"when they both are in the same direction?" is not all that clear to me. Who is in which direction, and who else ?
In your second problem, a conceptual dwelling becomes a bit clearer.
Basically, there is no Fc. For an object to execute a circular motion, some force has to play that role.
In the first problem, the horizontal component of the normal force plays that role. Hence also the equality Nc sin θ = mv^2 / r.
In the second problem, the vertical component of the gravitational force plays that role. Not all of it, so there remains some normal force. (**)
A "much better" (ahem) way to write this would be mg - N = the force to cause a circular motion.
Since we generally like short notation, we often use Fc for "the force to cause a circular motion", so now that name is back again. But remember it is shorthand for "the force to cause a circular motion" (or the force that changes the direction of the velocity vector...)
(**) Well, if v is big enough, all of mg is needed to keep the object on the circular trajectory. Increasing v beyond that, the car will loose contact with the hill, since there are no other contribuant forces that might keep it on there.
[edit] Ah, I see it's not a car but an unspecified "mass". Story doesn't change.