How the tilt of the earth's axis and the revolution cause changes in the altitudes of the midday sun at different times of the year?

The tilt of the Earth's axis (approximately 23.5 degrees) and its revolution around the Sun result in varying angles of sunlight received at different times of the year. During summer in a given hemisphere, the Sun appears higher in the sky at noon, leading to increased solar intensity and longer daylight hours. Conversely, in winter, the Sun is lower in the sky, resulting in shorter days and less intense sunlight. This seasonal variation in the altitude of the midday Sun is a direct consequence of the Earth's axial tilt and its orbital position around the Sun.