Javascript must be enabled to continue!
Two severe famines (1809–1810, 1814–1814) in Korea during the last stage of the little ice age (1809–1819)
View through CrossRef
Abstract. From the eruption of an unknown volcano in 1809 until that of Tambora in April 1815, large and small volcanoes erupted in succession, causing various climatic changes around the Earth. During this period, the monsoon climate zone of East Asia, including Korea, had a very dry summer, and the rice yield was very poor, which resulted in two severe famines that lasted until early summer in the following years. During the famines in 1809–1810 and 1814–1815, about 24 percent of the population of Korea (approx. 14 million people) died. The severity of the drought varied widely depending on the region in Korea. Famine was more severe in the southern region, due to the higher degree of drought than in the northern region that suffered less of a drought and reported a fewer number of deaths. Based on the works of a Korean bureaucrat-scholar, Chŏng Yak-yong, this article shed lights on the famines in Chŏlla-do Province, caused by the droughts in the last stages of the “little ice age” (1809–1819).
Title: Two severe famines (1809–1810, 1814–1814) in Korea during the last stage of the little ice age (1809–1819)
Description:
Abstract.
From the eruption of an unknown volcano in 1809 until that of Tambora in April 1815, large and small volcanoes erupted in succession, causing various climatic changes around the Earth.
During this period, the monsoon climate zone of East Asia, including Korea, had a very dry summer, and the rice yield was very poor, which resulted in two severe famines that lasted until early summer in the following years.
During the famines in 1809–1810 and 1814–1815, about 24 percent of the population of Korea (approx.
14 million people) died.
The severity of the drought varied widely depending on the region in Korea.
Famine was more severe in the southern region, due to the higher degree of drought than in the northern region that suffered less of a drought and reported a fewer number of deaths.
Based on the works of a Korean bureaucrat-scholar, Chŏng Yak-yong, this article shed lights on the famines in Chŏlla-do Province, caused by the droughts in the last stages of the “little ice age” (1809–1819).
Related Results
Ground ice detection and implications for permafrost geomorphology
Ground ice detection and implications for permafrost geomorphology
Most permafrost contains ground ice, often as pore ice or thin veins or lenses of ice. In certain circumstance, larger bodies of ice can form, such as ice wedges, or massive lenses...
Ice Management for Floating Ice Offshore Operations
Ice Management for Floating Ice Offshore Operations
Abstract
This paper describes the practicalities and principles of use of icebreakers in support of ice offshore operations, and specifically their efficiency in ...
Modelling very recent ice ages on Mars with the Planetary Climate Model
Modelling very recent ice ages on Mars with the Planetary Climate Model
Protected by centimeters of dry sediments, a planetary-scale mantle of relatively pure water ice covers the entire mid and high latitudes of Mars. Its presence down has been shown ...
Constraining Ceres' exposed ice: grain size, abundance, and is it salty?
Constraining Ceres' exposed ice: grain size, abundance, and is it salty?
Ubiquitous phyllosilicates and carbonates in Ceres’ surface regolith reveal extensive water-rock interaction in the past [1]. A key area of continued study is the water i...
Two severe famines (1809–1810, 1814–1815) in Korea during the last stage of the Little Ice Age
Two severe famines (1809–1810, 1814–1815) in Korea during the last stage of the Little Ice Age
Abstract. From the eruption of an unknown volcano in 1809 until that of Tambora in April 1815, large and small volcanoes erupted in succession, causing various climatic changes aro...
Effect of ocean heat flux on Titan's topography and tectonic stresses
Effect of ocean heat flux on Titan's topography and tectonic stresses
INTRODUCTIONThe thermo-mechanical evolution of Titan's ice shell is primarily controlled by the mode of the heat transfer in the ice shell and the amount of heat coming from the oc...
Viscous relaxation of Pluto's ice shell below Sputnik Planitia
Viscous relaxation of Pluto's ice shell below Sputnik Planitia
AbstractThe surface of Pluto is dominated by the Sputnik Planitia basin, possibly caused by an impact ~ 4 Gyr ago. To explain basin's unlikely position close to tidal axis with Cha...
Grain growth of polycrystalline ice doped with soluble impurities
Grain growth of polycrystalline ice doped with soluble impurities
The grain size of polycrystalline ice affects key parameters related to planetary evolution such as the rheological and dielectric properties of Earth's glaciers and ice sheets as ...

