Because fusion of any kind requires VERY high temperature and pressure, which can take place only in the core of a star.
When hydrogen stocks run out
The fusion of Hydrogen into Helium.
The helium in the Sun's core does not undergo fusion because it primarily consists of helium-4, which is a product of hydrogen fusion. While temperatures and pressures in the core are extremely high, the conditions required for helium fusion—such as even higher temperatures (around 100 million Kelvin) and sufficient density—are not met until much of the hydrogen has been fused into helium. Helium fusion, known as the triple-alpha process, will occur later in the Sun’s life cycle, once it exhausts its hydrogen fuel.
The fusion of Hydrogen into Helium causes heat and radiation to occur.
Helium is formed in the universe through nuclear fusion processes that occur in stars. During the fusion of hydrogen atoms in the core of a star, helium is produced as a byproduct. This process releases a large amount of energy and is responsible for the creation of helium in the universe.
When two hydrogen atoms fuse to become one helium atom.
In stars. As far as I know this is the only place.
Not enough pressure or temperature.
Hydrogen fusion does not occur in the corona of the sun. Fusion reactions occur in the sun's core where conditions are hot and dense enough for hydrogen nuclei to combine to form helium, releasing energy in the process. The corona is cooler and less dense than the core, so fusion cannot take place there.
In the core of the Sun, hydrogen atoms fuse to form helium in a process known as hydrogen fusion. This is the primary fusion process occurring in the Sun. As the core hydrogen is depleted, helium fusion into heavier elements like carbon and oxygen will occur in later stages of the Sun's evolution.
Nuclear fusion occurs in the solar core.
Most likely, that will be helium fusion. This is expected to occur when most of the hydrogen in the core has burnt out, and the Sun has expanded into a red giant. The core will then contract, its own weight no longer supported by hydrogen fusion, until the temperature and density has reached sufficient levels to initiate helium fusion. It is expected that the helium fusion will proceed at an initially uncontrolled rate, producing a helium flash. The sun probably has not enough mass to also reach critical levels required for carbon fusion, which would be the next stage in more massive stars.