Report On a Conference of Dynamics of Ionized Media
Report On a Conference of Dynamics of Ionized Media
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In our eReader you can find the full English version of the book. Read Report On a Conference of Dynamics of Ionized Media Online - link to read the book on full screen. Our eReader also allows you to upload and read Pdf, Txt, ePub and fb2 books. In the Mini eReder on the page below you can quickly view all pages of the book - Read Book Report On a Conference of Dynamics of Ionized Media
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Chapman and Ferraro studied the motion of an extremely rare ionized stream in the presence of the earth's magnetic field. They first asstuned 1. = ^J" E which was wrong. This assumption was modified in later work. Put p = m V + e kjc, If H = at the start, then p = - grad ^ and the law of conductivity is similar to that for superconductors: caxl i = - He^ H/mc^, Here H Is the number of the ions. Now curl H « Utt 1 80 that curl curl H = - UtT Ne ^mo, and since V»H » 0, It follows that V ^ H « Utt... He^ H/iac^ -17- The solution of this is H = H e — — o -Xx where X^ = Utt Ne^/mc^ The depth necessary to reduce the current to e~ times its level is d = 5, 5 X 10^ N'^/^ cms.
For actual cases this is 5 x 10 cm. Since the thickness of the stream is 11 12 10 - 10 cm, , then the inside of the stream is shielded hy a current sheath.
As the stream approaches the earth, there is a retardation of the front so that a hollow space Is formed.
earth \ et^^, tfc^e« This hollow thickens the ma^etic lines of force and so increases the mRgnetic field.
What to read after Report On a Conference of Dynamics of Ionized Media?
You can find similar books in the "Read Also" column, or choose other free books by Bernard Friedman to read onlineMoreLess
To quickly assess the difficulty of the text, read a short excerpt:
Chapman and Ferraro studied the motion of an extremely rare ionized stream in the presence of the earth's magnetic field. They first asstuned 1. = ^J" E which was wrong. This assumption was modified in later work. Put p = m V + e kjc, If H = at the start, then p = - grad ^ and the law of conductivity is similar to that for superconductors: caxl i = - He^ H/mc^, Here H Is the number of the ions. Now curl H « Utt 1 80 that curl curl H = - UtT Ne ^mo, and since V»H » 0, It follows that V ^ H « Utt... He^ H/iac^ -17- The solution of this is H = H e — — o -Xx where X^ = Utt Ne^/mc^ The depth necessary to reduce the current to e~ times its level is d = 5, 5 X 10^ N'^/^ cms.
For actual cases this is 5 x 10 cm. Since the thickness of the stream is 11 12 10 - 10 cm, , then the inside of the stream is shielded hy a current sheath.
As the stream approaches the earth, there is a retardation of the front so that a hollow space Is formed.
earth \ et^^, tfc^e« This hollow thickens the ma^etic lines of force and so increases the mRgnetic field.
What to read after Report On a Conference of Dynamics of Ionized Media?
You can find similar books in the "Read Also" column, or choose other free books by Bernard Friedman to read onlineMoreLess
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