It might be. It is difficult to achieve accuracy in these types of experiments.
FE sun cannot be at 700 miles and 3,000 miles at the same time. He made a mistake didn't he?
Nor can the sun be 3,391,200 and 12,376,800 miles at the same time under the Round Earth model. The discrepancy is clearly due to issues in accuracy.
Nobody here has been quoted to say that the sun is 3,391,200 or 12,376,800 miles away. On the other hand YOU have been quoted at 3,000 miles and here is Cartesian showing you that your highly regarded Rowbotham calculated 700 miles. RE'ers do respect the process of science and we also recognize that these numbers can change when experiments are done incorrectly. Today things are different though. Today we can use radar signals to find the distance to Venus. Signals sent from earth will bounce off the surface of Venus and then travel back to earth where we can detect them. Because radar travels at the speed of light (a quantity that is well known from laboratory experiments) you can easily calculate the distance between Venus and Earth at any time.
distance = 0.5*(time for radar to travel both ways)*(speed of light)
Now that we know the distance to Venus we can calculate the distance from the Earth to the Sun using trigonometry. Both Venus and Earth travel in almost perfect circles around the earth, so this is a fairly easy calculation. It might help to envision the situation if you draw two concentric circles on a piece of paper to represent the orbits of the Venus and Earth. Now imagine that the earth is set at one position in its orbit, as Venus travels along its orbit there are two points where the Venus-Sun line and the Earth-Sun are perpendicular (90 degrees apart). From our perspective on earth this is the point where Venus is the farthest it will get from the Sun. By keeping track of Venus over time we determine exactly when this will happen. When this happens we make the radar measurements mentioned above and we also measure the angle between the Sun and Venus at this point (here's where the trigonometry comes in!). It turns out that the distance from the Sun to the Earth is:
(distance of Sun-Earth) = (distance of Earth-Venus)*(cosine(angle))
This is how we get the distance of Sun-Earth to be 92,955,830 miles! This is also known as one astronomical unit (AU).
source:
http://www.ucolick.org/~mountain/AAA/aaawiki/doku.php?id=what_is_the_easiest_way_to_measure_the_distance_between_the_earth_and_the_sun