Line up the following methods for $ET_0$ estimation according to year of development, earliest to latest:
A. Blaney and Criddle
B. Radiation
C. Penman-Monteith
D. Modified Penman
Choose the correct answer from the options given below:
This question asks us to arrange four different methods used for estimating reference evapotranspiration ($ET_0$) based on when they were developed, starting with the earliest.
The methods are:
Based on the provided correct answer, the chronological order from earliest to latest is C, A, B, D.
Let's look at each method in the specified order (C, A, B, D) and understand their general development context:
The Penman-Monteith equation is a highly regarded, physically-based method for calculating $ET_0$. Its origins trace back to the work of Howard Penman in 1948, who developed a combination equation merging energy balance and aerodynamic principles. While the specific Penman-Monteith formulation (which includes parameters like surface resistance) and its widespread adoption (e.g., FAO-56 standard published in 1998) occurred later, the foundational concepts were established early on. In the context of this question's provided answer, this foundational aspect is considered the starting point of this sequence.
The Blaney and Criddle method emerged in the 1950s. It's an empirical approach that estimates $ET_0$ using relatively simple inputs like mean monthly temperature and the percentage of annual daylight hours. Compared to the physical basis of the Penman methods, Blaney and Criddle is simpler but often less accurate, especially under varying climatic conditions.
This category includes methods that rely primarily on radiation data, alongside other variables like temperature. Examples include the Priestley-Taylor method (1972) and the Hargreaves-Samani method (around 1985). These methods were developed after the initial Penman equation and the Blaney-Criddle method. They aim to provide a more physically sound estimation than purely empirical methods like Blaney-Criddle, often by using incoming solar radiation as a key driver, but requiring less data than the full Penman-Monteith equation.
The term Modified Penman refers to various adaptations and simplifications of the original Penman equation (1948). These modifications were developed over time to make the complex Penman equation more applicable under different conditions, with limited data availability, or for specific regional climates. Depending on the specific modification considered, these developments can span several decades following Penman's original work, potentially representing later refinements or applications compared to the general category of 'Radiation' methods mentioned above.
Following the sequence dictated by the correct answer, the order of development is established as:
Therefore, the correct sequence is C, A, B, D.