TL; DR

Around $8$ kg.

You can calculate the tidal force using Newton's law of gravitation, $$F = G\frac{m_1m_2}{r^2}$$ where $G$ is the universal gravitational constant, $m_1$ and $m_2$ are the masses of the two bodies, and $r$ is the distance between the body centres.

It is often convenient to work with gravitational acceleration. Now $F=ma$, so the gravitational acceleration due to a body of mass $M$ is simply $$a = \frac{GM}{r^2}$$ As Wikipedia mentions, it's hard to measure $G$, but it's easy to obtain quite precise values of $GM$ for bodies with satellites. According to JPL Horizons, $GM$ for Jupiter is $126686531.9\,\rm{km^3/s^2}$.

The tidal force is a differential force. For this scenario with Earth orbiting Jupiter, we need to calculate the force due to Jupiter at the centre of the Earth and subtract that from the force due to Jupiter at the surface of the Earth. So the tidal acceleration at the surface of the Earth is $$a = GM\left(\frac1{(R+\Delta r)^2} - \frac1{R^2}\right)$$ where $R$ is the orbital radius ($128000$ km), and $\Delta r$ is the radius of the Earth ($6378.1$ km).

Wikipedia gives an approximation equation, which is ok when $\Delta r$ is much smaller than $R$: $$a = 2\Delta r GM / R^3$$

We're using units of km, so we need to multiply the results by $1000$ to convert the acceleration to $\rm{m/s^2}$. And we can divide by $g = 9.80665\,\rm{m/s^2}$ to express the result in terms of standard Earth gravity.

Using that formula, I get $$a \approx 0.0785780\,\rm{m/s^2} = 0.0785780\,g$$ Thus a $100$ kg person would feel roughly $7.86$ kg lighter when Jupiter is directly above or below them.

Using the more accurate equation, $$a = 0.83226 \,\rm{m/s^2} = 0.084867\,g$$ when Jupiter is at the zenith, and $$a = 0.71659 \,\rm{m/s^2} = 0.073072\,g$$ when Jupiter is at the nadir.

These calculations are only approximate. If Earth were in that orbit, its shape would change due to the tidal force.

TL; DR

Around $8$ kg.

You can calculate the tidal force using Newton's law of gravitation, $$F = G\frac{m_1m_2}{r^2}$$ where $G$ is the universal gravitational constant, $m_1$ and $m_2$ are the masses of the two bodies, and $r$ is the distance between the body centres.

It is often convenient to work with gravitational acceleration. Now $F=ma$, so the gravitational acceleration due to a body of mass $M$ is simply $$a = \frac{GM}{r^2}$$ As Wikipedia mentions, it's hard to measure $G$, but it's easy to obtain quite precise values of $GM$ for bodies with satellites. According to JPL Horizons, $GM$ for Jupiter is $126686531.9\,\rm{km^3/s^2}$.

The tidal force is a differential force. For this scenario with Earth orbiting Jupiter, we need to calculate the force due to Jupiter at the centre of the Earth and subtract that from the force due to Jupiter at the surface of the Earth. So the tidal acceleration at the surface of the Earth is $$a = GM\left(\frac1{(R+\Delta r)^2} - \frac1{R^2}\right)$$ where $R$ is the orbital radius ($128000$ km), and $\Delta r$ is the radius of the Earth ($6378.1$ km).

Wikipedia gives an approximation equation, which is ok when $\Delta r$ is much smaller than $R$: $$a = 2\Delta r GM / R^3$$

We're using units of km, so we need to multiply the results by $1000$ to convert the acceleration to $\rm{m/s^2}$. And we can divide by $g = 9.80665\,\rm{m/s^2}$ to express the result in terms of standard Earth gravity.

Using that formula, I get $$a \approx 0.0785780\,\rm{m/s^2} = 0.0785780\,g$$ Thus a $100$ kg person would feel roughly $7.86$ kg lighter when Jupiter is directly above or below them.

Using the more accurate equation, $$a = 0.83226 \,\rm{m/s^2} = 0.084867\,g$$ when Jupiter is at the zenith, and $$a = 0.71659 \,\rm{m/s^2} = 0.073072\,g$$ when Jupiter is at the nadir.

These calculations are only approximate. If Earth were in that orbit, its shape would change due to the tidal force.

And of course, it's not safe for humans to be near Jupiter. It's too cold, and the radiation is too intense. Jupiter's radiation belts are huge, and far more energetic than Earth's. See The in-situ exploration of Jupiter’s radiation belts for details.