The hemisphere tilted towards the Sun has longer days and shorter nights. That's why days are longer during the summer than during the winter. In general, the further away from the equator you travel, the cooler summer and winter temperatures become. Angle of solar radiation and temperature at higher latitudes, the angle of solar radiation is smaller, causing energy to be spread over a larger area of the surface and cooler temperatures. The higher latitudes have a greater temperature range with a peak in July and January. The temperature lags the solstice as the atmosphere responds to the heating of the surface. The ocean heats up more slowly than land because water has a higher specific heat capacity. Climate change is occurring faster in high-latitude regions due to the phenomenon of Arctic amplification, the positive feedback effects that spur further warming of the climate. For example: Sea ice reflects the sun's rays back into space, reflecting more heat than it absorbs, which helps keep the planet cool. A second factor relating to sun angle, which helps make the high latitudes cooler, is the depth of atmosphere that the sun's rays must pass through on the way to the earth's surface. Because at high latitudes the sun is lower in the sky, it shines through the atmosphere on a slanting path.
Places at Earth's higher latitudes have more extreme seasonal changes in temperature than places at lower latitudes due to several factors:
The tilt of the Earth's axis: The Earth is tilted on its axis at an angle of approximately 23.5 degrees. As a result, at higher latitudes, the angle at which sunlight hits the Earth's surface changes more dramatically throughout the year. In the summer, the angle of sunlight is more direct and intense, leading to warmer temperatures, while in the winter, the angle of sunlight is more oblique and less intense, leading to cooler temperatures.
Day length: At higher latitudes, the length of daylight varies more dramatically throughout the year. During the summer months, there are more hours of daylight, which allows for more time for solar energy to be absorbed and for temperatures to warm up. Conversely, during the winter months, there are fewer hours of daylight, which means less time for solar energy to be absorbed and for temperatures to warm up.
Atmospheric circulation patterns: Atmospheric circulation patterns, such as the jet stream and prevailing winds, can also contribute to more extreme seasonal changes in temperature at higher latitudes. These circulation patterns can create temperature gradients that lead to cold air masses from the poles moving southward, leading to colder temperatures.
Overall, the combination of these factors leads to more extreme seasonal changes in temperature at higher latitudes, while places at lower latitudes tend to experience more consistent temperatures throughout the year.
The factor relating to sun angle, which helps make the high latitudes cooler, is the depth of atmosphere that the sun's rays must pass through on the way to the earth's surface. Because at high latitudes the sun is lower in the sky, it shines through the atmosphere on a slanting path. Angle of solar radiation at higher latitudes is smaller, causing energy to be spread over a larger area of the surface and cooler temperatures. At higher latitudes, the Sun's rays are less direct. The farther an area is from the equator, the lower its temperature. At the poles, the Sun's rays are least direct. Much of the area is covered with ice and snow, which reflect a lot of sunlight. The Earth receives the most solar radiation at the Equator and the least solar radiation at the Poles. Therefore, the warm temperatures experienced at the Equator are due to the intense solar radiation that is experienced year round relative to the Poles. Due to the spherical shape of the Earth, sunlight falls on different parts at different angles. Direct and focused sun rays falls on the equator and hence, the regions here are hotter and warmer.