DIP
The altitude of an object in the sky is the angular distance of the object above the observer's horizon. It is measured in degrees or radians from the horizon to the object.
Altitude of a celestial body is the angular distance between the horizon and the body when viewed from a specific location on Earth. It is measured in degrees and ranges from 0° at the horizon to 90° at the zenith, directly overhead.
The angular distance from the horizon to the height of a celestial object is known as its altitude. It is measured in degrees, ranging from 0° at the horizon to 90° at the zenith (directly overhead). This measurement helps observers determine how high an object appears in the sky, which is essential for navigation and astronomy.
radio signal bents around the curvature of earth and hence travel longer distance than the line of sight signal. At ultra high frequencies signal follows the line of sight path and hence maximum communication distance is limited due to curvature of earth for given height of transmitting and receiving antenna
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The altitude of an object in the sky is the angular distance of the object above the observer's horizon. It is measured in degrees or radians from the horizon to the object.
The appearance of a flat horizon when viewed from a distance is caused by the curvature of the Earth.
Altitude of a celestial body is the angular distance between the horizon and the body when viewed from a specific location on Earth. It is measured in degrees and ranges from 0° at the horizon to 90° at the zenith, directly overhead.
The angular distance from the horizon to the height of a celestial object is known as its altitude. It is measured in degrees, ranging from 0° at the horizon to 90° at the zenith (directly overhead). This measurement helps observers determine how high an object appears in the sky, which is essential for navigation and astronomy.
radio signal bents around the curvature of earth and hence travel longer distance than the line of sight signal. At ultra high frequencies signal follows the line of sight path and hence maximum communication distance is limited due to curvature of earth for given height of transmitting and receiving antenna
If the reference point and an object are both on the horizon then the angular distance to the object, relative to the reference point is simply the angle formed between the two rays from the observer to object and to the reference point. If either the object or reference point (or both) are not in the plane of the horizon then the appropriate rays are the projections of the rays from the observer onto the plane containing the horizon.
Azimuth is the horizontal angular distance measured clockwise from true north, while altitude is the vertical angular distance above the horizon. Together, these coordinates help locate a star's position in the sky.
To get an "approximate" distance to the oceanic horizon from a particular observation point, take the square root of the height of the observation point, add 22.5%, and that will give you the distance in statute miles. For example, if your eyes were 6 feet off the ground, and you stood atop a 50' tower, your observation point would be 56'. The square root of 56' is 7.48. Add 22.5% of 7.48 (1.68) to 7.48 and you have 9.16 statute miles from your eyes to the horizon.
You need to get to a sufficiently high altitude or distance from the Earth to being to see the curvature. A minimum heihgt of around 60 to 70,000 ft is required to be able the see the curvature of the horizon.
Because the earth is a sphere. The horizon is the curvature of the earth (or other planet) as it falls away from you.
The horizon appears to recede as you move towards it because of the curvature of the Earth. This curvature makes it seem like the horizon is always at a distance, no matter how far you travel towards it.
If you can see the horizon in the distance (like on a ship) you can notice the curvature of the earth. It's harder to notice when buildings and hills are in the way.