>2</sub> bond (λ < 242 nm), otherwise controlled by ozone absorption and Rayleigh scattering alone during volcanically quiescent conditions. Our NASA GISS ModelE simulations of the Toba eruption reveal up to 50% global ozone loss due to the overall photochemistry perturbations of the sulfate aerosols. We also consider and quantify the radiative effects of SO<sub>2</sub>, which partially compensated for the ozone loss by inhibiting the photolytic O<sub>3</sub> sink.</p><p>Our analysis shows that the magnitude of the ozone loss and UV-induced health-hazardous effects after the Toba eruption are similar to those in the aftermath of a potential nuclear conflict. These findings suggest a “Toba ozone catastrophe" as a likely contributor to the historic population decline in this period, consistent with a genetic bottleneck in human evolution.</p>


2020 ◽  
Vol 457 ◽  
pp. 117730 ◽  
Author(s):  
Qiu-Yue He ◽  
Mei-Jie Yan ◽  
Yoshiyuki Miyazawa ◽  
Qiu-Wen Chen ◽  
Ran-Ran Cheng ◽  
...  

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