How Is Current Density Calculated for Protons in the Solar Wind?

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Homework Help Overview

The discussion revolves around calculating the current density of protons in the solar wind, specifically near Earth, where the density and speed of protons are provided. The problem involves understanding the relationship between current density, charge density, and particle velocity.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss the formula for current density (J = nqv) and the interpretation of the number density (n) of protons. There is a focus on unit conversions and the correct application of given values. Some participants express confusion regarding the interpretation of density and the calculations involved.

Discussion Status

Some participants have provided insights into the correct interpretation of the number density of protons, while others are seeking clarification on their calculations and conversions. There is an ongoing exploration of the problem, with no clear consensus yet on the correct approach or solution.

Contextual Notes

Participants are working under the constraints of specific units (cm-3 to m-3 and km/s to m/s) and are addressing potential misunderstandings regarding the density of protons in the solar wind.

Sanjay101
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Near Earth, the density of protons in the solar wind (a stream of particles from the Sun) is 8.90 cm-3 and their speed is about 490 km/s.

(a) Find the current density of these protons.(b) If Earth's magnetic field did not deflect the protons, what total current would Earth receive?For part a I used Current density (J) = nqv, we know q and v. I tried finding n(number of protons) by finding the volume by m/density. Then using Avogadro's number/volume to get n.

For part b I said that the Current would just me Part a answer multiplied by the cross sectional area, but i did not get part a right.
 
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Sanjay101 said:
Near Earth, the density of protons in the solar wind (a stream of particles from the Sun) is 8.90 cm-3 and their speed is about 490 km/s.

For part a I used Current density (J) = nqv, we know q and v. I tried finding n(number of protons) by finding the volume by m/density. Then using Avogadro's number/volume to get n.

In n.q.v, n represents the NUMBER density (that means, the number of charges with charge q per unit of volume). In this case, this would mean the number of protons per m^3, or per cm^3 (depending on the unit system in which you work). But that's given! The solar wind consists of 8.9 PROTONS per cubic cm (and not, as you seem to think, 8.9 GRAM of protons per cubic cm - which would be a terribly dense charge density!)
 
o, i cannot believe i mistook that info. Thanks.
 
im having trouoble with part a myself i am using vne=J
i have to convert km/s to m/s cm^-3 to m^-3 and e is 1.6e-19

i plug
500000*840*1.6x10^-19 but its wrong can i get help U_U ?
 

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